FOCUS_December, 2014 - Delaware Astronomical Society Website
Transcription
FOCUS_December, 2014 - Delaware Astronomical Society Website
. to eet.. y art ap M P y w lida NT S o H al a GIA u n An ature Fe n i a Ag Vol. 59, No. 10, DECEMBER, 2014 Next Meeting – December 16th, 2014 at 7:00 PM ANNUAL HOLIDAY PARTY & Swap Meet! at the Mt. Cuba Astronomical Observatory ~ Please Join Us for Fellowship and Fun!! ~ IN THIS ISSUE: The sky is getting bigger around the Sawin Observatory. Well, I guess it’s more accurate to say that the VIEW of the sky is getting bigger. It started last Summer when Mt Cuba was doing some clean-up of the grounds and, as an extension of that project, they offered to remove the big tangle of vines and small scrubby trees next to our observing pad. Suddenly our view to the East was much more open. It was then easy to identify which of the bigger trees most encroached on our view and I was able to gain permission from Mt Cuba to remove them - even though it did not help the view from the main dome. To minimize the cost the DAS Board decided to only have trees dropped and to cut up the logs and limbs ourselves. Several boardmembers have volunteered and we’ll be calling for help from the membership. The 4 largest trees have now been cut down with four more smaller ones soon to follow. FREE FIREWOOD! - ALL YOU CAN CARRY! Check out the progress when you come to the Holiday Party on Tuesday the 16th.. Remember to bring your swap-table items and snack goodies to share at our annual Holiday party/Swap Meet/ Meeting on December 16. Peace and Happy Holidays to all! Each issue of FOCUS is full of useful hyperlinks. Just click on any graphic or telltale blue web address and your browser should take you to additional linked web resources. From the Observing Chair Mt. Cuba Public Nights Schedule AstroPhotos by Frank Colosimo DAS Looks for Education Chair Swap Table Information for the Holiday Party AstroPhotos by Ron Worden Sawin Obs. Reminder & DAS Loaner Equipment DAS Yahoo Forum Email Site Info DAS Star Parties, Upcoming Events & Activities Branched Alkyl Found in Space Info of Interest to DAS Members Pages Page Pages Page Page Page Page Page Page Page Page 2-3 2 4-5 6 6 6 7 7 8 8 9 NASA Science News: Japan Launches Asteroid Mission The Yin-Yang of Polar Sea Ice Young Volcanoes on the Moon Rosetta: Probe Drops Lander on Comet “New Horizons” wakes up on Pluto’s door Page 10 Page 11 Page 12 Page 13 Page 14 Astro-Photo and Website of the Month DAS Special Interest Groups Information Info on Memberships and Magazine Subscriptions Info on Board Members and Contact Information The Last Word by Editor Joe Neuberger Page 15 Page 16 Page 17 Page 18 Page 18 The Bubble Nebula: Photo taken by DAS member Rick Davis. Observing with the Delaware Astronomical Society... By Fred De Lucia, DAS Observing Chairperson On October 15 a number of DASers and I were observing from chairs of quite a different sort. Greg Lee, Rob Lancaster, Bill McKibben, Jeff Lawrence, Bill Hanagan, Glenn Bentley, Bob Mentzer, Dave Groski, Greg Weaver, Diana Metzger, Jim Barkley, Ted Trevorrow and others, whom I’m sure I missed, attended “A Decade at Saturn” at the University of Delaware’s Clayton Hall which was sponsored by the Delaware Asteroseismic Research Center at UD and the Mount Cuba Astronomical Observatory, the annual Harcourt “Ace” Vernon Memorial Lecture. From my 4th row observation chair my perspective was near perfect for me. Other DASers chose their observing posts according to their own preferences, be it up front and personal or further back for a more encompassing view (kind of like choosing a Plossl over a wide-field ocular). Introduced by Harry Shipman, the speaker for the evening was planetary scientist Carolyn Porco, imaging team leader for the Cassini mission at Saturn. Ironically, that evening was the 17th anniversary of the launch of the Cassini-Huygens spacecraft aboard a Titan IVB/Centaur. Seven years later and after gravitational assists via flybys of Earth, Venus and Jupiter Cassini arrived in orbit around Saturn on July 1, 2004. On December 25 of that year the Huygens probe separated from Cassini to begin its journey to Saturn’s moon Titan for the first outer solar system landing in January 2005. Dr. Porco’s eyebrow raising presentation included insightful facts and eyepopping pictures from the past 10 years of the Cassini mission at Saturn. The wealth of information she imparted to the audience about the discovery of water on Enceladus, the lakes and methane rain of (Continued on Following Page) “PUBLIC NIGHTS” at the Mt. CUBA OBSERVATORY... MCAO PUBLIC NIGHTS Greg Weaver The Mt. Cuba Observatory Public Nights continue year round! In addition to learning about many aspects of the heavens, you’ll have a chance to visit and view our all-digital full-dome planetarium. You can pick up a schedule when you next come to a meeting or get the latest updated version off the website at: http:// MountCuba.org. Programs are presented on Monday nights at 8pm. Please check the website for full details and updates on programs planned. Interested individuals or groups can apply by letter or call 654-6407 (preferably between the hours of 9 and 11 am, Monday through Friday) to the Observatory to obtain reservations for these “Public Nights”. The Public Nights schedule for 2014 follows: Date Speaker 15 Dec. Judy Provencal Topic The Music of the Stars. 2015 dates for which topics and speakers have yet to be chosen: 12 Jan. 9 March 26 Jan. 23 March 9 Feb 23 Feb. -2- From the Observing Chair (contined from page 2) Titan, the composition of the rings of Saturn and the enormous accomplishments of an international team of the still ongoing mission were humbling enough, but the image which most impressed this earthbound sentient life form was that of the view from Saturn’s rings of the Earth and the Moon (it was the advanced announcement that such a picture would be taken that galvanized tens of thousands of people to wave in the direction of Saturn at the moment that Cassini took the picture in 2013). Seen at a distance of some 900 million miles there were no visible continents. Earth, largely featureless, looked different from other solar system objects only due to its bluish reflection of sunlight. Completely unnoticed were 7 billion people inhabiting the Earth interacting in complex social structures. Also undetected were the varieties of ecosystems with innumerable components affected by countless internal and external factors. Nor were there any traces of evidence linking that blue planet with a spacecraft orbiting a distant world. But, nonetheless, all that and more were there, playing out in the infinite expanse of hostile space but under the fragile protective bubble of our atmosphere, where encouragement and inspiration give rise to anticipation for the continuing exploration of the Solar System… and beyond. Later that evening I couldn’t help but contemplate that the diminutive signatures of the atmospheres of extra-solar planets are now being revealed. What complexities lay unnoticed amidst that increasing count of such worlds that are so much more distant than our neighboring planets? Perhaps in generations to come as the layers of the mysteries of the universe ever so slowly peel away we will finally conclude that life in its unimaginable diversity of forms is as common among the stars as it is on Earth. Have a Happy Holiday Season, everyone. The PRESIDENT’S DAS BOARD MEETING AGENDA for DECEMBER Tuesday, December 16th, 2014 There will be no DAS Board Meeting in December due to the Annual Holiday Party and Swap Meet that is Scheduled for this Date. Don’t forget to JOIN IN and stop by for GREAT Camaraderie and Eats, . along with a FABULOUS SWAP MEET to take care of some of those on your Holiday Gift List!! SEE YOU THERE! 