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Messier Plus Marathon Text
Messier Plus Marathon Object List by Wally Brown & Bob Buckner with additional objects by Mike Roos Object Data - Saguaro Astronomy Club Score is most numbered objects in a single night. Tiebreaker is count of un-numbered objects Observer Name Date Address Marathon Obects __________ Tiebreaker Objects ________ SEQ OBJECT TYPE CON R.A. DEC. RISE TRANSIT SET MAG SIZE NOTES TIME M 53 GLOCL COM 1312.9 +1810 7:21 14:17 21:12 7.7 13.0' NGC 5024, !B,vC,iR,vvmbM,st 12.. NGC 5272, !!,eB,vL,vsmbM,st 11.., Lord Rosse-sev dark 1 M 3 GLOCL CVN 1342.2 +2822 7:11 14:46 22:20 6.3 18.0' marks within 5' of center 2 M 5 GLOCL SER 1518.5 +0205 10:17 16:22 22:27 5.7 23.0' NGC 5904, !!,vB,L,eCM,eRi, st mags 11...;superb cluster M 94 GALXY CVN 1250.9 +4107 5:12 13:55 22:37 8.1 14.4'x12.1' NGC 4736, vB,L,iR,vsvmbM,BN,r NGC 6121, Cl,8 or 10 B* in line,rrr, Look for central bar M 4 GLOCL SCO 1623.6 -2631 12:56 17:27 21:58 5.4 36.0' structure M 80 GLOCL SCO 1617.0 -2258 12:36 17:21 22:06 7.3 10.0' NGC 6093, st 14..., Extremely rich and compressed M 62 GLOCL OPH 1701.2 -3006 13:49 18:05 22:21 6.4 15.0' NGC 6266, vB,L,gmbM,rrr, Asymmetrical M 19 GLOCL OPH 1702.6 -2615 13:34 18:06 22:38 6.8 17.0' NGC 6273, vB,L,R,vCM,rrr, One of the most oblate GC 3 M 107 GLOCL OPH 1632.5 -1303 12:17 17:36 22:55 7.8 13.0' NGC 6171, L,vRi,vmC,R,rrr, H VI 40 M 106 GALXY CVN 1218.9 +4718 3:46 13:23 22:59 8.3 18.6'x7.2' NGC 4258, !,vB,vL,vmE0,sbMBN, H V 43 M 63 GALXY CVN 1315.8 +4201 5:31 14:19 23:08 8.5 12.6'x7.2' NGC 5055, BN, vsvB stell. -
Wynyard Planetarium & Observatory a Autumn Observing Notes
Wynyard Planetarium & Observatory A Autumn Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn Tour of the Sky with the Naked Eye CASSIOPEIA Look for the ‘W’ 4 shape 3 Polaris URSA MINOR Notice how the constellations swing around Polaris during the night Pherkad Kochab Is Kochab orange compared 2 to Polaris? Pointers Is Dubhe Dubhe yellowish compared to Merak? 1 Merak THE PLOUGH Figure 1: Sketch of the northern sky in autumn. © Rob Peeling, CaDAS, 2007 version 1.2 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. Close to the horizon is a group of stars like the outline of a saucepan with the handle stretching to your left. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The two right-hand stars are called the Pointers. Can you tell that the higher of the two, Dubhe is slightly yellowish compared to the lower, Merak? Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white- hot. 2. Use the Pointers to guide you upwards to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the left are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris. -
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. -
Ghost Hunt Challenge 2020
Virtual Ghost Hunt Challenge 10/21 /2020 (Sorry we can meet in person this year or give out awards but try doing this challenge on your own.) Participant’s Name _________________________ Categories for the competition: Manual Telescope Electronically Aided Telescope Binocular Astrophotography (best photo) (if you expect to compete in more than one category please fill-out a sheet for each) ** There are four objects on this list that may be beyond the reach of beginning astronomers or basic telescopes. Therefore, we have