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Journal of the South Bay Astronomical Society – October 2016 on line at http://sbastro.net/ On Facebook at facebook.com/SBAstroSociety On Yahoo Groups at: https://groups.yahoo.com/neo/groups/SBASTRO/info Monthly General Meeting: Friday October 7th 7:30 PM “TBA” Tim Thompson The September 9 Meeting President Greg Benecke began the meeting by welcoming newcomers Mike and Sophia. Ken Munson then gave an observing report that included his efforts to find a good observing location for next year’s total solar eclipse, and his visit to a meeting of the Big Sky Astronomy Club in Kalispell, Montana. Ken also observed last-month’s conjunction of Venus and Jupiter, and he had a dark but windy observing session at Red Rock Canyon. Finally, Ken set up a couple of telescopes during Labor Day, and showed dozens of passersby the Sun in hydrogen-alpha, as well as the Moon, Venus, Jupiter, Mars and Saturn and even a few stars. President Benecke then read out an article that contrasted the Webb and Hubble Space Telescopes. He also announced that the eight-week Astronomy for City Dwellers course will be starting on September 28. He also pointed out that the SBAS annual elections will occur during the October meeting, and that members should seriously consider helping the Society out by volunteering. Ken Rossi announced plans for an upcoming star night at the South Coast Botanic Garden. After a ten-minute break, George Nestojko gave a short presentation to the twenty people present about the RR Lyrae stars and the Blazhko effect, which is still not fully understood. The meeting then ended at 8:50. - Dr. Steven Morris One Incredible Galaxy Cluster Yields Two Types of Gravitational Lenses By Ethan Siegel There is this great idea that if you look hard enough and long enough at any region of space, your line of sight will eventually run into a luminous object: a star, a galaxy or a cluster of galaxies. In reality, the universe is finite in age, so this isn't quite the case. There are objects that emit light from the past 13.7 billion years—99 percent of the age of the universe—but none before that. Even in theory, there are no stars or galaxies to see beyond that time, as light is limited by the amount of time it has to travel. But with the advent of large, powerful space telescopes that can collect data for the equivalent of millions of seconds of observing time, in both visible light 1 and infrared wavelengths, we can see nearly to the edge of all that's accessible to us. The most massive compact, bound structures in the universe are galaxy clusters that are hundreds or even thousands of times the mass of the Milky Way. One of them, Abell S1063, was the target of a recent set of Hubble Space Telescope observations as part of the Frontier Fields program. While the Advanced Camera for Surveys instrument imaged the cluster, another instrument, the Wide Field Camera 3, used an optical trick to image a parallel field, offset by just a few arc minutes. Then the technique was reversed, giving us an unprecedentedly deep view of two closely aligned fields simultaneously, with wavelengths ranging from 435 to 1600 nanometers. With a huge, towering galaxy cluster in one field and no comparably massive objects in the other, the effects of both weak and strong gravitational lensing are readily apparent. The galaxy cluster— over 100 trillion times the mass of our sun— warps the fabric of space. This causes background light to bend around it, converging on our eyes another four billion light years away. From behind Galaxy cluster Abell S1063 (left) as imaged with the Hubble Space Telescope as part of the Frontier the cluster, the light Fields program. The distorted images of the background galaxies are a consequence of the warped from distant galaxies space dues to Einstein's general relativity; the parallel field (right) shows no such effects. Image is stretched, credit: NASA, ESA and Jennifer Lotz (STScI) magnified, distorted, and bent into arcs and multiple images: a classic example of strong gravitational lensing. But in a subtler fashion, the less optimally aligned galaxies are distorted as well; they are stretched into elliptical shapes along concentric circles surrounding the cluster. A visual inspection yields more of these tangential alignments than radial ones in the cluster field, while the parallel field exhibits no such shape distortion. This effect, known as weak gravitational lensing, is a very powerful technique for obtaining galaxy cluster masses independent of any other conditions. In this serendipitous image, both types of lensing can be discerned by the naked eye. When the James Webb Space Telescope launches in 2018, gravitational lensing may well empower us to see all the way back to the very first stars and galaxies. If you’re interested in teaching kids about how these large telescopes “see,” be sure to see our article on this topic at the NASA Space Place: http://spaceplace.nasa.gov/telescope-mirrors/en/ This article is provided by NASA Space Place. With articles, activities, crafts, games, and lesson plans, NASA Space Place encourages everyone to get excited about science and technology. Visit spaceplace.nasa.gov to explore space and Earth science! SBAS Executive Board President Vice-President Secretary Greg Benecke Ryan Parker 310-217-1512 213-454-1766 [email protected] [email protected] Steve Pedersen 310-378-6479 [email protected] Treasurer & Astronomical League Rep. 2 SBAS Committees Program Chairman Astronomical League Liaison Outreach Committee Newsletter Reproduction Publications Committee: SBAS Website Webmaster First Light Editor Observing Committee Membership Committee Cathy Brassell [email protected] Ken Rossi 310-515-1586 [email protected] Ken Munson Greg Benecke Craig Gates Ray Grace 310-257-1971 310-217-1512 310-376-6387 310-370-1913 [email protected] [email protected] [email protected] [email protected] Publicity Committee Property Committee Manhattan Bch Blvd Harbor Fwy (110) San Diego Fwy (405) Monthly General Meetings We normally meet on the first Friday of each month at 7:30 p.m. in the Planetarium at El Camino College (16007 Crenshaw Bl. In Torrance). If the first Friday is on or close to a holiday, we usually defer the meeting until the second Friday of the month. The Planetarium is on the south side of Manhattan Beach Blvd., one block west of Crenshaw Blvd. (near the center of the map at left). Crenshaw Blvd The planetarium is the only round, domed building on campus. There is on-street parking, and we can often use