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A publication of the Lunar Section of ALPO Edited by David Teske: [email protected] 2162 Enon Road, Louisville, Mississippi, USA Recent issues: http://moon.scopesandscapes.com/tlo_back.html July 2020 In This Issue Online readers, ALPO Conference November 6-7, 2020 2 July 2020 3 click on images An Invitation to Join ALPO 3 for hyperlinks. Observations Received 4 By the Numbers 7 Submission Through the ALPO Image Achieve 4 When Submitting Observations to the ALPO Lunar Section 9 Call For Observations Focus-On 9 Focus-On Announcement 10 2020 ALPO The Walter H. Haas Observer’s Award 11 Sirsalis T, R. Hays, Jr. 12 Long Crack, R. Hill 13 Musings on , H. Eskildsen 14 Almost Full, R. Hill 16 Northern , H. Eskildsen 17 Northwest Moon and Horrebow, H. Eskildsen 18 A Bit of Thebit, R. Hill 19 D in the Landscape of the (and Two Kipukas?), A. Anunziato 20 On the South Shore, R. Hill 22 Focus On: The Lunar 100, Features 11-20, J. Hubbell 23 Recent Topographic Studies 43 Lunar Geologic Change Detection Program T. 120 Key to Images in this Issue 134

These are the modern Golden Days of lunar studies in a way, with so many new resources available to lu- nar observers. Recently, we have mentioned Robert Garfinkle’s opus Luna Cognita and the new lunar map by the USGS. This brings us the updated, 7th edition of the Virtual Moon . These are all wonderful resources for your lunar studies.

This month, The Lunar Observer features Jerry Hubbell’s Focus On article, Lunar 100, Features 11-20. This has proven to be an incredibly popular series! My new page By the Numbers (page 7) tells of 34 ob- servers submitting 215 lunar observations for this issue. Many of those images grace these pages, and all are in the ALPO Lunar Image Gallery. Also be sure to check out page 10, the 2020 ALPO Walter H. Haas Observer’s Award. All this, plus articles by Alberto Anunziato, Rik Hill, Howard Eskildsen and Tony Cook. Enjoy and be safe.

The Lunar Observer/July 2020/ 1

ALPO Conference November 6-7, 2020

Interested parties are hereby invited to submit papers and research posters on the astronomy-related topics of their choice for presentation at the next ALPO conference to be held jointly with the Georgia Regional As- tronomers Meeting (GRAM) when that group meets on November 6 and 7, 2020.

This will be the second time the ALPO has participated with the GRA group, the first time being the autumn of 2017.

Like last time, the was made after an online discussion and vote by the ALPO board of directors.

This year's conference will be at North Georgia College in , Georgia, approximately a one-and-a-half- hour drive north of downtown Atlanta. The ALPO portion of the conference will commence with the ALPO board meeting on Friday, November 6, to be followed by an informal gathering that evening with a lecture, social gathering with snacks and observing at the school’s on-campus observatory.

All papers will be presented the following day, Saturday, November 7, between 9 a.m. and 5 p.m.

Also as we did in 2017, there will be an ALPO dinner on Saturday evening where the Walter Haas Observ- ing Award and the Peggy Haas Service Award will be presented.

We have been allotted up to at least four (4) time slots for ALPO papers of no more than 15 minutes in length; the preferred method is 12 minutes for the paper presentation plus 3 minutes for follow-up questions. The preferred format is Microsoft PowerPoint.

We have also been invited to participate with wall-mounted research posters which are also commonly done at academic and professional conferences everywhere.

Participants are encouraged to submit research papers, presentations, and experience reports concerning var- ious aspects of Earth-based observational astronomy. Suggested topics for papers and presentations include the following: • New or ongoing observing programs and studies, specifically, how those programs were designed, im- plemented and continue to function. • Results of personal or group studies of solar system or extra-solar system bodies. • New or ongoing activities involving astronomical instrumentation, construction or improvement. Challenges faced by Earth-based observers such as changing interest levels, deteriorating observing condi- tions brought about by possible global warming, etc. A hard-copy version of your paper should be made available for future web site publication.

More details about paper presentations and to whom they should be sent will be published in the Summer issue of the ALPO Journal for release in early June.

The Lunar Observer/July 2020/ 2

Lunar Calendar July 2020

Date Time UT Event July 2020 5 Moon greatest southern declination -24.1o 5 0444 5 2200 1.9o north of Moon 6 0900 2o north of the Moon 6 East limb most exposed +5.0o 11 North limb most exposed +6.8o 11 2000 2.0o north of the Moon 12 1900 Moon at apogee 404,199 km 12 2329 Last Quarter Moon 17 0700 3o south of the Moon 19 West limb most exposed -5.4o 19 Moon greatest northern declination +23.9o 20 1733 Lunation 1207 25 South limb most exposed -6.7o 25 0500 Moon at perigee 368,361 km 27 1232 First Quarter Moon

The Lunar Observer welcomes all lunar related images, drawings, articles, reviews of equipment and reviews of books. You do not have to be a member of ALPO to submit material, though membership is highly encouraged. Please see below for membership and near the end of The Lunar Observer for submission guidelines.

Comments and suggestions? Please send to David Teske, contact information page 1. Need a hard copy, please contact David Teske.

AN INVITATION TO JOIN THE A.L.P.O.

The Lunar Observer is a publication of the Association of Lunar and Planetary Observers that is available for access and participation by non- members free of charge, but there is more to the A.L.P.O. than a monthly lunar newsletter. If you are a nonmember you are invited to join our organization for its many other advantages. We have sections devoted to the observation of all types of bodies found in our solar system. Section coordinators collect and study members’ observations, correspond with observers, encourage beginners, and contribute reports to our Jour- nal at appropriate intervals. Our quarterly journal, The Journal of the Association of Lunar and Planetary Observers-The Strolling Astronomer, contains the results of the many observing programs which we sponsor including the drawings and images produced by indi- vidual amateurs. Additional information about the A.L.P.O. and its Journal is on-line at: http://www.alpo-astronomy.org. I invite you to spend a few minutes browsing the Section Pages to learn more about the fine work being done by your fellow amateur astronomers. To learn more about membership in the A.L.P.O. go to: http://www.alpo- astronomy.org/main/member.html which now also provides links so that you can enroll and pay your membership dues online.

The Lunar Observer/July 2020/ 3

Lunar Topographic Studies

Acting Coordinator – David Teske - [email protected]

Assistant Coordinator – William - [email protected]

Assistant Coordinator – Jerry Hubbell – [email protected] Assistant Coordinator-Wayne Bailey– [email protected] Website: http://moon.scopesandscapes.com/

Observations Received

Name Location and Organization Article/image Aylen Borgatello Alaniz AEA - Oro Verde, Entre Rios, Ar- Image of (2), Proclus and gentina . Jay Worth, Florida, USA Images of , (2), and drawing of Posido- nius. Alberto Anunziato Paraná, Argentina, SLA Article and drawing Euclides D in the Landscape of Mare Cognitum (and Two Kipukas?), images of Peta- vius (2), Aristarchus (2), Gassendi (3), Sinus Iridum (2) and Jorge. Arranz Lunar Group of the Madrid Astro- Drawing of Gassendi. nomical Association (AAM), Ma- drid, Spain Sergio Babino Montevideo, Uruguay Image of Tycho, Proclus, Gassendi, Vallis Schröteri (3), Mare Serenita- tis (2), Vallis Alpes and . Francisco Alsina Cardinalli Oro Verde, Argentina, SLA Images of Aristarchus (7), Proclus (6), Gassendi, Sinus Iridum, Recta (3), Vallis Schröteri (4), (4), Vallis Alpes and Po- sidonius (2). Jairo Chavez Popayán, Colombia, SLA Image of Gassendi, Sinus Iridum, Vallis Schröteri and Mare Serenitatis David Emiliano Gonzalez Cian AEA - Oro Verde, Entre Rios, Ar- Image of Aristarchus, , gentina Langrenus and . Leonardo Alberto Córdoba, Argentina Image of the waxing gibbous Moon. Michel Deconinck Aquarellia Observatory, south France Sketches and pastels of Aristarchus, Proclus, Gassendi, Sinus Iridum, Straight Wall, Petavius, Schröter’s , Dark Edges of Mare Sereni- tatis, Alpine Valley and Posidonius. Walter Ricardo Elias AEA - Oro Verde, Entre Rios, Ar- Image of (2), Aristar- gentina chus, and Plato. Desiré Godoy Oro Verde, Argentina, SLA Image of Aristarchus, Proclus and Gassendi. Many thanks for all these observations, images, and drawings.

The Lunar Observer/July 2020/ 4

Name Location and Organization Article/image Eskildsen, Howard Ocala, Florida, USA Article and image Musing on The- ophilus, Northern Moon, Northwest Moon and Horrebow, image of Mons Rumker, , Lichtenberg, Gri- maldi and Sirsalis. Fernando Gimenez Montevideo, Uruguay Image of Tycho. Fernando Gomez Montevideo, Uruguay,SAO Image of Sinus Iridum. Martín Queirolo Gomez Montevideo, Uruguay, SAO Image of Proclus, Sinus Iridum (2) and Mare Serenitatis (2) and Marcelo Mojica Gundlach Cochabamba, Bolivia, SLA Image of Gassendi, Sinus Iridum, Mare Serenitatis and Vallis Alpes (3). Robert H. Hays, Jr. Worth, Illinois, USA Drawing and article Sirsalis T. Rik Hill Tucson, Arizona, USA Image and article Almost Full, Long Crack, On the South Shore and A Bit of Thebit. Jerry Hubbell Wilderness, Virginia, USA Article Focus-On Lunar 11-20 Carlos Lobato San José de Carrasco, Uruguay, SAO Drawing of Gassendi. Ángel Manuel López Lunar Group of the Astronomical Image of Mare Serenitatis. Association from Madrid, Spain Frank Melillo Holtsville, New York, USA Image of Lunar X Luigi Morrone SNdR Luna UAI, Agerola, Italy Image of Rima , Lade, , Atlas and Hercules, Aris- toteles and , Theophilus and , Vallis Alpes, Rima Hygi- nus, , , Meton, Maurolycus, and Albate- gnius. Rafael Lara Muñoz Guatemala, Guatemala, SLA Images of Earthshine, Mare Serenita- tis, , Copernicus and Aristarchus. Cyntia Olivera Santiago del Estero, Argentina, SLA Image of Sinus Iridum. Raúl Roberto Podestá Formosa, Argentina, SLA Image of Rupes Recta. Re, Gabriel AEA - Oro Verde, Entre Rios, Ar- Image of Aristarchus (2), Gassendi gentina and . Sid, Leandro AEA - Oro Verde, Entre Rios, Ar- Image of (2), Copernicus, gentina , Waxing Gibbous Moon, Plato, Tycho, Aristarchus, Cassini and Proclus. Fernando Surà San Nicolás de los Arroyos, Argenti- Image of Proclus. na, SLA-LIADA Michael Sweetman Tucson, Arizona, USA. Sky Crest Image of Mare Crisium and Anaxag- Observatory oras.

Many thanks for all these observations, images, and drawings.

The Lunar Observer/July 2020/ 5

Observations Received

Name Location and Organization Article/image Steve Thornton Images of the Straight Wall and Ptol- emaeus. Fabio Verza UAI Italy Moon Section SNdR Luna Image of Sinus Iridum (3), Full UAI - Italy Moon, , Theophilus (3), At- las, Piccolomini (2), , Longomontanus, , Montes Apenninus (2), Last Quarter Moon, , Ptolemaeus, Coper- nicus, Clavius, , Archi- medes, Montes Recta, Plato, Pur- bach, Pythagoras, Rupes Recta (2), Bullialdus, , Waxing Crescent Moon (2), Grove, Mare Crisium, Mare Serenitatis, Burg, Janssen, , (2), Mare Tranquillita- tis, Posidonius, , Endymion, , , , Julius Caesar, Manilius, Maurolycus, Meton, Playfair and Vallis Alpes. Dennis Wilde Transit Dreams Observatory, Cam- Image of Proclus. pobello, South Carolina, USA

Many thanks for all these observations, images, and drawings.

The Lunar Observer/July 2020/ 6

July 2020 The Lunar Observer By the Numbers

This month there were 215 observation by 34 observers from 10 countries.

The Lunar Observer/July 2020/ 7

SUBMISSION THROUGH THE ALPO IMAGE ARCHIVE ALPO’s archives go back many years and preserve the many observations and reports made by am- ateur astronomers. ALPO’s galleries allow you to see on-line the thumbnail images of the submitted pictures/observations, as well as full size versions. It now is as simple as sending an email to include your images in the archives. Simply attach the image to an email addressed to [email protected] (lunar images). It is helpful if the filenames follow the naming convention : FEATURE-NAME_YYYY-MM-DD-HHMM.ext YYYY {0..9} Year MM {0..9} Month DD {0..9} Day HH {0..9} Hour (UT) MM {0..9} Minute (UT) .ext (file type extension) (NO spaces or special characters other than “_” or “-”. Spaces within a feature name should be replaced by “-”.) As an example the following file name would be a valid filename: Sinus-Iridum_2018-04-25-0916.jpg (Feature Sinus Iridum, Year 2018, Month April, Day 25, UT Time 09 hr16 min) Additional information requested for lunar images (next page) should, if possible, be included on the image. Alternatively, include the information in the submittal e-mail, and/or in the file name (in which case, the coordinator will superimpose it on the image before archiving). As always, additional commentary is always welcome and should be included in the submittal email, or attached as a separate file. If the filename does not conform to the standard, the staff member who uploads the image into the data base will make the changes prior to uploading the image(s). However, use of the recommended for- mat, reduces the effort to post the images significantly. Observers who submit digital versions of draw- ings should scan their images at a resolution of 72 dpi and save the file as a 8 1/2'“x 11” or A4 sized picture. Finally a word to the type and size of the submitted images. It is recommended that the image type of the file submitted be jpg. Other file types (such as png, bmp or tif) may be submitted, but may be converted to jpg at the discretion of the coordinator. Use the minimum file size that retains image detail (use jpg quality settings. Most single frame images are adequately represented at 200-300 kB). How- ever, images intended for photometric analysis should be submitted as tif or bmp files to avoid lossy compression. Images may still be submitted directly to the coordinators (as described on the next page). However, since all images submitted through the on-line gallery will be automatically forwarded to the coordinators, it has the advantage of not changing if coordinators change.

The Lunar Observer/July 2020/ 8

When submitting observations to the A.L.P.O. Lunar Section In addition to information specifically related to the observing program being addressed, the fol- lowing data should be included:

Name and location of observer Name of feature Date and time (UT) of observation (use month name or specify mm-dd-yyyy-hhmm or yyyy-mm-dd-hhmm) Filter (if used) Size and type of telescope used Magnification (for sketches) Medium employed (for photos and electronic images) Orientation of image: (North/South - East/West) Seeing: 0 to 10 (0-Worst 10-Best) Transparency: 1 to 6

Resolution appropriate to the image detail is preferred-it is not necessary to reduce the size of im- ages. Additional commentary accompanying images is always welcome. Items in bold are re- quired. Submissions lacking this basic information will be discarded.

