Astronomy July 2014

Total Page:16

File Type:pdf, Size:1020Kb

Astronomy July 2014 IMAGER PROFILE With remote observatories in GERALD Namibia and the Alpen foothills, this Austrian imager can lock his lens RHEMANN on any comet or nebula he likes. text and images by imaging from Gerald Rhemann near and far My first encounter with astronomy wasn’t until 1986. Intrigued by the frequent media reports about the return of Halley’s Comet, I decided to have a look through a big telescope myself. I trav- eled to the western suburbs of Vienna — the capital city of Austria and my hometown — where the historic Kuffner Observatory and its 10.6-inch (270 millimeters) refract- ing telescope live. But what I saw through the eyepiece dis- appointed me. Even through this big refrac- tor, Comet 1P/Halley appeared as nothing more than a foggy patch — no evidence of the impressive tails that shone through in photographs. Still, Halley aroused my inter- est enough that a couple of years later, in 1989, I purchased a telescope and mount. I wanted to make images that captured the For several months, the author (pictured above) had same level of detail I had seen in photos of the opportunity to remotely control an astrograph that comet, detail that the eye alone can’t located in Nerpio, Spain. With it, he captured IC 2177, the Seagull Nebula in Monoceros (right). see. Plus, because I was the owner of a pho- This image had 21.9 total hours of exposure — the tography shop, I had ready access to all the longest of any object the author has ever captured. other stuff I needed — cameras, lenses, a (ASA 8-inch f/2.9 hyperbolic astrograph, FLI PL darkroom, and experience. 16803 CCD camera, HαLRGB image with 180, 555, 224, 140, and 217 minutes of exposure, respectively) Comets in the foothills My backyard, however, was not an ideal Austria. Because Jäger and I share an inter- observing spot. Vienna’s light-polluted skies est in taking portraits of the solar system’s didn’t lead to photographic success. Fortu- oldest inhabitants, a deep and lasting friend- nately, I met Michael Jäger, the most experi- ship developed between us. He showed me enced and successful comet imager in his favorite dark-sky sites: observation- friendly spots in the Austrian Voralpen. In Gerald Rhemann has been sky-shooting since these foothills of the Alps, less than an 1989. His work has been featured in scientific hour’s drive from my home, light pollution papers and on NASA websites. is nearly nonexistent. 46 ASTRONOMY • JULY 2014 The author captured Comet Lovejoy (C/2013 R1) on the morning of December 14 from Jauerling, a mountain in the Austrian Voralpen. The CCD’s sensor was sensitive to blue light and therefore accentuated the ion tail structures, whose carbon monoxide causes the hue. The comet was active and powerful enough that its ion tail visibly changed from one day to the next. The image is The region around Antares (Alpha [α] Scorpii) is one of the most amazing and beautiful in the entire sky, a two-panel mosaic. (8-inch f/2.9 ASA hyperbolic containing a complex mix of emission and reflection nebulae, dust lanes obscuring background stars, and astrograph, FLI PL 16070 CCD camera, LRGB im- star clusters. The author took this six-panel mosaic from Namibia over the course of three nights. (8-inch age with 5-minute exposures through each filter f/2.9 ASA hyperbolic astrograph, FLI PL 16070 CCD camera, LRGB image with exposures of 35, 25, 25, and for each panel) 40 minutes, respectively, for each panel) For imaging bright comets or comets at moves in the field during the exposure — The era of chemical film low altitude under the transparent Voralpen and sometimes its tail structure changes I first imaged deep-sky objects and comets skies, I have portable equipment: an Astro- quite quickly as well — processing observa- through an 8-inch Celestron and later a 5.2- systeme Austria (ASA) DDM60 mount and tions isn’t straightforward. To get both pin- inch Takahashi Epsilon 130 astrograph. an ASA 8-inch f/2.9 hyperbolic astrograph. point star shots and a sharp comet image, I After I became more proficient, I decided to Although trekking out there is a challenge first remove the stars. Then, going back to purchase a Schmidt camera, then the most and requires discipline, especially on a cold the original picture, I remove the comet suitable instrument for comet imaging. winter night, it feels worth the effort when I from the star field, and — finally — I put The camera was a small one, only suit- can capture crisp shots of comet tails them back together again. That might sound able for use with 35mm film, and it was