7 to 9pm. -3- Images by Member Frank Colosimo from His Blue Mountain Vista Observatory at New Ringgold, PA IC 2118 (aka Witch Head Nebula) in Eridanus is a large and faint reflection nebula thought to be an old supernova remnant. It glows from radiation from Rigel and is 900 light-years from Earth. Date: Oct-Nov 2014 Location: New Ringgold PA Optics: Takahashi FSQ106ED 530 mm focal length Mount: Paramount MX Camera: SBIG STL 11000 Guiding: internal chip Exposure: RGB R:14x10 min, G:14x10 min, B:15x10 min for a total of 7.2 hrs Processing: Image acquisition using CCD Autopilot. Initial processing was done using Maxim DL with subsequent processing with Photoshop. The Crab Nebula, Messier 1 (M1, NGC 1952), is the most famous and conspicuous supernova remnant, an expanding cloud of gas created in the explosion of a star (supernova) that was observed in the year 1054 AD. It shines as a nebula of magnitude 8.4 near the southern “horn” of Taurus, the Bull. It has apparent dimensions of 6 x 4 arc minutes and is about 6,400 light years away. Imaging data: Date: Jan 3,16 2009 Location: New Ringgold PA Optics: Meade LX200R 14 at f/7.87 Mount: Paramount ME Camera/Filters: Apogee Alta U8300 FLI CFW-2-7 FLI Filters Guiding: Orion Starshoot Autoguider in Orion ST-80 Exposure: Luminance: 8x5 minutes 2x2, R:3x5 min G:4x5 min B:4x8 min Ha: 9X5 min all binned 3x3 for a total of 2.5 hours Processing: Image acquisition using CCD Autopilot. Initial processing was done using Maxim DL with subsequent processing using Photoshop. I combined the HA and R subs in Photoshop to create the Red layer for this image. -4- NGC 185 (aka Caldwell 18) is a dwarf elliptical galaxy about 2 million light-years away in the constellation of Cassiopeia. It is a member of our Local Group of galaxies and is a satellite of the Andromeda Galaxy Messier 31. Unlike most ellipticals which are smooth and featureless, NGC 185 contains young stellar clusters and other features like the dark spot/dark lane that can be seen in the image. Date: Sep - Oct 2014 Location: New Ringgold PA Optics: Hyperion f/8 12.5 inch, FL 2540 mm Mount: Paramount ME Camera: Apogee U8300 Guiding: ST-402 on Innovations Foresight On-Axis Guider Exposure: LRGB: L:21x15 min R:15x10 min, G:11x8 min, B:13x10 min for a total of 11.4 hrs. Processing: Image acquisition using CCD Autopilot. Initial processing was done using Maxim DL with subsequent processing with Photoshop. NGC 1514 is a planetary nebula in Taurus, aka the Crystal Ball Nebula. It has apparent magnitude 9.4 but it is only 2.2 arc minutes in diameter. The wideview field shows the nebula nestled between two brighter magnitude 8 stars the white one to the upper right and the yellow K0 star to the lower left. The nebula’s central star is mag 9 - quite bright for a planetary cs. Two small background stars can be seen near the central star. There is a faint outer envelope around the main nebula, just visible in the image. Date: Nov 20-28, 2014 Location: New Ringgold PA Optics: Hyperion f/8 12.5 inch, FL 2540 mm Mount: Paramount ME Camera: Apogee U8300 Guiding: ST-402 on Innovations Foresight On-Axis Guider, SharpLock focusing method Exposure: LRGB: L:5x10min R:10x8 min, G:10x5 min, B:11x11 min for a total of 5 hrs. Processing: Image acquisition using CCD Autopilot. Initial processing was done using Maxim DL with subsequent processing with Photoshop. -5- DAS Looks for Education Chair--This is a Board Level Position The DAS Board of Directors is seeking a member interested in serving as our Education Chairman. If you’re looking for a way to get more involved in the club and its affairs, please consider looking into volunteering for this Board level position. You can get details and discuss the position with President Greg Lee at 302-762-5358 or [email protected]. The Swap Tables at Past Holiday Parties were a GREAT SUCCESS, So We’re Doing it AGAIN...SO BRING OUT YOUR STUFF--MAKE A MEMBER HAPPY & Put some Extra Holiday Money in Your Pocket as Well!! Past year’s Swap Tables at the Annual Holiday Christmas Party were such a huge success that we’re going to do it again this year--ONLY BIGGER. So rummage through those drawers and aluminum briefcases for what you’re no longer putting to use, for there is a member out there who will likely think “This is just what I’ve been needing” and will take it off of your hands and put in them some extra cash for Holiday gifts for your family and friends! There will be PLENTY of table space to display your wares, so start thinking now of that astronomical equipment, books, telescopes, binoculars, software, etc. that have been collecting dust. Something you’ve been thinking of getting rid of, to sell or just give away. There’s someone in the Club that could put those items to good use! So check what you’ve got, and bring it to the December Holiday Party & Swap Meet. You’ll be glad you did!! Attend, Mix with Your Fellow Members & Enjoy! Images from Member Ron Worden’s Snobie Observatory Messier 42: Taken with STV Camera LRGB; Telescope: Meade LX200 10” FL 1575mm Venus Transit Photo 6/5/2012 Taken on Orion 4" 20x-60x Spotting Scope with a Canon 40D DSLR at ISO 400 Messier 42: STV Camera B&W; Telescope: Meade LX200 10” FL 2500mm -6- SAWIN OBSERVATORY REMINDER AND DAS LOANER TELESCOPES AND EQUIPMENT Bill Hanagan The DAS owns and maintains The Sawin Observatory on the grounds of the Mt. Cuba Astronomical Observatory. The Sawin Observatory houses the club’s equatorially mounted 12.5" reflecting telescope. The Sawin is also currently home base for our 17.5" split-tube Dobsonian telescope. DAS members can obtain a key for access to the Sawin Observatory by being checked out on these telescopes and the use of the observatory. Naturally, all DAS members are invited to look through these telescopes during our Member Star Parties (MSPs) at the Sawin. DAS members who are interested in becoming key holders of the Sawin Observatory should contact Greg Lee to receive training in the use of the facility and the telescopes. LOANER TELESCOPES and EQUIPMENT 80 mm Celestron Refractor (on loan from Bill McKibben) The club currently has on loan from our Secretary, Bill McKibben, an 80 mm Celestron Refractor with a Nextar GOTO mount. As soon as we can pair this up with an eyepiece set, we’d like to put