Digitally submitted images should be sent to: David Teske – [email protected] Jerry Hubbell –[email protected] Wayne Bailey—[email protected]

Hard copy submissions should be mailed to David Teske at the address on page one.

CALL FOR OBSERVATIONS: FOCUS ON: Lunar 100 Focus on is a bi-monthly series of articles, which includes observations received for a specific fea- ture or class of features. The subject for the July 2020 edition will be the Lunar 100 numbers 11- 20. Observations at all phases and of all kinds (electronic or film based images, drawings, etc.) are welcomed and invited. Keep in mind that observations do not have to be recent ones, so search your files and/or add these features to your observing list and send your favorites to (both): Jerry Hubbell –[email protected] David Teske – [email protected]

Deadline for inclusion in the Lunar 100 numbers 11-20 article is June. 20, 2020

FUTURE FOCUS ON ARTICLES: In order to provide more lead time for contributors the following future targets have been selected: The next series of three will concentrate on subjects of the Selected Areas Program.

Subject TLO Issue Deadline Lunar 100 (numbers 21-30) September 2020 August 20, 2020 Lunar 100 (numbers 31-40) November 2020 October 20, 2020

The Lunar Observer/July 2020/ 9

Focus-On Announcement

We are pleased to announce the future Focus-On topics. These will be based on the Lunar 100 by Charles Wood. Every other month starting in May 2020 , the Focus-On articles will explore ten of the Lunar 100 targets. Targets 21-30 will be featured in the September 2020 The Lunar Observer. Submissions of arti- cles, drawings, images, etc. due by August 20, 2020 to David Teske and Jerry Hubbell.

L Feature Name Significance Rükl Chart 21 Crater with subsided and fractured floor 58 22 Aristarchus Plateau Uplifted region with pyroclastics 18 23 Pico Isolated Imbrium basin-ring fragment 11 24 Rille containing rimless collapse pits 34 25 Messier and Messier A Oblique ricochet-impact pair 48

26 Mare Frigoris Arcuate mare of uncertain origin 2-6

27 Archimedes Large crater lacking central peak 12, 22

28 Hipparchus First drawing of a single crater 44, 45 29 Ariadaeus Rille Long, linear graben 34 30 Schiller Possible oblique impact 71

Explore the Lunar 100 on the link below: https://www.skyandtelescope.com/observing/celestial-objects-to-watch/the-lunar-100/

The Lunar 100: Features 1-10 May 2020 Issue – Due April 20, 2020 The Lunar 100: Features 11-20 July 2020 Issue – Due June 20, 2020 The Lunar 100: Features 21-30 September 2020 Issue – Due August 20, 2020 The Lunar 100: Features 31-40 November 2020 Issue – Due October 20, 2020 The Lunar 100: Features 41-50 January 2021 Issue – Due December 20, 2020 The Lunar 100: Features 51-60 March 2021 Issue – Due February 20, 2021 The Lunar 100: Features 61-70 May 2021 Issue – Due April 20, 2021 The Lunar 100: Features 71-80 July 2021 Issue – Due June 20, 2021 The Lunar 100: Features 81-90 September 2021 Issue – Due August 20, 2021 The Lunar 100: Features 91-100 November 2021 Issue – Due October 20, 2021 Jerry Hubbell –[email protected] David Teske – [email protected]

The Lunar Observer/July 2020/ 10

Howard-

As the Chairman of the 2020 ALPO The Walter H. Haas Observer’s Award, it is my extreme pleasure to let you know that you have been selected to be the recipient of the 2020 The Walter H. Haas Observer’s Award.

The Walter H. Haas Observer’s Award is bestowed annually (generally when the ALPO meets in the sum- mer), to an amateur astronomer for excellence in observational Solar System astronomy. This award is named after our founder and original executive director and was established in 1985. The selection of this award is conducted by a committee convened by its committee chairman, Timothy Robertson. The composi- tion of the committee changes from year to year so that the responsibility of selection is shared by a wider group of members in the ALPO that are well qualified, while allowing others that vote one year, to be con- sidered for the award in another year, when not serving on the committee.

This award is given for excellence in Solar System observational amateur astronomy. Work done as part of the observer’s job must be regarded as professional work and is not considered as an amateur effort for this award. However, a professional astronomer can be recognized for work done when he or she was an ama- teur.

The Award itself consists of an engraved plaque. The awardee also receives a two-year complimentary membership in the ALPO.

This year the ALPO conference is at the University of North Georgia in Dahlonega, Georgia, where this No- vember's ALPO meeting is scheduled to be held in conjunction with the Georgia Regional Astronomers Meeting on November 6 and 7. However, with the current situation, discussions are in place on canceling or changing the dates of the event.

Congratulations of being selected as the 2020 ALPO The Walter H. Haas Observer’s Award winner.

Tim Robertson

Howard,

Congratulations on your being awarded the 2020 ALPO Walter H. Haas Observer’s award! You are very well deserving of this honor. The Lunar Observer is frequently graced with images and articles provided by you. These are always enlightening to our readers. In addition to the work with The Lunar Observer, you are a frequent contributor to the Lunar Domes Gallery with high resolution images on said domes. Along with these lunar contributions, you frequently supply the ALPO Solar Program with daily images of the Sun in white light, hydrogen alpha and calcium wavelengths. These all take much time and work to produce.

Thank you and congratulations for your award!

David Teske

The Lunar Observer/July 2020/ 11

Sirsalis T Robert H. Hays, Jr.

Sirsalis T, Robert H. Hays, Jr. Worth, Illinois, USA. 07 March 2020 0242-0326; 0344-0356 UT. 15 cm reflector, 170 x. Seeing 8-9/10, transparency 6/6.

I observed this crater and vicinity on the evening of March 6/7, 2020. This area is in far southwest . Sirsalis T is a half-crater at the southern end of a wide ridge. It is open to the southwest. This configuration resembles the end of a wrench. A detached peak is off the west end of Sirsalis T, and another peak is south of its center. Three short ridges are south of its east end. A tiny pit and a small peak are just east of the center-ridge junction, and a short ridge is to their north. A long, broken ridge is northwest of Sirsalis T. The north end of the ridge is quite substantial with interior shadowing and with small peaks near- by. There is a low half-crater well north of Sirsalis T. This crater is open to the north, nearly the opposite of Sirsalis T. Its west rim is wider but shorter than the narrow east rim. The wide, curved ridge farther to the west is Sirsalis epsilon. This is part of the broken ring Sirsalis E. Two peaks and a are to its north.

The Lunar Observer/July 2020/ 12

Long Crack Rik Hill

The Moon is almost full and it seems like there is little to see. But on the southwest is a grouping of craters that lead us to one of the longest cracks on the Moon. Near the top of the image are two overlap- ping craters. The one on the top is Sirsalis (43 km). You will notice a rima running north-south just to the right of it. This is, appropriately enough, Rimae Sirsalis, one main rima with several smaller, shorter, thin- ner ones on the side. The main Rima is 309 km long, its southern end in shadow here and the northern end of the top of this image. Just to the right of the nameplate on this image is the faintest traces of the upper edge of a crater wall. This is the crater Crüger (48 km) with the satellite crater Crüger A (27 km), the sharp crater next to the rima. Further on the same direction is a shallow flat-bottomed crater, (32 km). In the lower corner of this image is the half-illuminated crater (20 km). Lastly, is the odd dark feature on the far eastern (right) edge of this image below the overlap insert. This is , listed as 49 km diameter but it was hardly circular. It appears to be a small piece of the Oceanus Procellarum material to the north. In fact, it is the flooded remains of an ancient crater whose eastern wall rises 1.3 km above the sur- rounding interior. I’s sure this range would be an impressive sight at sunset from the flooded floor!

Sirsalis, Richard Hill, Tucson, Arizona, USA, Loudon Observatory. 04 June 2020 0550 UT, co- 66.7o. Dynamax 6 telescope plus 2x bar- low, 850 nm filter, Skyris 132M camera. Seeing 8/10.

The Lunar Observer/July 2020/ 13

Musings on Theophilus Howard Eskildsen

Theophilus dominates this image with its sharp crater rim, multiple terraces, complex central peak and pools of impact melt indicated on Figure 1 with an “I.” The area with the “?” label is also likely impact melt as well, probably first from Theophilus and later covered over by ejecta or melt from Mӓdler which lies to the lower right of the “?” label. While the cause for confusion is not readily visible in Figure 1, Figure 2 shows a close-up view from the LROC QuickMap and reveals the reason for question of origin.

Note the density of the small craters on the impact melt in the interior of Theophilus on Figure 2. Compared to the impact melt outside its north rim the crater density appears about the same, but on the area of the “?”, craterlets are nearly absent and are more like the crater density in Mӓdler. Also, the LROC image shows this area to have a darker than the other melt areas. Assuming this area contains impact melt from The- ophilus, it should have the same craterlet density as the melt on the interior of the crater and similar albedo, so something must have covered any melt from Theophilus. I suspect that impact melt, fluidized ejecta, or probably both, from Mӓdler covered over of the older deposit and changed the albedo and crater count.

The pools of impact melt outside Theophilus are located to the north and east of the crater, and the rim ele- vation is lower on those sides as well. LROC QuickMap measurements north-south and west-east paths through the central peak area show a western rim elevation of 900 meters above mean lunar radius (MLR), while the eastern rim is 890 meters below MLR, a difference of 1790 meters over a measured distance of 103 km. Similarly, the southern rim is 63 meters above MLR while the north rim is 520 meters below MLR, or 583 meters higher than the southern rim over a measured distance of 97m. I wonder if this contributed to the location of melt pools on that side or if they are simply a result of asymmetrical ejection of the melted material.

Using the LROC QuickMap measurements, the average of the two diameters is 100 km, the depth 4640 me- ters with a depth/diameter ratio of 0.046. The highest central peak measured 2780 meters above the lowest part of the crater floor. This compares to diameter of 98.59 km, depth of 4100 meters, with central peak height of 1810 as listed in Luna Cognita, page 11-26, by Robert Garfinkle. These differences are not surpris- ing since the crater is not exactly round and measurement techniques of the crater depths and central peak heights is challenging due to the uneven elevation of the crater floor, even with LROC data. Also, the rim of Theophilus is not even in elevation. The southwest rim that overlaps Cyrillus has collapsed and is nearly 800 meters lower than the western rim of the crater, so the two measurements done probably overestimate the mean rim elevation and therefore the depth of the crater.

It also raises another question, should the rim elevation be estimated using all parts of the rim, including are- as where slumping occurred, or should only the original intact rim be used to measure mean rim height and be used to calculate crater depths?

Online readers, click on images for hyperlinks.

The Lunar Observer/July 2020/ 14

Figure 1, Theophilus, Howard Eskildsen, Ocala, Florida, USA. 10 June 2020 0949 UT, colongitude 142.0 degrees. Celestron 9.25 inch Schmidt- telescope, f/10, fl 2395 mm, Celestron Skyris 236M camera. Seeing 6/10, transparency 4/6.

Figure 2, The- ophilus, Image from LROC Quickmap

The Lunar Observer/July 2020/ 15

Almost Full Rik Hill

About a day before Full Moon you can see this amazing landscape in the center of the terminator. The large dark crater just left of center is (228 km), one of the stepping stones to when the libra- tion is right. There’s a cluster of craters east (right) of Grimaldi. The easternmost one is Dam- oiseau (37 km). South of this is a well-defined crater near the bottom of the image, Sirsalis (43 km). In the lower right corner is the dark crater (48 km), distinctive for its dark floor, darker than the surrounding Oceanus Procellarum making it stick out visu- ally.

Grimaldi, Richard Hill, Tucson, Arizona, USA, Loudon Observatory. 06 May 2020 0548 UT, colon- gitude 70.0o. Dynamax 6 telescope plus barlow, 665 nm filter, Skyris 445M cam- era. Seeing 8/10.

Above Grimaldi is anoth- er large crater (109 km) with the small crater Lohrmann (32 km) just below. Above Hevelius is a deeper crater, (60 km). Notice the apparent gash between Hevelius and Grimaldi. There is a shallow valley here, seen on the LROC Quick Map, and a couple of small craters add to the effect, but it looks more dramatic than the true topography at this lighting. On both sides of Lohrmann, note the unnamed system of rimae. I’s quite surprised they are not named. Another curious gash is below to the right of Grimaldi. It appears to pass through two craters but in fact is a linear alignment of around 10 eroded craters. Then south of Grimaldi are more rimae. These are named Rimae Grimaldi. They lead into a flat area further to the south that is Rocca W (102 km). As big as Hevelius but, alas, only a satellite crater to Rocca. This is definitely a region worthy of careful examina- tion… just when you thought the Moon was almost full and there was nothing left to see!

The Lunar Observer/July 2020/ 16

Northern Moon Howard Eskildsen

This image shows favorable of the northern Moon. Just west of the terminator, a distinctive group of craters form what I think of as steppingstones to the north pole. is easy to spot above Meton at any libration, and Main overlap just above Scoresby, and beyond them lies indented by the crater Gioja. In the darkness north of Byrd lies Peary and the north pole rests on its upper rim somewhere in the darkness to the left of the center of Byrd.

A seldom-seen crater, Hermite peers from the top of the image and behind it is another surprise crater that will be revealed in the next image I send.

North Pole Region, Howard Eskildsen, Ocala, Florida, USA. 10 June 2020 0941 UT, colongitude 142.0 degrees. Celestron 9.25 inch Schmidt-Cassegrain telescope, f/10, fl 2395 mm, Celestron Skyris 236M camera. Seeing 6/10, transparency 4/6.

Online readers, click on images for hyperlinks.

The Lunar Observer/July 2020/ 17

Northwest Moon and Horrebow Howard Eskildsen

This image also shows the northwestern Moon including and beyond, with selected craters la- beled. One of the strangest craters is Horrebow. An obvious slump of the rim occurred on the southwest part of the crater, but a strange ridge appears to the northeast where it overlaps with Horrebow A. It almost ap- pears as if part of the lower rim of Horrebow A persisted in the face of the Horrebow impact, or perhaps part of Horrebow's NE rim slumped into Horrebow A. Maybe there is another explanation, but I find this to be another intriguing part of the Moon.

Northwest Moon, Howard Eskildsen, Ocala, Florida, USA. 12 June 2020 0950 UT, colongitude 166.4 degrees. Celestron 9.25 inch Schmidt-Cassegrain telescope, f/10, fl 2395 mm, Celestron Skyris 236M camera. Seeing 7/10, transparency 3/6.

The Lunar Observer/July 2020/ 18

A Bit of Thebit Rik Hill

Here we have a wonderful area on the Moon that bears a lot of study. Our crater that lends its name to this image, Thebit (60 km) is in the center with Thebit A (20 km) breaching its upper left (northwest) wall. Above this crater and a little to the right (east) is the wonderfully terraced crater (100 km) with nice rimae on its floor. A little to the northwest of this is the unusual crater (41 km) with a broad round central peak. It has been appropriately likened to an egg in a basket. Due west of Thebit you’ll see a dark slash. This is the 114 km long Rupes Recta or the “Straight Wall”. It is not terribly straight and given a little more resolution than we have here you would see that. The wall looks like an abrupt cliff but actually is fairly sloped but as we see it here it is only about 1-1.5 km wide. Consider what this is from your home. Most people can easily see a kilometer in some direction unless they live in a forest. West of this is the relatively young crater (17 km). A small rima extends to the northwest from the north wall of this crater. This is Rima Birt and it too is only about a kilometer wide!

