SIAC Newsletter March 2015

Total Page:16

File Type:pdf, Size:1020Kb

SIAC Newsletter March 2015 March 2015 The Sidereal Times Southeastern Iowa Astronomy Club A Member Society of the Astronomical League Club Officers: Minutes February 19, 2015 Executive Committee President Jim Hilkin President Jim Hilkin the checking account is snow on the observatory Vice President Libby Snipes Treasurer Vicki Philabaum called the meeting to or- $1,895.92 which includes dome. Dave announced Secretary David Philabaum th th Chief Observer David Philabaum der at 6:30 pm with the $160.89 in grant funds. that a group of 4 and 5 Members-at-Large Claus Benninghoven following members in at- Vicki will send out dues grade Girl Scouts is Duane Gerling Blake Stumpf tendance: Judy Smithson, notices as they come due. scheduled to come to the rd Board of Directors Paul Sly, Claus Benning- Dave reported that he had observatory on March 3 . Chair Judy Hilkin Vice Chair Ray Reineke hoven, Duane Gerling, received some brochures Jim reported that the Secretary David Philabaum Members-at-Large Bill Stewart, Carl Snipes, about the 2015 Nebraska Witte Observatory will be Frank Libe Blake Stumpf and Dave Philabaum. Star Party. It will be held painted this spring. A Jim Wilt Three guests were also in July 12-17 at the Merritt grant has been submitted Audit Committee Dean Moberg (2012) attendance. Jim ex- reservoir near Valentine, to Diamond Vogel for the JT Stumpf (2013) John Toney (2014) pressed condolences to Nebraska. Jim reported paint. In preparation for Newsletter Carl on the recent death that a group of Girl Scouts this the bushes on the Karen Johnson of his mother. Dave pre- was at the observatory on north side of the class- sented the Treasurer's February 3 rd , but the only room will be removed. A report in Vicki's absence. viewing was through a couple of evergreens have Inside this issue: The current balance in portable scope because of already been cut back. (Minutes continued on page 3) In The News 2 Mutual Events 2 Upcoming Dates Convention Letter 3 ~ Dues are due in April ~ First Friday Public Viewing, April 3 (weather Minutes (cont.) 3 ~ Nominations for club permitting) Looking Back 4 officers in April ~ Deadline for the April ~ Election of officers in Treasurer’s Report 4 newsletter is Wednesday, May Observer’s Report 5-6 April 8, 2015 ~ The next meeting will ~ April meeting on the Calendar 7 be Thursday, March 19, at 17 th the Burlington Public Li- Sky Maps 8-9 brary, 6:30—7:30 Page 2 The Sidereal Times In The News The Maven spacecraft has served by the Hubble exposed them to ultravio- detected a high-altitude Space Telescope. It’s esti- let radiation, and have dust cloud and aurora in mated to be 60 miles thick produced uracil, cytosine, the atmosphere of Mars. and buried under an icy and thymine. All three crust 95 miles deep. are found in RNA and Amateur astronomers can DNA, showing that these now help discover new Four new spacecraft, the components of life can be asteroids by analyzing im- MMS, launched on March made non-biologically in a ages using a desktop soft- 12, will study magnetic lab under conditions ware application devel- reconnection, a process found in space. oped by NASA and Plane- where magnetic fields tary Resources, Inc. The connect and disconnect software is free and can be and reconnect in new con- Sources: downloaded at http:// figurations, converting http://www.nasa.gov/news/ topcoder.com/asteroids magnetic energy into ki- releases/latest/#.VQntQI7F_K1 netic energy, thermal en- On Friday, March 27, the ergy, and particle acceler- http://www.nasa.gov/topics/ first one-year crew will ation, resulting in bursts universe/ launch for the Interna- of energy. index.html#.VQop147F_K0 Did You Know? tional Space Station. Scientists at the Ames Re- Ganymede is only Evidence for an under- search Center in Califor- slightly smaller than ground saltwater ocean on nia have taken ice samples Ganymede has been ob- containing pyrimidine, Mars. Although Gali- leo called it Jupiter III, it was renamed in the mid-1800s. a er Gan- Deep Mutual Events of Jupiter's Moons ymede , a Trojan Begin End prince in Greek my- Date Type ∆m thology. (Local) (Local) 3/20/2015 0:39:59 0:44:44 1E2 0.6 3/24/2015 1:03:35 1:11:24 3E2 0.5 3/27/2015 2:53:22 2:58:18 1E2 0.6 4/11/2015 20:41:15 20:50:37 2E3 1.0 4/13/2015 20:28:20 20:33:36 1E2 0.6 4/17/2015 20:27:45 20:37:01 4O3 1.0 Type - type of the event is given in the form "nEm" or "nOm" where n is the number of eclips- ing or occulting satellite, m is the number of eclipsed or occulted one. "E" denotes an eclipse and "O" denotes an occultation. 