streaming through space. easy, but it is not. tricky to work with: I had to cut the film But creating those pictures is no small My images are so precise that I report and load the pieces into the film holder task. Both the imaging and the processing of positional observations to the International without scratching them or getting any dynamic observations like these are time- Astronomical Union, which has designated dust or moisture on them — and I had to consuming. Because a comet perceptibly my observatory in Eichgraben C14. do this in an improvised darkroom in the 48 ASTRONOMY • JULY 2014 Observing hot spots Eichgraben, Austria EUROPE Voralpen, Austria AFRICA : ROEN KELLY ROEN : Tivoli, Namibia ASTRONOMY This portrait of reflection nebula IC 4592 also shows IC 4601 in the lower left. (8-inch f/2.9 ASA hyperbolic astrograph, FLI PL 16803 CCD camera, LRGB image with exposures of 55, 30, 20, and 50 minutes, respectively) back of my car. But the hardship provided installed my first CCD camera, a Starlight valuable practice, and I worked myself up Xpress SXV-H9. to a larger Schmidt camera that was suit- Imaging with this camera opened a able for 6x6cm plates. With a focal length of whole new world and new feeling for me. 450mm and a focal ratio of f/2.0, this cam- Because I could immediately see what I was era was fast and produced great images photographing, I could be sure the image across the entire field of view. was in focus and the mount was tracking In those days, commercial film just properly. Moreover, the digital “darkroom” wasn’t ready for astroimaging. We photogra- rendered unimaginable possibilities in pro- phers had to alter it a bit. Using nitrogen gas, cessing plausible, as the throughput we hypersensitized the film to reduce reci- increased enormously. There are always procity failure, which makes the film less trade-offs, though: lots of cables and lots of responsive after a certain amount of expo- electricity — both of which made traveling sure time. We also had to develop and print to observing sites difficult. the film ourselves, which required access to Not one to be deterred, I solved the a darkroom. In view of all these difficulties, problem by building an observatory in the only a few amateurs worldwide attempted backyard of my weekend house in Eichgra- serious astrophotography. With the Schmidt ben, Lower Austria. It has a roll-off roof and camera, however, and doing considerable is fully remote-controlled — I can obtain preparatory work, I obtained several hun- images wherever I am. The observatory has dred images of comets and deep-sky objects. a 12-inch ASA 12N astrograph at f/3.6 on an ASA DDM85 direct drive mount and a Step into the digital age Finger Lakes Instrumentation ML8300 In 2003, I recognized that the time of film CCD camera. had passed, and I switched to CCD astro- The author’s remote-controlled observatory in Eichgraben, Lower Austria, contains a 12-inch ASA photography. Meanwhile I had acquired a Under southern skies 12N astrograph at f/3.6 on an ASA DDM85 mount. 14-inch Cassegrain telescope with a prime Even though I now have many nearby He also observes from the Austrian Voralpen and focus option at f/3.0. On this instrument, I observing options, the summer nights at Namibia, where he has a remote setup. WWW.ASTRONOMY.COM 49 On an average night, the seeing in Eichgraben is only moderately good. But in spring, it sometimes is decent enough to use the ASA Barlow Corrector to get a longer focal length (2,070mm) with a 12-inch ASA 12N astrograph at f/6.8, as the author did to obtain this image of Bode’s Galaxy (M81). (FLI ML8300 CCD camera, LRGB image with exposures of 240, 110, 70, and 140 minutes, respectively) In this April 1997 giving visitors like me full access to our gal- image, Comet Hale- axy’s core wonders. Bopp’s (C/1995 O1) tail stretches up to During my 2010 stay in Namibia, I the Double Cluster in installed the same type of equipment that I Perseus (NGC 869/884). have in my observatory in Eichgraben in a The observations were friend’s nearby Southern Hemisphere obser- recorded on Kodak Pro Gold 6x6cm plates. vatory. By 2012, that observatory was fully (225/255/450mm remote-controlled, and I have access to this Schmidt camera, expo- 12-inch astrograph whenever I want. sure of 5 minutes) In the future, I plan to use this telescope for comet searching. The probability of find- ing a new visitor to the inner solar system is much greater in the Southern Hemisphere Austrian latitudes are short and the weather are available — even in the middle of the than in the north, where several professional is unstable.