Below Thebit is a large shallow crater, Purbach (121 km) with a very unusual central peak, probably the remnants of a previous crater wall. To the east is a flat floored crater, (70 km) and south of it is (also 70 km). Purbach lays on top of an even older crater to the south, Regiomontanus (129 km) with a central peak that has a more-or-less central crater. (No, it is not a volcano.) Lastly, we have that very circular crater with thin terraced walls in the lower right corner of the image. This is Werner (71 km) with a fresh crater and white ejecta blanket on the north inner slope. We know its fresh (relatively) because it is lighter colored. Its composed of the same material as the rest of the crater but when it’s crushed and pulver- ized it takes on a higher albedo, or reflectivity and thus look white.

Thebit, Richard Hill, Tucson, Ari- zona, USA, Loudon Observa- tory. 03 April 2020 0211 UT, colongitude 28.8o. Dynamax 6 tele- scope plus 1.5 x barlow, 610 nm filter, Skyris 132M camera. Seeing 8/10.

The Lunar Observer/July 2020/ 19

Euclides D in the Landscape of the Mare Cognitum (and Two Kipukas?) Alberto Anunziato

The intricate landscape of the Mare Cognitum is fascinating as the terminator passes through it, and oblique sunlight illuminates an expressionist setting in which the resolution of small telescopes like mine is substan- tially improved. The always remembered Peter Grego says in “The Moon and How to Observe It” (page 173): “Mare Cognitum is a dark lava plain, somewhat oval in shape, measuring 330 km from Montes Riphaeus in the northwest to its southeastern shoreline near Guericke. Mare Cognitum, the “Known Sea”, takes its name from the fact that the probe, Ranger 7, secured the first detailed close-up photographs of the Moon's surface prior to its (intended) crash-landing on the sea in July 1964”. In the sketch we can see the small Euclid D (5 kilometers in diameter) casting a long shadow to the northwest, with its bright outline, although brighter in the east than in the west. We have to imagine that the Riphaeus Mountains are located exactly to the west of the image, shining beautifully in the terminator (beautiful vision of impossible execu- tion). A dorsum extends from west to east, interrupted by Euclid D. We can venture that it is the least elevat- ed, since it is perceived only by the brightness of its elevated areas. Another shorter one extends in the same direction further north, casting partly shadow, so it would be higher than the previous one (and brighter). A third extends from north to south and is clearly the highest: brighter, with a blacker shadow and more distin- guishable shapes, at its northern end the light and shadow glimpses a crater. South of Euclid D there is an imprecise bright spot and further to the south a second one, smaller but casting a small shadow. The first one seemed to correspond to a brighter ground coloration, but the second one looks like a dome, as I can see a dome with my 105mm telescope. The search in the charts was unsuccessful. In Grego's quoted book we read that “Near its western shoreline can be found a teardrop-shaped dome 20 km long. Unique among lunar domes, it is composed of brighter material than the surrounding mare, and it can be seen under a high illumi- nation. A group of hills to its west also have a high albedo. It is possible that the dome and the nearby hills are the remnants of a submerged crater, the dome representing the crater’s central uplift”. Clearly it is not the dome quoted by Grego, which would be much larger. In "Lunar Domes. Properties and Formation Pro- cesses” (Raffaello Lena et al.), a formation is mentioned in Mare Cognitum (page 54), a kipuka “surface parts surrounded by the flooding mare lavas. Kipukas usually consist of a different material than the sur- rounding mare, such that a spectral contrast would have to be observed. A typical example of a lunar kipuka is the formation Darney Chi located in western Mare Cognitum, an elevated section of Highland terrain em- bayed by mare lava”. But Darney Crater is much further south. Perhaps it is one of the hills to which Grego refers "A group of hills to its west also have a high albedo". And these hills could be two 6-kilometer kipu- kas west of Darney Chi, according to "Lunar kipukasas evidence for an Extended Tectonic and Volcanic History of the Maria" (D.J. Nichols et. Al.). After reading the sources quoted, I was left with a bit of remorse for not having pointed out more precisely, while observing, these two oddities in that strange landscape, full of wonders, which is Mare Cognitum.

The Lunar Observer/July 2020/ 20

Euclides D, Alberto Anunziato, Paraná, Argentina. 31 May 2020 2220-2245 UT. 105 mm Maksutov-Cassegrain tele- scope (Meade EX 105), 154 x.

The Lunar Observer/July 2020/ 21

On the South Shore Rik Hill

The whole rim of Mare Nectaris is populated with wonderful features. Here we have the south side of the big scarp below and left of center stretching from the beautiful crater Piccolomini (90 km) at the bottom going all the way up past Catarina (104 km) some 495 km. You can just barely see another pressure ridge, concentric to Mare Nectaris, running from down south of the large “U” shaped crater above center, Fracastorius (128 km). Unfortunately, the nice east-west rima that bisects this crater is just beyond the resolution of this image. But there are many secondary craters on its floor and a splattering of them in the upper left covering (54 km), a little brother to Fracastorius. These secondaries are likely ejec- ta from the Theophilus impact to the north which must have been a fantastic sight!

Fracastorius, Richard Hill, Tucson, Arizona, USA, Loudon Observatory. 28 May 2020 0211 UT, colongitude 339.8o. Dynamax 6 telescope plus 2x barlow, 850 nm filter, Skyris 132M camera. Seeing 8/10.

The Lunar Observer/July 2020/ 22

Focus On: The Lunar 100 Features 11 through 20

Jerry Hubbell Assistant Coordinator, Lunar Topographical Studies

This is the second article of ten in a series on Chuck Wood’s Lunar 100 list. Chuck Wood, the founder of the Lunar Photo of the Day (LPOD) (Ref.), first discussed this in a Sky & Telescope article published in 2004, and later published on the Sky & Telescope website (Ref.). This series will run from May 2020 until January 2022. I may insert a few other topics in between this series so the end date for this series may extend out to the end of 2022. Chuck wanted this list of lunar features (L1 to L100) to be like the well-known list of Messier objects that would give lunar observers a way to progress in their study of the moon and become life-long observers. The list contains all the diverse features of the Moon including Mare, Craters, , Mountains, and Volcanic Domes. The list starts out with the naked eye view of the full disk of the Moon and progresses through more difficult features.

This series of Focus On articles is meant to be the basis for a lunar visual observing program but is not lim- ited to that. It can be the basis for starting your own image-based study of the Moon, which will enable you to use the Lunar Terminator Visualization Tool (LTVT) (Ref.), a sophisticated software program used to do topographical measurements of the lunar surface. These articles will introduce and show each of the Lunar 100 features as observed and submitted by our members through drawings, images, and narrative descrip- tions. Although you can use your naked eye and binoculars to start observing objects L1 – L20, observing objects L21 – L80 will require the use of a 3-inch (76-mm) telescope. Features at the end of the list (L81 – L100) will require a 6 to 8-inch (152 to 203-mm) telescope. Many of the features are best observed at differ- ent phases of the Moon.

One of the best ways to help you learn the features of the Moon is through sketching the lunar surface. Dur- ing this series of articles, we will highlight drawings of many of the Lunar 100 features. Springer Books publishes an excellent book, released in 2012, called Sketching the Moon (Handy, et al.) (Ref.). There are other resources on the Internet to help you get started observing and sketching the Moon including the ALPO’s excellent Handbook of the ALPO Training Program (Ref.)

In this article we continue with features 11 through 20 on Chuck’s list. This article highlights the excellent drawings of each of these features submitted by Michel Deconinck from Provence, France. Here is a list of features 11 – 20:

Designation Feature Name Description/Significance L11 Aristarchus Very Bright Crater with Dark Bands on its Walls L12 Proclus Oblique-Impact Rays L13 Gassendi Floor Fractured Crater L14 Sinus Iridum Very Large Crater with Missing Rim L15 Rupes Recta AKA “Straight Wall” - Best Example of a Lunar Fault L16 Petavius Crater with a Domed and Fractured Floor L17 Schröter's Valley Giant Sinuous Rille L18 Mare Serenitatis Distinct Mare Areas with Different Compositions L19 Alpine Valley Lunar Graben L20 Posidonius Floor Fractured Crater

The Lunar Observer/July 2020/ 23

The Lunar 100: Feature 11 and 17—Aristarchus and Schröter's Valley

Figure 1. Aristarchus & Schröter's Valley Sketch, Michel Deconinck, Artignosc-sur-Verdon, Provence, France, 09 June 2014, 2100 UT, Colongitude 53.8°, Bresser refractor 102/1000, 10mm Delos eyepiece, Magnification 100x, pas- tels Conté grey, black and white + blending stump on Canson paper 240gr black. North/Up, East/Right. Online readers, click on images for hyperlinks.

The Lunar Observer/July 2020/ 24

The Lunar 100: Feature 11 and 17—Aristarchus and Schröter's Valley

Figure 2. Ar- istarchus & Schröter's Valley, Alberto Anunziato (Paraná, Argentina, SLA), 19 June 2016 0215 UT, Colongitude 77.9°, 250 mm. Schmidt-Cassegrain (Meade LX 200), QHY5-II Camera, North/Left, East/Up.

The Lunar Observer/July 2020/ 25

The Lunar 100: Feature 12 Proclus

Figure 3. Proclus Sketch, Michel Deconinck, Artignosc-sur-Verdon, Provence, France, 04 May 2014, 2100 UT, Co- longitude 334.1°, Bresser refractor 102/1000, 26mm Bresser eyepiece, 10mm Delos eyepiece, Magnification 38x, 100x, pastels Conté grey, black and white + blending stump on Canson paper 240gr black. North/Down, East/Right.

The Lunar Observer/July 2020/ 26

The Lunar 100: Feature 12 Proclus

Figure 4. Proclus, Sergio Babino, Montevideo, Uruguay, SAO, 29 April 2020, 2244 UT, Colongitude 356.2°, 8-inch (200 mm) Schmidt-Cassegrain, Camera ZWO174mm. North/Up, East/Right.

The Lunar Observer/July 2020/ 27

The Lunar 100: Feature 13 Gassendi

Figure 5. Gassendi Sketch (rotated 180°), Jorge Arranz, Lunar Group of the Madrid Astronomical Association (AAM), Madrid, Spain, 07 March 2009, 2227 UT, Dobsonian 250mm f/5, 15 mm eyepiece, 282x magnification, pastels Conté grey, black and white + blending stump on Canson paper 240gr black. Colongitude 47.4°, North/Up, East/ Right.

The Lunar Observer/July 2020/ 28

The Lunar 100: Feature 13 Gassendi

Figure 6. Gassendi, Jerry Hubbell, Lake of the Woods Observatory (I24) Locust Grove, Virginia, USA, 04 February 2012 0058 UT, Colongitude 48.2°, Meade 10-inch LX5 Schmidt-Cassegrain, DMK21AU04AS camera. Seeing 6/10, Transparency 5/6. North/Up, East/Right.

The Lunar Observer/July 2020/ 29

The Lunar 100: Feature 14 Sinus Iridum

Figure 7. Sinus Iridum Sketch, Michel Deconinck, Artignosc-sur-Verdon, Provence, France, 05 June 2017, 1930 UT, Colongitude 45.3°, Bresser refractor152mm/1200mm, 10mm Delos eyepiece, Magnification 120x, pastels Conté grey, black and white + blending stump on Canson paper 240gr black. North/Up, East/Left

The Lunar Observer/July 2020/ 30

The Lunar 100: Feature 14 Sinus Iridum

Figure 8. Sinus Iridum, Jay Albert, Lake Worth, Florida, USA, 05 October 2019 at 0103 UT. Colongitude 345.3°, 200 mm f/10 Celestron 8” NexStar Evolution SCT, 7mm Orthoscopic eyepiece projection, iPhone 6s Camera, Seeing 5/10, Transparency 3/6 North/Up, East/Left.

The Lunar Observer/July 2020/ 31

The Lunar 100: Feature 15 Straight Wall

Figure 9. Rupes Recta “Straight Wall” Sketch, Michel Deconinck, Artignosc-sur-Verdon, Provence, France, 07 May 2014 2140 UT, Colongitude 10.8°, Bresser refractor 102/1000, 26mm Bresser eyepiece, 10mm Delos eyepiece, Mag- nification 38x, 100x, pastels Conté grey, black and white + blending stump on Canson paper 240gr black. North/Up, East/Left.

The Lunar Observer/July 2020/ 32

The Lunar 100: Feature 15 Straight Wall

Figure 10. Rupes Recta “Straight Wall”, Francisco Alsina Cardinalli, Oro Verde, Argentina, SLA. 20 December 2015 0031 UT, Colongitude 19.6°. 250 mm Meade LX200 SCT, Canon EOS Digital Rebel XS camera, North/Up, East/Right.

The Lunar Observer/July 2020/ 33

The Lunar 100: Feature 16 Petavius

Figure 11. Petavius, Alberto Anunziato, Oro Verde, Argentina, SLA, 04 March 2018 at 0748 UT. Colongitude 114.6°, 280 mm f/10 Celestron CPC 1100 SCT, Canon EOS Digital Rebel XS, Seeing 6/10, North/Up, East/Right.

The Lunar Observer/July 2020/ 34

The Lunar 100: Feature 18 Mare Serenitatis

Figure 12. Mare Serenitatis Sketch, Michel Deconinck, Artignosc-sur-Verdon, Provence, France, 05 April 2018, 2000 UT, Colongitude 150.1°, Mewlon CRS (Dall Kirkham) 250mm f10 Ethos 13mm eyepiece 192x magnification, pastels Conté grey, black and white + blending stump on Canson paper 240gr black. North/Up, East/Right.

The Lunar Observer/July 2020/ 35

The Lunar 100: Feature 18 Mare Serenitatis

Figure 13. Mare Serenitatis, Marcelo Mojica Gundlach, Cochabamba, Bolivia, SLA, 30 April 2020, 2324 UT, Colon- gitude 8.8°, 6-inch Maksutov FL=1800mm SkyWatcher, ZWO ASI178. Seeing 7/10, Transparency 5/6, North/Up, East/Right.

The Lunar Observer/July 2020/ 36

The Lunar 100: Feature 19 Alpine Valley

Figure 14. Alpine Valley Sketch, Michel Deconinck, Artignosc-sur-Verdon, Provence, France, 03 May 2020, 2115 UT, Colongitude 44.3°, Mewlon CRS (Dall Kirkham) 250mm f15 Ethos 13mm eyepiece 288x magnification, pastels Conté grey, black and white + blending stump on Canson paper 240gr black. North/Left, East/Up.

