Desert Skies
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
CONSTELLATION VULPECULA, the (LITTLE) FOX Vulpecula Is a Faint Constellation in the Northern Sky
CONSTELLATION VULPECULA, THE (LITTLE) FOX Vulpecula is a faint constellation in the northern sky. Its name is Latin for "little fox", although it is commonly known simply as the fox. It was identified in the seventeenth century, and is located in the middle of the northern Summer Triangle (an asterism consisting of the bright stars Deneb in Cygnus (the Swan), Vega in Lyra (the Lyre) and Altair in Aquila (the Eagle). Vulpecula was introduced by the Polish astronomer Johannes Hevelius in the late 17th century. It is not associated with any figure in mythology. Hevelius originally named the constellation Vulpecula cum ansere, or Vulpecula et Anser, which means the little fox with the goose. The constellation was depicted as a fox holding a goose in its jaws. The stars were later separated to form two constellations, Anser and Vulpecula, and then merged back together into the present-day Vulpecula constellation. The goose was left out of the constellation’s name, but instead the brightest star, Alpha Vulpeculae, carries the name Anser. It is one of the seven constellations created by Hevelius. The fox and the goose shown as ‘Vulpec. & Anser’ on the Atlas Coelestis of John Flamsteed (1729). The Fox and Goose is a traditional pub name in Britain. STARS There are no stars brighter than 4th magnitude in this constellation. The brightest star is: Alpha Vulpeculae, a magnitude 4.44m red giant at a distance of 297 light-years. The star is an optical binary (separation of 413.7") that can be split using binoculars. The star also carries the traditional name Anser, which refers to the goose the little fox holds in its jaws. -
The State of Anthro–Earth
The Rosette Gazette Volume 22,, IssueIssue 7 Newsletter of the Rose City Astronomers July, 2010 RCA JULY 19 GENERAL MEETING The State Of Anthro–Earth THE STATE OF ANTHRO-EARTH: A Visitor From Far, Far Away Reviews the Status of Our Planet In This Issue: A Talk (in Earth-English) By Richard Brenne 1….General Meeting Enrico Fermi famously wondered why we hadn't heard from any other planetary 2….Club Officers civilizations, and Richard Brenne, who we'd always suspected was probably from another planet, thinks he might know the answer. Carl Sagan thought it was likely …...Magazines because those on other planets blew themselves up with nuclear weapons, but Richard …...RCA Library thinks its more likely that burning fossil fuels changed the climates and collapsed the 3….Local Happenings civilizations of those we might otherwise have heard from. Only someone from another planet could discuss this most serious topic with Richard's trademark humor 4…. Telescope (in a previous life he was an award-winning screenwriter - on which planet we're not Transformation sure) and bemused detachment. 5….Special Interest Groups Richard Brenne teaches a NASA-sponsored Global Climate Change class, serves on 6….Star Party Scene the American Meteorological Society's Committee to Communicate Climate Change, has written and produced documentaries about climate change since 1992, and has 7.…Observers Corner produced and moderated 50 hours of panel discussions about climate change with 18...RCA Board Minutes many of the world's top climate change scientists. Richard writes for the blog "Climate Progress" and his forthcoming book is titled "Anthro-Earth", his new name 20...Calendars for his adopted planet. -
The Professor Comet's Report Late Summer/Early Autumn – September
The Professor Comet’s Report 1 Messier 71 and C/2009 P1 Garradd © Steve Grimsley of Houston Astronomical Society, 2011 Welcome to the comet report which is a monthly article on the observations of comets by the amateur astronomy community and comet hunters from around the world! This article is dedicated to the latest reports of available comets for observations, current state of those comets, future predictions, & projections for observations in comet astronomy! Late Summer/Early Autumn – September 2011 The Professor Comet’s Report 2 The Current Status of the Predominant Comets for July 2011! Comets Designation Orbital Magnitude Trend Observation Constellations Visibility (IAU – MPC) Status Visual (Range in Lat.) (Night Sky Location) Period Garradd 2009 P1 C 7.0 – 7.2 Getting 60°N – 60°S Between Sagitta and Vulpecula All Night Brighter (heading WNW towards Hercules) Honda – 45P P 8.0 Getting 50°N – 85°S Undergoing a wide retrograde motion! Early Morning Mrkos - Brighter Currently the comet is north of Hydra Pajdusakova heading NE towards Leo Elenin 2010 X1 C 8.6 – 9.4 Getting 45°N – 75°S Currently undergoing retrograde Early Evening Brighter motion in the S region of Leo (Just after Dusk) Crommelin 27P P 9.5 Possibly N/A Poor Elongation N/A Fading? (lost in the daytime glare!) LINEAR 2011 M1 C 10.4 Brightening 60°N – 45°N Moving SE of Ursa Major and All Night heading across the E edge of Leo Minor Hill 2010 G2 C 11.1 Fading 60°N – 10°N Between Ursa Major and Lynx All Night (Moving SSW of Muscida) Gibbs 2011 A3 C 11.4 Brightening 55°N -