Recommended publications
  • Orion Newtonian Astrograph Instruction Manual
    INSTRUCTION MANUAL Orion 8" and 10" f/3.9 Newtonian Astrographs #8297 8" f/3.9, #8296 10" f/3.9 #8296 Providing Exceptional Consumer Optical Products Since 1975 OrionTelescopes.com Customer Support (800) 676-1343 • E-mail: [email protected] Corporate Offices (831) 763-7000 • 89 Hangar Way, Watsonville, CA 95076 © 2011 Orion Telescopes & Binoculars IN 406 Rev. A 07/11 2" Finder scope Accessory bracket collar 9x50 Finder Scope Optical tube Tube rings Focus wheel Drawtube Fine focus wheel tensioning thumbscrew Focus wheel Figure 1. The Orion 8" f/3.9 Newtonian Astrograph Congratulations on your purchase of an Orion f/3.9 Newtonian Astrograph! These powerful imaging telescopes feature “fast,” high-quality parabolic optics, a 2" dual-speed Crayford focuser, and excellent mechanical construction with some special features. Optimized for astrophotography with DSLR and astronomical CCD imaging cameras, our f/3.9 Newtonian Astrographs are capable of delivering breathtak- ing imaging performance – for beginning to advanced astrophotographers. This instruction manual covers both the 8" and 10" mod- Parts List els of f/3.9 Newtonian astrograph. Although they differ • Optical tube assembly in aperture and focal length, physical size, and weight, they are otherwise very similar in mechanical construc- • Optical tube dust cap tion and features. So we will use the 8" model to illus- • 1.25" eyepiece holder trate the features of both astrographs. Any exceptions • 9x50 finder scope with bracket related to the 10" model will be noted. • Pair of hinged tube rings This instruction manual will help you to set up and • 2" thread-on extension adapter, 30mm properly use your telescope.
    [Show full text]
  • U. S. Naval Observatory Washington, D. C. 20392-5420 Ued to Advance for the Astronomical Almanac and Astro- Nomical Phenomena
    633 U. S. Naval Observatory Washington, D. C. 20392-5420 ued to advance for The Astronomical Almanac and Astro- nomical Phenomena. The Astronomical Almanac for 2001 was published at the earliest date in over 15 years. Proceed- I. PERSONNEL ings of the U.S. NAO Sesquicentennial Symposium, held last A. Civilian Personnel year, were published during this reporting period. USNO Circular 178, ‘‘List of Active Professional Observatories,’’ Retirements included Alan Bird. by M. Lukac and R. Miller, went to press in June 2000. Tom Corbin retired on Oct. 2, 1999 after a 35-year career Exchange of material also continued with both the Institut de at USNO. F.S. Gauss retired on 2 June, after a 37-year career Mechanique Celeste ͑France͒ and HMNAO. at USNO. A major effort to streamline almanac production is ongo- ing within the NAO. S. Stewart continued to review, docu- B. DoD Science and Engineering Apprenticeship ment, upgrade, and standardize production of Sections E and Program HofThe Astronomical Almanac, as well as documenting the rest of the sections prepared by the U.S. NAO. This infor- The USNO summer intern program for high school and mation and the status of all publications are now on-line college students continued in the summer of 1999. This pro- within the department for easier access and timeliness. Al- gram, called the Science and Engineering Apprentice Pro- manac production software is being moved into an auto- gram ͑SEAP͒, is sponsored by the Department of Defense mated version control system for the purposes of standard- ͑DoD͒ and managed by George Washington University.