The Lunar Observer/July 2020/ 37

The Lunar 100: Feature 19 Alpine Valley

Figure 15. Alpine Valley, Marcelo Mojica Gundlach, Cochabamba, Bolivia, SLA, 05 January 2020, 2254 UT, Colon- gitude 36.2°, 6-inch Maksutov SkyWatcher FL=1800 mm, ZWO ASI178. Seeing 5/10, Transparency 5/6, North/Up, East/Right.

The Lunar Observer/July 2020/ 38

The Lunar 100: Feature 20 Posidonius

Figure 16. Alpine Valley, Jay Albert, Lake Worth, Florida, USA, 20 May 2011, 0615 UT, Colongitude 120.8°, 11- inch Celestron SCT, 311x magnification. Seeing 5/10, Transparency 4/6, Northeast/Up, Northwest/Right.

The Lunar Observer/July 2020/ 39

The Lunar 100: Feature 20 Posidonius

Figure 17. Posidonius, Sergio Babino, Montevideo, Uruguay, SAO, 14 March 2020, 0458 UT, Colongitude 145.3°, 203 mm SCT, ZWO 174mm camera, North/Up, East/Right. Once again, we had a very large response to our request for images and drawings for the second set of 10 features of the Lunar 100 (L11 – L20). As in the last article, we again had images taken with cellphone cam- eras. I am grateful for all the submissions. We had a total of 87 images and drawings submitted from over 20 astronomers. Most of the images came from Alberto Anunziato’s groups, SAO-SLA, and LIADA. Previ- ously he prefaced the images he sent on behalf of his group this way:

The Lunar Observer/July 2020/ 40

“LUNAR 100 PROGRAM Sociedad Astronómica Octante-Sociedad Lunar Argentina

When we found out that the next objectives of the Focus On Section would be the features listed in the Charles Wood's famous Lunar 100, the members from Sociedad Lunar Argenti- na (SLA) and Sociedad Astronómica Octante (SAO) of the República Oriental del Uruguay, we considered interesting to join the initiative of "The Lunar Observer" (TLO) and therefore we launched our Lunar 100 Program, under the auspices of the Lunar Section of the Liga Iberoamericana de Astronomía (LIADA). The objective is twofold. We will report the images submitted to the program to "The Lunar Observer". And we will also publish them in all the media of SLA, SAO and LIADA. We think it is a great opportunity to stimulate amateur lu- nar observation and if the call is successful, we can dream of some final joint publication.”

We look forward to future drawings and images submitted by ALPO, SLA, SAO, LIADA members. Please share with us any images you have in your image catalog, we hope to see everyone participate in these Focus On articles.

– Jerry Hubbell

COMPUTER PROGRAMS

Virtual Moon Atlas https://sourceforge.net/projects/virtualmoon/

Lunar Terminator Visualization Tool (LTVT) http://www.alpoastronomy.org/lunarupload/LTVT/ ltvt_20180429-HTML.zip

REFERENCES

Chuck Wood, The Lunar 100 (November 2012), Sky & Telescope Magazine (website), https:// skyandtelescope.org/observing/celestial-objects-to-watch/the-lunar-100/ (retrieved April 26, 2020)

Handy R., Kelleghan D., McCague Th., Rix E., Russell S., Sketching the Moon, 2012 Springer Books, https://www.springer.com/us/book/9781461409403 (retrieved April 26, 2020)

Association of Lunar and Planetary Observers, Handbook of the ALPO Training Program, http:// www.cometman.net/alpo/ (retrieved April 26, 2020)

Chuck Wood, Lunar Photo Of the Day (LPOD), https://www2.lpod.org/wiki/LPOD:About (retrieved April 26, 2020)

Lunar Reconnaissance Office ACT-REACT Quick Map, http://target.lroc.asu.edu/q3/ (retrieved October 31, 2017)

Patrick Chevalley, Christian Legrand, Virtual Moon Atlas, http://ap-i.net/avl/en/start (retrieved June 30, 2018)

International Astronomical Union Gazetteer of , Crater Tycho, https://planetarynames.wr.usgs.gov/Feature/6163 (retrieved March 1, 2020)

Wikipedia, The Lunar 100 , https://en.wikipedia.org/wiki/Lunar_100 (retrieved April 26, 2020)

The Lunar Observer/July 2020/ 41

Aeronautical Chart Information Center (ACIC), United States Air Force, LAC Series Chart Reference, host- ed by the Lunar and Planetary Institute, https://www.lpi.usra.edu/resources/mapcatalog/LAC/ lac_reference.pdf (retrieved September 1, 2019)

Lunar and Planetary Institute, Digital Lunar Orbiter Photographic Atlas of the Moon, http:// www.lpi.usra.edu/resources/lunar_orbiter/ (retrieved September 1, 2017).

ADDITIONAL READING

Bussey, Ben & . 2004. The Atlas of the Moon. Cambridge University Press, New York.

Byrne, Charles. 2005. Lunar Orbiter Photographic Atlas of the . Springer-Verlag, London.

Chong, S.M., Albert C.H. Lim, & P.S. Ang. 2002. Photographic Atlas of the Moon. Cambridge University Press, New York.

Chu, Alan, Wolfgang Paech, Mario Wigand & Storm Dunlop. 2012. The Cambridge Photographic Moon Atlas. Cambridge University Press, New York.

Cocks, E.E. & J.C. Cocks. 1995. Who’s Who on the Moon: A biographical Dictionary of Lunar Nomencla- ture. Tudor Publishers, Greensboro

Gillis, Jeffrey J. ed. 2004. Digital Lunar Orbiter Photographic Atlas of the Moon. Lunar & Planetary Insti- tute, Houston. Contribution #1205 (DVD). (http://www.lpi.usra.edu/resources/lunar_orbiter/).

Grego, Peter. 2005. The Moon and How to Observe It. Springer-Verlag, London.

IAU/USGS/NASA. Gazetteer of Planetary Nomenclature. (http://planetarynames.wr.usgs.gov/Page/MOON/ target).

North, Gerald. 2000. Observing the Moon, Cambridge University Press, Cambridge.

Rukl, Antonin. 2004. Atlas of the Moon, revised updated edition, ed. Gary Seronik, Sky Publishing Corp., Cambridge.

Schultz, Peter. 1972. Moon Morphology. University of Texas Press, Austin. The-Moon Wiki. http://the- moon.wikispaces.com/Introduction

Wlasuk, Peter. 2000. Observing the Moon. Springer-Verlag, London.

Wood, Charles. 2003. The Moon: A Personal View. Sky Publishing Corp. Cambridge.

Wood, Charles & Maurice . 2012. 21st Century Atlas of the Moon. Lunar Publishing, UIAI Inc., Wheeling.

The Lunar Observer/July 2020/ 42

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 11, Aristarchus

Aristarchus Plateau, Jay Albert, Lake Worth, Florida, USA. 05 May 2020 0223 UT. Celes- tron NexStar Evolution 8 inch Schmidt- Cassegrain telescope, iPhone 6s, Photoshop El- ements. Seeing 6/10, transparency 3/6.

Online readers, click on images for hyperlinks.

Aristarchus, Michel Deconinck, southern France. 21 May 2013 2015 UT. Bresser 102mm/1000mm refractor telescope, 100 x with Delos 10mm eyepiece.

The Lunar Observer/July 2020/ 43

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 11, Aristarchus

Aristarchus, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 17 February 2019 0441 UT. 200 mm refrac- tor telescope, 742 nm filter, QHY5-II camera.

The Lunar Observer/July 2020/ 44

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 11, Aristarchus

Aristarchus, Francisco Alsina Cardinalli ,Oro Verde, Argenti- na, SLA. 19 April 2019 0209 UT. 105 mm Meade ETX Mak- sutov-Cassegrain telescope, QHY5-II camera.

Aristarchus, Desiré Godoy, Oro Verde, Argentina, SLA. 21 August 2016 0337 UT. 250 mm Meade LX 200 Schmidt-Cassegrain tele- scope, QHY5-II camera.

The Lunar Observer/July 2020/ 45

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 11, Aristarchus

Aristarchus, Francisco Alsina Cardinalli ,Oro Verde, Argenti- na, SLA. 20 December 2015 0045 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, Canon EOS Digital Rebel XS camera.

Aristarchus, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 21 April 2016 2209 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, Canon EOS Digital Rebel XS cam- era.

The Lunar Observer/July 2020/ 46

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 11, Aristarchus

Aristarchus, Alberto Anunziato, Paraná, Argen- tina, SLA . 19 April 2019 0645 UT. 105 mm Meade ETX Maksutov-Cassegrain telescope, QHY5-II camera.

Aristarchus, Rafael Lara Muñoz, Guatema- la, Guatemala, SLA. 17 May 2020 0535. 114 mm reflector telescope, Samsung Note 9 cell phone camera.

The Lunar Observer/July 2020/ 47

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 11, Aristarchus

Aristarchus, Walter Ricardo Elias, AEA - Oro Verde, Entre Rios, Argentina. 03 June 2020 0225 UT. Meade LX200 10 inch Schmidt-Cassegrain telescope, ZWO ASI 120 mm/s camera.

Aristarchus, Leandro Sid, AEA - Oro Verde, Entre Rios, Argentina. 03 June 2020 0026 UT. Meade StarNavigator NG 90 mm fl 1250 mm Maksutov- Cassegrain telescope, Samsung J7 Prime camera.

The Lunar Observer/July 2020/ 48

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 11, Aristarchus

Aristarchus, Gabriel Re, AEA - Oro Verde, Entre Rios, Argentina. 02 June 2020 2212 UT. Meade LX200 10 inch Schmidt- Cassegrain telescope, ZWO ASI 120 mm/s camera.

Below, Aristarchus, Abel David Emiliano Gonzalez Cian, AEA - Oro Verde, Entre Rios, Argentina. 03 June 2020 0109 UT. 10 inch Meade Light Bridge reflector tele- scope, Nikon 3100 camera.

The Lunar Observer/July 2020/ 49

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 12, Proclus

Proclus, Dennis Wilde, Transit Dreams Observa- tory, Campobello, South Carolina, USA. 27 April 2020 2359 UT. 250 mm Schmidt- Cassegrain tele- scope, Canon 60 da camera, 100 frames, BYEOS, Registax, Pho- toshop Seeing 7/10, top of image is 20 east of North.

Proclus, Francisco Alsina Cardinalli ,Oro Verde, Argenti- na, SLA. 14 May 2016 0216 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, Astronomik ProPlanet 742 IR-pass filter, QHY5-II camera.

The Lunar Observer/July 2020/ 50

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 12, Proclus

Mare Crisium, Michael Sweetman, Sky Crest Obser- vatory, Tucson, Arizona, USA. 07 June 2020 1043 UT. 8 inch f/12 Guan Sheng Classical Cassegrain tele- scope, Skyris132M camera, Orion red filter. East up North left. Seeing-3-4/10, Transparency- 3/6. Two panel mosaic.

Proclus, Martín Queirolo Gomez, Montevideo, Uru- guay, SAO. 28 De- cember 2015 1937 UT. 114 mm Newto- nian reflector tele- scope, Nikon D5100 camera.

The Lunar Observer/July 2020/ 51

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 12,Proclus

Proclus, Francisco Alsina Cardinal- li ,Oro Verde, Argentina, SLA. 09 December 2016 0400 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, Astronomik ProPlanet 742 IR-pass filter, QHY5-II camera.

Proclus, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 11 December 2016 0433 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, Astronomik ProPlanet 742 IR-pass filter, QHY5-II camera.

The Lunar Observer/July 2020/ 52

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 12, Proclus

Proclus, Francisco Alsi- na Cardinalli ,Oro Verde, Argentina, SLA. 20 Au- gust 2018 2343 UT. 200 mm refractor telescope, QHY5-II camera.

Proclus, Fernando Surà, San Nicolás de los Ar- royos, Argentina, SLA- LIADA . 09 May 2020 2220 UT. 127 mm. Mak- sutov-Cassegrain tele- scope, filter, Neximage 5 camera.

The Lunar Observer/July 2020/ 53

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 12, Proclus

Proclus, Francisco Alsina Cardinalli, Oro Verde, Argentina, SLA. 11 Sep- tember 2018 0101 UT. 279 mm Celestron 11 Edge HD Schmidt- Cassegrain telescope, QHY5-II camera.

Proclus, Desiré Godoy, Oro Verde, Argentina, SLA. 08 November 2019 0126 UT. 200 mm Newtonian reflector telescope, QHY5-II camera.

The Lunar Observer/July 2020/ 54

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 12, Proclus

Proclus and Mare Crisium, Fabio Verza, Milan, Italy. 26 June 2020 2011 UT. Celestron 4 inch Maksutov-Cassegrain telescope, Astronomik IR filter, ZWO ASI 290 MM camera.

Proclus, Leandro Sid, AEA - Oro Verde, Entre Rios, Argentina. 27 June 2020 2219 UT. Meade StarNavigator NG 90 mm fl 1250 mm Maksutov-Cassegrain telescope, Samsung J7 Prime camera.

The Lunar Observer/July 2020/ 55

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 12, Proclus

Mare Crisium and Proclus, Abel David Emiliano Gonzalez Cian, AEA - Oro Verde, Entre Rios, Argentina. 08 June 2020 0306 UT. 10 inch Meade Light Bridge reflector tele- scope, Nikon 3100 camera.

Proclus, Aylen Borgatello Alaniz, AEA - Oro Verde, Entre Rios, Argentina. 27 June 2020 2121 UT. Meade LX200 10 inch Schmidt-Cassegrain telescope, ZWO ASI 120 mm/s camera.

The Lunar Observer/July 2020/ 56

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 13, Gassendi

Gassendi, Jay Albert, Lake Worth, Florida, USA. 04 April 2020 0156 UT. Celestron NexStar Evolution 8 inch Schmidt-Cassegrain telescope, iPhone 6s, Pho- toshop Elements. Seeing 6/10, transparency 2/6.

Gassendi, Michel Deconinck, southern France. 02 May 2012 1820 UT. Bresser 102mm/1000mm refrac- tor telescope, 100 x with Delos 10mm eyepiece.

The Lunar Observer/July 2020/ 57

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 13, Gassendi

Gassendi, Francisco Alsina Cardinalli, Oro Verde, Argentina, SLA. 20 January 2016 2145 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, Canon Eos Digital Rebel XS camera.

Gassendi, Gabriel Re, AEA - Oro Verde, Entre Rios, Argentina. 02 June 2020 2238 UT. Meade LX200 10 inch Schmidt- Cassegrain telescope, ZWO ASI 120 mm/s camera.

The Lunar Observer/July 2020/ 58

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 13, Gassendi

Gassendi, Alberto Anunziato, Oro Verde, Argentina, SLA. 30 April 2016 0906 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, QHY5-II camera.

Gassendi, Desiré Godoy, Oro Verde, Argentina, SLA. 14 August 2016 0353 UT. 130 mm. Newtonian reflec- tor (Celestron Astromaster 130). .

The Lunar Observer/July 2020/ 59

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 13, Gassendi

Gassendi, Alberto Anunziato, Oro Verde, Argentina, SLA. 30 April 2016 0902 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, QHY5- II camera.

Gassendi, Jairo Chavez, Popayán, Colombia, SLA. 10 Oc- tober 2019 0129 UT. 10 inch truss Dobsonian telescope, Sony DSC-WX 50 camera.