1=Io, 2=Europa, 3=Ganymede, 4=Callisto ∆m - expected maximum drop of the combined magnitude. MarchNovember 2015 2013 Page 3 NCRAL Convention Cancelled "We of the Fargo-Moorhead Astronomy Club regret to inform you that we are unable to host the NCRAL 2015 convention, and the June 5-6 event in Fargo is cancelled. We apologize for any disappointment or inconvenience this causes you. Our club has had a trying year with a series of setbacks. Economic circumstances have affected our university partners and mem- bership; half of our core members are gone due to job relocations out of our metro area, the state, and even the country. The remaining members have been discussing what the future of the FMAC will be. We wish your clubs the best for the future, and that they may live long and prosper. Sincerely, Scarlet Gray Bernard President, Fargo-Moorhead Astronomy Club" Did You Know? The bright stars in Gemini are Castor and Minutes (continued from page 1) Pollux, which are also the names of the Jim said he has postponed sending some photos and then gave a presentation brothers in the movie working on the panels for posters. She reported that on the constellation Gemi- “Face/Off.” the south end of the Prugh the Rand Foundation ni. After his presentation -Carver Observatory until would like to sponsor a Jim said that former mem- warmer weather returns. talk by Dr. Stone, possibly ber Terry Durbin was sell- Jim reported that he and this fall, and asked if the ing his 18" Obsession tele- Dave met with Kent Rector SIAC would like to help. scope and passed around to go over the cooperative She told them that we pictures of it. Carl passed agreement with the Con- would. Jim reported that around a binder of pic- servation Board to see if Dr. Steven Spangler of the tures that Libby Snipes there are any issues that University of Iowa would has recently taken for the need be addressed. No like to come sometime and members to look at. Libby changes were made. The look through the Clark. He wasn't able to be at the Conservation Board ap- would also be available to meeting. With no further proved and signed the give a talk. He is from the business to discuss, Duane agreement, but Partner's Houghton, IA area. Jim moved to adJourn, Bill se- for Conservation did not went over the list of up- conded, and the meeting sign. Jim reminded every- coming dates noting that was adJourned. one that nominations for the next meeting will also Respectfully submitted, club officers will take place be at the Burlington Public Dave Philabaum in April and elections will Library on March 19 th at be in May. Judy reported 06:30 pm. Dave gave the that Dr. Stone will be Observer's report. Jim Page 4 The Sidereal Times Looking Back in the Sidereal Times 25 Years Ago—March 1990 The March 1990 Sky & was four megapixels and as and a 50 megapixel Telescope magazine had a most observatories were astronomical CCD cam- picture of the largest CCD using one megapixel im- era is available to ama- made. It was a 16 mega- agers. A spokesperson for teurs. The Large Synoptic pixel chip made by Ford JPL said that the new Survey Telescope (LSST) Aerospace. It took over 11 chip is "too new and too will contain a 3.2 gi- minutes to read out the big for serious considera- gapixel camera made data from the chip and tion at this time". (Today up of an array of CCD took up 32 megabytes of it is not unusual to find chips. It will begin sur- storage. At that time the 20 megapixel chips in veying the heavens from largest astronomical CCD consumer digital camer- Chile in 2022.) Looking Back in the Sidereal Times 10 Years Ago—March 2005 In the Observer's Report Titan’s atmosphere and Huygens probe descend- it was noted that the Cas- 35 hydrocarbon lakes ed through Titan's at- sini Space Probe had and seas have been mosphere and landed on Did You Know? made its fourth flyby of named . The surface tem- the surface. The mission Saturn's moon Titan, fly- perature on Titan is - has been extended until According to Greek ing within 982 miles of its 290 °F and the surface 2017 which will include mythology, the surface. (Since then Cas- pressure is almost 50% over 50 more flybys of sini-Huygens mission has Titan.) Olympians overthrew more than on Earth. In identified 17 molecules in addition to flying by, the the elder gods that ruled the earth. Those elders, brothers of Saturn, were called Treasurer’s Report Titans.