campus parking: check inside to see if you need a FREE parking permit for your car. We enjoy the planetarium facilities through the courtesy of the El Camino College Administration, and have several faculty members of the Astronomy Department as members of our Club. Our meetings always include an informal opening, when new attendees are invited to introduce themselves and let us know about their interests in astronomy. Members share their latest news and observations at this time. The rest of the evening is devoted to guest speakers, who range from amateur astronomers to professional astronomers to representatives from local aerospace companies to college professors. We are fortunate to have all these talented people in our area, willing to come and talk to us. Monthly Planning Meeting Committee members (and anyone else with an interest in Society activities) meet each month, usually on the Monday following the general meeting. Meetings are sometimes rescheduled due to travel and other circumstances. Exact date and time of each month’s meeting will be announced in the monthly meeting. The October planning meeting will be held at the home of TBD. 3 SBAS Dues Month Join/Due Member (Family) Student Expires Email Only January _$40.00 $25.00 Dec February _$36.67 $22.92 Dec March _$33.33 $18.75 Dec April _$30.00 $20.83 Dec May $26.67 $18.75 Dec June _$23.33 $16.67 Dec July _$20.00 $14.58 Dec August _$16.67 $12.50 Dec September _$13.33 $10.42 Dec October _$10.00 $8.33 Dec November _$6.67 $6.25 Dec December _$3.33 $4.17 Dec Note to Current U.S. Mail Members: The SBAS Board has decided that it is no longer cost effective to publish and mail out hard copies of the FirstLight. Since this decision was made after some 2016 renewals for U.S. Mail memberships were received, we will either refund the difference or extend your full 2015 membership though March of 2016. To simplify the dues, we suggest that all membership expire in December. Dues are $40.00/year ($25.00/year for students) and expire on December 31, of the current year. The FirstLight is now only available via Email notification and on our web site. New members use Month Join, and current members select your expiring Month to calculate the amount. Members that expire in October or November may wish to write one check and include next year’s membership. Make checks payable to the South Bay Astronomical Society. Dues may be paid at the general meeting or mailed to: South Bay Astronomical Society Attn: Greg Benecke P.O. Box 1937 Redondo Beach, CA 90278 SBAS Membership Benefits Contact Greg Benecke for magazine subscriptions at club rates: “Sky & Telescope” $32.95 and “Astronomy” $34.00/1 year or $60.00/2 years! Note: S&T subscribers at the club rate renew their subscriptions by mailing their renewal notice and check or calling the 800# on the renewal notice. Only new subscribers or subscribers converting their subscription to the club rate need to contact Arnie or send a check to the PO Box. Astronomy subscriptions and renewals still go through Arnie or via the PO Box. Astronomy Technology Today has become a digital only magazine. They have stated that current print subscribers will continue to be able to access digital issues without any cost. New subscribers should check their website for ordering details and subscription costs (www.astronomytechnologytoday.com). 4 Online Subscribe/Renew Instructions Astronomy Magazine US Subscription Rate: 1 year/12 Issues…..$34.00 2 years/24 issues….$60.00 3 years/36 Issues….$85.95 This year, there is an additional option for club member to order or renew. If you prefer, you can complete your individual transaction online with a credit card. Please follow the instructions below: 1) Go to www.astronomy.com/promo 2) When prompted for the promotion code, type in your club’s unique offer code “RCLUB165” and click the “Get Offer” button. 3) Select the order term (1 year, 2 years, or 3 years). 4) Enter your name, address and credit card information. Please note: you do not need to enter the promotion code a second time on this order page. That entry field can be disregarded. 5) Click on the “Submit” button. You will receive a confirmation page immediately. Please print this page for your records. If you have any questions, call one of our Customer Service Representatives at 1-800-533-6644, Monday – Friday 8:30 AM – 4:30 PM CT. Outside the US and Canada, please call 262-796-8776. Astronomical League Observing Clubs All SBAS members in good standing are also members of the Astronomical League and are eligible to participate in the League’s Observing Clubs. The Astronomical League provides many different observing programs (clubs). These programs are designed to provide a direction for your observations and to provide a goal. The programs have certificates and pins to recognize the observers’ accomplishments and for demonstrating their observing skills with a variety of instruments and objects. For more information, go to: http://www.astroleague.org/observing.html. New Free Astronomy Technology Today Subscription Offer Astronomy Technology Today offers a free 12-month online subscription for members. Go to the following URL for instructions on how to subscribe: http://www.cnyo.org/2016/02/01/12-free-months-of-astronomy-technology-todaytellem-cnyo-or-your-own-club-sent-you/ Useful and Interesting Astronomy Websites Website http://www.calsky.com/ https://www.aavso.org/ http://www.cleardarksky.com/csk/prov/California_clocks.html http://ssd.jpl.nasa.gov/horizons.cgi http://heavens-above.com 5 Description A useful site for planning an evening's star gazing if you don't have your own planetarium software. Information for observers with an interest in tracking variable stars. Good site to check to know what the weather will be like where you might be planning on going. Great site to use when you want to find a new comet or asteroid that isn't already in your planetarium software's list. See the Ephemeris Generator file on the SBAS Yahoo group site for instructions. Check this site to find out what satellites may be visible in your sky. http://www.lunar-occultations.com/iota/iotandx.htm http://pictures.ed-morana.com/ISSTransits/predictions/ http://www.aerith.net/comet/weekly/current.html http://sohowww.nascom.nasa.gov/ Website for the International Occultation Timing Association. Good place to find information on asteroid occultations of background stars. Find out when the ISS will transit in front of the Sun or Moon as seen from your location. Weekly information on bright comets. Good place to learn where there are