Online readers, click on images for hyperlinks.

The Lunar Observer/July 2020/ 60

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 13, Gassendi

Gassendi, Sergio Babino, Montevideo, Uruguay. 08 March 2020 0134 UT. 203 mm Schmidt-Cassegrain telescope, ZWO ASI 174 mm camera.

Gassendi, Carlos Lobato, San José de Carrasco, Uru- guay, SAO. 04 April 2020 2230 to2233 UT. 130 mm Newtonian reflector telescope, 257 x.

The Lunar Observer/July 2020/ 61

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 13, Gassendi

Gassendi, Alberto Anunziato, Oro Verde, Argentina, SLA. 11 December 2016 0155 UT. 250 mm Meade LX 200 Schmidt- Cassegrain tele- scope, Astronomik ProPlanet 742 IR- pass QHY5-II camera.

Gassendi, Marcelo Mo- jica Gundlach, Cochabamba, Bolivia, SLA . 04 May 2020 0330 UT. 150 mm fl 1800 mm Skywatch- er Maksutov- Cassegrain telescope, ZWO ASI 178 b/w camera.

The Lunar Observer/July 2020/ 62

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 14, Sinus Iridum

Sinus Iridum, Jay Albert, Lake Worth, Florida, USA. 24 July 2018 0209 UT. Celestron NexStar Evolution 8 inch Schmidt-Cassegrain telescope, iPhone 6s, Photoshop Elements. Seeing 6510.

Mare Imbrium, Fabio Verza, Milan, Italy. 13 June 2020 0742 UT. Celestron CPC800 Schmidt -Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

The Lunar Observer/July 2020/ 63

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 14, Sinus Iridum

Sinus Iridum, Fabio Verza, Milan, Italy. 04 May 2020 1945 UT, colongitude 55.7 degrees. Celestron CPC800 Schmidt-Cassegrain tele- scope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

Sinus Iridum, Martín Queirolo Gomez, Mon- tevideo, Uruguay, SAO. 11 October 2016 2044 UT. 114 mm Newtonian reflector tele- scope, Celestron Nextimage 5 camera.

The Lunar Observer/July 2020/ 64

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 14, Sinus Iridum

Sinus Iridum, Martín Queirolo Gomez, Montevideo, Uruguay, SAO. 23 January 2016 2226 UT. 114 mm Newtonian reflector telescope, Nikon D5100 camera.

The Lunar Observer/July 2020/ 65

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 14, Sinus Iridum

Sinus Iridum, Jairo Chavez, Popayán, Colombia, SLA. 25 April 2018 2041 UT. 10 inch truss Dobsonian tele- scope, Y360 camera.

Sinus Iridum, Francisco Alsina Cardinalli ,Oro Verde, Argenti- na, SLA. 21 August 2016 0413 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, Astronomik ProPlanet 742 IR- pass filter, QHY5-II camera.

The Lunar Observer/July 2020/ 66

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 14, Sinus Iridum

Sinus Iridum, Al- berto Anunziato, Oro Verde, Argenti- na, SLA. 11 Decem- ber 2016 0221 UT. 250 mm Meade LX 200 Schmidt- Cassegrain tele- scope, Astronomik ProPlanet 742 IR- pass filter. .

Sinus Iridum, Marcelo Mojica Gundlach, Co- chabamba, Bolivia, SLA . 16 May 2019 0257 UT. 150 mm re- fractor telescope, Ori- on V-block filter, ZWO ASI 120 b/w camera.

The Lunar Observer/July 2020/ 67

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 14, Sinus Iridum

Sinus Iridum, Fer- nando Gomez, Mon- tevideo, Uruguay, SAO. 22 January 2013 2324 UT. Meade LX 200 305 mm Schmidt- Cassegrain tele- scope, Canon 1000D camera.

Sinus Iridum, Alberto Anun- ziato, Oro Verde, Argenti- na, SLA. 24 October 2015 0442 UT. 250 mm Meade LX 200 Schmidt- Cassegrain tele- scope, Phillips SPC900NC webcam.

The Lunar Observer/July 2020/ 68

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 14, Sinus Iridum

Sinus Iridum, Cyntia Olivera, Santiago del Estero, Argentina, SLA. 19 March 2020 0654 UT. 114 mm reflector tele- scope, Samsung Galaxy J5 camera.

Plato and Sinus Iridum, Leandro Sid, AEA - Oro Verde, Entre Rios, Argentina. 01 June 2020 0058 UT. Meade StarNavigator NG 90 mm fl 1250 mm Maksutov- Cassegrain telescope, Samsung J7 Prime camera.

The Lunar Observer/July 2020/ 69

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 15, the Straight Wall

Straight Wall, Steve Thornton. 30 May 2020 1645 UT. 9.25 inch Celestron Schmidt-Cassegrain telescope, 2 x bar- low, Optolong 685 nm IR Pass filter, ZWO ASI 120mm/s camera.

Rupes Recta, Fabio Verza, Milan, Italy. 13 June 2020 0744 UT. Celestron CPC800 Schmidt- Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

The Lunar Observer/July 2020/ 70

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 15, the Straight Wall

Rupes Recta, Francisco Alsina Cardinalli, Oro Verde, Argen- tina, SLA. 10 September 2015 2251 UT. 11 inch Celestron Edge HD Schmidt-Cassegrain telescope, QHY5-II camera.

Rupes Recta, Raúl Roberto Podestá, Formosa, Argentina, SLA . 03 January 2020 2343 UT. 127 mm Maksutov-Cassegrain telescope, Hokenn CCD Imager.

The Lunar Observer/July 2020/ 71

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 15, the Straight Wall

Rupes Recta, Martín Queirolo Gomez, Montevideo, Uruguay, SAO. 22 September 2016 2245 UT. 114 mm Newtoni- an reflector telescope, Nextimage 5 camera.

Online readers, click on images for hyperlinks.

The Lunar Observer/July 2020/ 72

Recent Topographic Studies Additional Focus-On Images of Lunar Feature 16, Petavius

Petavius, Michel Deconinck, southern France. 10 March 2016 1830 UT. Bresser 152mm/1200mm refractor telescope, 120 x with Delos 10mm eyepiece.

Petavius, Alberto Anunziato, Oro Verde, Argentina, SLA . 15 September 2019 0402 UT. 180 mm reflector telescope, QHYII-5 camera.

The Lunar Observer/July 2020/ 73

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 17, Schröter’s Valley

Vallis Schroteri, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 30 April 2016 0538 UT. 250 mm Meade LX 200 Schmidt-Cassegrain telescope, QHY5-II camera.

The Lunar Observer/July 2020/ 74

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 17, Schröter’s Valley

Vallis Schroteri, Francisco Alsi- na Cardinalli ,Oro Verde, Argen- tina, SLA. 11 December 2016 0317 UT. 250 mm Meade LX 200 Schmidt-Cassegrain tele- scope, Astronomik ProPlanet 742 IR-pass filter, QHY5-II camera.

Vallis Schroteri, Sergio Babino, Montevideo, Uruguay. 08 April 2020 0141 UT. 203 mm Schmidt-Cassegrain tele- scope, ZWO ASI 174 mm camera.

The Lunar Observer/July 2020/ 75

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 17, Schröter’s Valley

Vallis Schroteri, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 12 December 2016 0034 UT. 8 inch Meade Starfinder reflector telescope, As- tronomik ProPlanet 742 IR-pass filter.

Vallis Schroteri, Sergio Babino, Montevideo, Uruguay. 08 March 2020 0129 UT. 203 mm Schmidt-Cassegrain telescope, ZWO ASI 174 mm camera.

The Lunar Observer/July 2020/ 76

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 17, Schröter’s Valley

Vallis Schroteri, Sergio Babino, Montevideo, Uruguay. 05 De- cember 2019 0110 UT. 203 mm Schmidt-Cassegrain telescope, ZWO ASI 174 mm camera.

Vallis Schroteri, Jairo Chavez, Popayán, Colombia, SLA. 19 January 2019 0156 UT. 10 inch truss Dobsonian telescope, Sony DSC-WX 50 camera.

The Lunar Observer/July 2020/ 77

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 18, Mare Serenitatis Dark Edge

Mare Seren- itatis, Mar- tín Queirolo Gomez, Montevideo, Uruguay, SAO. 19 December 2016 1839 UT. 114 mm Newto- nian reflec- tor tele- scope, Nikon D5100 cam- era.

Mare Serenitatis, Jairo Chavez, Popayán, Colombia, SLA. 15 December 2018 2329 UT. 10 inch truss Dobsonian telescope, Sony DSC-WX 50 camera.

The Lunar Observer/July 2020/ 78

Recent Topographic Studies

Additional Focus-On Images of Mare Serenitatis Lunar Feature 18, Dark Edge

Mare Serenitatis, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 01 July 2017 2334 UT. 200 mm refractor telescope, QHY5-II camera.

Mare Serenitatis, Ángel Manuel López. Lunar Group of the Astronomical Association from Madrid, Spain. 29 May 2020 1955 UT. 5 inch Schmidt-Cassegrain telescope, QHY5-II camera.

The Lunar Observer/July 2020/ 79

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 18, Mare Serenitatis Dark Edge

Mare Serenitatis, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 14 May 2016 0232 UT. 250 mm Meade LX 200 Schmidt-Cassegrain tele- scope, Astronomik ProPlanet 742 IR-pass filter, QHY5-II camera.

Mare Serenitatis, Sergio Babino, Montevideo, Uruguay. 15 December 2018 0055 UT. 8”Astrotech RC Ritchety Chretien telescope, ZWO ASI 174 mm camera.

The Lunar Observer/July 2020/ 80

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 18, Mare Serenitatis Dark Edge

Mare Serenitatis, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 17 February 2019 0214 UT. 200 mm refractor telescope, Astronomik ProPlanet 742 IR-pass filter, QHY5-II camera.

Mare Serenitatis, Fabio Verza, Milan, Italy. 26 June 2020 2032 UT. Celestron 4 inch Maksutov-Cassegrain telescope, Astronomik IR filter, ZWO ASI 290 MM cam- era.

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Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 18, Mare Serenitatis Dark Edge

Mare Serenitatis, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 25 February 2018 0135 UT. 200 mm refractor telescope, QHY5-II camera.

Mare Serenitatis, Sergio Babino, Montevideo, Uru- guay. 14 April 2019 0037 UT. 8”Astrotech RC Ritchety Chretien telescope, ZWO ASI 174 mm cam- era.

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Recent Topographic Studies

Additional Focus-On Images of Mare Serenitatis Dark Edge

First Quarter Moon, Mare Serenitatis, Rafael Lara Muñoz, Guatemala, Guatemala, SLA. 29 May 2020 1934. 114 mm reflector telescope, Samsung Note 9 cell phone camera.

Calippus, Fabio Verza, Milan, Italy. 27 June 2020 2005 UT. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x bar- low, Astronomik IR Pro 807 filter, ZWO ASI 290 MM camera.

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Recent Topographic Studies

Additional Focus-On Images of the Alpine Valley

Vallis Alpes, Marcelo Mojica Gundlach, Cocha- bamba, Bolivia, SLA . 22 July 2018 2338 UT. 150 mm fl 1800 mm refractor telescope, Orion V-block filter, SWO CMOS camera.

Vallis Alpes, Francisco Alsina Cardinali ,Oro Verde, Argentina, SLA. 25 February 2018 0057 UT. 200 mm refractor telescope, QHY5- II camera.

The Lunar Observer/July 2020/ 84

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 19, the Alpine Valley

Vallis Alpes, Alberto Anunziato, Oro Verde, Argentina, SLA . 10 September 2016 2312 UT. Celestron 11 inch Edge HD Schmidt-Cassegrain telescope, QHYII-5 camera.

Mare Serenitatis, Sergio Babino, Montevideo, Uruguay. 14 March 2020 0446 UT. 8”Astrotech RC Ritchety Chretien telescope, ZWO ASI 174 mm camera.

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Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 19, the Alpine Valley

Vallis Alpes, Marcelo Mojica Gundlach, Cochabamba, Bolivia, SLA . 30 April 2020 2330 UT. 150 mm fl 1800 mm Maksutov- Cassegrain Sky Watcher tele- scope, ZWO-ASI 178 mm camera.

Plato and Vallis Alpes, Walter Ricar- do Elias, AEA - Oro Verde, Entre Rios, Argentina. 29 June 2020 0134 UT. Meade LX200 10 inch Schmidt- Cassegrain tele- scope, ZWO ASI 120 mm/s camera.

The Lunar Observer/July 2020/ 86

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 19, the Alpine Valley

Mons Piton and Vallis Alpes, Wal- ter Ricardo Elias, AEA - Oro Verde, Entre Rios, Argentina. 01 June 2020 0123 UT. Meade LX200 10 inch Schmidt-Cassegrain telescope, ZWO ASI 120 mm/s camera.

Mare Frigoris and Alpine Valley, Gabriel Re, AEA - Oro Verde, Entre Rios, Argentina. 29 June 2020 0135 UT. Meade LX200 10 inch Schmidt-Cassegrain telescope, ZWO ASI 120 mm/s camera.

The Lunar Observer/July 2020/ 87

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 19, the Alpine Valley

Plato and the Alpine Valley, Aylen Borgatello Alaniz, AEA - Oro Verde, Entre Rios, Argenti- na. 29 June 2020 0310 UT. Meade LX200 10 inch Schmidt- Cassegrain telescope, ZWO ASI 120 mm/s camera.

Vallis Alpes, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1956 UT. Celes- tron 14 Edge ED Schmidt- Cassegrain telescope, Fornax mount, Zeiss barlow, Baa- der R + IR 610 nm filter, ZWO ASI 174 m camera.

The Lunar Observer/July 2020/ 88

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 20, Posidonius

Posidonius, Michel Deconinck, southern France. 05 April 2018 2200 UT. 250 mm Dall Kirkham f/10 telescope, 192 x with Ethos 13mm eye- piece.

Posidonius, Francisco Alsina Cardinalli ,Oro Verde, Argentina, SLA. 27 March 2016 0445 UT. Celestron 11 Edge HD Schmidt-Cassegrain telescope, Canon Eos Digital Rebel XS cam- era.

The Lunar Observer/July 2020/ 89

Recent Topographic Studies

Additional Focus-On Images of Lunar Feature 20, Posidonius

Posidonius and Grove, Fabio Verza, Milan, Italy. 26 June 2020 2040 UT. Celestron 4 inch Maksutov- Cassegrain telescope, Astronomik IR filter, ZWO ASI 290 MM camera.

Posidonius, Francisco Alsina Cardinalli ,Oro Verde, Argenti- na, SLA. 28 March 2016 0445 UT. Celestron 11 Edge HD Schmidt-Cassegrain telescope, Canon Eos Digital Rebel XS camera.

The Lunar Observer/July 2020/ 90

Recent Topographic Studies

Ptolemaeus, Steve Thornton. 30 May 2020 1615 UT. 9.25 inch Celestron Schmidt-Cassegrain tele- scope, 2 x barlow, Optolong 685 nm IR Pass filter, ZWO ASI 120mm/s camera.