Recommended publications
  • Astronomy Magazine Special Issue
    γ ι ζ γ δ α κ β κ ε γ β ρ ε ζ υ α φ ψ ω χ α π χ φ γ ω ο ι δ κ α ξ υ λ τ μ β α σ θ ε β σ δ γ ψ λ ω σ η ν θ Aι must-have for all stargazers η δ μ NEW EDITION! ζ λ β ε η κ NGC 6664 NGC 6539 ε τ μ NGC 6712 α υ δ ζ M26 ν NGC 6649 ψ Struve 2325 ζ ξ ATLAS χ α NGC 6604 ξ ο ν ν SCUTUM M16 of the γ SERP β NGC 6605 γ V450 ξ η υ η NGC 6645 M17 φ θ M18 ζ ρ ρ1 π Barnard 92 ο χ σ M25 M24 STARS M23 ν β κ All-in-one introduction ALL NEW MAPS WITH: to the night sky 42,000 more stars (87,000 plotted down to magnitude 8.5) AND 150+ more deep-sky objects (more than 1,200 total) The Eagle Nebula (M16) combines a dark nebula and a star cluster. In 100+ this intense region of star formation, “pillars” form at the boundaries spectacular between hot and cold gas. You’ll find this object on Map 14, a celestial portion of which lies above. photos PLUS: How to observe star clusters, nebulae, and galaxies AS2-CV0610.indd 1 6/10/10 4:17 PM NEW EDITION! AtlAs Tour the night sky of the The staff of Astronomy magazine decided to This atlas presents produce its first star atlas in 2006.
    [Show full text]
  • A Basic Requirement for Studying the Heavens Is Determining Where In
    Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun­ damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short).
    [Show full text]
  • Exoplanet.Eu Catalog Page 1 # Name Mass Star Name
    exoplanet.eu_catalog # name mass star_name star_distance star_mass OGLE-2016-BLG-1469L b 13.6 OGLE-2016-BLG-1469L 4500.0 0.048 11 Com b 19.4 11 Com 110.6 2.7 11 Oph b 21 11 Oph 145.0 0.0162 11 UMi b 10.5 11 UMi 119.5 1.8 14 And b 5.33 14 And 76.4 2.2 14 Her b 4.64 14 Her 18.1 0.9 16 Cyg B b 1.68 16 Cyg B 21.4 1.01 18 Del b 10.3 18 Del 73.1 2.3 1RXS 1609 b 14 1RXS1609 145.0 0.73 1SWASP J1407 b 20 1SWASP J1407 133.0 0.9 24 Sex b 1.99 24 Sex 74.8 1.54 24 Sex c 0.86 24 Sex 74.8 1.54 2M 0103-55 (AB) b 13 2M 0103-55 (AB) 47.2 0.4 2M 0122-24 b 20 2M 0122-24 36.0 0.4 2M 0219-39 b 13.9 2M 0219-39 39.4 0.11 2M 0441+23 b 7.5 2M 0441+23 140.0 0.02 2M 0746+20 b 30 2M 0746+20 12.2 0.12 2M 1207-39 24 2M 1207-39 52.4 0.025 2M 1207-39 b 4 2M 1207-39 52.4 0.025 2M 1938+46 b 1.9 2M 1938+46 0.6 2M 2140+16 b 20 2M 2140+16 25.0 0.08 2M 2206-20 b 30 2M 2206-20 26.7 0.13 2M 2236+4751 b 12.5 2M 2236+4751 63.0 0.6 2M J2126-81 b 13.3 TYC 9486-927-1 24.8 0.4 2MASS J11193254 AB 3.7 2MASS J11193254 AB 2MASS J1450-7841 A 40 2MASS J1450-7841 A 75.0 0.04 2MASS J1450-7841 B 40 2MASS J1450-7841 B 75.0 0.04 2MASS J2250+2325 b 30 2MASS J2250+2325 41.5 30 Ari B b 