this out on loan to members to see if they find it useful as a loaner telescope. Contact Bill McKibben if you would like to give this scope a try. 6” Orion Dobsonian Telescope We have a 6" Orion Sky-Quest XT6 Dobsonian reflector, complete with eyepiece set, available for loan to members. You can keep the telescope out on loan for a month or more. However, we use this telescope heavily for outreach star parties at the Woodside Farm Creamery, so if you have it on loan from April through October you may be asked to bring it out to one or more of these events. Meade 8” LX-10 Telescope We also have an 8” Meade LX-10 Schmidt Cassegrain Telescope (SCT) available for loan. If you have any thoughts about buying a telescope, especially an SCT, you are strongly advised to take this one out on loan so you can learn the advantages and disadvantages of this design. Barlowed Laser Collimator Toolset Also available for loan to DAS members is Howie Glatter’s version of the Barlowed Laser Colimator. This is actually made up of a set of three very nice tools: 1) a 1.25” Glatter laser collimator (which is useful on its own for collimating the secondary mirror); 2) a 1.25” “TuBlug”, which converts the straight beam laser collimator into a “Barlowed” laser collimator, complete with a target screen that’s visible from the back end of your Newtonian telescope; and 3) an Orion 2” to 1.25” centering adapter for use with 2” focusers. Along with the center donut or triangle on your Newtonian primary mirror, a Barlowed laser collimator is a very accurate and incredibly easy way to collimate your Newtonian or Dobsonian telescope. It may sound complicated, but using the Barlowed laser collimator is incredibly quick and easy compared to earlier generations of collimation tools. As one person noted “It’s one of the handiest and most useful tools the club has ever offered for loan to the membership!” Obviously, no one DAS member can keep these collimation tools out on loan forever, but borrowing this set of tools is a great way to become familiar with the new “Barlowed Laser Collimator” approach to collimation without having to buy the tool set sight unseen. If you’re interested in borrowing any of the club’s loaner telescopes or other items, please contact Bill Hanagan, Jeff Lawrence, or Greg Lee at one of our monthly meetings. When adding or editing your profile, you will need to enter your actual name in the “Real Name” box so you can be identified as a DAS member so Don Shedrick can approve your application to join the DAS group, and everyone will know to whom they are communicating. Finally, specify your desired email address for delivery of messages. Note: You may choose to not have your name and email address displayed to any-one other than DAS members who are members of the Yahoo DAS email group. For more detailed instructions, go to the DAS website under DAS Resource Links. DAS FORUM / E-MAIL SITE ON YAHOO This is a restricted e-mail service for use by DAS members for DAS purposes. To use this site, go to http://groups.yahoo.com; search for Delaware Astronomical Society; and click on the link that comes up. To join, you must have a Yahoo ID and password; if you don’t, you can register at this time by following Yahoo’s instructions. You will then be allowed to “Join the group” upon clicking in that box. You must then register for the DAS group and add your profile by clicking on “add new profile” and completing the form -7- Star Parties, Upcoming Events and Activities December 13, 2014-- 7:00 pm - 10:00 pm Delaware Museum of Natural History: Geminid Meteor Shower Astronomy presentation in the lecture hall on the Geminid Meteor shower (that peaks tonight and the next night) and if weather permits a star party on the rear lawn where we can, also, watch for the Geminids. DAS and the MCAO Partners with DelMNH for this event. Speaker is Greg Lee. December 16, 2014-- 7:00 pm - 9:00 pm DAS Holiday Party at MCAO DAS Holiday Party & Swap Meet for DAS members and invited guests only; No Board Meeting tonight. January 20, 2015-- 7:00 pm - 9:30 pm DAS January 2015 Monthly Meeting 7PM: DAS Board meeting, all are welcome. 8PM: General meeting - This Evening’s Presentation: ¤Near-Earth Objects and Other Dangers from Space presented by: John Conrad NASA/JPL Solar System Ambassador. February 13, 2015-- 5:30 pm - 7:30 pm Bellevue State Park Introduction to the Night Sky Bellevue State Park offers an evening of stargazing as DAS shows constellations and gives an introduction to observing the night sky. Equipment will be available, or you may bring your own. Red-filtered lights only please. No fee for this program. Call the Park to pre-register 302-761-6963. Meet in the Hunter Barn parking lot. -8- The Cocoon Nebula: Photo by DAS Member Rick Davis Sawin Certification Program Fred De Lucia The Sawin is the major centerpiece of DAS. In the past it was in use much more often and by a number of members on every clear Friday night. It has been largely underutilized for a number of reasons. One reason, I believe, is that newer members or members who do not own a telescope might feel intimidated by the equipment and the observatory’s layout. We hope to address this by instituting the Sawin Certification Program. With the new upgrades installed, its use will be more inviting and user friendly to both new and experienced members. Certified Key Holders of the Sawin have access to its use at any time without supervision . The Program will consist of a minimum of 2 sessions, scheduled at the Sawin, to obtain the necessary knowledge and experience in using the Sawin equipment. These sessions will be supervised by a current Sawin Key Holder. The first session, likely set for a weekend in the daylight (even if it’s cloudy), will familiarize learners with the layout of the Sawin and overall operation, including opening the roof, uncovering and covering the telescopes, handling eyepieces and pointing the telescopes, etc. If the supervising Sawin Key Holder determines that progression during the first session is acceptable, then the second session will be scheduled for a clear sky night session to address night time use of the equipment. The Sawin Certification Program is for DAS members only who are in good standing and 16 years of age or older. Participants in the program who are under 18 years of age must be accompanied by a parent or guardian. For information or sign-up, please, contact Greg Lee, DAS President at [email protected]. Call for DAS AstroImages for Display in Mt. Cuba Lobby MCAO is asking for any DAS members to submit their astroimages for display in the Observatory. It would like to display the club member’s talents and update some of the images currently on display in the lobby of the Observatory. Images will be displayed for up to a year and replaced as new images are submitted. Full credits to the imager will be included. Please include all technical information with the image (date, telescope and camera used, exposure time, image processing software, etc.). You may email digital images