bright comets to be seen. Refer to the Horizons website above to generate ephemerides. See the sun in ways you might never have imagined! You can even create your own movies of the sun in different the different frequencies imaged by the SOHO spacecraft. Travels I took a two-week vacation in August, ostensibly to visit relatives in north-central Montana. My secret mission was to do a reconnaissance of some sites for observing the total solar eclipse next year. I headed north through Utah on Interstate 15 then east on I-70 to Colorado and then north on I-25 to Wyoming. Casper and the area around it had beautifully blue skies with a number of puffy clouds formed in the turbulent airflow over the Rockies to the west. It didn’t seem like a big show stopper for eclipse watching. After visiting my mother and brother, I headed for home, first stopping off in Kalispell, Montana. There, I met up with the Big Sky Astronomical Club. They are a small group of dedicated astronomers in the beautiful Flathead Valley. Luckily, their monthly meeting was being held a week later than normal due to their recent public observing session atop the Continental Divide at Logan Pass in Glacier National Park. That’s nearly 7000 feet above sea level! Wish I could have been there with them. I meet them at their meeting site, a local fire station outside of Kalispell. I’d hoped we’d be able to do some observing afterwards but the weather was too bad to allow that. Anyway, when I’d arranged to meet them I’d offered to do a talk so I did one of the presentations I’d done for SBAS, “Tales from the Edge: When Things Go Wrong in Geostationary Orbit”. It was a lot of fun meeting and doing the talk for them and the emails I got afterwards told me they really enjoyed having such an unusual guest speaker. On the way home I came down the west side of the Rockies passing through central Oregon on Highway 97. Madras, Oregon is going to be dead center on the path of totality. I’d thought the high desert of central Oregon would be clear but instead, the sky was covered by solid clouds. Thin in some areas but still the whole sky was just a bland grey. These are one-point data samples so not a whole lot can be taken with them. Still, I’m planning on going to the Casper area next August. - Ken Munson Observing Reports Harbor City – On Saturday evening, August 27th, just before sunset, I got my binoculars out and walked down to the corner where I had a good view to the west. Without any good marks to use for sighting, it took me a while to find the small bright speck of Venus in the fading sunset. It took about another 10 minutes before I was finally able to see distant Jupiter just barely 10’ away. What a neat sight to see! I saw several neighbors who were out so I went 6 over and invited them to take a look at this fairly rare conjunction of these two planets. A couple of girls came by on bicycles and asked what I was looking at. One of them was really excited at hearing about the conjunction and asked to take a look. Turns out she was interested in astronomy and her several most recent school science projects were on astronomy. - Ken Munson Inyokern Road – Having been on-call the previous week, I’d been unable to make a dark-sky trip prior to new moon. Since new moon occurred on a Thursday, it was still going to be a small crescent and would set early on Saturday. So, on September 3 rd, I packed up and headed off to Inyokern Road area by Redrock Canyon for a night of observing. Predictions were for some fairly good conditions. Unfortunately, it turned out to be a lot windier than I’d anticipated. Too windy for doing any photography, I set the scope up for visual observing. A huge cloud had formed over the mountains to the north which must have been influenced by spiral winds rising over the mountains. It made a really striking shape and by sunset, lit by the red light, it almost appeared to glow from fire within the cloud. Wished I’d had my SLR camera to snap a picture. Even before the sunset, I was able to find the Moon, Venus and Jupiter. Not a lot of detail to be seen on Jupiter with it being so low and with low clouds on the horizon. Once it was fully dark, the observing really got underway. First up was Saturn, beautiful as always but a bit shaky with air turbulence couple with vibration of the scope in the wind. Next, it was on to Mars. Equally watery but with filtering and patience I could still make out a fair amount of surface detail. I decided to work my way up the Milky Way, starting on the southern horizon in the Scorpio/Sagittarius region. Even though it was pretty windy throughout the night, initially, at least, the sky was very transparent and I was able to see a lot of faint objects. I started out hunting through all the different globular clusters that swarm around the galactic core like moths around a light. Many were small and faint, but some were small yet very bright. I was way late getting around to M5 which, even though low, was still magnificent. M19 was high in the sky when I came across it and it made a very beautiful sight. Using the 12mm Nagler eyepiece I could resolve many stars in the cluster. NGC 6302, the Bug Nebula, was a very bright oblong planetary nebula. According to Starry Night it was a magnitude 13 planetary yet it appeared to be much brighter. Also in Scorpio, I checked out IC 4606. This is a patch of diffuse nebula, part of the Rho Ophiuchi Complex. For the first time, using the 35mm Panoptic eyepiece and my Comet Filter (really an ultra-high contrast filter), I was actually able to make out the hazy nebulosity. Moving into Ophiuchus, I came across NGC 6369, a planetary nebula. This was just a small hazy patch with a 10 th magnitude star nearby. In the 12mm eyepiece, it appeared to be a ring-type nebula as the circumference appeared brighter than the center. M8, the Lagoon Nebula, was absolutely magnificent, probably the best I’ve ever seen it. Using the 35mm eyepiece and the Comet Filter, I could see more nebulosity around the star cluster even details far away from the cluster that I’d never seen before. NGC 6445, the Little Gem, really is a little gem of a planetary nebula. This one, in the 12mm eyepiece, looked like a double ring, similar to the Helix Nebula. M17, the Swan Nebula, was another familiar object made even better with the 35mm and Comet Filter. There was more nebulosity visible to a greater extent than I’d ever seen before. NGC 6818, another planetary in Sagittarius looked like it might be another ring-type nebula. There did appear to be some structure but with the