    [Show full text]
  • Orion® Ritchey-Chrétien Astrographs
    INSTRUCTION MANUAL Orion® Ritchey-Chrétien Astrographs #8268 6" f/9 RC #8267 8" f/8 RC #8266 10" f/8 RC #8267 #8266 #8268 Providing Exceptional Consumer Optical Products Since 1975 OrionTelescopes.com Customer Support (800) 676-1343 • E-mail: [email protected] Corporate Offices (831) 763-7000 • 89 Hangar Way, Watsonville, CA 95076 IN 361 Rev. B 5/15 Congratulations on your purchase of an Orion Unpacking Your Telescope Ritchey-Chretien astrograph. These compact but large-aperture telescopes are designed and opti- Use care when unpacking the shipping carton. We recom- mized for high-performance astrophotography mend keeping the boxes and all original packaging materi- als. In the event that the telescope needs to be shipped to with CCD and DSLR cameras. Sporting an optical another location, or returned for warranty repair, having the design comprising hyperbolic primary and second- proper packaging will ensure that your telescope will survive ary mirrors, the RC is highly regarded by advanced the journey intact. Returns for refund or exchange will not be astrophotographers and professional observato- accepted without all of the original packaging. Once all items ries worldwide. Even the vaunted Hubble Space have been removed from the box take a moment to confirm Telescope is an RC! Orion RCs deliver exceptional that all pieces are present and intact. Refer to the Parts List to aid in identifying the included items. image quality and resolution with zero image shift, minimal coma, a highly baffled steel tube for out- standing contrast, and exclusive mounting options The Focuser for optional finder scopes and guide scopes.
    [Show full text]
  • The Wide Field Cassegrain: Exploring Solution Space Peter Ceravolo Ceravolo Optical Systems [email protected]
    The Wide Field Cassegrain: Exploring Solution Space Peter Ceravolo Ceravolo Optical Systems www.ceravolo.com [email protected] Abstract This article illustrates the use of an internal aperture stop in a high speed, wide field Cassegrain optical system. The astrograph features a well corrected and uniformly illuminated focal plane. Opto-mechanical design and manufacturing issues are also discussed. 1. Introduction Of all the conventional astronomical telescope Aperture Stop designs used in amateur astronomy the Cassegrain is the least likely to be considered a candidate for wide field imaging applications. This perception is a hangover from the era of visual observing where minimizing the central obscuration was critical to preserving image fidelity. The resulting long focal length, slow telescopes did not lend themselves to photography. The central obscuration in reflector astrographs need not be so constrained since ground based amateur instruments never achieve diffraction limited performance, primarily due to poor seeing, image sampling limitations and tracking errors. Cassegrain astrographs with a large obscuration (50% of the aperture diameter or greater) and a fast primary will permit a relatively short overall focal length, a wider field of view and more uniform focal plane illumination. While the larger obscuration does reduce system through put, the light loss can be compensated for with longer exposures. Figure 1, internal stop Cassegrain astrograph In addition to the benefits of a larger obscuration, allowing the aperture stop position to move from the primary mirror to a more central location in the Cassegrain optical system offers the potential to achieve very wide fields of view in a fast system 2.
    [Show full text]
  • Comets in UV
    Comets in UV B. Shustov1 • M.Sachkov1 • Ana I. G´omez de Castro 2 • Juan C. Vallejo2 • E.Kanev1 • V.Dorofeeva3,1 Abstract Comets are important “eyewitnesses” of So- etary systems too. Comets are very interesting objects lar System formation and evolution. Important tests to in themselves. A wide variety of physical and chemical determine the chemical composition and to study the processes taking place in cometary coma make of them physical processes in cometary nuclei and coma need excellent space laboratories that help us understand- data in the UV range of the electromagnetic spectrum. ing many phenomena not only in space but also on the Comprehensive and complete studies require for ad- Earth. ditional ground-based observations and in-situ exper- We can learn about the origin and early stages of the iments. We briefly review observations of comets in evolution of the Solar System analogues, by watching the ultraviolet (UV) and discuss the prospects of UV circumstellar protoplanetary disks and planets around observations of comets and exocomets with space-born other stars. As to the Solar System itself comets are instruments. A special refer is made to the World Space considered to be the major “witnesses” of its forma- Observatory-Ultraviolet (WSO-UV) project. tion and early evolution. The chemical composition of cometary cores is believed to basically represent the Keywords comets: general, ultraviolet: general, ul- composition of the protoplanetary cloud from which traviolet: planetary systems the Solar System was formed approximately 4.5 billion years ago, i.e. over all this time the chemical composi- 1 Introduction tion of cores of comets (at least of the long period ones) has not undergone any significant changes.