Copernicus, Rafael Lara Muñoz, Guatemala, Gua- temala, SLA. 02 May 2020 1845. 114 mm re- flector telescope, Sam- sung Note 9 cell phone camera.

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Recent Topographic Studies

Just Past Full Moon, Fabio Verza, Milan, Italy. 07 May 2020 2140 UT colongitude 93.0 degrees. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x barlow, IR- Pro 807 filter, ZWO ASI 290 MC-S camera.

Marius Hills, Howard Eskildsen, Ocala, Florida, USA. 17 June 2020 1327 UT, colongitude 229.4 degrees. Celestron 9.25 inch Schmidt-Cassegrain telescope, f/10, fl 2395 mm, Celestron Skyris 236M camera. Seeing 6/10, transparency 4/6.

The Lunar Observer/July 2020/ 92

Recent Topographic Studies

Last Quarter Moon, Fabio Verza, Milan, Italy. 13 June 2020 0739 UT, colongitude 177.9 degrees. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S cam- era.

Montes Apenninus, Rafael Lara Muñoz, Guatemala, Guatemala, SLA. 30 April 2020 1932. 114 mm reflector telescope, Samsung Note 9 cell phone camera.

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Recent Topographic Studies

Lade, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1931 UT. Celestron 14 Edge ED Schmidt- Cassegrain telescope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m camera.

Waxing Crescent Moon, Fabio Verza, Milan, Italy. 26 June 2020 1958 UT, colongitude 343.4 degrees. Celestron 4 inch Maksutov-Cassegrain telescope, Astronomik IR filter, ZWO ASI 290 MM camera. Mosaic of six images.

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Recent Topographic Studies

Grimaldi, Howard Eskildsen, Ocala, Florida, USA. 17 June 2020 1329 UT, colongitude 229.5 degrees. Celestron 9.25 inch Schmidt- Cassegrain telescope, f/10, fl 2395 mm, W-25 red filter, Celestron Skyris 236M camera. Seeing 6/10, transparency 4/6. Howard writes:

This image shows the mare patches in Gri- maldi and in . Directly west of the pair, the crater near the limb is Schluter. Mountains from the Rook Range can be seen on the south of Schluter. Just north of Grimaldi are a trio of craters that remind me of an elf with big horizontal ears. They are, from south to north, Lohrmann, Heve- lius, and Cavalerius.

Tycho, Fernando Gimenez, Montevideo, Uru- guay. 29 August 2012 0248 UT. 230mm f/13 refractor telescope, BENQ camera.

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Recent Topographic Studies

Endymion, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1919 UT. Celestron 14 Edge ED Schmidt- Cassegrain telescope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m camera.

Waxing Crescent Moon, Fabio Verza, Milan, Italy. 27 June 2020 2036 UT, colongitude 355.8 degrees. Celestron CPC800 Schmidt-Cassegrain tele- scope, 1.3 x barlow, Astronomik IR Pro 807 filter, ZWO ASI 290 MM camera. Mosaic of four images.

The Lunar Observer/July 2020/ 96

Recent Topographic Studies

Clavius, Fabio Verza, Milan, Italy. 13 June 2020 0810 UT. Celestron CPC800 Schmidt- Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

Waxing Gibbous Moon, Leonardo Alber- to Colombo, Córdoba, Argentina. 30 May 2020 2345 UT. 35 mm telescope, Green “Bronica” YG-2 filter, QHY5LII-M cam- era.

The Lunar Observer/July 2020/ 97

Recent Topographic Studies

Bullialdus, Fabio Verza, Milan, Italy. 14 June 2020 0822 UT. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter and W-23A red filter, ZWO ASI 290 MC-S camera.

Tycho, Sergio Babino, Montevideo, Uruguay. 08 May 2020 0248 UT. 203 mm catadrioptic telescope, ZWO ASI 174 mm camera.

Online readers, click on images for hyperlinks.

The Lunar Observer/July 2020/ 98

Recent Topographic Studies

Janssen, Fabio Verza, Milan, Italy. 27 May 2020 2006 UT. Celestron CPC800 Schmidt- Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

Sirsalis, Howard Eskildsen, Ocala, Flor- ida, USA. 17 June 2020 1330 UT, colon- gitude 229.5 degrees. Celestron 9.25 inch Schmidt-Cassegrain telescope, f/10, fl 2395 mm, Celestron Skyris 236M cam- era. Seeing 6/10, transparency 4/6.

Howard adds:

This image shows Sirsalis and A with associated rille. On the limb of the moon Mare Orientale is just visible. The Moon is rising in declination and will have favorable position for more morning imaging over the next few . I hope to do more late-phase lunar imaging of this area to try and tease out details of Orientale's moun- tainous rings before and sometimes after local sunrise if necessary.

The Lunar Observer/July 2020/ 99

Recent Topographic Studies

Rima Ariadaeus, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1847 UT. Celestron 14 Edge ED Schmidt-Cassegrain telescope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m cam- era.

Montes Apenninus, Fabio Verza, Milan, Italy. 13 June 2020 0750 UT. Celestron CPC800 Schmidt-Cassegrain tele- scope, 1.3 x barlow, IR-Pro 807 filter and W-23A red filter, ZWO ASI 290 MC-S camera.

The Lunar Observer/July 2020/ 100

Recent Topographic Studies

Theophilus, Fabio Verza, Milan, Italy. 27 May 2020 2023 UT. Celestron CPC800 Schmidt- Cassegrain telescope, 1.3 x barlow, IR-Pro 807 fil- ter, ZWO ASI 290 MC-S camera.

Below, Atlas and Hercu- les, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1922 UT. Celestron 14 Edge ED Schmidt-Cassegrain tele- scope, Fornax mount, Zeiss Abbe barlow, Baa- der R + IR 610 nm filter, ZWO ASI 174 m camera.

The Lunar Observer/July 2020/ 101

Recent Topographic Studies

Anaxagoras, Michael Sweetman, Sky Crest Ob- servatory, Tucson, Arizo- na, USA. 07 June 2020 1051 UT. 8 inch f/12 Guan Sheng Classical Casse- grain telescope, Skyr- is132M camera, Orion red filter. East upper right, North upper left. Seeing-3- 4/10, Transparency- 3/6. Two panel mosaic.

Aristoteles, Fabio Verza, Milan, Italy. 27 June 2020 2003 UT. Celestron CPC800 Schmidt- Cassegrain telescope, 1.3 x barlow, Astronomik IR Pro 807 filter, ZWO ASI 290 MM camera.

The Lunar Observer/July 2020/ 102

Recent Topographic Studies

Archimedes, Fabio Verza, Milan, Italy. 31 May 2020 1943 UT. Celestron CPC800 Schmidt- Cassegrain telescope, 1.3 x barlow, IR-Pro 807 fil- ter, ZWO ASI 290 MC-S camera.

Aristoteles and Eudoxus, Luigi Morrone, SNdR Luna UAI, Ager- lla, Italy, 27 June 2020 1912 UT. Celestron 14 Edge ED Schmidt -Cassegrain tele- scope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm fil- ter, ZWO ASI 174 m camera.

The Lunar Observer/July 2020/ 103

Recent Topographic Studies

Theophilus and Cyrillus, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1904 UT. Celestron 14 Edge ED Schmidt-Cassegrain telescope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m camera.

Bossingault, Fabio Verza, Milan, Italy. 27 June 2020 2016 UT. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x barlow, Astronomik IR Pro 807 filter, ZWO ASI 290 MM camera.

The Lunar Observer/July 2020/ 104

Recent Topographic Studies

Julius Caesar, Fabio Verza, Milan, Italy. 27 June 2020 2010 UT. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x barlow, Astronomik IR Pro 807 filter, ZWO ASI 290 MM camera.

Deslandres, Walter Ricardo Elias, AEA - Oro Verde, Entre Rios, Argentina. 03 June 2020 0126 UT. Meade LX200 10 inch Schmidt-Cassegrain telescope, ZWO ASI 120 mm/s camera.

The Lunar Observer/July 2020/ 105

Recent Topographic Studies

Waxing Gibbous Moon, Leandro Sid, AEA - Oro Verde, Entre Rios, Argentina. 01 June 2020 0038 UT. Meade Star- Navigator NG 90 mm fl 1250 mm Maksutov-Cassegrain tele- scope, Samsung J7 Prime cam- era.

Langrenus, Abel David Emiliano Gon- zalez Cian, AEA - Oro Verde, Entre Rios, Argentina. 08 June 2020 0305 UT. 10 inch Meade Light Bridge reflec- tor telescope, Nikon 3100 camera.

The Lunar Observer/July 2020/ 106

Recent Topographic Studies

Messier, Aylen Borgatello Alaniz, AEA - Oro Verde, Entre Rios, Argentina. 28 June 2020 0030 UT. Meade LX200 10 inch Schmidt-Cassegrain tele- scope, ZWO ASI 120 mm/s camera.

Rima Hyginus, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1940 UT. Celestron 14 Edge ED Schmidt-Cassegrain telescope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m cam- era.

The Lunar Observer/July 2020/ 107

Recent Topographic Studies

Purbach, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1944 UT. Celestron 14 Edge ED Schmidt-Cassegrain telescope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m camera.

Cassini, Luigi Morrone, SNdR Lu- na UAI, Agerlla, Italy, 27 June 2020 1837 UT. Celestron 14 Edge ED Schmidt-Cassegrain telescope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m camera.

The Lunar Observer/July 2020/ 108

Recent Topographic Studies

Piccolomini, Fabio Verza, Mi- lan, Italy. 27 May 2020 2003 UT. Celestron CPC800 Schmidt -Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

Tycho, Leandro Sid, AEA - Oro Verde, Entre Rios, Argentina. 01 June 2020 0059 UT. Meade StarNavigator NG 90 mm fl 1250 mm Maksutov- Cassegrain telescope, Samsung J7 Prime cam- era.

The Lunar Observer/July 2020/ 109

Recent Topographic Studies

Earthshine, Rafael Lara Muñoz, Guatemala, Guate- mala, SLA. 24 May 2020 0245. 114 mm reflector tel- escope, Samsung Note 9 cell phone camera.

The Lunar X, Frank J. Melillo, Holts- ville, New York, USA. 28 June 2020 0235 UT. Celestron 8 inch f/10 Schmidt -Cassegrain telescope, DMK 21AU618.AS camera.

The Lunar Observer/July 2020/ 110

Recent Topographic Studies

Longomontanus, Fabio Verza, Milan, Italy. 31 May 2020 2001 UT. Celestron CPC800 Schmidt- Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

Bullialdus, Leandro Sid, AEA - Oro Verde, Entre Rios, Argentina. 01 June 2020 0031 UT. Meade StarNavigator NG 90 mm fl 1250 mm Maksutov- Cassegrain telescope, Samsung J7 Prime camera.

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Recent Topographic Studies

Purbach, Fabio Verza, Milan, Italy. 13 June 2020 0803 UT. Celestron CPC800 Schmidt-Cassegrain tele- scope, 1.3 x barlow, IR-Pro 807 and W-23A red filter, ZWO ASI 290 MC- S camera.

Lichtenberg, Howard Eskildsen, Ocala, Florida, USA. 17 June 2020 1326 UT, colongitude 229.4 degrees. Celestron 9.25 inch Schmidt-Cassegrain telescope, f/10, fl 2395 mm, W-25 red filter, Celestron Skyris 236M camera. Seeing 6/10, transparency 4/6.

Howard writes:

This image taken was about three hours after sunrise, so a W -25 filter was used to minimize atmospheric glare. The crater Lichtenberg is in the center of the image with rays visible north and west of the crater but erased by later volcanic activity. It is quite an unusual crater with very interesting geologic history.

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Recent Topographic Studies

Petavius, Abel David Emiliano Gonzalez Cian, AEA - Oro Verde, Entre Rios, Argentina. 08 June 2020 0304 UT. 10 inch Meade Light Bridge reflector telescope, Nikon 3100 camera.

Meton, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1926 UT. Celestron 14 Edge ED Schmidt- Cassegrain telescope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m camera.

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Recent Topographic Studies

Pythagoras, Fabio Verza, Milan, Italy. 13 June 2020 0757 UT. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x barlow, IR-Pro 807 and W-23A red filter, ZWO ASI 290 MC-S camera.

Mons Rumker, Howard Eskildsen, Ocala, Florida, USA. 17 June 2020 1325 UT, colongitude 229.4 degrees. Celes- tron 9.25 inch Schmidt-Cassegrain telescope, f/10, fl 2395 mm, Celestron Skyris 236M camera. Seeing 6/10, trans- parency 4/6.

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Recent Topographic Studies

Bullialdus, Leandro Sid, AEA - Oro Verde, Entre Rios, Argentina. 01 June 2020 0029 UT. Meade StarNavigator NG 90 mm fl 1250 mm Maksutov-Cassegrain telescope, Samsung J7 Prime camera.

Mons Hadley, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1848 UT. Celestron 14 Edge ED Schmidt-Cassegrain tel- escope, Fornax mount, Zeiss Abbe barlow, Baader R + IR 610 nm filter, ZWO ASI 174 m camera.

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Recent Topographic Studies

Montes Apenninus, Fabio Verza, Milan, Italy. 31 May 2020 1828 UT. Celestron CPC800 Schmidt-Cassegrain tele- scope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

Maurolycus, Luigi Morro- ne, SNdR Luna UAI, Ager- lla, Italy, 27 June 2020 1921 UT. Celestron 14 Edge ED Schmidt- Cassegrain telescope, For- nax mount, Zeiss Abbe bar- low, Baader R + IR 610 nm filter, ZWO ASI 174 m cam- era.

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Recent Topographic Studies

Albategnius, Luigi Morrone, SNdR Luna UAI, Agerlla, Italy, 27 June 2020 1947 UT. Celestron 14 Edge ED Schmidt- Cassegrain tele- scope, Fornax mount, Zeiss Ab- be barlow, Baa- der R + IR 610 nm filter, ZWO ASI 174 m cam- era.

Anaximenes, Fabio Verza, Milan, Italy. 13 June 2020 0824 UT. Celestron CPC800 Schmidt-Cassegrain tele- scope, 1.3 x barlow, IR-Pro 807 and W-23A red filter, ZWO ASI 290 MC-S camera.

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Recent Topographic Studies

Copernicus, Fabio Verza, Milan, Italy. 13 June 2020 0748 UT. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x barlow, IR-Pro 807 and W-23A red filter, ZWO ASI 290 MC-S camera.

Clavius, Fabio Verza, Milan, Italy. 31 May 2020 1954 UT. Celestron CPC800 Schmidt-Cassegrain telescope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

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Recent Topographic Studies

Plato, Fabio Verza, Milan, Italy. 13 June 2020 0753 UT. Celestron CPC800 Schmidt- Cassegrain telescope, 1.3 x barlow, IR-Pro 807 and W-23A red filter, ZWO ASI 290 MC-S camera.

Atlas, Fabio Verza, Milan, Italy. 27 May 2020 2027 UT. Celestron CPC800 Schmidt-Cassegrain tele- scope, 1.3 x barlow, IR-Pro 807 filter, ZWO ASI 290 MC-S camera.