to the Mt. Cuba website. Photos may be sent to the Observatory or brought to a DAS meeting. The Observatory looks forward to displaying your beautiful images! Contact Greg at [email protected]. DAS Now has a Discount Subscription Rate for Astronomy Technology Today Magazine and Amateur Astronomy Magazine Astronomy Technology Today: : Members can subscribe directly on-line and then in the appropriate box enter the club’s discount code which is: DAS. During the order process, members simply enter the discount code and they will receive the discounted rate at checkout. Print subscribers also have unlimited access to all current and past digital issues at no additional cost. Normal print subscriptions are $18 per year. The club rate is $14 per year. The magazine is issued bi-monthly. https://www.astronomytechnologytoday.com/ Amateur Astronomy Magazine: DAS members must print, fill out and mail the form found in the “Files” section of our Yahoo email list website. . The magazine is issued quarterly. http://www.amateurastronomy.com/index.htm. -9- Japan Launches Asteroid Mission On missions for the Dec. 4, 2014: Dec. 3, the Japan Journey to Mars. Aerospace ExploraComets and tion Agency (JAXA) asteroids contain successfully material that formed launched its in a disk surrounding Hayabusa2 mission our infant sun. The to rendezvous with an hundreds of thouasteroid, land a small sands of known probe plus three mini asteroids are leftrovers on its surface, overs from material and then return that didn't coalesce samples to Earth. into a planet or moon NASA and JAXA are in the inner solar cooperating on the system. The thouscience of the sands of known mission and NASA comets likely formed will receive a portion in the outer solar of the Hayabusa2 system, far from the sample in exchange Asteroid Explorer “Hayabusa2” is a successor of “Hayabusa” (MUSES-C), which revealed sun's heat, where several new technologies and returned to Earth in June 2010. for providing Deep water exists as ice. Image Credit: JAXA and Akihiro Ikeshita Space Network Larger objects like dwarf planets Pluto and Ceres also formed in the communications and navigation support for the mission. outer solar system, where water ice is stable. Pluto and Hayabusa2 builds on lessons learned from JAXA’s Ceres will soon be explored by NASA missions New Horiinitial Hayabusa mission, which collected samples from a zons and Dawn, respectively. Asteroids and comets are of small asteroid named Itokawa and returned them to Earth in unique interest to scientists, though, because they could June 2010. Hayabusa2’s target is a 750 meter-wide asteroid hold clues to the origins of life on Earth. named 1999 JU3, because of the year when it was discovThese missions have greatly increased scientific ered by the NASA-sponsored Lincoln Near-Earth Asteroid knowledge on Earth about our solar system and the history Research project, Lexington, Massachusetts. This is a Cof our planet. Many scientists suspect we could find organic type asteroid which are thought to contain more organic material in asteroids and comets, like amino acids—critical material than other asteroids. Scientists hope to better building blocks for life, which could help answer questions understand how the solar system evolved by studying about the origins of life on Earth. These questions drive us to samples from these asteroids. continue exploring the intriguing asteroids and comets of our “We think of C-type asteroids as being less altered solar system. than others,” says Lucy McFadden, a planetary scientist at Multiple missions that are operating in space or in NASA’s Goddard Space Flight Center in Greenbelt, Marydevelopment by NASA and international partners could bring land. “Bringing that material back and being able to look at it us much closer to answering that question in our lifetimes in the lab — I think it’s going to be very exciting.” On Nov. 17, NASA and JAXA signed a Memorandum and also help identify Near-Earth Objects that might pose a risk of Earth impact, and further help inform developing of Understanding for cooperation on the Hayabusa2 mission options for planetary defense. and NASA’s Origins, Spectral Interpretation, Resource Follow the latest missions and discoveries at: http:// Identification, Security – Regolith Explorer (OSIRIS-REx) www.nasa.gov/asteroid-and-comet-watch/ mission to mutually maximize their missions’ results. OSIRIS-REx is scheduled to launch in 2016. It will be the Credits: first U.S. asteroid sample return mission. OSIRIS-REx will | Production Editor: Dr. Tony Phillips | Credit: Science@NASA rendezvous with the 500-meter-sized asteroid Bennu in 2019 for detailed reconnaissance and a return of samples to Earth in 2023. Illustration of Hayabusa2 and OSIRIS-REx will further strengthen Comet Siding’s the two space agencies’ relationship in asteroid exploration. Mars Flyby The missions will also help NASA choose its target this coming Spring. for the first-ever mission to capture and redirect an asteroid. NASA's Asteroid Redirect Mission (ARM) in the 2020s will help NASA test new technologies needed for future human -10- T h e Y i n - Ya n g o f P o l a r S e a I c e Dec. 4, 2014: The "That's one world is getting warmer. theory," says Meier. It comes as no "I think that winds are surprise, therefore, definitely playing a when researchers substantial role. But announce as they did other factors could be this past September at work, too." For that Arctic sea ice instance, he points extent is still below out that glaciers normal, continuing a melting around the years-long downward edges of the continent trend, covering less and could, ironically, less of the north polar produce more ice in seas with a frozen the surrounding crust. On the heels of ocean. "Fresh that announcement, meltwater from A new ScienceCast video explores the curious differences between north- and southcame another, a little glaciers is easier to polar sea ice. Click to Play it. more puzzling. While freeze than briny seawater," he explains. Arctic sea ice was melting, Antarctic sea ice was at an allSnowfall could be important, too. Snow landing on time high. In 2014, sea ice surrounding Antarctica covered thin sea ice can weigh the ice down and push it just below more of the southern oceans than it has since satellite the water. Cold ocean water seeps up through the ice and record began in the late 1970s. floods the snow – leading to a slushy mixture that freezes Is this also a sign of global warming? and thickens the sea ice. "There is no doubt that climate change is real," says Some scientists feel that these processes could Walt Meier of NASA's Goddard Space Flight Center. "The simply be due the natural variations in the Antarctic region's two poles are just responding in their own unique way to the climate. While it is clear that global warming is playing a same global phenomenon." significant role in the loss of Arctic sea ice, the trend in the He points out that Earth, taken as a whole, is losing Antarctic is small enough that it