    [Show full text]
  • J'/ 7 ~,J,,F42~OD'/ 4~Z T 0014- AL4 '4 N 444 4 V-~ V~'4,,/C4D4 ;/L X' 3* ''(N I /I -- -K
    4'T,4 "~ J, itI' ~ " 4 4~~~~~~t f"- N'. 4 tV34 '' '4~~~~~~~r "''',) m/4' - 4 / .,~~~~t 4f {'NW ' I, '~ / . 4 4'~~~~~-' ~~~~-"" ' ' A '' " I \ ' o A4 j'/ 7 ~,j,,f42~OD'/ 4~z t 0014- AL4 '4 N 444 4 v-~ v~'4,,/C4D4 ;/l x' 3* ''(N I /I -- -K . 2 . /-, -, 1 '> 97 (; ' '-I' -4 )-' Ni\iS ,L -I-' "1/ iT h 'i l I .=.,, ca ec~- fr ain ivsoOd* .: 25 C , '-A- ", ---.- a a en .- -_ . - ; . - - '1 (N, -< I' 4 -I --. N ?- j -. Thspprpeet h veso h uhrs adde o eesr .I ~rf~c :";athethe vieio oddr Spce ight Cenbitr o: NASA r 7-ref e.'th viGods th~ar ddSpace', Fligt . enter. .. orN-/- " -- -' -- I / -I- _ . - " . -,t -" , *-*- . : TABLE OF CONTENTS Page LIST OF ATTENDEES 3 FOREWORD 6 INTRODUCTION TO SPACELAB/SHUTTLE 8 ASTRONOMY PAYLOADS 12 I. A Very High Resolution Spectrograph for Interstellar Matter 15 Research - E. Jenkins and D. York, Princeton University Observatory 2. Schmidt Camera/Spectrograph for Far Ultraviolet Sky Survey 20 G. Carruthers and C. Opal, Naval Research Laboratory 3. UV Telescope with Echelle Spectrometer - Y. Kondo and 25 C. Wells, Johnson Spacecraft Center 4. Small Infrared Cryogenic Telescope - R. Walker, Air Force 29 Cambridge Research Laboratory 5. Two EUV Experiments - S. Bowyer, University of California 33 at Berkeley 6. Ultraviolet Photometer - A. Code and R. Bless, University 39 of Wisconsin 7. Schwarzschild Camera - A. Smith, Goddard Space Flight Center 43 8. Three Rocket-Class Payloads for Spacelab - C. Lillie, 49 University of Colorado 9. Additional Payloads 57 ASTRONOMY MISSION STUDIES - W. Scull, Goddard Space Flight Center 60 SMALL INSTRUMENT POINTING SYSTEM (SIPS) - C.
    [Show full text]
  • To Photographing the Planets, Stars, Nebulae, & Galaxies
    Astrophotography Primer Your FREE Guide to photographing the planets, stars, nebulae, & galaxies. eeBook.inddBook.indd 1 33/30/11/30/11 33:01:01 PPMM Astrophotography Primer Akira Fujii Everyone loves to look at pictures of the universe beyond our planet — Astronomy Picture of the Day (apod.nasa.gov) is one of the most popular websites ever. And many people have probably wondered what it would take to capture photos like that with their own cameras. The good news is that astrophotography can be incredibly easy and inexpensive. Even point-and- shoot cameras and cell phones can capture breathtaking skyscapes, as long as you pick appropriate subjects. On the other hand, astrophotography can also be incredibly demanding. Close-ups of tiny, faint nebulae, and galaxies require expensive equipment and lots of time, patience, and skill. Between those extremes, there’s a huge amount that you can do with a digital SLR or a simple webcam. The key to astrophotography is to have realistic expectations, and to pick subjects that are appropriate to your equipment — and vice versa. To help you do that, we’ve collected four articles from the 2010 issue of SkyWatch, Sky & Telescope’s annual magazine. Every issue of SkyWatch includes a how-to guide to astrophotography and visual observing as well as a summary of the year’s best astronomical events. You can order the latest issue at SkyandTelescope.com/skywatch. In the last analysis, astrophotography is an art form. It requires the same skills as regular photography: visualization, planning, framing, experimentation, and a bit of luck.
