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A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: Wayne Bailey [email protected] 17 Autumn Lane, Sewell, NJ 08080 RECENT BACK ISSUES: http://moon.scopesandscapes.com/tlo_back.html FEATURE OF THE MONTH – JULY 2013 DAMOISEAU-A Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA February 24, 2013 05:05-05:45 UT, 15 cm refl, 170x, seeing 7-8/10 I observed this area on the evening of Feb. 23/24, 2013 after the moon hid kappa Cancri. This area is just south-east of Grimaldi. Lunar librations were favorable for it that evening. Damoiseau A has a low but complete rim from its south end counter-clockwise around to its west side where it meets Damoiseau D. Southward from D, the rim of A becomes ill-defined and peters out, leaving a gap in its south end. Damoiseau D is an egg-shaped crater with its tapered end to the south. Damoiseau AA is the small pit inside the north rim of Damoiseau A, and Damoiseau AB is the similar pit to the east. The floor of Damoiseau A otherwise appears very smooth. Low ridges and strips of shadow protrude from various points on its rim. The southeast rim of Damoiseau A merges smoothly into a strip of dark shadow that ends at Damoiseau F. The Lunar Quadrant map shows a fault there. A small crater is just south of F and a larger shallower crater is to i s east. Neither of these two craters are shown on the Lunar Quadrant map. A shadowless bright spot and a tiny peak are also in this area. An attention-getting crater chain is farther south. From west to east, the three largest craters are Damoiseau C, BB and B. Damoiseau B and BB overlap, but no rim is evident between them. Two modest craters are between Damoiseau C and BB, and three smaller ones are east of Damoiseau 1 B. A low mound and a small bright spot are east of this group. Damoiseau CA is the small, shallow crater west of Damoiseau C. A low ridge is farther to the south. A dark strip of shadow starts south of Damoiseau C, winds between C and CA, and angles toward F, but peters out before reaching that crater. This strip is bright on its sunward side south of C, but not farther north. The Lunar Quadrant map actually shows a fault to be continuous between Damoiseau A and C, but I didn't see it that way. There is a dusky area between the crater chain and Damoiseau F, merging with the fault's interruption. More dusky areas are south of the crater chain. ***************************************** LUNAR CALENDAR JULY-AUGUST 2013 (UT) July 06 12:00 Moon 3.7 Degrees S of Mars July 07 00:37 Moon at Apogee (406,491 km – 252,582 miles) July 07 02:00 Moon 3.6 Degrees SSW of Jupiter July 08 07:15 New Moon (Start of Lunation 1120) July 08 12:00 Moon 0.14 Degrees NW of Mercury July 10 19:00 Moon 6.7 Degrees SSW of Venus July 16 03:19 First Quarter July 16 24:00 Moon 3.2 Degrees SSW of Saturn July 20 03:12 Extreme South Declination July 21 09:00 Moon 1.2 Degrees NW of Pluto July 21 20:28 Moon at Perigee (358,401 km – 222,700 miles) July 22 18:15 Full Moon July 25 02:00 Moon 5.4 Degrees NNW of Neptune July 27 22:00 Moon 3.3 Degrees N of Uranus July 29 17:44 Last Quarter Aug. 03 08:54 Moon at Apogee (405,833 km – 252,173 miles) Aug. 03 22:00 Moon 4.0 Degrees S of Jupiter Aug. 04 09:00 Moon 5.2 Degrees SSW of Mars Aug. 05 05:00 Moon 4.3 Degrees SSW of Mercury Aug. 06 21:50 New Moon (Start of Lunation 1121) Aug. 09 23:00 Moon 4.8 Degrees SSW of Venus Aug. 13 05:00 Moon 3.0 Degrees SW of Saturn Aug. 14 10:56 First Quarter Aug. 16 12:12 Extreme South Declination Aug. 17 20:00 Moon 1.6 Degrees NE of Pluto Aug. 19 01:27 Moon at Perigee (362,264 km – 225,100 miles) Aug. 21 01:44 Full Moon Aug. 21 12:00 Moon 5.3 Degrees NNW of Neptune Aug. 22 22:00 Moon 1.9 Degrees SE of asteroid 324-Bamberga Aug. 24 03:00 Moon 3.2 Degrees NNW of Uranus Aug. 28 09:35 Last Quarter Aug. 29 17:06 Extreme North Declination Aug. 30 23:47 Moon at Apogee (404,882 km – 251,582 miles) Aug. 31 17:00 Moon 4.5 Degrees S of Jupiter 2 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 Journal at appropriate intervals. Our quarterly journal, The Strolling Astronomer, contains the results of the many observing programs which we sponsor including the drawings and images produced by individual amateurs. Additional information about the A.L.P.O. and its Journal is on-line at: http://www.alpoastronomy.org/index.htm 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. 