9.88 30 Ari B 39.4 1.22 38 Vir b 4.51 38 Vir 1.18 4 Uma b 7.1 4 Uma 78.5 1.234 42 Dra b 3.88 42 Dra 97.3 0.98 47 Uma b 2.53 47 Uma 14.0 1.03 47 Uma c 0.54 47 Uma 14.0 1.03 47 Uma d 1.64 47 Uma 14.0 1.03 51 Eri b 9.1 51 Eri 29.4 1.75 51 Peg b 0.47 51 Peg 14.7 1.11 55 Cnc b 0.84 55 Cnc 12.3 0.905 55 Cnc c 0.1784 55 Cnc 12.3 0.905 55 Cnc d 3.86 55 Cnc 12.3 0.905 55 Cnc e 0.02547 55 Cnc 12.3 0.905 55 Cnc f 0.1479 55
    [Show full text]
  • High-Precision Asteroseismology of Dense Stellar Fields
    Experimental Astronomy https://doi.org/10.1007/s10686-021-09711-1 ORIGINAL ARTICLE HAYDN High-precision AsteroseismologY of DeNse stellar fields Andrea Miglio1,2,3 · Leo´ Girardi4 · Frank Grundahl5 · Benoit Mosser6 · Nate Bastian7 · Angela Bragaglia3 · Karsten Brogaard5,8 · Gael¨ Buldgen9 · William Chantereau7 · William Chaplin1 · Cristina Chiappini10 · Marc-Antoine Dupret11 · Patrick Eggenberger9 · Mark Gieles12,13 · Robert Izzard14 · Daisuke Kawata15 · Christoffer Karoff5 · Nadege` Lagarde16 · Ted Mackereth1,17,18,19 · Demetrio Magrin4 · Georges Meynet9 · Eric Michel20 · Josefina Montalban´ 1 · Valerio Nascimbeni4 · Arlette Noels11 · Giampaolo Piotto21 · Roberto Ragazzoni4 · Igor Soszynski´ 22 · Eline Tolstoy23 · Silvia Toonen1,24 · Amaury Triaud1 · Fiorenzo Vincenzo1,25 Received: 29 July 2020 / Accepted: 9 February 2021 / © The Author(s) 2021 Abstract In the last decade, the Kepler and CoRoT space-photometry missions have demon- strated the potential of asteroseismology as a novel, versatile and powerful tool to perform exquisite tests of stellar physics, and to enable precise and accurate char- acterisations of stellar properties, with impact on both exoplanetary and Galactic astrophysics. Based on our improved understanding of the strengths and limitations of such a tool, we argue for a new small/medium space mission dedicated to gath- ering high-precision, high-cadence, long photometric series in dense stellar fields. Such a mission will lead to breakthroughs in stellar astrophysics, especially in the metal poor regime, will elucidate the evolution and formation of open and globular clusters, and aid our understanding of the assembly history and chemodynamics of the Milky Way’s bulge and a few nearby dwarf galaxies. Keywords Stars: low-mass · Globular clusters · Galaxy: bulge · Galaxies: dwarf · Asteroseismology A list of people who have expressed interest for HAYDN is available here: https://www.asterochronometry.eu/haydn/people.html Andrea Miglio [email protected] Extended author information available on the last page of the article.