    [Show full text]
  • Lick Observatory Records: Correspondence UA.036.Ser.01
    http://oac.cdlib.org/findaid/ark:/13030/c8dj5m3f No online items Guide to the Lick Observatory Records: Correspondence UA.036.Ser.01 Alix Norton University of California, Santa Cruz 2015 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Guide to the Lick Observatory UA.036.Ser.01 1 Records: Correspondence UA.036.Ser.01 Language of Material: English Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Correspondence Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.01 Physical Description: 148.5 Linear Feet257 boxes and 54 microfilm reels Date (inclusive): 1833-2009 Date (bulk): 1870-1960 Access Collection is open for research. The physical copybooks are restricted due to the fragile nature of the material. All use is directed to the microfilm of these volumes. The microfilm reels can be accessed by requesting them from Special Collections via the Library Catalog. Historical note The Lick Observatory was completed in 1888 and continues to be an active astronomy research facility at the summit of Mount Hamilton, near San Jose, California. It is named after James Lick (1796-1876), who left $700,000 in 1875 to purchase land and build a facility that would be home to "a powerful telescope, superior to and more powerful than any telescope yet made". The completion of the Great Lick Refractor in 1888 made the observatory home to the largest refracting telescope in the world for 9 years, until the completion of the 40-inch refractor at Yerkes Observatory in 1897. Since its founding in 1887, the Lick Observatory facility has provided on-site housing on Mount Hamilton for researchers, their families, and staff, making it the world's oldest residential observatory.
    [Show full text]
  • Astrometry with Small Instruments
    ASTROMETRY WITH SMALL INSTRUMENTS Petre Popescu1, Alin Nedelcu1, Radu Popescu1, Octavian Bădescu1,2 1Astronomical Institute of Romanian Academy: [email protected]; [email protected]; [email protected]; 2Technical University of Civil Engineering, Faculty of Geodesy: [email protected] Abstract Based on an analyze concerning Bucharest astrometric instruments, a modernization project was elaborated. There are exposed the general aims of the project and the preliminary results obtained: the selection of data from astronomical catalogues, data acquisition concerning instrument positioning and tracking, data selection from astronomical image acquisition system and data processing by means of specific procedures. I. Observational astrometry in Romania Main topics of research in Romanian astrometry were connected with the use of 4 instruments: Prin-Merz Astrograph, Meridian Circle Gauthier- Prin, Zeiss Transit Telescope and Danjon Astrolabe. Meridian Circle Gauthier-Prin 19/235 cm was installed in 1926, it had an important contribution in improving, in an extended international cooperation, stellar catalogues. Zonal and local catalogues for different purposes were built using this instrument. The developments of CCD astrometry and the difficulties of financing such a special project obliged us to stop visual observations. Now the Meridian Circle is preserved and we are studying the opportunity of future modernization. Zeiss Transit Telescope 10/100 cm was set up in 1956 and was used for Earth rotation monitoring. After using 30 years, taking into account the new development of this class of instruments we stopped the observations. In the future, such an astronomic instrument has no use, except for education. Danjon Astrolabe 10/100 cm was borrowed from Brussels Observatory and installed in 1993.