3 When submitting observations to the A.L.P.O. Lunar Section In addition to information specifically related to the observing program being addressed, the following data should be included (Bold items are required): Name and location of observer Name of feature Date and time (UT) of observation Size and type of telescope used Magnification (for sketches) Orientation of image: (North/South - East/West) Seeing: 1 to 10 (1-Worst 10-Best) Transparency: 1 to 6 Medium employed (for photos and electronic images) Additional commentary accompanying images is always welcome. CALL FOR OBSERVATIONS: FOCUS ON: Mons Rumker Focus on is a bi-monthly series of articles, which includes observations received for a specific feature or class of features. The subject for the September 2013 edition will be Mons Rumker. Mons Rumker is most visible on observations close to the terminator, although 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 this to your observing list and send your favorites to: Wayne Bailey - [email protected] Deadline for inclusion in the Mons Rumker article is August 20, 2013 FUTURE FOCUS ON ARTICLES: In order to provide more lead time for potential contributors the following targets have been selected: Subject TLO Issue Deadline Schickard-Wargentin November 2013 October 20, 2013 Aristarchus January 2014 December 20, 2013 4 ALCon 2013 In Atlanta This year, the annual ALPO meeting will again be held in conjunction with the Astronomical League’s ALCon, Wednesday July 24, 2013 through Saturday July 27, 2013 at Fernbank Science Center, near Atlanta, GA. Detailed information can be found in the JALPO vol. 55, #2, Spring 2013, which is freely available at http://www.alpo-astronomy.org/djalpo/55-2/JALPO55-2 - FREE with ALCon 2013 Registration.pdf or on the Astronomical League’s website http://alcon2013.astroleague.org/. A discounted room rate is available at the Emory Conference Center Hotel. This year, all technical papers will be mainstreamed and presented at one location. Previously, the ALPO technical papers were presented separately from the others. Papers will be presented on Wednesday, July 24, and Thursday, July 25. If you would like to present a paper please submit by June 15, 2013, the following: • Title of the paper being presented. • A four- or five-sentence abstract of each paper. • The format in which the presentation will be. • A 100-word biography and a recent photograph of the presenter for posting on the ALCon 2013 website and inclusion in the printed program guide. 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  • Lunar Sourcebook : a User's Guide to the Moon

    Lunar Sourcebook : a User's Guide to the Moon

    4 LUNAR SURFACE PROCESSES Friedrich Hörz, Richard Grieve, Grant Heiken, Paul Spudis, and Alan Binder The Moon’s surface is not affected by atmosphere, encounters with each other and with larger planets water, or life, the three major agents for altering throughout the lifetime of the solar system. These terrestrial surfaces. In addition, the lunar surface has orbital alterations are generally minor, but they not been shaped by recent geological activity, because ensure that, over geological periods, collisions with the lunar crust and mantle have been relatively cold other bodies will occur. and rigid throughout most of geological time. When such a collision happens, two outcomes are Convective internal mass transport, which dominates possible. If “target” and “projectile” are of comparable the dynamic Earth, is therefore largely absent on the size, collisional fragmentation and annihilation Moon, and so are the geological effects of such occurs, producing a large number of much smaller internal motions—volcanism, uplift, faulting, and fragments. If the target object is very large compared subduction—that both create and destroy surfaces on to the projectile, it behaves as an “infinite halfspace,” Earth. The great contrast between the ancient, stable and the result is an impact crater in the target body. Moon and the active, dynamic Earth is most clearly For collisions in the asteroid belt, many of the shown by the ages of their surfaces. Nearly 80% of the resulting collisional fragments or crater ejecta escape entire solid surface of Earth is <200 m.y. old. In the gravitational field of the impacted object; many of contrast, >99% of the lunar surface formed more than these fragments are then further perturbed into 3 b.y.