THE CHANTICLEER Jacksonville State University Jacksonville
Jacksonville State University JSU Digital Commons Chanticleer Historical Newspapers 1985-01-11 Chanticleer | Vol 32, Issue 15 Jacksonville State University Follow this and additional works at: https://digitalcommons.jsu.edu/lib_ac_chanty Recommended Citation Jacksonville State University, "Chanticleer | Vol 32, Issue 15" (1985). Chanticleer. 871. https://digitalcommons.jsu.edu/lib_ac_chanty/871 This Book is brought to you for free and open access by the Historical Newspapers at JSU Digital Commons. It has been accepted for inclusion in Chanticleer by an authorized administrator of JSU Digital Commons. For more information, please contact [email protected]. C Entertainment THE CHANTICLEER Jacksonville State university Jacksonville. Alabama Vol. &No. W January 11, 1985 Mild controversy erupts over - senate resolution By JAN DICKINSON A resolution calling for a faculty-wide vote of "no confidence" in Resident Theron Montgomery was presented to the Faculty Senate at its December 10 meeting, two days before Montgomery anriounced his resignation to the Board of Trustees. Now the sponsor of the resolution, Dr. Gene Blanton, of the English Department, says that he intends to withdraw the resolution at the January 14 meeting of the senate. 13lanton stated in the January 6 edition of the Anniston Star that, because of comments made by several members of the Board of bstees, the wssibility of dropping the resolution was strong. According to that article, trustee Paul Carpenter said, "It (the vote) wouid make absolutely no difference in my opinion. We have studied the entire situation, and we are satisfied with the decision." Another board member, Dwaine Luce, stated, "....the bard is responsible for running the school, and the faculty is responsible for iristructing the students." Echoing the sentiments of Carpenter, he added, "'I'he board has inade its decision and the board, in my pinion, will stand by its decision." According to Dr. -
Central Coast Astronomy Virtual Star Party December 19Th 7Pm Pacific
Central Coast Astronomy Virtual Star Party December 19th 7pm Pacific Welcome to our Virtual Star Gazing session! We’ll be focusing on objects you can see with binoculars or a small telescope, so after our session, you can simply walk outside, look up, and understand what you’re looking at. CCAS President Aurora Lipper and astronomer Kent Wallace will bring you a virtual “tour of the night sky” where you can discover, learn, and ask questions as we go along! All you need is an internet connection. You can use an iPad, laptop, computer or cell phone. When 7pm on Saturday night rolls around, click the link on our website to join our class. CentralCoastAstronomy.org/stargaze Before our session starts: Step 1: Download your free map of the night sky: SkyMaps.com They have it available for Northern and Southern hemispheres. Step 2: Print out this document and use it to take notes during our time on Saturday. This document highlights the objects we will focus on in our session together. Celestial Objects: Moon: The moon is 5 days past new, really good for star gazing. Be sure to look at the moon tonight with your naked eyes and/or binoculars! Jupiter and Saturn are getting closer and closer, and on the 21st, they will be close enough to BOTH fit in the view of the eyepiece! If you start watching now, you’ll notice them draw closer and closer together. It’s pretty neat that this date also lines up with the Winter Solstice. This is the first Jupiter-Saturn conjunction since 2000, and the closest since 1623 (only 14 years after Galileo made this first telescope). -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
In Pdf Format
lós 1877 Mik 88 ge N 18 e N i h 80° 80° 80° ll T 80° re ly a o ndae ma p k Pl m os U has ia n anum Boreu bal e C h o A al m re u c K e o re S O a B Bo l y m p i a U n d Planum Es co e ria a l H y n d s p e U 60° e 60° 60° r b o r e a e 60° l l o C MARS · Korolev a i PHOTOMAP d n a c S Lomono a sov i T a t n M 1:320 000 000 i t V s a Per V s n a s l i l epe a s l i t i t a s B o r e a R u 1 cm = 320 km lkin t i t a s B o r e a a A a A l v s l i F e c b a P u o ss i North a s North s Fo d V s a a F s i e i c a a t ssa l vi o l eo Fo i p l ko R e e r e a o an u s a p t il b s em Stokes M ic s T M T P l Kunowski U 40° on a a 40° 40° a n T 40° e n i O Va a t i a LY VI 19 ll ic KI 76 es a As N M curi N G– ra ras- s Planum Acidalia Colles ier 2 + te . -
A Study of Ultraviolet Spectra of Delta Sagittae A