intermittent bouncing of the telescope, I couldn’t get enough of a steady look to make out the detail. NGC 6572, in Ophiuchus was a small, bright planetary. Not a lot of detail could be seen. Interesting thing here was that it makes the point on two pairs of stars off to one side. Moving into Aquila, I checked out NGC 6571. This is a small, faint planetary. Even so, it looked nice in the 12mm eyepiece even without any filter. NGC 6772, also in Aquila, is a very faint, 14 th magnitude planetary. This is a new low for me in visual planetary nebula observing. Looked better in the 35mm eyepiece with the Comet Filter than it did in the 12mm with or without any filter. It was getting towards midnight and the wind was picking up. Literally picking it. It picked up my mouse pad and blew it and the mouse several yards away! The telescope was bouncing so bad I gave up on it for a while and sat back on my astronomy chair and used the binoculars. It was kind of fun to see how many objects I could recognize in the binoculars. Among them, M39, M29, M103, all open star clusters. While roving around Cassiopeia, I noticed 7 a large fuzzy object off of Caph, near Rho Cassiopeia. I noted the position and kept roving around. Off one right arm of Perseus I noted another fuzzy object that couldn’t be resolved with the binoculars. Its position was just off of b Persei and formed a triangle with Lambda Persei. After a while, the wind settled down and I went back to the scope. First, I checked out the two objects that I’d found in binoculars. The one in Cassiopeia turned out to be NGC 7789, a dense open cluster of faint stars. Looked very nice. The one in Perseus turned out to be NGC 1528, another dense open cluster made of faint stars. I tried finding Campbell’s Red Hydrogen Star in Cygnus. Still couldn’t find it. Easy enough to see in the 60-inch, it seems to be hard to identify in a small telescope. Checked out NGC 6905, a 12 th magnitude planetary nebula in Delphinus. It makes a nice tight triangle with a pair of stars. NGC 1491 is an emission nebula in Perseus. Located in a patch of dark nebula, it was just barely noticeable. It looked slightly better with the Comet Filter. Nearby, in Cassiopeia is NGC 281. Also an emission nebula, this one was much more visible. In fact, this was the first time I’d ever seen it, even though I’d tried many times. Once again, the Comet Filter really does a great job of bringing out the “faint fuzzies”! I could see why it got its nickname, the Pacman Nebula. By this time the wind was starting to gust again. I checked out a couple of carbon stars, most notable of which was DS Pegasus. This bright, orange colored star is surrounding by a huge number of white stars. By now it was after 2 AM and it was cold and windy and clouds were moving in. All night I’d been plagued by the scope seeming to lose its tracking and the GoTos getting more and more inaccurate. I’d had to re-align the scope several times through the night. When I started taking things apart I found out why. I hadn’t fully locked the elevation clutch down! This allowed the scope to slip in elevation a bit with every move. Stupid mistake! Not a terrific night but one of the best I’ve had in some time. - Ken Munson Columbia Park – I decided to take advantage of the holiday and the recent new moon to take the scope and my PST over to Columbia Park in Torrance. I set up at about 10:30 AM with the sky covered in cloud but figured they would break up around noon like they usually did. I figured with the holiday there’d be a lot of people in the park and I could do a bit of astronomy outreach. I wasn’t disappointed and there were a lot of people in the park that day. A large church group set up at the tables and barbecue grills not too far from me. This group was really curious and a lot of their young people mostly teens, came over repeatedly to take a look. For most of the day, I alternated from the Sun, to the Moon and then Venus. The sun had a really good grouping of large sunspots. In the PST, the biggest two spots were visible as well as a bright plage area between them, a dark river of a filament and some large prominences around the edge. People were really amazed to see a planet, even one as dull as Venus, in broad daylight. As the sky grew clearer, I swung over to Jupiter. I could see it but no one else could. It was just a faint, faint pale ghost of its usual self. Late in the afternoon, I tried finding Saturn but didn’t have any luck so it was back to the initial trio. After a bit more time, by about 4 PM, I tried Saturn again and thought I’d seen it but couldn’t be sure. So I swung down to Mars. And there it was! Its reddish orange color made it stand out more clearly against the blue sky background. The kids and their parents were really thrilled to see Mars. Then, swinging back up to Saturn, I could definitely see it. After a bit of patient observing, one by one the young people who were around were also able to finally spot the ringed planet. With that success, I decided to go for the gold and try to find a star with the sun still shining brightly. Swung the scope up to Arcturus and, yes! There is was, glowing with a fiery orange color in the deep blue sky overhead. Once again, it amazed people and it seemed like half the church group lined up to get a look at a star in daylight. By this time the marine layer was starting to move in and patchy clouds were beginning to crowd the sky. One of the young people who’d been with me most of the day, Jonathan, really wanted to see Vega. So, I decided to try since it should be almost straight overhead, even though I feared its white color would make it less visible in daylight. But, no, it stood out like a sore thumb against the deep blue sky! As luck would have it, it happened to be in a patch of clear sky between the branches of a tree. Again other members of the church group lined up to see it. People were just so amazed and stunned to be able to see a star with the sun still up in the sky. 8 With clouds moving in rapidly and the temperature dropping and the park emptying out, I decided it was time to shut down. It had been an incredibly fun and worthwhile day and I was glad I’d decided to do this. - Ken Munson Ridgecrest School – On Saturday night, September 24th, club members Ken Rossi, George Nestojko, Justin Fuller, Larry Kinney, Steve Pedersen (who arrived around midnight) and Ken Munson gathered at Ridgecrest Middle School in RPV at sunset for an evening of in-town observing. Conditions looked favorable with clear skies, only a light breeze and warm