marked these objects with an * and provided alternate replacements for you just below the designated entry. We will use the primary objects to break a tie if that’s needed. Page 1 TAS Ghost Hunt Challenge - Page 2 Time # Designation Type Con. RA Dec. Mag. Size Common Name Observed Facing West – 7:30 8:30 p.m. 1 M17 EN Sgr 18h21’ -16˚11’ 6.0 40’x30’ Omega Nebula 2 M16 EN Ser 18h19’ -13˚47 6.0 17’ by 14’ Ghost Puppet Nebula 3 M10 GC Oph 16h58’ -04˚08’ 6.6 20’ 4 M12 GC Oph 16h48’ -01˚59’ 6.7 16’ 5 M51 Gal CVn 13h30’ 47h05’’ 8.0 13.8’x11.8’ Whirlpool Facing West - 8:30 – 9:00 p.m. 6 M101 GAL UMa 14h03’ 54˚15’ 7.9 24x22.9’ 7 NGC 6572 PN Oph 18h12’ 06˚51’ 7.3 16”x13” Emerald Eye 8 NGC 6426 GC Oph 17h46’ 03˚10’ 11.0 4.2’ 9 NGC 6633 OC Oph 18h28’ 06˚31’ 4.6 20’ Tweedledum 10 IC 4756 OC Ser 18h40’ 05˚28” 4.6 39’ Tweedledee 11 M26 OC Sct 18h46’ -09˚22’ 8.0 7.0’ 12 NGC 6712 GC Sct 18h54’ -08˚41’ 8.1 9.8’ 13 M13 GC Her 16h42’ 36˚25’ 5.8 20’ Great Hercules Cluster 14 NGC 6709 OC Aql 18h52’ 10˚21’ 6.7 14’ Flying Unicorn 15 M71 GC Sge 19h55’ 18˚50’ 8.2 7’ 16 M27 PN Vul 20h00’ 22˚43’ 7.3 8’x6’ Dumbbell Nebula 17 M56 GC Lyr 19h17’ 30˚13 8.3 9’ 18 M57 PN Lyr 18h54’ 33˚03’ 8.8 1.4’x1.1’ Ring Nebula 19 M92 GC Her 17h18’ 43˚07’ 6.44 14’ 20 M72 GC Aqr 20h54’ -12˚32’ 9.2 6’ Facing West - 9 – 10 p.m. -
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. -
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). -
Cassiopeia - the Queen
May 18 2021 Cassiopeia - The Queen Observed: No Object Her Type Mag Alias/Notes NGC 7801 Non-Existent IC 11 Non-Existent NGC 358 Non-Existent NGC 629 Non-Existent IC 155 Non-Existent NGC 771 Non-Existent IC 1795 Non-Existent NGC 896 IC 1824 Non-Existent Single Star IC 1831 Non-Existent IC 1851 Non-Existent NGC 7438 Non-Existent IC 5366 Non-Existent NGC 7795 Non-Existent Sub Total: 13 Observed: Yes Object Her Type Mag Alias/Notes ABELL 82 Pl Neb 12.7 IC 1454 BERK 2 Open Cl I 1 m BERK 58 Open Cl IV 2 p 9.7 CR 15 Open Cl II 2 p 8.1 Tr 1 CR 26 Open Cl II 3 m n 6.5 Mel 15 Inside IC 1805 LBN CR 34 Open Cl I 3 p 6.8 CR 36 Open Cl III 2 m 7 Tr 3 CR 463 Open Cl III 2 m 5.7 IC 10 Glxy IBm 11.8 UGC 192 MCG 10-1-1 IRAS 177+5900 PGC 1305 IC 59 Brt Nebula E+R Sh2-185 Gamma Cassiopiae LBN 620 IC 63 Brt Nebula E+R LBN 623 Ghost Nebula IC 166 Open Cl II 1 r 11.7 IC 289 Pl Neb 4+2 12.3 Hubble 1 PK 138+2.1 PNG 138.8+2.8 IC 1590 Open Cl n 7.4 Cr 8 (Inside of NGC 281) IC 1747 Pl Neb 3b 13.6 PK 130+1.1 PNG 130.2+1.3 IC 1805 Brt Nebula E Sh2-190 LBN 654 (Cr 26 in brightest part) Heart Nebula IC 1848 Open Cl I 3 p n 6.5 Cr 32 (Inside LBN 667 Soul Nebula) IC 1871 Brt Nebula E KING 13 Open Cl II 2 m KING 14 Open Cl III 1 p 8.5 KING 16 Open Cl I 2 m 10.3 LBN 667 Brt Nebula E Soul Nebula (Surrounds IC1848) NGC 103 Open Cl II 1 m 9.8 NGC 110 Open Cl IV 1 p NGC 129 H79-8 Open Cl III 2 m 6.5 Cr 2 NGC 133 Open Cl IV 1 p 9.4 NGC 136 H35-6 Open Cl II 1 p Cr 4 Page 1 of 2 May 18 2021 Cassiopeia - The Queen Observed: Yes Object Her Type Mag Alias/Notes NGC 146 Open Cl II -
IC 1805, NGC 654 and NGC 6823