A STUDY OF ULTRAVIOLET SPECTRA OF DELTA SAGITTAE A. AKALIN and S. ENGIN University of Ankara Dept. of Astronomy and Space Sciences 06100 Tandogan, Ankara Turkiye ABSTRACT. High resolution spectrum of the VV Cephei type star Ô Sge (M2 II + AO V) observed with the IUE satellite between 1979-1985 have been analysed. The radial velocity curves of non blended absorption features have been formed. Observed radial velocities are compared with the theoretical radial velocity curve due to orbital motion. We found that observed radial velocity variation is the resultant of radial velocity of hotter component and wind velocity around this star. The wind is perturbed by hotter component. Matching the UV continuum fluxes obtained from IUE high resolution spectra to fluxes of Kurucz model atmospheres yields Te=11000±500 °K. Thus the spectral type of hot component was found as AO. 1. Introduction Delta Sagittae - classified as M2II+B by Batten and Fisher (1981) and M211+AO V by Batten (1986) is a spectroscopic binary of VV Cephei type with an orbital period of 3720 days. Β type component is eclipsed by the atmosphere of the M giant.The system must have an orbital inclination greater than 70°, since atmospheric eclipses have been observed. The last periastron passage occurred in the second week of April 1990. Distance to the system was determined 300 pc by Reimers and Kudritzki (1981), 224 pc by Batten and Fisher (1981) and 170±30 pc by Reimers and Schroder (1983). 2. Observations We have collected twelve IUE images of Ô Sge from to IUE-VILSPA data bank, The spectra cover the period between May 26, 1979 and May 14, 1985. -
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 -
Desert Skies Tucson Amateur Astronomy Association
Desert Skies Tucson Amateur Astronomy Association Volume LIII, Number 10 October, 2007 Spitzer Space Telescope Studies Binary Stars ♦ Learn about the ♦ Constellation of the month ♦ School star parties ♦ All-Arizona Star Party ♦ Opportunities to Volunteer Cover Photo: Artist concept of the circumbinary disk. Credit: P. Marenfeld and NOAO/AURA/NSF, http://www.noao.edu/ outreach/press/pr06/pr0604.html TAAA Web Page: http://www.tucsonastronomy.org TAAA Phone Number: (520) 792-6414 Office/Position Name Phone E-mail Address President Bill Lofquist 297-6653 [email protected] Vice President Ken Shaver 762-5094 [email protected] Secretary Steve Marten 307-5237 [email protected] Treasurer Terri Lappin 977-1290 [email protected] Member-at-Large George Barber 822-2392 [email protected] Member-at-Large Keith Schlottman 290-5883 [email protected] Member-at-Large Teresa Plymate 883-9113 [email protected] Chief Observer Wayne Johnson 586-2244 [email protected] AL Correspondent (ALCor) Nick de Mesa 797-6614 [email protected] Astro-Imaging SIG Steve Peterson 762-8211 [email protected] Computers in Astronomy SIG Roger Tanner 574-3876 [email protected] Beginners SIG JD Metzger 760-8248 [email protected] Newsletter Editor George Barber 822-2392 [email protected] School Star Party Scheduling Coordinator Paul Moss 240-2084 [email protected] School Star Party Volunteer Coordinator Claude -
Jeans Escape
TheThe lossloss ofof thethe earlyearly MartianMartian atmosphereatmosphere andand itsits waterwater inventoryinventory duedue toto thethe activeactive youngyoung SunSun H. Lammer (1), Yu. N. Kulikov (2), N. Terada (3), I. Ribas (4), D. Langmayr (1), N. V. Erkaev (5), G. Jaritz (6), H. K. Biernat (1,6) (1) Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, A-8042 Graz, Austria (2) Polar Geophysical Institute (PGI), Russian Academy of Sciences, Khalturina Str. 15, Murmansk, 183010, Russian Federation (3) Solar-Terrestrial Environment Laboratory, Nagoya University, Japan (4) Institute for Space Studies of Catalonia (IEEC) and Instituto de Ciencias del Espacio (CSIC), E-08034, Barcelona, Spain (5) Institute for Computational Modelling, Russian Academy of Sciences, Ru-660036 Krasnoyarsk 36, Russian Federation (6) Institute for Geophysics, Astrophysics, and Meteorology, University of Graz, Universitätsplatz 5, A-8010 Graz, Austria IEEC/CSIC TheThe casecase forfor aa wet,wet, warmwarm Mars:Mars: ButBut wherewhere isis allall thethe waterwater andand thethe atmosphereatmosphere ?? ¾ Observations of a network of valleys in crater rich areas of the southern hemisphere suggests that Mars had once a significant hydrologic activity [e.g., Carr Nature 326, 30, 1987; Baker Nature 412, 228, 2001; Carr & Head III JGR 108, E5, 5042, 2003] ¾ Asteroids and comets from beyond 2.5 AU provide the source of Mars’ water, which totals 6 – 27 % of the Earth’s present ocean equivalent to 600 – 2700 m depth on the Martian surface or in the crustal regolith [Lunine et al. Icarus 165, 1, 2003] ¾ Enrichment and fractionation of heavy isotopes [e.g., Pepin Icarus 111, 289, 1994] ¾ Estimations of volumes of potential early Martian water reservoirs from geo-morphological analysis of possible shorelines by MGS images and MOLA data → d ≈ 150 - 160 m [Carr & Head III JGR 108, E5, 5042, 2003] - Stored in present polar caps → d ≈ 20 - 30 m - Surface ground water → d ≈ 80 m ? - Escaped to space → d ≈ 50 - 80 m ? ¾ Early atmosphere ≈ 1 – 5 bars [e.g., Pollack, Kasting et al.