temperatures. In fact, it was so warm, it was shirt-sleeve weather all night long. By 1 AM, the temperature was still 75o F on top of PV. It was actually colder down below. Larry Kinney was busy trying out his new, home-made, hand-crafted wooden equatorial mount. George did a number of astro-images of stellar spectra while the rest of us pursued our own observing plans. The evening started off with some easy targets, Venus, Mars and Saturn. A family passed by as a father’s son ran laps around the playing field. I offered them a view of Saturn. Even though it turned out the seeing was not all that great, they were amazed to see the rings of Saturn. As the sky gradually darkened, one by one the moons of Saturn became visible. Kent, the young boy in the family, was the first to spot a moon and was thrilled to discover it was a large moon and the only one in the solar system to have an atmosphere. Mars was also still very good to see, clearly in a gibbous phase and showing a fair amount of surface detail in spite of the unsteady air. Once it was fully dark, observing really got underway. A surprise target was provided by George who directed us to check out the second Double-Double in Lyra. This is another pair of stars similar to the famous Double-Double of Epsilon Lyra 1&2. Identified as HIP 94043 and HIP 94075 in my Starry Night software, the pair of double stars makes a nearly equilateral triangle with another star, TYC 24648-965-1. The doubles are not quite as close as the famous pair, having a fairly good separation, which was fortunate given the poor seeing this night. The doubles are also of slight different magnitudes. Still, a nice sight to see and fun to find another pair of close double stars that can fit in the FOV of an eyepiece. Having set up for visual observing, I spent a good portion of the evening flitting through a lot of globular and open star clusters. I’d mounted my 80mm Onyx scope on my Nexstar 11 and would use it for those clusters or objects that were a bit too big to really appreciate in the smaller FOV of the Nexstar. M22, M13, M92 and M15 were magnificent examples of globular clusters in the 12mm Nagler eyepiece. M11 was all but invisible in the Onyx, being made of many faint stars. Yet in the 12mm on the Nexstar, it was really beautiful, the many faint stars standing out clearly. Open cluster NGC 6633 in Ophiuchus made a nice gem with a wide spacing of bright stars. Surprisingly, in the Onyx, it wasn’t all that attractive. I tried for some nebulas, as well. M57 was very nice in the 12mm with an OIII filter. My old friend, 12 th magnitude NGC 6905 also looked nice in the Nagler eyepiece. M27 was really magnificent in the 12mm in the Nagler with the OIII filter. The Saturn Nebula, NGC 7009, was very bright, clearly looking like a slightly fuzzy version of its namesake. The Helix Nebula, NGC 7293, however, was all but invisible even with the my 35mm Panoptic eyepiece and the high contrast Comet Filter. I decided to try for interesting doubles, first just going through the stars in a constellation and using the Starry Night software to identify which stars were doubles. One drawback with SN, is that it only says a double has a separation of < or > 10”. Many of the doubles I found using SN were quite nice but not truly spectacular. A few were so widely separated that it was impossible to tell in the scope whether they were doubles or not. I switched from using SN to the Nexstar Observing List, or NSOL. This program, designed by an early user of the Nexstar series of scopes, has a number of lists provided by other users and the ability to create new lists. I started it up and opened a list of double stars for September-November. I found a few doubles that were challenging to split with the seeing conditions that prevailed all night. 12 Aqr was one such as it had a separation of only 2.9” and a huge magnitude difference between the stars of the pair. 49 Cyg was another close double that could just barely be separated as it was only 2.5” apart. After hunting down doubles, I opened the list for Carbon Stars for September-November. Carbon stars are late age stars similar to red giants but with a distinctive spectral signature. That signature is dominated by Carbon in various combinations. Carbon stars come in two varieties, one which creates carbon from fusing helium into carbon which then gets lofted into the star’s atmosphere through convection, and the other which is believed to be a red giant pair 9 with what is now a white dwarf. Here the giant siphoned material from its companion which had been a carbon star and pulled the carbon into its own atmosphere. Carbon stars are often dim and hard to see since they often don’t radiate enough energy to trigger the color rods in the human eye. Still, they can be very beautiful to see, especially in a crowded field among white stars. Hence, the effect I call being a ruby among diamonds. UX Dra is one such carbon star. It’s a nice, bright, very pretty deeply red carbon star surrounded by a sprinkling of similar magnitude white stars. S Cep is absolutely beautiful, a deep cherry red carbon star. Very pretty to see. By now, it was nearing 1 AM and I decided to shut down, having been up since before 4 AM. I took one last look at an old favorite, M45. Here, the Nexstar showed its limitations since it’s FOV was too small to appreciate this huge open cluster. It looked spectacular in the Onyx with it really wide field, using my 20mm Wide-angle eyepiece. A very satisfactory way to end an enjoyable evening! - 10 Ken Munson Astronomy for City Dwellers Enjoy the Night Sky! Experience the wonder of the night sky through… Learning constellations Understanding amazing truths about the cosmos Seeing planets, galaxies, star clusters, nebula and other deep-sky objects through a variety of modern telescopes No experience required Begins September 28; 8 weekly Wednesday evening classes 7:00-9:00 pm Rancho Del Mar School, 38 Crest Road West, Rolling Hills, CA 90274 Instructor: Steve Lindsey www.nightglories.com Course Fee: $92 Registration Info: CALL 310-541-7626 ext. 290 Website: http://www.pvpusd.net/adulted 11 Astronomy App Luminos Introduces Advanced Features and Visuals September 1, 2016 FandomFare Displayed with permission from Fandom Fare California-based Wobbleworks LLC today releases Luminos 9.1, the most recent free feature update to its awardwinning astronomy app for iOS devices. Whether you want to admire ancient constellations, watch satellites soaring overhead, find out what that brilliant dot is on the horizon, or recreate