could be explained simply sea ice. According to satellite measurements from NASA due to natural variations in the region's climate. "Ultimately," and the National Snow and Ice Data Center, the Arctic has says Meier, "we expect that continued warming will take its lost an average of 20,800 square miles of sea ice a year toll, and even Antarctic sea ice will begin to decline." since the late 70s. Meanwhile, the Antarctic has gained an What we are seeing, he suggests, is the quirky average of 7,300 square miles per year—not enough to regional way Earth responds to a global stimulus. Earth's balance loses at the other end of the planet. climate system is complex, and climate change will continue But why do the Arctic and Antarctic behave in to have fascinatingly unpredictable consequences in the different ways? years ahead. "The increase we've seen in Antarctic sea ice is a little bit of a mystery," allows Meier. "We're still trying to Credits: figure out how a warmer global climate leads to these Author: Dr. Tony Phillips | Production Editor: Dr. Tony Phillips regional increases in ice cover." | Credit: Science@NASA The culprit could be weather. Climate change is altering weather patterns around the planet, and one of those More information: changes is an increase in windiness around the continent of Antarctic Sea Ice Reaches New Record Maximum -- Science@NASA Antarctica. Cold air blows from the ice-covered continent out The Cloudy Future of Arctic Sea Ice -- Science@NASA over the sea, freezing the waters and pushing sea ice outward to cover record-setting areas. 2014 Arctic Sea Ice Minimum 6th Lowest on Record -- Science@NASA Click to and Stay Informed About EVERYTHING to do with Man’s Exploration of the Universe! -11- Young Volcanoes on the Moon IMPs are too Back in 1971, Apollo small to be seen 15 astronauts from Earth, averaging orbiting the Moon less than a third of a photographed mile (500 meters) something very odd. across in their Researchers called it largest dimension. "Ina," and it looked That's why, other like the aftermath of than Ina, they haven't a volcanic eruption. been found before. There's Nevertheless, they nothing odd about appear to be widevolcanoes on the spread around the Moon, per se. Much nearside of the of the Moon's ancient Moon. surface is covered "Not only are A new ScienceCast video explores the mystery of recent lunar volcanism. Click to Play it. with hardened lava. the IMPs striking The main features of the "Man in the Moon," in fact, are old landscapes, but also they tell us something very important basaltic flows deposited billions of years ago when the Moon about the thermal evolution of the Moon," says Mark was wracked by violent eruptions. The strange thing about Robinson of Arizona State University, the principal investigaIna was its age. tor for LRO's high resolution camera. "The interior of the Planetary scientists have long thought that lunar Moon is perhaps hotter than previously thought." volcanism came to an end about a billion years ago, and "We know so little of the Moon!" he continues. "The little has changed since. Yet Ina looked remarkably fresh. Moon is a large mysterious world in its own right, and its For more than 30 years Ina remained a mystery, a "one-off only three days away! I would love to land on an IMP and oddity" that no one could explain. take the Moon's temperature first-hand using a heat probe." Turns out, the mystery is bigger than anyone Some people think the Moon looks dead, "but I imagined. Using NASA's Lunar Reconnaissance Orbiter, a never thought so," says Robinson, who won't rule out the team of researchers led by Sarah Braden of Arizona State possibility of future eruptions. "To me, it has always been an University has found 70 landscapes similar to Ina. They call inviting place of magnificent beauty, a giant magnet in our them "Irregular Mare Patches" or IMPs for short. sky drawing me towards it." "Discovering new features on the lunar surface was Young volcanoes have only turned up the heat on the thrilling!" says Braden. "We looked at hundreds of highMoon's allure. Says Robinson … "let's go!" resolution images, and when I found a new IMP it was Credits: always the highlight of my day." Author: Dr. Tony Phillips | Production Editor: Dr. Tony Phillips | "The irregular mare patches look so different than Credit: Science@NASA more common lunar features like impact craters, impact Examples of smooth and uneven melt, and highlands material," she says. "They really jump deposits marked out at you." with ‘S’ and ‘U’. a, On the Moon, it is possible to estimate the age of a Topographic landscape by counting its craters. The Moon is pelted by a depression containing the slow drizzle of meteoroids that pepper its surface with impact Sosigenes IMP . b, scars. The older a landscape, the more craters it contains. Maskelyne IMP. Some of the IMPs they found are very lightly Circular topocratered, suggesting that they are no more than 100 million graphic high right of centre. c, Manilus-1 years old. A hundred million years may sound like a long IMP. Sharp, lobate time, but in geological terms it's just a blink of an eye. The contacts (white volcanic craters LRO found may have been erupting during arrows) where the the Cretaceous period on Earth--the heyday of dinosaurs. smooth deposits superposed the Some of the volcanic features may be even younger, 50 uneven deposit .d, million years old, a time when mammals were replacing IMP inside Hyginus dinosaurs as dominant lifeforms. crater. e, Carrel-1 "This finding is the kind of science that is literally IMP. Narrow, discontinuous sections of uneven deposits may be a vent rim remnant. The inset highlights three lobate contacts (white arrows). going to make geologists rewrite the textbooks about the f, IMP north of Aristarchus crater. g, Maclear-1 IMP. Black arrows point Moon," says John Keller, LRO project scientist at the to lobate margins. h, Cauchy-5 IMP. Superposed on a 6 km diameter Goddard Space Flight Center. volcano. i, Ina exhibits numerous connected and isolated smooth Nov 24, 2014: deposits. Images: NASA/GSFC/Arizona State University. Click for larger image -12- Rosetta: Space probe drops Robotic Lander on Comet 67P From 88.5 WFDD, Public Radio for the Piedmont, part of the NPR Digital Network By SHAWN FITZMAURICE--SciWorks Radio is a production of 88.5 WFDD and SciWorks, the Science Center and Environmental Park of Forsyth County, located in Winston-Salem. WFDD: On November 12th, after a 10-year journey, the European Space Agency’s space probe, Rosetta, dropped the robotic lander Philae onto the surface of Comet 67P. This is the first-ever landing on a comet. This week, we invited Jonathan Ward, author of an upcoming book about launching the Apollo missions, and NASA-sanctioned JPL Solar System Ambassador, to discuss what we know so far from the lander. The European Space Agency has placed a six-month embargo on information, but Mr. Ward has pieced together what is available. Ward: There was an upward-facing thruster that was supposed