    [Show full text]
  • 00E the Construction of the Universe Symphony
    The basic construction of the Universe Symphony. There are 30 asterisms (Suites) in the Universe Symphony. I divided the asterisms into 15 groups. The asterisms in the same group, lay close to each other. Asterisms!! in Constellation!Stars!Objects nearby 01 The W!!!Cassiopeia!!Segin !!!!!!!Ruchbah !!!!!!!Marj !!!!!!!Schedar !!!!!!!Caph !!!!!!!!!Sailboat Cluster !!!!!!!!!Gamma Cassiopeia Nebula !!!!!!!!!NGC 129 !!!!!!!!!M 103 !!!!!!!!!NGC 637 !!!!!!!!!NGC 654 !!!!!!!!!NGC 659 !!!!!!!!!PacMan Nebula !!!!!!!!!Owl Cluster !!!!!!!!!NGC 663 Asterisms!! in Constellation!Stars!!Objects nearby 02 Northern Fly!!Aries!!!41 Arietis !!!!!!!39 Arietis!!! !!!!!!!35 Arietis !!!!!!!!!!NGC 1056 02 Whale’s Head!!Cetus!! ! Menkar !!!!!!!Lambda Ceti! !!!!!!!Mu Ceti !!!!!!!Xi2 Ceti !!!!!!!Kaffalijidhma !!!!!!!!!!IC 302 !!!!!!!!!!NGC 990 !!!!!!!!!!NGC 1024 !!!!!!!!!!NGC 1026 !!!!!!!!!!NGC 1070 !!!!!!!!!!NGC 1085 !!!!!!!!!!NGC 1107 !!!!!!!!!!NGC 1137 !!!!!!!!!!NGC 1143 !!!!!!!!!!NGC 1144 !!!!!!!!!!NGC 1153 Asterisms!! in Constellation Stars!!Objects nearby 03 Hyades!!!Taurus! Aldebaran !!!!!! Theta 2 Tauri !!!!!! Gamma Tauri !!!!!! Delta 1 Tauri !!!!!! Epsilon Tauri !!!!!!!!!Struve’s Lost Nebula !!!!!!!!!Hind’s Variable Nebula !!!!!!!!!IC 374 03 Kids!!!Auriga! Almaaz !!!!!! Hoedus II !!!!!! Hoedus I !!!!!!!!!The Kite Cluster !!!!!!!!!IC 397 03 Pleiades!! ! Taurus! Pleione (Seven Sisters)!! ! ! Atlas !!!!!! Alcyone !!!!!! Merope !!!!!! Electra !!!!!! Celaeno !!!!!! Taygeta !!!!!! Asterope !!!!!! Maia !!!!!!!!!Maia Nebula !!!!!!!!!Merope Nebula !!!!!!!!!Merope
    [Show full text]
  • Exoplanet.Eu Catalog Page 1 Star Distance Star Name Star Mass
    exoplanet.eu_catalog star_distance star_name star_mass Planet name mass 1.3 Proxima Centauri 0.120 Proxima Cen b 0.004 1.3 alpha Cen B 0.934 alf Cen B b 0.004 2.3 WISE 0855-0714 WISE 0855-0714 6.000 2.6 Lalande 21185 0.460 Lalande 21185 b 0.012 3.2 eps Eridani 0.830 eps Eridani b 3.090 3.4 Ross 128 0.168 Ross 128 b 0.004 3.6 GJ 15 A 0.375 GJ 15 A b 0.017 3.6 YZ Cet 0.130 YZ Cet d 0.004 3.6 YZ Cet 0.130 YZ Cet c 0.003 3.6 YZ Cet 0.130 YZ Cet b 0.002 3.6 eps Ind A 0.762 eps Ind A b 2.710 3.7 tau Cet 0.783 tau Cet e 0.012 3.7 tau Cet 0.783 tau Cet f 0.012 3.7 tau Cet 0.783 tau Cet h 0.006 3.7 tau Cet 0.783 tau Cet g 0.006 3.8 GJ 273 0.290 GJ 273 b 0.009 3.8 GJ 273 0.290 GJ 273 c 0.004 3.9 Kapteyn's 0.281 Kapteyn's c 0.022 3.9 Kapteyn's 0.281 Kapteyn's b 