eclipses, Luminos has what you need. Luminos now supports translucent 3D terrain, orientation modes, a 3D view of recently explored Comet 67P, and a hypothetical model of the undiscovered Planet Nine. San Jose, California – Wobbleworks LLC has released the latest version of its flagship astronomy app Luminos, bringing visual improvements and stargazing additions to existing customers. Luminos 9.1 expands on the application features with new visuals such as Comet 67P and the theoretical Planet Nine, and new settings such as orientation modes. Luminos 9.1 is a free update for current iOS device and Apple Watch owners. Users of Luminos will now see translucent versions of the terrain at their current location, as determined by their device sensors. Translucent terrain allows quicker identification of celestial objects below the horizon, and these objects can be tracked even when they are obscured by the ground. The translucent terrain is an addition to the Luminos dynamic terrain engine, which downloads 3D representations of hills and valleys based on current GPS coordinates. To support more advanced users, Luminos has added orientation modes that allow the user to change the view from the default "horizontal" system to "ecliptic", "equatorial", or "galactic" orientations. While the traditional horizontal view appears as though the user is standing on a planet surface, the new options re-orient the screen interaction along a different baseline. For example, the ecliptic option adjusts the view along the plane of the Solar System planet orbits. Orientation modes provide easier tracking for many celestial objects. The Luminos app now calls out variable stars with magnitude changes over time. Users can also sort star categories to find the largest, fastest changing, or closest stars with single taps. The ESA Rosetta mission recently mapped the structure of Comet 67P/Churyumov-Gerasimenko during its closeup study of that object, and Luminos has utilized the data from the Rosetta mission to include a 3D representation of the comet nucleus which users can rotate and explore. The theoretical Planet Nine, a body as yet unseen but proposed by noted astronomers is now modeled in Luminos 9.1 using the best-known calculations of its hypothetical position. Planet Nine is thought to exist in the outer reaches of the Solar System due to observed fluctuations on known bodies that would be caused by the gravitational pull of another large body. While scientists search for proof of the planet, users of the Luminos app can simulate orbiting Planet Nine and observing the rest of the Solar System from its remote location. Luminos is the recent recipient of a 2015 PC Magazine Editor's Choice award. Previous versions of Luminos added the largest star catalog available on mobile, the most comprehensive built-in deep space image library, live sky charts for Apple Watch, and 3D meteor shower simulations. App Highlights: * Now in its sixth year of free feature updates * Realistic sky visualizations * Largest astronomy database on mobile, up to 113 million stars * Smooth animations and 3D flight to any destination in the solar system * Thousands of years of simulated solar and lunar eclipses * Satellite, comet, meteor, and asteroid tracking * Telescope control Device Requirements: * iPad, iPhone, or iPod touch 12 * Optional Apple Watch app included * iOS version 9.0 or later * 700 MB device space Ancient UK Standing Stones Proven To Be Astronomical In Nature August 19, 2016 STEAM Displayed with permission from STEAM Register Register New research proves that the earliest standing stone monuments of Britain were constructed to track the specific movements of the Sun and Moon. New research has statistically proven that the earliest standing stone monuments of Britain, constructed around 5,000 years ago, were indeed constructed to track the specific movements of the Sun and Moon. The research, which was conducted by experts at the University of Adelaide, relied on the use of innovative 2D and 3D technology to construct quantitative tests of the patterns of alignment of the standing stones. "Nobody before this has ever statistically determined that a single stone circle was constructed with astronomical phenomena in mind – it was all supposition," said project leader and University of Adelaide Visiting Research Fellow Dr. Gail Higginbottom. The research team focused their studies on the oldest great stone circles built in Scotland (Callanish, on the Isle of Lewis, and Stenness, Isle of Orkney - both predating Stonehenge‘s standing stones by about 500 years). They found that there was evidence of a great concentration of alignments towards the Sun and Moon at different times of their cycles. They also found that much simpler monuments were still being built that had at least one of the same astronomical alignments some 2,000 years later in Scotland. The Standing Stones of Stenness, Isle of Orkney. Credit: iStockphoto More Than Meets The Eye The stones aren't just connected to the Sun and the Moon, however. The researchers uncovered a complex relationship between the alignment of the stones, the surrounding landscape and horizon, and the movements of the Sun and the Moon across that landscape, reports Adelaide's Robyn Mills. "This research is finally proof that the ancient Britons connected the Earth to the sky with their earliest standing stones, and that this practice continued in the same way for 2,000 years," Dr. Higginbottom said. 13 The team also found that about half the sites were surrounded by one landscape pattern and the other half by the complete reverse. "These chosen surroundings would have influenced the way the Sun and Moon were seen, particularly in the timing of their rising and setting at special times, like when the Moon appears at its most northerly position on the horizon, which only happens every 18.6 years," Dr. Higginbottom said. "For example, at 50% of the sites, the northern horizon is relatively higher and closer than the southern and the summer solstice Sun rises out of the highest peak in the north. At the other 50% of sites, the southern horizon is higher and closer than the northern, with the winter solstice Sun rising out of these highest horizons. These people chose to erect these great stones very precisely within the landscape and in relation to the astronomy they knew. They invested a tremendous amount of effort and work to do so. It tells us about their strong connection with their environment, and how important it must have been to them, for their culture and for their culture's