to push Philae onto the surface so that the ice screws on the feet could drill into the comet surface. They knew before they released the lander that the thruster wasn't working, but there was no way to fix it. There was also a set of harpoons that were supposed to anchor the lander to the Rosetta selfie from 10 miles out. Credit: nasa.gov comet. Those did not fire. They think that the propellant in there was not Click to Hear the Program stable over the course of the 10 years. Philae’s feet went through a couple of inches of soft dust and then they hit a hard surface. It looks like one of the legs may have hit a rock which caused it to tip slightly and the lander came to rest at an angle against what appears to be a cliff or a crater wall. WFDD: Among the unexpected challenges, Philae’s landing site is problematic. The solar powered lander is hidden in shadow, and its exact location is unknown. Ward: When the European Space Agency scientists realized that it wasn’t getting a lot of sunlight they decided just to go ahead and run as many of the experiments as they could. They had ten instruments on the lander and they used all ten of them, and then tried to get as much of that data back as they could before the batteries finally died. WFDD: From what we know so far, results are mixed. Ward: There’s an instrument called MUPUS which is a hammer and a probe that are intended to penetrate into the comet surface and get a temperature of the comet. Unfortunately, part of that instrument was in the harpoons, and since those didn’t fire, that part didn’t get into the surface. The hammer had three increasing strength settings, but none of those was strong enough to be able to get through the surface of the comet. In fact there was a secret setting of 4, and even that wasn’t strong enough to break through. What it did show was that, instead of being crumbly, as was initially expected, the comet surface was as hard as ice. They had a drill on board that was supposed to try to drill into the surface and bring back some material that would be dumped into a chemical analyzer oven, but apparently there was nothing but trace amounts of gas when they ran the analyzer. An instrument that was intended to measure the chemical composition of the surface of the comet also didn’t work. It appears that the cover of the instrument didn’t come off. WFDD: While each failure still may tell us something about the comet, Philae’s successes give a tantalizing look at what we may know after the European Space Agency’s embargo. Ward: Another instrument was able to determine that there are organic molecules on the comet, and that was a very important finding. Organic molecules contain carbon and they are the building blocks of life. So the analyzer was designed to tell if these molecules are left handed or right handed. WFDD: Amino acids, in theory, can form as left or right handed, one being a mirror image of the other. Life should be compatible with either, but all life on earth is based on left handed molecules. We don’t know why. Determining the handedness of the comet’s organic material could give insight to the part comets may have played in seeding Earth with the building blocks of life. So what’s in the future for Rosetta and Philae? Ward: Just before the lander went silent, they commanded it lift itself up off the surface and and rotate so that once the comet gets closer to the sun it will start getting more light and maybe they’ll be able to re-awaken the lander. Rosetta is going to stay in orbit around the comet as it approaches the sun over the coming year, and they’re going to watch the comet begin to develop as it gets closer, gets warmer, and the ice begins to form kind of a gas cloud around the comet. At a recent on-line question-and-answer event, someone asked one of the scientists to summarize what he’d learned so far about the comet, and he said that “the main thing that I take away from this is that the comet is much more complex than I ever thought it would be.” He said, “I saw scientists who’ve done only comets for all of their careers staring in unbelief at the images they’ve been seeing from this. It makes it a really cool place where everybody has to take a step back and learn new things. Philae Lander on its way to the surface of Comet 67P -13- New Horizons Wakes Up on Pluto's Doorstep After With a a voyage of nearly seven-instrument nine years and three science payload billion miles —the that includes farthest any space advanced imaging mission has ever infrared and ultraviotraveled to reach its let spectrometers, a primary target – compact multicolor NASA’s New Horizons camera, a highspacecraft came out resolution teleof hibernation on Dec. scopic camera, two 6th for its long-awaited powerful particle 2015 encounter with spectrometers and the Pluto system. a space-dust Operators at detector, New New Horizons Mission Operations Manager Alice Bowman and operations team member the Johns Hopkins Horizons will begin Karl Whittenburg watch the screens for data confirming that the New Horizons spacecraft University Applied observing the Pluto had transitioned from hibernation to active mode on Dec. 6. Click for ScienceCast Video. Physics Laboratory in system on Jan. 15. Laurel, Md., confirmed at 9:53 p.m. (EST) that New HoriNew Horizons’ closest approach to Pluto will occur zons, operating on pre-programmed computer commands, on July 14, but plenty of highlights are expected before then, had switched from hibernation to “active” mode. Moving at including, by mid-May, views of the Pluto system better than light speed, the radio signal from New Horizons – currently what the Hubble Space Telescope can provide of the dwarf more than 2.9 billion miles from Earth, and just over 162 planet and its moons. million miles from Pluto – needed four hours and 26 minutes A Musical Wake-Up to reach NASA’s Deep Space Network station in Canberra, New Horizons joins the Australia. astronauts on four space “This is a watershed event that signals the end of shuttle missions who New Horizons crossing of a vast ocean of space to the very “woke up” to English tenor frontier of our solar system, and the beginning of the Russell Watson’s inspirmission’s primary objective: the exploration of Pluto and its ational "Where My Heart many moons in 2015,” said Alan Stern, New Horizons Will Take Me" – in fact, principal investigator from Southwest Research Institute, Watson himself recorded For New Horizons, Russell Watson Records Special Version of ‘Where My Boulder, Colo. a special greeting and Heart Will Take Me.’ Listen to it here Since launching on January 19, 2006, New Horizons version of the song to has spent 1,873 days — about two-thirds of its flight time — honor New Horizons! The song was played in New Horizons in hibernation. Its 18 separate hibernation periods, from midmission operations upon confirmation of the spacecraft’s 2007 to late 2014, ranged from 36 days to 202 days in wake-up on Dec. 6. length. The team used hibernation to save wear and tear on The Sleeping Spacecraft: How Hibernation Worked spacecraft components and reduce the risk of system failures. During hibernation mode, much of the New Horizons “Technically, this was routine, since the wake-up spacecraft was unpowered. The onboard flight computer was a procedure that we’d done many times before,” said monitored system health and broadcast a weekly beaconGlen Fountain, New Horizons project manager at APL. status tone back to Earth. Onboard sequences sent in “Symbolically, however, this is a big deal. It means the start advance by mission controllers woke New Horizons two or of our pre-encounter operations.” three times each year to check out critical systems, caliThe wake-up sequence had been programmed into brate instruments, gather some science data, rehearse New Horizons' onboard computer in August, and started Pluto-encounter activities, and perform course corrections. aboard the spacecraft at 3 p.m. EST on Dec. 6. About 90 New Horizons pioneered routine cruise-flight hibernaminutes later, New Horizons began transmitting word to tion for NASA. Not only has hibernation reduced wear and Earth on its condition, including the report that it is back in tear on the spacecraft's electronics, it also lowered opera"active" mode. tions costs and freed up NASA Deep Space Network trackThe New Horizons team will spend the next several ing and communication resources for other missions. weeks checking out the spacecraft, making sure its systems Credits: and science instruments are operating properly. They’ll also Production Editor: Dr. Tony Phillips | Credit: Science@NASA continue to build and test the computer-command seMore: quences that will guide New Horizons through its flight to and The Johns Hopkins Applied Physics Laboratory manages the New Horizons mission for NASA's Science Mission Directorate. New reconnaissance of the Pluto system. Dec. 7, 2014: Horizons is part of the New Frontiers Program managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. APL designed, built and operates the New Horizons spacecraft. -14- ASTRO-PHOTO of the MONTH The Veil Nebula Photo by DAS Member Rob Lancaster The Veil Nebula was taken in October, 2012 at a site called the “RV Lot,” a place in Fred De Lucia’s community in north Wilmington where they park RV’s. Setup Details: 10" Newtonian telescope, Losmandy G-11 Telescope Mount, Canon XSi DSLR that I modified by removing the IR filter and replacing it with one more sensitive to H-Alpha Light, Astronomik 2" UHC Nebula Filter, Macbook Pro Computer for Data Collection and Analysis. WEBSITE of the MONTH Astronomers Without Borders www.astronomerswithoutborders.org/ The Global Pairing Project program will allow an exchange of our cultures as well as sharing new techniques in science and astronomy. We believe both paired member clubs will benefit and learn from our expanded common interests. We have no planned agenda and only expect the engagements will go as far as the two mutually desire. In addition to the benefits of pairing, the Las Cumbres Observatory Global Telescope (LCOGT) Network will also allot some telescope time for the AWB Club Pairing program participants. These mutual cultural exchanges will not only benefit both clubs, but individuals will have a chance to advance their interest in astronomy and science. Through live web connections, both clubs will be able to expand on basic to advanced concepts in astronomy, astrophotography and even telescope operation. Budding stargazers in remote regions that otherwise may not have opportunities to expand their horizons in the hobby, will even have a chance to learn about observing techniques and the wonders of the night sky. Check it all out at www.astronomerswithoutborders.org/. -15- DAS ASTROPHOTOGRAPHY SPECIAL INTEREST GROUP Bill Hanagan The DAS astro-photography special interest group (DAS AP-SIG) meets monthly at Mt. Cuba and at our members’ homes. The AP SIG sometimes meets regardless of the weather, but some meetings are planned around specific imaging demonstrations and are “Flex-Scheduled” using email on 1-2 day notice to synchronize with the weather. AP-SIG meetings are regularly announced via the DAS Yahoo Group as well as by email to AP-SIG members. See the sidebar for a brief rundown on how to get started taking astro-photos. To join the AP-SIG, send me an email at [email protected] with your name, address, and phone number and tell me that you want to join the AP-SIG. AP-SIG meetings are informal and typically include the presentation of astrophotos taken by the members along with an extended question and answer period. The topics discussed during our Q&A sessions have covered the entire gamut of astrophotography, from how to get started with a minimum of equipment, to polar aligning your telescope, to the fine points of using auto-guiders and post-processing digital images. In addition, we often have special presentations on topics of particular interest at the time. For example, we’ve had special presentation on the ways a telescope can be polar aligned, the nature of various noise sources in electronic detectors including CCD cameras, how to make high dynamic range (HDR) photos, and how to photograph many different particular subjects, including: aurora, lunar eclipses, meteors, and the planets. Even if you aren’t an AP-SIG member, you’re welcome to attend the AP-SIG meetings to learn more. Our next “On Site” AP-SIG meeting is scheduled to be hosted by Rob Lancaster on Friday, December 12 at 7:30 PM at his home at 508 Brentwood Drive in Wilmington, DE. Rob is planning a tutorial demonstration of PixInsight, a program and flexible development environment designed specifically for astronomical image processing. PixInsight runs on Windows, MAC, and Linux based computers. A fully functional trial version can be downloaded from http://pixinsight.com/ The subsequent meeting of the AP-SIG is tentatively scheduled for the weekend of January 23 / 24. Please mark these dates on your calendar! On How to Get Started in Astro-Photography Bill Hanagan You can get started in astrophotography with your current camera mounted on a tripod by taking wide field photographs of meteor showers, conjunctions, constellations, and star trails. Mounting your camera “piggyback” on a motorized telescope that tracks the movement of the stars allows you to photograph a few more subjects, mostly large and bright nebulas and comets. At this level, some smaller subjects may benefit from the use of a telephoto lens. As you move to progressively fainter and smaller subjects, the demands on your equipment will grow considerably. However, as you improve your equipment, the number of subjects that you can photograph will also increase exponentially. Joining the AP SIG is a great way to learn what equipment you’ll need to photograph the subjects that interest you and to find out what specific equipment works well (or doesn’t work) before you spend your money. DAS AMATEUR TELESCOPE MAKING SPECIAL INTEREST GROUP Bill Hanagan The DAS Amateur Telescope Making (ATM) Special Interest Group (SIG) is made up of DAS members who get together to work on their own as well as club related telescope making projects. When and where AP-SIG members meet depends on what ATM projects are currently active. The general range of activities of the ATM SIG includes all manner of telescope making including Newtonian mirror making, the testing of complete telescopes as well as individual optics, and the making of telescope accessories. In the past, we’ve made several Newtonian telescope mirrors from scratch and completed some that members brought in as works in progress, including one that was started in the mid-60’s! We’ve also made new telescope tubes, made secondary mirror holders, tested numerous telescope objectives, manufactured spiders, and made many solar filters for telescopes and binoculars. We recently completed the refiguring of the DAS 17.5” Newtonian mirror. Anyone interested in joining the ATM SIG should email their name, address, and phone number to me at [email protected]. FOCUS uses plenty of photos in banners & elsewhere each issue, and So how about you?? HAVE ANY OLD or NEW ASTROPHOTOS?? we want to use YOURS...not Hubble’s!! PLEASE email to FOCUS editor (or tell us where they can be found on the web if your photos reside there) Photos need NOT be current. -16- INFORMATION ON DAS MEMBERSHIPS AND MAGAZINE SUBSCRIPTIONS DAS MEMBERSHIP · DAS membership dues are $30.00 per year and due on November 1 for all members. - There is no need to renew membership until the treasurer contacts you during the membership renewal drive starting in mid-October. · New members joining at various times of the year may be eligible for a prorated dues amount. - $20 when joining March-May - $10 when joining June-August - $30 for joining September-October through November 1 of the following year. ASTRONOMICAL LEAGUE MEMBERSHIP · · · The DAS offers an optional membership in the Astronomical League (AL) at a discounted rate. AL membership dues are $7.50 per year and are due on June 1 for all members. The AL does not offer any prorated discounts for new memberships starting mid-year. SKY & TELESCOPE MAGAZINE · · · · · · The DAS offers subscriptions to Sky & Telescope at a discounted rate of $32.95 per year. Subscriptions to S&T will be processed by the club for the first subscription year only. The publisher should then send renewal notices directly to the subscriber at the club rate of $32.95. You may receive renewal offers for amounts other than $32.95. If so, check to see if they are special offers and how close you are to your renewal date. Your subscription expiration date should be displayed on the mailing label on your magazine. If you are within 3 months of your renewal date and still have not received the correct renewal notice, please contact the publisher and tell them you should receive the member rate. ASTRONOMY MAGAZINE · · · · The DAS offers subscriptions to Astronomy magazine at a discounted rate of $34.00 per year. Subscriptions to Astronomy will be processed by the club for the first subscription year only. Your subscription expiration date should be displayed on the mailing label on your magazine. Renewals can be handled by all club members on the Astronomy.com website using the following steps: a. go to www.astronomy.com b. select the ‘customer service’ link in the upper right corner c. select the ‘renew your subscriptions’ link d. enter your customer number (found on the mailing label), postal code, and the renewal code of ‘RCLUB040’ and click ‘continue’ e. follow the remaining steps from there. NEW MEMBERSHIP FORM · · Please review the membership and magazine information above carefully. PLEASE fill out the membership form below completely. - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -- -- - - - NEW MEMBERSHIP FORM Please be sure to review the Membership and Magazine information above carefully. Please make checks payable to DAS and forward to: Jeff Lawrence, Treasurer, 815 Leeds Lane, Newark, DE 19711 Senior / Family Membership Junior Membership (15 or under) $30.00 $10.00 Astronomical League Sky & Telescope Magazine $ 7.50 $32.95 Astronomy Magazine $34.00 Total: Name_________________________________________________Email Address________________________________ Street Address_________________________________________________Phone Number________________________ City___________________________________________________________State______Zip_______________________ Notes_________________________________________________________________________________________________ For questions or concerns, contact Jeff Lawrence, DAS Treasurer at (302) 668-8277 or [email protected] -17- DAS CONTACTS Please call any of us with your concerns! Board members: Officers: President: Greg Lee -- 302-762-5358 or [email protected], Vice-President: Rob Lancaster -- also, Program Chair & Future Web Site Development -- [email protected] Secretary: Bill McKibben, Secretary [email protected] Treasurer: Jeff Lawrence [email protected]; (302) 668-8277also Sky & Telescope & Astronomy magazine issues Board Members at Large: Terry Lisansky [email protected] Glenn Bentley -- 610-869-0706 or [email protected] Bill Hanagan -- 302-239-0949 or [email protected], also Astronomical Photography Special Interest Group; Amateur Telescope Making Special Interest Group; By-Laws;Observatory and Equipment Improvements Standing Chairs: Publications: Joe Neuberger -- 302-723-2734 or [email protected], also, FOCUS Newsletter article/photo contributions Observing: Fred DeLucia -- 609-410-8943 or [email protected], also, Elections Chair and Awards Chair Education: Open Position (contact Pres. Greg Lee with questions) Observatory: Open Position (contact Pres. Greg Lee with questions) Library Maria Lavalle and Sue Bebon Other Chairs: Web Site Maintenance and Operation: Daniel Chester-- [email protected] Other Contacts: Astronomical League Coordinator: MCAO Web Page: www.MountCuba.org DAS Web Page: www.DelAstro.org Lynn King - [email protected] SEE PRECEEDING PAGE FOR NEW MEMBERSHIP FORM If you have questions, call any of the member representatives listed. Otherwise, just check the appropriate boxes and complete the form on the preceeding page. Print it or cut it off and send it with your check to Jeff Lawrencet his address on the form. The magazine prices are group rates to DAS members. If you’re just joining us for the first time, THANK YOU VERY MUCH, and WELCOME to the DAS! It’s GREAT to have you with us! The Last Word. . . FOCUS editor Joe Neuberger I can hardly believe that this is my 64th issue as Your Publications Chair and FOCUS Editor, which I have been doing since September, 2008. And it has been my Pleasure to serve the membership in this manner. I strive to make each issue of the FOCUS a little better than the last, and hope I succeed in that effort. I look forward to another year in 2015. So, before 2014 comes to a close, let me say “Thank You” for your wide ranging support, and to wish Everyone a sincere “Happy Holidays!” And “Best Wishes for a Safe & Happy New Year to ALL!”