0.015 4.3 Wolf 1061 0.250 Wolf 1061 d 0.024 4.3 Wolf 1061 0.250 Wolf 1061 c 0.011 4.3 Wolf 1061 0.250 Wolf 1061 b 0.006 4.5 GJ 687 0.413 GJ 687 b 0.058 4.5 GJ 674 0.350 GJ 674 b 0.040 4.7 GJ 876 0.334 GJ 876 b 1.938 4.7 GJ 876 0.334 GJ 876 c 0.856 4.7 GJ 876 0.334 GJ 876 e 0.045 4.7 GJ 876 0.334 GJ 876 d 0.022 4.9 GJ 832 0.450 GJ 832 b 0.689 4.9 GJ 832 0.450 GJ 832 c 0.016 5.9 GJ 570 ABC 0.802 GJ 570 D 42.500 6.0 SIMP0136+0933 SIMP0136+0933 12.700 6.1 HD 20794 0.813 HD 20794 e 0.015 6.1 HD 20794 0.813 HD 20794 d 0.011 6.1 HD 20794 0.813 HD 20794 b 0.009 6.2 GJ 581 0.310 GJ 581 b 0.050 6.2 GJ 581 0.310 GJ 581 c 0.017 6.2 GJ 581 0.310 GJ 581 e 0.006 6.5 GJ 625 0.300 GJ 625 b 0.010 6.6 HD 219134 HD 219134 h 0.280 6.6 HD 219134 HD 219134 e 0.200 6.6 HD 219134 HD 219134 d 0.067 6.6 HD 219134 HD
    [Show full text]
  • The Monitor Project: Searching for Occultations in Young Open Clusters
    Mon. Not. R. Astron. Soc. 000, 1–26 (2002) Printed 26 June 2018 (MN LATEX style file v2.2) The Monitor project: Searching for occultations in young open clusters S. Aigrain1⋆, S. Hodgkin1, J. Irwin1, L. Hebb2, M. Irwin1, F. Favata3, E. Moraux4, F. Pont5 1Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom 2School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, Scotland 3ESA/ESTEC, Keplerlaan 1, PO Box 299, 2200 AG Noordwijk, The Netherlands 4Laboratoire d’Astrophysique, Observatoire de Grenoble, BP 53, F-38041 Grenoble C´edex 9, France 5Observatoire Astronomique de l’Universit´ede Gen`eve, 51, chemin des Maillettes, CH-1290 Sauverny, Switzerland Accepted . Received . ; in original form . ABSTRACT The Monitor project is a photometric monitoring survey of nine young (1–200Myr) clus- ters in the solar neighbourhoodto search for eclipses by very low mass stars and brown dwarfs and for planetarytransits in the light curves of cluster members.It beganin the autumnof 2004 and uses several 2 to 4m telescopes worldwide. We aim to calibrate the relation between age, mass, radius and where possible luminosity, from the K-dwarf to the planet regime, in an age range where constraints on evolutionary models are currently very scarce. Any detection of an exoplanet in one of our youngest targets (. 10Myr) would also provide important constraints on planet formation and migration timescales and their relation to proto-planetary disc life- times. Finally, we will use the light curves of cluster members to study rotation and flaring in low-mass pre-main sequence stars.