survival." Results of this research, which is part of the Western Scotland Megalithic Landscape Project, are published in the Journal of Archaeological Science: Reports. Ripples in fabric of space-time? Hundreds of undiscovered black holes ScienceDaily 7 September 2016 - New research by the University of Surrey published today in the journal Monthly Notices of the Royal Astronomical Society has shone light on a globular cluster of stars that could host several hundred black holes, a phenomenon that until recently was thought impossible. Globular clusters are spherical collections of stars which orbit around a galactic centre such as our Milky-way galaxy. Using advanced computer simulations, the team at the University of Surrey were able to see the un-see-able by mapping a globular cluster known as NGC 6101, from which the existence of black holes within the system was deduced. These black holes are a few times larger than the Sun, and form in the gravitational collapse of massive stars at the end of their lives. It was previously thought that these black holes would almost all be expelled from their parent cluster due to the effects of supernova explosion, during the death of a star. "Due to their nature, black holes are impossible to see with a telescope, because no photons can escape," explained lead author Miklos Peuten of the University of Surrey. "In order to find them we look for their gravitational effect on their surroundings. Using observations and simulations we are able to spot the distinctive clues to their whereabouts and therefore effectively 'see' the un-seeable." It is only as recently as 2013 that astrophysicists found individual black holes in globular clusters via rare phenomena in which a companion star donates material to the black hole. This work, which was supported by the European Research Council (ERC), has shown that in NGC 6101 there could be several hundred black holes, overturning old theories as to how black holes form. Hubble Space Telescope Observation of the Co-author Professor Mark Gieles, University of Surrey central region of the Galactic globular cluster continued, "Our work is intended to help answer fundamental NGC 6101: Compared to the majority of Galactic questions related to dynamics of stars and black holes, and globular clusters, NGC 6101 shows a less the recently observed gravitational waves. These are emitted concentrated distribution of observable stars. when two black holes merge, and if our interpretation is right, Credit: NASA the cores of some globular clusters may be where black hole mergers take place." The researchers chose to map this particular ancient globular cluster due to its recently found distinctive makeup, which suggested that it could be different to other clusters. Compared to other globular clusters NGC 6101 appears 14 dynamically young in contrast to the ages of the individual stars. Also the cluster appears inflated, with the core being under-populated by observable stars. Using computer simulation, the team recreated every individual star and black hole in the cluster and their behaviour. Over the whole lifetime of thirteen billion years the simulation demonstrated how NGC 6101 has evolved. It was possible to see the effects of large numbers of black holes on the visible stars, and to reproduce what was observed for NGC6101. From this, the researchers showed that the unexplainable dynamical apparent youth is an effect of the large black hole population. "This research is exciting as we were able to theoretically observe the spectacle of an entire population of black holes using computer simulations. The results show that globular clusters like NGC 6101, which were always considered boring are in fact the most interesting ones, possibly each harboring hundreds of black holes. This will help us to find more black holes in other globular clusters in the Universe. " concluded Peuten. First stars formed even later than previously thought ScienceDaily 2 September 2016 - ESA's Planck satellite has revealed that the first stars in the Universe started forming later than previous observations of the Cosmic Microwave Background indicated. This new analysis also shows that these stars were the only sources needed to account for reionising atoms in the cosmos, having completed half of this process when the Universe had reached an age of 700 million years. With the multitude of stars and galaxies that populate the present Universe, it's hard to imagine how different our 13.8 billion year cosmos was when it was only a few seconds old. At that early phase, it was a hot, dense primordial soup of particles, mostly electrons, protons, neutrinos, and photons -- the particles of light. In such a dense environment the Universe appeared like an 'opaque' fog, as light particles could not travel any significant distance before colliding with electrons. As the cosmos expanded, the Universe grew cooler and more rarefied and, after about 380,000 years, finally became 'transparent'. By then, particle collisions were extremely sporadic and photons could travel freely across the cosmos. Today, telescopes like Planck can observe this fossil light across the entire sky as the Cosmic Microwave Background, or CMB. Its distribution on the sky reveals tiny fluctuations that contain a wealth of information about the history, composition and geometry of the Universe. The release of the CMB happened at the time when electrons and protons joined to form hydrogen atoms. This is the first moment in the history of the cosmos when matter was in an electrically neutral state. Cosmic reionisation. Credit: ESA – C. Carreau After that, a few hundred million years passed before these atoms could assemble and eventually give rise to the Universe's first generation of stars. As these first stars came to life, they filled their surroundings with light, which subsequently split neutral atoms apart, turning them back into their constituent particles: electrons and protons. Scientists refer to this as the 'epoch of 15 reionisation'. It did not take long for most material in the Universe to become completely ionised, and -- except in a very few, isolated places -- it has been like that ever since. Observations of very distant galaxies hosting supermassive black holes indicate that the Universe had been completely reionised by the time it was about 900 million years old. The starting point of this process, however, is much harder to determine and has been a hotly debated topic in recent years. "The CMB can tell us when the epoch of reionisation started and, in turn, when