    [Show full text]
  • JUNE 2011 Sky Tch
    WESTCHESTER AMATEUR ASTRONOMERS JUNE 2011 Sky tch Sea of Rains Rick Bria took this picture of the Moon on May 12th at the Mary Aloysia Hardey Observatory. Explains Rick: Just right of center is Mare Imbrium, Latin for “Sea of Rains”. It’s a 1200 kilometer wide circular smooth area created by a large impact 4 billion years ago. The impact formed 7km high mountains chains that encircle Mare Imbrium. Lava then filled the crater giving it a smooth look. The crater Plato is also lava filled and very smooth. Formed by an impact just after the formation of Mare Imbrium, Plato is 100 kilometers across. Copernicus is an impact crater 93 kilometers in diameter and 4 kilometers deep. At only 800 million years old, Copernicus is much younger than Plato. As a result, its shape is noticeably more sharp and detailed. Copernicus has a rather obvious ray system formed by ejected material blasted out by the impact. This ray system is most obvious at full Moon, but can be seen in the attached picture taken just after first quarter phase. SERVING THE ASTRONOMY COMMUNITY SINCE 1983 Page 1 WESTCHESTER AMATEUR ASTRONOMERS JUNE 2011 Events for June 2011 WAA Lectures WAA Club Picnic “Exploring Exotic Matter of the Saturday June 18th, 2pm Universe” Friday June 3rd, 7:30pm Trailside Museum, Ward Pound Ridge Miller Lecture Hall, Pace University The event is for WAA members and their guests only. Club members are encouraged to bring side-dishes, Pleasantville, NY salads and desserts. Tell the guard at gatehouse you Deirdre Frost will speak on the search for unusual are going to WAA Picnic.
    [Show full text]
  • Innovative Astronomy Gear Products Our 16Th Annual Roundup of Hot Products Highlights the for Most Intriguing New Astronomy Gear in the Worldwide Market
    Innovative Astronomy Gear Products Our 16th annual roundup of Hot Products highlights the for most intriguing new astronomy gear in the worldwide market. 2014 By the Editors of Sky & Telescope Wow! What a year it’s been for product introductions. When we fi nished compiling our “short list” of candidates for this year’s Hot Products, we had the biggest list ever in the history of pre- paring our annual survey. Furthermore, when the dust settled and we had our fi nal selection, it too comprised the most items ever. While it’s been a great year for new products, things need to be more than just “new” to make our list. They need to introduce new technologies, off er solutions to old problems, or deliver unprecedented value. As such, our selection aims to honor the products that help our hobby evolve. This year’s picks range from the elegantly simple (the dual fi nder bracket on page 68) to the mind-bogglingly complex (the Diff erential Autoguider System on page 66). The costs are equally varied, ranging from a free smartphone app to telescopes costing $15,000 and more. As always, we hope you enjoy reading about the new products that intrigued us the most for 2014. ▶ StarSense AutoAlign Celestron • celestron.com U.S. price: $329.95 Celestron’s SkyProdigy telescopes (reviewed in our March 2013 issue, page 62) introduced the company’s StarSense Technology, which uses a dedicated imaging module to provide foolproof initialization of the scopes’ computerized Go To pointing. The new StarSense AutoAlign system now brings that technology to the company’s full line of Go To telescopes.
    [Show full text]
  • January's Sky in Memoriam 29 Things About Comets
    January 2013 - Volume 8, Number 1 David Garner, Editor We welcome your comments on the Bulletin. Email them to the Editor at [email protected]. A PDF version of the Bulletin is available here. A Web-based version of the Bulletin is available here. January's Sky According to the 2013 Observer's Handbook, the Quadrantid meteors peak on January 3rd. Mercury will not be visible all month but will reappear in the evening sky at month's end. Venus continues dropping lower in the early morning eastern sky whereas Mars is low in the SW evening sky. Look for Jupiter on the northern edge of the Hyades and will be occulted by the Moon on the night of the 21st/22nd (for some observers). Saturn is in the dawn sky whereas Uranus and Neptune are low in the western evening sky. The next full Moon occurs on January 27th. In Memoriam British astronomer and broadcaster Sir Patrick Moore has died on 2012 December 9, aged 89. He presented the BBC programme The Sky At Night for 55 years, making him the longest-running host of the same television show ever. 29 Things About Comets by Ron Macnaughton Toronto Centre, Chair, Education Committee Here is a list of 29 things about comets that you might not know: • Edmund Halley noticed that comet sightings in 1531, 1607 and 1682 all had similar retrograde motion. • He suggested in 1705 that all were the same comet and calculated the orbit – a first for an object that was not a planet. • In 1759, it returned later than Halley predicted because Jupiter and Saturn affected its orbit.
    [Show full text]