    [Show full text]
  • SPIRIT Target Lists
    JANUARY and FEBRUARY deep sky objects JANUARY FEBRUARY OBJECT RA (2000) DECL (2000) OBJECT RA (2000) DECL (2000) Category 1 (west of meridian) Category 1 (west of meridian) NGC 1532 04h 12m 04s -32° 52' 23" NGC 1792 05h 05m 14s -37° 58' 47" NGC 1566 04h 20m 00s -54° 56' 18" NGC 1532 04h 12m 04s -32° 52' 23" NGC 1546 04h 14m 37s -56° 03' 37" NGC 1672 04h 45m 43s -59° 14' 52" NGC 1313 03h 18m 16s -66° 29' 43" NGC 1313 03h 18m 15s -66° 29' 51" NGC 1365 03h 33m 37s -36° 08' 27" NGC 1566 04h 20m 01s -54° 56' 14" NGC 1097 02h 46m 19s -30° 16' 32" NGC 1546 04h 14m 37s -56° 03' 37" NGC 1232 03h 09m 45s -20° 34' 45" NGC 1433 03h 42m 01s -47° 13' 19" NGC 1068 02h 42m 40s -00° 00' 48" NGC 1792 05h 05m 14s -37° 58' 47" NGC 300 00h 54m 54s -37° 40' 57" NGC 2217 06h 21m 40s -27° 14' 03" Category 1 (east of meridian) Category 1 (east of meridian) NGC 1637 04h 41m 28s -02° 51' 28" NGC 2442 07h 36m 24s -69° 31' 50" NGC 1808 05h 07m 42s -37° 30' 48" NGC 2280 06h 44m 49s -27° 38' 20" NGC 1792 05h 05m 14s -37° 58' 47" NGC 2292 06h 47m 39s -26° 44' 47" NGC 1617 04h 31m 40s -54° 36' 07" NGC 2325 07h 02m 40s -28° 41' 52" NGC 1672 04h 45m 43s -59° 14' 52" NGC 3059 09h 50m 08s -73° 55' 17" NGC 1964 05h 33m 22s -21° 56' 43" NGC 2559 08h 17m 06s -27° 27' 25" NGC 2196 06h 12m 10s -21° 48' 22" NGC 2566 08h 18m 46s -25° 30' 02" NGC 2217 06h 21m 40s -27° 14' 03" NGC 2613 08h 33m 23s -22° 58' 22" NGC 2442 07h 36m 20s -69° 31' 29" Category 2 Category 2 M 42 05h 35m 17s -05° 23' 25" M 42 05h 35m 17s -05° 23' 25" NGC 2070 05h 38m 38s -69° 05' 39" NGC 2070 05h 38m 38s -69°
    [Show full text]
  • Photometry and Membership for Low Mass Stars in the Young Open Cluster NGC 2516
    A&A 375, 863–889 (2001) Astronomy DOI: 10.1051/0004-6361:20010918 & c ESO 2001 Astrophysics Photometry and membership for low mass stars in the young open cluster NGC 2516 R. D. Jeffries1,?,M.R.Thurston2, and N. C. Hambly3 1 Department of Physics, Keele University, Keele, Staffordshire ST5 5BG, UK 2 School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK 3 Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK Received 15 May 2001 / Accepted 26 June 2001 Abstract. We present the results of a 0.86 square degree CCD photometric survey of the open cluster NGC 2516, which has an age of about 150 Myr and may have a much lower metallicity than the similarly-aged Pleiades. Our BVIc survey of cluster members is complete to V ' 20 and is used to select a preliminary catalogue of 1254 low mass (0.2 <M<2.0 M ) cluster candidates, of which about 70–80 percent are expected to be genuine. After applying corrections for contamination by non-members and adding data for higher mass stars from the literature, we investigate the cluster binarity, luminosity and mass function, mass segregation and total mass. We find a binary fraction of 26 5 percent, for A to M-type systems with mass ratios between 0.6 and 1, which is very similar to the Pleiades. The mass function is metallicity and evolutionary-model dependent, but consistent with a Salpeter-like law (dN/dlogM ∝ M −α, α =+1.47 0.11 or α =+1.67 0.11 for the solar and half-solar metallicity models of Siess et al.