the first stars formed in the Universe," explains Jan Tauber, Planck project scientist at ESA. To make this measurement, scientists exploit the fact that a fraction of the CMB is polarised: part of the light vibrates in a preferred direction. This results from CMB photons bouncing off electrons -- something that happened very frequently in the primordial soup, before the CMB was released, and then again later, after reionisation, when light from the first stars brought free electrons back onto the cosmic stage. "It is in the tiny fluctuations of the CMB polarisation that we can see the influence of the reionisation process and deduce when it began," adds Tauber. A first estimate of the epoch of reionisation came in 2003 from NASA's Wilkinson Microwave Anisotropy Probe (WMAP), suggesting that this process might have started early in cosmic history, when the Universe was only a couple of hundred million years old. This result was problematic, because there is no evidence that any stars had formed by then, which would mean postulating the existence of other, exotic sources that could have caused the reionisation at that time. This first estimate was soon to be corrected, as subsequent data from WMAP pushed the starting time to later epochs, indicating that the Universe had not been significantly reionised until at least some 450 million years into its history. This eased, but did not completely solve the puzzle: although the earliest of the first stars have been observed to be present already when the Universe was 300 to 400 million years old, it remained unclear whether these stars were the main culprits for reionising fully the cosmos or whether additional, more exotic sources must have played a role too. In 2015, the Planck Collaboration provided new data to tackle the problem, moving the reionisation epoch even later in cosmic history and revealing that this process was about half-way through when the Universe was around 550 million years old. The result was based on Planck's first all-sky maps of the CMB polarisation, obtained with its LowFrequency Instrument (LFI). Now, a new analysis of data from Planck's other detector, the High-Frequency Instrument (HFI), which is more sensitive to this phenomenon than any other so far, shows that reionisation started even later -- much later than any previous data have suggested. "The highly sensitive measurements from HFI have clearly demonstrated that reionisation was a very quick process, starting fairly late in cosmic history and having half-reionised the Universe by the time it was about 700 million years old," says Jean-Loup Puget from Institut d'Astrophysique Spatiale in Orsay, France, principal investigator of Planck's HFI. "These results are now helping us to model the beginning of the reionisation phase." "We have also confirmed that no other agents are needed, besides the first stars, to reionise the Universe," adds Matthieu Tristram, a Planck Collaboration scientist at Laboratoire de l'Accélérateur Linéaire in Orsay, France. The new study locates the formation of the first stars much later than previously thought on the cosmic timeline, suggesting that the first generation of galaxies are well within the observational reach of future astronomical facilities, and possibly even some current ones. In fact, it is likely that some of the very first galaxies have already been detected with long exposures, such as the Hubble Ultra Deep Field observed with the NASA/ESA Hubble Space Telescope, and it will be easier than expected to catch many more with future observatories such as the NASA/ESA/CSA James Webb Space Telescope. 16 Schedule of Coming Events Date Event 3-9 October Friday Astronomy Week 4-10 October World Space Week Astronomy Day is a world-wide event observed each spring and fall. The next Astronomy Day this year is October 8, 2016; Astronomy Day next spring will be May 14, 2016. Local astronomical societies, planetariums, museums, and observatories will be sponsoring public viewing sessions, presentations, workshops, and other activities to increase public awareness about astronomy and our wonderful universe. Since its United Nations declaration in 1999, World Space Week has grown into the largest public space event on Earth. More than 1,800 events in 73 countries celebrated the benefits of space and excitement about space exploration in 2015. With our new Theme “Remote Sensing – Enabling Our Future” we aim to inspire even more events around the world in October 2016. See http://www.worldspaceweek.org/ for more information. 7 October Friday Night 7:30PM Monthly General Meeting 9 October Draconids Meteor Shower Peak Topic: TBD Speaker: TBD The maximum rate typically reaches 1-2 per hour, but outbursts of hundreds or thousands per hour occurred several times during the 20th century. 11 October Monthly Planning Meeting Monday Night See directions on Page 4. 7:30 PM 14 October Friday Evening 6-10 PM O-tsumkimi Festival Japanese Harvest Moon festival being held at the South Coast Botanical Garden at 26300 Crenshaw Blvd, Palos Verdes Estates. While few Japanese are lucky enough to have tearooms, let alone a pond with a view to the east, this ancient festival is meant to celebrate the beauty of the moon, and the fall harvest. 18 September UCLA Meteorite Gallery Lecture Series Saturday 2:30 “Calcium-Aluminum-rich Inclusions: The Solar System's First Rocks” by Kevin McKeegan, PM Professor of Geochemistry and Cosmochemistry, UCLA 21 October Orionid Meteor Shower Peak The Orionid meteor shower is the second of two showers that occur each year as a result of Earth passing through dust released by Halley's Comet, with the first being the Eta Aquarids. The point from where the Orionid meteors appear to radiate is located within the constellation Orion. Observers in the Northern Hemisphere will see around 20 meteors per hour at maximum 22 October Saturday Evening In Town Dark Sky Observing Session at Ridgecrest Middle School– 28915 NortbBay Rd. RPV, Weather Permitting: Please contact Greg Benecke to confirm that the gate will be opened! 17 Date Event 29 October Saturday Night Out of Town Dark Sky Observing Session 30 October Venus Passes 3 Degrees from Saturn Contact Greg Benecke to coordinate a location. 4 November Monthly General Meeting Friday Topic: Update on JUNO Evening 7:30 Speaker: Theo Clarke, JPL PM 18 South Bay Astronomical Society ********* Next General Meeting at El Camino College Planetarium: Friday, October 7th, at 7:30 P.M. “TBD” Tim Thompson ********* South Bay Astronomical Society P.O. Box 1937 Redondo Beach, CA 90278 19