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Lunar Geologic Change Detection Program Coordinator Dr. Anthony Cook- [email protected] Assistant Coordinator David O. Darling [email protected]

2020 July LUNAR GEOLOGICAL CHANGE DETECTION PROGRAM

Reports have been received from the following observers for May: Jay Albert (Lake Worth, FL, USA - ALPO) observed: , Aristarchus, Atlas, , Copernicus, , , Kepler, Plato, Ross D, and Tycho. Alberto Anunziato (Argentina - SLA) observed: , Bullialdus, Daniel, Gassen- di, Hyginus N, Messier, Plato, Proclus, Ross D and Tycho. Aylen Borgatello (Argentina – AEA) imaged Hy- ginus N. Luis Francisco Alsina Cardinali (SLA) imaged: Messier, Plato, Plato, Ross D, Tycho and several features. Maurice Collins (New Zealand – ALPO/BAA/RASNZ) imaged: Aristarchus, , Copernicus, earthshine, Grimaldi, Hevelius, Kepler, , Plato, Schickard, Tycho and several features. Tony Cook (ALPO/BAA) videoed the Moon in the thermal IR and imaged several features in near-IR wavebands. Rob Davies (Mid-West Wales, UK - BAA/NAS) imaged the Montes Apenninus and several features. Daryl Dobbs (Risca, UK – BAA) observed: Mare Frigoris, Maurolycus, and Ptolemaeus. Valerio Fontani (Italy – UAI) made a time lapse video of: Vallis Schroteri. Walter Elias (Argentina – AEA) imaged Copernicus, Pla- to, Ross D and Tycho. Les Fry (Mid-West Wales, UK – NAS) imaged: , Bailly, Bullialdus, Byr- gius, Cassini, de Vico, , Hipparchus, Hommel, Mare Crisium, , Messier, Plato, Rein- hold, Riccius, Theophilus, Tycho, and . Abel Gonzalez Cian (Argentina – AEA) imaged Alphonsus and Copernicus. Facundo Gramer (Argentina – AEA) imaged Tycho. Rik Hill (Tucson, AZ, USA - ALPO/ BAA) imaged Copernicus, Fracastorius, Gassendi, Grimaldi and Gutenburg. Leatherbarrow (Sheffield, UK – BAA) imaged: , Maurolycus, and Sinus Iridum. Nigel Longshaw (Oldham, UK - BAA) observed: Daniell, earthshine, Mons Piton and Proclus. Gabriel Re (Argentina – AEA) imaged Messier, Plato and Tor- ricelli B. Leandro Sid (Argentina – AEA) imaged Hyginus. Phil Sheperdson (York, UK – BAA) observed/ imaged Ptolemaeus. Trevor Smith (Codnor, UK – BAA) observed: Aristarchus, Bailly, Plato and Proclus. Bob Stuart (Rhayader, UK – BAA/NAS) imaged: Agrippa, Albategnius, Alphonsus, Arzachel, Birt, Bulli- aldus, Cassini, , Clavius, Copernicus, , Cyrillus, , Deslandres, , , Geminus, Gutenberg, , Hercules, Hyginus, , Janssen, Kaiser, , Langrenus, Montes Apenninus, , Petavius, Piccolomini, Plato, Posidonius, Ptolemaeus, Rheita, , Theophilus, Torricelli, , Tycho, Vallis Alpes, , Werner and several features. Fran- co Taccogna (Italy – UAI) imaged: Herodotus, and Vallis Schroteri. David Teske (Louisville, MS, USA – ALPO) imaged Herodotus. Gary Varney (Pembroke Pines, FL, USA – ALPO) imaged: Bullialdus, Clavius, Plato, Sinus Iridum Tycho and several features. Fabio Verza (Italy – UAI) imaged: Herodotus, Mare Frigor- is, and Vallis Schrotri. Derick Ward (Swindon, UK – BAA) imaged: Alphonsus, , Daniell, Mons Piton, Plato, Proclus, and Ross D. Luigi Zanatta (Italy – UAI) imaged: Herodotus.

LTP reports: No LTP were reported in May, however a likely candidate impact flash was recorded from France on 2020 May 27 UT 20:49. If you were recording earthshine then, perhaps for an occultation, then please let me know if you spot a flash in any video that you captured.

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News: As you can see from the list of observers above, this is now occupying half of a page. This emphasizes a healthy observing program. Now I really do enjoy writing and doing a quick analysis on ob- servations from you all, however I am also now getting into a bit of a space and time problem. Space-wise this month we occupy 13 pages of my submitted word file. Time-wise it took me 2.5 days to sort through the observations write, format and perform a quick analysis, and I still didn’t have time to include: Abel Gonzalez Cian, Leandro Sid, and Facundo Gramer’s reports (My apologies over this – but they will be used in the database of observations). I am not complaining and strongly encourage observers to send in their observation. However, I think we need to do things differently to get future LGC newsletters down to a more manageable production time and page size. I propose keeping the list of observations received at the top of the newsletter, to let you know who has observed what, but will have to be more selective in which observations to show. I haven’t decided upon the right way to do this yet, but may have this implemented by next month. Watch this space!

Routine Reports: Below are a selection of reports received for May that can help us to re-assess unusual past lunar observations – if not eliminate some, then at least establish the normal appearance of the surface features in question.

Plato: On 2020 May 01 UT Gabriel Re (AEA) at 22:15 and at 23:40 Walter Elias (AEA) observers took images of similar illumination (±0.5°) to the following two LTP reports:

On 1995 Sep 03 at UT19:40-20:15 P. Moore (Selsey, UK, 15" reflector at x400) observed that the floor of Plato was much darker than he would normally expect and furthermore no interior craterlets were seen. There was however a white patch that was barely visible at the location of the central craterlet should have been. G. North (UK) attempted to observe but the Moon was too low and seeing terrible. F. Doherty reported Plato normal. 2006 catalog ID=475 and weight=3. ALPO/BAA weight=1.

Plato 1949 Mar 09 UT 02:00-03:00 E.J.Reese (6" reflector x240) and one hour later T.R.Hake (5" refractor x300) both unable to see any detail on the floor of Plato, despite both being able to see a "difficult to see" cleft near to the crater Connon. Reese was able to see detail under similar illumination back in 1948 and 1947 and saw the floor craterlets in Plato clearly then. ALPO/BAA weight=1.

Figure 1. Plato taken on 2020 May 01 by AEA observers and orientated with north towards the top. (Left) An image by Gabriel Re taken at 22:15UT. (Right) An image by Walter Elias taken at 23:40UT.

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As you can see from Fig 1, both images show no detail on the floor. Furthermore, the contrast in Fig 1 (Right) does make the floor of Plato look darkish. I will therefore lower the weights of both these reports to 0 to make them non-LTPs.

Figure 2. Tycho orientated with north towards the top. Image taken by Luis Francisco Alsina Cardinali (SLA) on 2020 May 01 UT 23:16-23:17. (Left) Image as captured with some slight sharpening. (Right) Contrast stretched ver- sion to show up detail in the shadows – if present.

Fig 2 shows none of the luminous marks in the shadow that Walter Haas reported in 1940. There- fore, we shall leave the weight of that LTP at 2 for now.

Daniell: On 2020 May 02 UT 21:52-21:54 Derick Ward (BAA) imaged the crater and Alberto Anunziato (SLA) sketched 22:20-22:25 this crater under similar illumination (±0.5°) to the following report:

Daniell 1979 Jul 04 UT 20:40-21:19 Observed by Saxton (UK?, 216mm refractor?, seeing III, transparency: Good) "noticed that the east end of Daniell was bright and fuzzy and had somewhat poorly defined edge to the bright part. A sketch was made, and possibly shows the same as in past reports" BAA Lunar Section Report. Cameron 2006 extension catalog ID=59 and weight=3. Observer located in Leeds, England and used a 9" reflector x250. Seeing=III and trans- parency=good. ALPO/BAA weight=2.

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Figure 3. Daniell. (Background) An image by Derick Ward (BAA) taken on 2020 May 02 UT 21:52-21:54 and orien- tated with north towards the top. (Bottom Left) A sketch by John Saxton (BAA) made on 1979 Jul 04 UT 20:40-21:19 orientation presumably with north towards the bottom? (Right) A sketch by Alberto Anunziatio made on 2020 May 02 UT 22:20-22:35 with an “N” indicating where north is – the numbers indicate relative brightness.

It is nice and clear from Derick’s image (Fig 3 - Background) that the floor of Daniell is dark, the west wall is nice and bright and the east wall diffuse. Alberto’s sketch (Fig 3 – Right) confirms the dark ap- pearance of the floor but also shows the relative brightness values of the rim. Now the sketch provided by Saxton (Fig 3 – Bottom Left) has no North indicator, but by convention (also looking at his sketches of oth- er craters) probably has north towards the bottom. So, in this case why does Saxton say that the east of Dan- iell was bright and fuzzy whereas in Derick’s image it is the west wall? Back in the late 1970’s the BAA Lunar Section transitioned from the “Classical” way of defining East and West on the Moon to the IAU system. Saxton does not make clear which system they were using, though in sketches submitted later that year it is clear that they use IAU as they start putting IAU in brackets every time they mention a direction. I therefore suggest that “noticed that the east end of Daniell was bright and fuzzy and had somewhat poorly defined edge to the bright part” should read: “noticed that the west end of Daniell was bright and fuzzy and had somewhat poorly defined edge to the bright part”. However, this still does not agree with Derick’s im- age which shows a bright west end and a fuzzy east end. We shall therefore leave the weight of this 1979 report at 2 for now.

Copernicus: On 2020 May 02 UT 04:43 Rik Hill (ALPO/BAA) imaged the crater in monochrome under similar illumination to the following two reports:

On 1995 Jul 07 at UT 04:22 R. Spellman (Los Angeles, CA, USA) noted that the floor of Copernicus was slightly darker in blue light. The ALPO/BAA weight=1. This report came from R. Spellman's web site.

Copernicus 1969 Nov 18 UT 21:10-21:11 Observed by Hedervari(Budapest, Hungary, 3.5" refractor) "Yellowish-red stripe on inner W. wall (chrom. aberr.? 12 watch)." NASA catalog weight=2. NASA catalog ID No. 1217. ALPO/BAA weight=1.

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Figure 4. Copernicus at 665nm as imaged by Rik Hill (ALPO/BAA) on 2020 May 02 UT 04:43 and orientated with north towards the top.

Although Rik’s image is monochrome, it does at least provide a very useful context image for what the overall appearance of Copernicus should have looked like to the respective observers back in 1995 and 1969. It can also prove useful for modelling atmospheric spectral dispersion, or chromatic aberration, to see if this could have generated the colors at the locations specified. We shall leave the weights as they are.

Plato: On May04 ALPO observers: Jay Albert observed (01:25-01:40UT) and Gary Varney imaged (02:44UT) the crater under both similar illumination and topocentric libration (±1°) to the following report:

On 1980 Jul 22 at UT20:08-21:50 G.North (Sussex, UK, 8" reflector, x144 and x207, seeing III-V and transparency fair) suspected an obscuration on the north and north west wall. The effect came and went. May have been due to see- ing and image contrast? Cameron 2006 catalog ID=101 and weight=1. ALPO/BAA weight=1.

…and for Gary Varney’s image, just similar illumination (±0.5°) to the following report:

Plato 1970 Dec 08 UT 18:00-23:59 UT Observed by Fitton (Oldham, England, 8.5" reflector, S=VG) "All surrounding detail perfect, but barely a trace of floor detail. A suggestion of 2 or 3 white spots including central A seen only on one examination out of five. "sector" beginning to show. ALPO/BAA weight=1.

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Figure 5. Plato on 2020 May 03 at 02:44 UT as imaged by Gary Varney (ALPO). The image has been rotated so that north was towards the top – hence the triangular section missing on the bottom left.

Jay comments that for the 1980 report that the central, N pair and S craterlets were seen, though the N pair and S craterlets were sometimes difficult and even momentarily missing. There was no hint of any obscuration or fuzziness on the N and NW walls. He did note however that part of the NE wall, which was also well detailed, appeared to have a lot of damage or deterioration. Gary’s image (Fig 5) confirms Jay’s description. We can quite see why seeing variability could cause the obscuration effect seen by Gerald north. So therefore, we shall lower the weight of that LTP to 0 and remove it from the LTP database.

Likewise, for the 1970 Fitton report, Fig 5 tells us that the craterlets could probably only be seen during the really best moments of atmospheric seeing. We shall therefore lower the weight of that report to 0 and remove it from the ALP/BAA database too.

Herodotus: On 2020 May 04 UAI observers: Luigi Zanatta (19:02UT), Franco Taccogna (10:39UT), and Fabio Verza (19:50 UT) attempted a repeat illumination request to try to detect the pseudo peak that occa- sionally has been reported on the floor of Herodotus:

BAA Request: Some astronomers have occasionally reported seeing a pseudo peak on the floor of this crater. However, there is no central peak! Please there- fore image or sketch the floor, looking for anything near the center of the crater resembling a light spot, or some highland emerging from the shadow. All reports should be emailed to: a t c @ a b e r . a c . u k

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Figure 6. Herodotus as imaged on 2020 May 04 by UAI members and orientated with north towards the top. (Left) Luigi Zanatta’s image from 19:02UT. (Center) Franco Taccogna’s image from 10:39UT. (Right) Fabio Verza’s im- age from 19:50 UT.

We have an extremely nice set of time sequence images from our UAI observers (See Fig 6), but alas no sign of the pseudo peak. It is possible that it was some kind of atmospheric effect e.g. image ghosting from different layers in our atmosphere travelling in different directions? We are definitely looking in the right colongitude range where it has been seen occasionally in the past – so whatever the cause of past sighting – lunar or atmospheric, it should hopefully recur given long enough.

Vallis Schroteri: On 2020 May 04 UAI observers: Valerio Fontani (1944 UT), 19:47 UT), Franco Taccog- na (19:47 UT) and Fabio Verza (19:54UT) imaged the following area under a repeat illumination request that corresponded to the following LTP report:

Aristarchus Area 2004 Nov 22 UT 04:58-05:49 Observed by Gray (Winnemucca, NV, USA, 152mm f/9 refractor, seeing 4-5, transparency 4-5, x114, x228) "Blinked Herodotus with Wratten filters Blue 38A and Red 25. The illuminated west crater wall stood out brilliantly in blue light, much more so than in white light. This was true also of Aristarchus. Red light did not increase contrasts in Herodotus any more than they were in white light. Shadows in Herodotus ap- peared as black as the night west of the terminator and remained that way throughout the observing period. No LTP seen in Herodotus tonight. A possible LTP was seen to the west of Herodotus near the terminus of Schroter’s Valley. It was noted at the beginning of the observing period that there were four very bright spots of light, one near the end of Schroter’s Valley, the other three grouped together a little further north. Although not far from the ter- minator they were definitely east of it. It was noted that all of them nearly vanished in the Blue 38A filter while Aristarchus and the rim of Herodotus gleamed brilliantly. At 5:19UT it was noted that the most brilliant of the four lights, the one near the terminus of Schroter’s Valley, had faded almost to invisibility in white light. When first seen it had been brighter than Ar- istarchus. It remained very dim after this through the remainder of the ob- serving period, and was unchanged at 7:35-7:49UT when I again examined the ar- ea. The other three bright spots remained brilliant and unchanged."