    [Show full text]
  • Caldwell Catalogue - Wikipedia, the Free Encyclopedia
    Caldwell catalogue - Wikipedia, the free encyclopedia Log in / create account Article Discussion Read Edit View history Caldwell catalogue From Wikipedia, the free encyclopedia Main page Contents The Caldwell Catalogue is an astronomical catalog of 109 bright star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled Featured content by Sir Patrick Caldwell-Moore, better known as Patrick Moore, as a complement to the Messier Catalogue. Current events The Messier Catalogue is used frequently by amateur astronomers as a list of interesting deep-sky objects for observations, but Moore noted that the list did not include Random article many of the sky's brightest deep-sky objects, including the Hyades, the Double Cluster (NGC 869 and NGC 884), and NGC 253. Moreover, Moore observed that the Donate to Wikipedia Messier Catalogue, which was compiled based on observations in the Northern Hemisphere, excluded bright deep-sky objects visible in the Southern Hemisphere such [1][2] Interaction as Omega Centauri, Centaurus A, the Jewel Box, and 47 Tucanae. He quickly compiled a list of 109 objects (to match the number of objects in the Messier [3] Help Catalogue) and published it in Sky & Telescope in December 1995. About Wikipedia Since its publication, the catalogue has grown in popularity and usage within the amateur astronomical community. Small compilation errors in the original 1995 version Community portal of the list have since been corrected. Unusually, Moore used one of his surnames to name the list, and the catalogue adopts "C" numbers to rename objects with more Recent changes common designations.[4] Contact Wikipedia As stated above, the list was compiled from objects already identified by professional astronomers and commonly observed by amateur astronomers.
    [Show full text]
  • The Star Clusters Young & Old Newsletter
    SCYON The Star Clusters Young & Old Newsletter edited by Holger Baumgardt, Ernst Paunzen and Pavel Kroupa SCYON can be found at URL: http://astro.u-strasbg.fr/scyon SCYON Issue No. 34 16 July 2007 EDITORIAL Here is the 34th issue of the SCYON newsletter. The current issue contains 35 abstracts from refereed journals, and an announcement for the MODEST-8 meeting in Bonn in December. The next issue will be sent out in September. We wish everybody a productive summer... Thank you to all those who sent in their contributions. Holger Baumgardt, Ernst Paunzen and Pavel Kroupa ................................................... ................................................. CONTENTS Editorial .......................................... ...............................................1 SCYON policy ........................................ ...........................................2 Mirror sites ........................................ ..............................................2 Abstract from/submitted to REFEREED JOURNALS ........... ................................3 1. Star Forming Regions ............................... ........................................3 2. Galactic Open Clusters............................. .........................................6 3. Galactic Globular Clusters ......................... ........................................16 4. Galactic Center Clusters ........................... ........................................23 5. Extragalactic Clusters............................ ..........................................24
    [Show full text]
  • Astronomy and Astrophysics Books in Print, and to Choose Among Them Is a Difficult Task
    APPENDIX ONE Degeneracy Degeneracy is a very complex topic but a very important one, especially when discussing the end stages of a star’s life. It is, however, a topic that sends quivers of apprehension down the back of most people. It has to do with quantum mechanics, and that in itself is usually enough for most people to move on, and not learn about it. That said, it is actually quite easy to understand, providing that the information given is basic and not peppered throughout with mathematics. This is the approach I shall take. In most stars, the gas of which they are made up will behave like an ideal gas, that is, one that has a simple relationship among its temperature, pressure, and density. To be specific, the pressure exerted by a gas is directly proportional to its temperature and density. We are all familiar with this. If a gas is compressed, it heats up; likewise, if it expands, it cools down. This also happens inside a star. As the temperature rises, the core regions expand and cool, and so it can be thought of as a safety valve. However, in order for certain reactions to take place inside a star, the core is compressed to very high limits, which allows very high temperatures to be achieved. These high temperatures are necessary in order for, say, helium nuclear reactions to take place. At such high temperatures, the atoms are ionized so that it becomes a soup of atomic nuclei and electrons. Inside stars, especially those whose density is approaching very high values, say, a white dwarf star or the core of a red giant, the electrons that make up the central regions of the star will resist any further compression and themselves set up a powerful pressure.1 This is termed degeneracy, so that in a low-mass red 191 192 Astrophysics is Easy giant star, for instance, the electrons are degenerate, and the core is supported by an electron-degenerate pressure.
    [Show full text]