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Figure 7. Vallis Schroteri as imaged on 2020 May 04 by UAI observers and orientated with north towards the top. (Far Left) Valerio Fontani’s color image from 1944 UT. (Left) Franco Taccogna’s image in red light from 19:47 UT. (Right) Franco Taccogna’s image in blue light from 19:47 UT. (Far Right) Fabio Verza’s monochrome image from 19:54UT.

It is a shame that I cannot show you in this PDF file that Valerio Fontani’s image (Fig 7 -Left) is part of an animated GIFF file or a time lapse video, as it is very impressive to watch. Franco’s images (Fig 7 - Left and Right) are color images but do not show up the effects that Robin Gray mentions. Fabio’s im- age (Fig 7 – far right) gives us the sharpest view. I am not quite sure what bright spots Robin Gray was re- ferring to in his LTP report as he did not include a sketch. There are however some sunlit mountains way to the NW of Herodotus on the northern side of Vallis Schroteri. I think we shall leave the weight of the LTP report as it is now, but at least we have some very useful context images from which to judge this report in the future.

Herodotus: On 2020 May 05 UT 02:20 David Teske (ALPO) imaged the crater some 28 min after the end of the repeat illumination window (±0.5°) for the following report:

On 1993 Sep 28 at UT 04:30-06:10 S.Beaumont (Cambridge, UK)observed that the north east edge of Herodotus appeared as a "highland area spilling over into" the Cobra's Head border or "overlook". The shadow on the elevation was contig- uous with a similar shadow over the Cobra's Head "like a darkening of the ter- rain. Shadow appears softer diffused without sharp bounds of most Lunar shad- ows. sketch. S. edge of crater started to appear at 0615". The Cameron 1978 catalog ID=468 and the weight=2. The ALPO/BAA weight=1 as the date or UT are wrong.

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Figure 8. Aristarchus and Herodotus on 2020 May 05 UT 02:20 as imaged by David Teske (ALPO) and orientated with north towards the top.

Jay Albert, who was also observing at the time, comments that contrary to the LTP description, He- rodotus was completely sunlit and visible with the terminator roughly 5 Herodotus diameters further W. The crater’s E wall was in shadow but the floor was sunlit. The Cobra Head stood out in high relief with some shadow on its W slope. This is confirmed in David’s image (Fig 8). I will take a look again at the re- port and try some alternative dates and times in the lunar schedule web site.

Plato: On 2020 May 06 UT 07:49 Maurice Collins (ALPO/BAA/RASNZ) imaged the crater under similar illumination to the following report:

Plato 1874 Jan 01 UT 20:00? Observed by Pratt (England?) Unusual appearance" NASA catalog weight=1. NASA catalog ID #183. ALPO/BAA weight=1.

Figure 9. Plato as imaged by Maurice Collins (ALPO/BAA/RASNZ) on 2020 May 06 UT and orientated with north towards the top.

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Note that the time of the 1874 report was estimated. Nevertheless, Maurice’s image (Fig 9) is the best guess as to what the normal appearance should have looked like – nothing unusual. We shall keep the weight of the 1874 report at 1 until we can find out more about it.

Bailly: On 2020 May 06 UT 21:50-22:20 Trevor Smith (BAA) sketched this crater using a 16” Newtonian under similar illumination to the following report: Bailly 1974 Oct 29 22:00-23:00 Observed by Lord (St Annes-on-Sea, UK), 25cm reflector, x125 & x400,seeing III, transparency 5/5. South west floor was darker in a blue filter than in other filters. Observer thought this was due to a natural green color here. Had seen this on 3 other occasions under early morning illumination. ALPO/BAA weight=1.

Figure 10. Bailly as sketched by Trevor Smith (BAA) on 2020 May 06 UT 21:50-22:20, using a Wratten 38 blue fil- ter. Trevor noted that indeed the SW floor had a slight darkening to it and when viewed through a blue filter appeared darker than through other filters. The interior ramparts to the SW of Bailly were bright with sunlight. The floor to the NE was lit by the rising Sun and looked the same color and intensity as all the nearby other craters. We shall therefore lower the weight of the 1974 LTP report from 1 to 0, thus removing it from our LTP database.

Ptolemaeus: On 2020 May 29 UT 21:10-21:35 Daryl Dobbs observed from 21:15-22:15, Les Fry (NAS) imaged at 22:47 and Phil Shepherdson observed (22:45-23:13UT) this crater under a BAA lunar schedule request for the following report: BAA Request: Examine the floor visually, sketch, or image to show the progres- sion of the shadow spires across floor and the emergence of the center of the floor into sunlight. If observing visually, how would you describe the appear- ance of the central lit area on the floor? If imaging, do a time lapse e.g. 1 image per minute to show the progression of the shadow spires. We are asking for these observations following an observation by P. Shepherdson (BAA) on 2020 Feb 01 UT 19:40-19:50 who commented on an unusual appearance to the floor. However, an image supplied suggests it is just shadow spires. Neverthe- less, we would like to check at a repeat illumination. As another challenge, because the light illuminating the floor may come from narrow horizontal gaps on the eastern rim, and maybe slightly polarized see if you can use a polar- ized filter in the field of view at the eyepiece, or in front of the camera, and rotate through different angles. Do you see any change in the appearance of the illuminated area of the floor? Any sketches, visual descriptions, or images taken, should be emailed to: a t c @ a b e r . a c. u k

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Figure 11. Ptolemaeus on 2020 May 29. (Left) an image taken by Les Fry (NAS) at 22:47 UT. (Right) an image by Phil Shepherdson (BAA) taken at 23:13 UT.

Daryl reports : “The object of this observing run was to see if the emerging floor and shadow spires had any unusual features. Observation terminated due to obscuring hill and houses. Throughout this ob- serving run I used a Baader polarizing filter swapping it out every 3-4 minutes, each time I used the filter I rotated it in the focuser 360 degrees, however I could not detect any discernible difference in using the fil- ter. When I started the observing run the floor was in deep shadow, by 21.15 a light elongated area became visible under the southern wall. As the shadow spires appeared the next area to come into illumination was in the center of the crater followed progressively towards the original area and slightly north of center, un- til at the end of the observing run an area approximately 1/3 of the crater width and 2/3rds its length was illuminated pierced with shadow spires. The area being illuminated had an even tone as the area increased in size. The first area to be illuminated between 22.18 and 22.30had an uneven edge facing the Southern wall of Ptolemaeus, this was in contrast to the sharp edges on the rest of the shadow spires. After 22.30 un- til the observing run ended this turned into a sharp edge. The seeing conditions however deteriorated from ii to iii, due most likely to rising heat from houses nearby. From 22.15 a dark line appeared run- ning SW to NE the area either side of this was a uniform shade, the dark line. I could not detect anything unusual compared to previous observations apart from the uneven edge on the luminated area under the southern wall”. A sketch was provided but is not shown here.

Phil Shepherdson comments that “Luckily last night (29 - early 30 May),I managed to observe once more the shadows within Ptolemaeus but this time, there was no bright 'ashen' light that I had observed on Feb1st. Please forgive my sticking to my guns, but I will stand by my observation however weird it appears to be. I have taken a picture of 30 May just after midnight of the crater, but it is not very good” (Fig 11 - Right). Les Fry also took an image that night, but it was too early for the shadow spires to occur (Fig 11 – Left) as the floor is completely shadow filled at that point.

Mons Piton: On 2020 May 29 UT 22:48 Rob Davies (BAA/NAS) imaged the area under similar illumina- tion (±0.5°) to the following report:

On 1983 May 20 at UT00:00-03:00 K. Marshall (Medellin, Columbia) noted that Mons Piton was too bright near the terminator and was surrounded by shadow. A sketch was made. The mountain appeared segmented with one thin shadow line. The mountain looked like a Mexican Sombrero hat. This appearance is normal. What was abnormal was that Piton was brighter than Proclus, and only slightly fainter than Censorinus. The CED brightness measurements were normal Pi- ton=3.6, Proclus=3.5 and Censorinus=3.7. Please check to see whether this is still the case. The Cameron 2006 catalog ID=221 and the weight=3. The ALPO/BAA weight=1. The Lunar Observer/July 2020/ 130

Figure 12. Mons Piton as imaged by Rob Davies (BAA/NAS) on 2020 May 29 UT 22:48 and orientated with north towards the top.

As you can see from Rob Davies’ image (Fig 12), Mons Piton is bright, but perhaps not “very bright”. We shall therefore leave the weight at 1 for now.

Proclus: On 2020 May 29 UT 22:50-23:05 Nigel Longshaw (BAA) sketched the crater under similar illu- mination (±0.5°) to the following report:

Proclus 1972 Jan 23 UT 15:20-16:50 observed by Stolzen (51.17N, 9.25E, 50mm refractor, T=2, S=2) "Pure bright white point within crater" - Hilbrecht and Kuveler, Earth, Moon & Planets, 30 (1984), p53-61. ALPO/BAA weight=1.

Figure 13. Proclus as sketched by Nigel Longshaw (BAA) on 2020 May 29 UT22:50-23:05.

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Nigel comments that the crater floor appeared uniform throughout (See Fig 13) and there were no bright spots noted within the crater, contradicting the appearance that Stolzen recorded. Nigel was using a 77mm refractor, which was comparable in size to the one that Stolzen used. We shall therefore keep the 1972 re- port at a weight of 1.

Alphonsus: On 2020 May 30 the crater was imaged by BAA members Bob Stuart (20:05UT) and Derick Ward (21:09-21:11) under similar illumination and topocentric libration (±1°) to the following LTP report:

Alphonsus 1966 Apr 28 UT 21:58 Observed by Smith (England, 10" reflector) and Corralitos Observatory (Organ Pass, NM, USA, 24" reflector+Moon Blink) "Reddish patches, (not confirmed at Corralitos with MB tho they give feature as Gassendi in their report)." NASA catalog weight=2. NASA catalog ID #930. ALPO/BAA weight=1.

Figure 14. Alphonsus on 2020 May 30 orientated with north towards the top. (Left) A detailed monochrome image by Bob Stuart (BAA/NAS) at 20:05UT. (Right) A color image by Derick Ward (BAA) at 21:09-21:11 with color saturation increased to 60% - some atmospheric spectral dispersions and/or chromatic aberration color fringes now shows up on contrasty edges in the image.

Looking at the Cameron description of the 1966 LTP, I would be very surprised if New Mexico and England had the Moon at good observing altitudes, and at night, at both sites at the same time. I suspect the Corralitos observation must have come a few hours after the Smith report. Therefore, it is probably incor- rect to say that Corralitos could not confirm the LTP if the LTP was short lived. Anyway, we now have views of what the crater should have looked like to Smith in Fig 14, and you can see from Fig 14 (Right) that there are not normally redish patches on the floor of Alphonsus. Although the dark pyroclastic patches on the floor are a slight blown, they would have been too faint to have seen visually. We shall therefore keep the weight of this LTP at 1, but will consider changing it to 2 once we get a few more color images of this area and perhaps find more details about the Smit report.

Autolycus: On 2020 May 30 UT 23:31 Aylen Borqatello Alaniz (AEA) was imaging the vicinity around Hyginus N, when they caught Autolycus in the field of view are similar illumination to the following re- port:

On 1984 Dec 01 at UT 20:00 a British Astronomical Association Lunar Section member (Southam, Warwickshire, UK) found no detail on the floor of Autolycus, despite there being plenty of detail on the floor of crater. Ac- cording to Foley, there should be some detail at this stage of illumination. Grego reports that the observation was from a Society for Popular Astronomy member and they described "a homogeneous grey veil over the 20 km floor of the crater". The Cameron 2006 catalog ID=255 and the weight=2. ALPO/BAA weight=2

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Figure 15. Autolycus as imaged by Aylen Borqatello Alaniz (AEA) on 2020 May 30 UT 23:31 and orien- tated with north towards the top.

Indeed, Aylen’s image (Fig 15) does show that at this stage in illumination, Autolycus should have detail upon its floor. Therefore, we will leave the weight of then1984 report at 2 because the description sounds unusual!

Mare Frigoris: On 2020 May 31 Daryl Dobbs sketched (21:00-21:42UT) and Bill Leatherbarrow imaged (20:30UT) this area for a repeat illumination request by the UAI:

Figure 16. Mare Frigoris on 2020 May 29 orientated with north towards the bottom. (Left) a sketch by Daryl Dobbs made at 21:00-21:42UT. (Right) An image by Bill Leatherbarrow (BAA) made at 20:30 UT.

As the observational request was from the UAI, these reports will be sent off to them. However, I just wanted to show you how useful the Lunar Schedule web site can be for purposes other than eliminating past LTP reports e.g. it is also useful for dome observing.

General Information: For repeat illumination (and a few repeat libration) observations for the coming month - these can be found on the following web site: http://users.aber.ac.uk/atc/ lunar_schedule.htm . By re-observing and submitting your observations, only this way can we fully resolve past observational puzzles. To keep yourself busy on cloudy nights, why not try “Spot the Difference” be- tween spacecraft imagery taken on different dates? This can be found on: http://users.aber.ac.uk/atc/tlp/ spot_the_difference.htm . If in the unlikely event you do ever see a LTP, firstly read the LTP checklist on http://users.aber.ac.uk/atc/alpo/ltp.htm , and if this does not explain what you are seeing, please give me a call on my cell phone: +44 (0)798 505 5681 and I will alert other observers. Note when telephoning from outside the UK you must not use the (0). When phoning from within the UK please do not use the +44! Twitter LTP alerts can be accessed on https://twitter.com/lunarnaut .

Dr Anthony Cook, Department of Physics, Aberystwyth University, Penglais, Aberystwyth, Ceredigion, SY23 3BZ, WALES, UNITED KINGDOM. Email: atc @ aber.ac.uk

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Key to Images In This Issue

1. Albategnius 19. Grimaldi 37. Plato 2. Alpine Valley 20. Horrebow 38. Posidonius 3. 21. Janssen 39. Proclus 4. Anaximenes 22. Julius Caesar 40. Ptolemaeus 5. Archimedes 23. Lade 41. Purbach 6. Aristarchus 42. Pythagoras 24. Langrenus 43. Rima Ariadaeus 7. Aristoteles 25. Lichtenberg 44. Rima Hyginus 8. Atlas 26. Longmontanus 45. Schoter’s Valley 9. Bossingault 27. Mare Serenitatis 46. Sinus Iridum 10. Bullialdus 28. Marius 47. Sirsalis 11. Cassini 29. Maurolycus 48. Straight Wall 12. Clavius 30. Messier 49. Thebit 13. Copernicus 31. Meton 50. Theophilus 14. Deslandres 32. Mons Apenninus 51. Tycho 15. Endymion 33. Mons Rumker 16. Euclides 34. North Pole 17. Fracastorius 35. Petavius 18. Gassendi 36. Piccolomini

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