ASTRONOMY & ASTROPHYSICS APRIL II 1999, PAGE 313 SUPPLEMENT SERIES Astron. Astrophys. Suppl. Ser. 136, 313–331 (1999) Spectroscopic observations of young open clusters: IC 1805, NGC 654 and NGC 6823 H.M. Shi1,2 and J.Y. Hu2,3 1 Shanghai Astronomical observatory, Chinese Academy of Sciences, Shanghai 200030, China 2 Joint Laboratories for Optical Astronomy, Chinese Academy of Sciences, China 3 Beijing Astronomical observatory, Chinese Academy of Sciences, Beijing, 100080, China Received September 30, 1998; accepted January 11, 1999 Abstract. Spectroscopic observations were made for a Table 1. Spectrographs and gratings sample of 263 stars from three young open clusters spectrograph grating dispersion central wavelenth IC 1805, NGC 654 and NGC 6823 with CCD detectors in name lines/mm A/mm˚ A/pixel˚ A˚ the blue and yellow-red spectral regions. MKK types were UNIVERSAL 300 195 4.7 6000 properly determined for these stars by carefully compar- OMR 300 200 4.8 6000 600 100 2.4 5000 ing spectra of program stars with those of a complete grid 1200 50 1.2 4375 of MKK standards, which were observed with the same in- struments as the program stars. For most of the observed stars precise MKK types were assigned for the first time. A few of early-type emission-line stars were discovered or status, to just cite a few. The study of clusters and as- confirmed. The presence of Be stars in the studied clusters sociations deeply relies upon the accumulation of various is discussed. Spectra of the observed MKK standards also kinds of precise data, be it astrometric, photometric or reveal lots of features showing temperature or luminosity spectroscopic. -
History of Globulettes in the Milky Way
History of Globulettes in the Milky Way Tiia Grenman1 • Erik Elfgren1 • Hans Weber1 Abstract Globulettes are small (radii < 10 kAU) dark small-sized globules within H II regions were first ob- dust clouds, seen against the background of bright neb- served by Bok & Reilly (1947), followed by Thackeray ulae. A majority of the objects have planetary mass. (1950) and Herbig (1974). They are dense, cold and These objects may be a source of brown dwarfs and neutral clouds with dark appearance in optical images. free floating planetary mass objects in the galaxy. In The pillars of gas and dust are pointing towards the ion- this paper we investigate how many globulettes could izing sources and are usually connected to the molecular have formed in the Milky Way and how they could con- shell. tribute to the total population of free floating planets. In such H II regions, a new distinct class of objects, In order to do that we examine H-alpha images of 27 globulettes, was noted by Gahm et al. (2007) and Gren- H II regions. In these images, we find 778 globulettes. man (2006). The globulettes are seen as silhouettes We find that a conservative value of the number of against the background of bright nebulae in optical im- 10 globulettes formed is 5:7 × 10 . If 10 % of the glob- ages. Typically, they are roundish objects that are ulettes form free floating planets then they have con- much smaller (< 10 kAU) than normal globules with a tributed with 5:7×109 free floating planets in the Milky mass of . -
Nd AAS Meeting Abstracts
nd AAS Meeting Abstracts 101 – Kavli Foundation Lectureship: The Outreach Kepler Mission: Exoplanets and Astrophysics Search for Habitable Worlds 200 – SPD Harvey Prize Lecture: Modeling 301 – Bridging Laboratory and Astrophysics: 102 – Bridging Laboratory and Astrophysics: Solar Eruptions: Where Do We Stand? Planetary Atoms 201 – Astronomy Education & Public 302 – Extrasolar Planets & Tools 103 – Cosmology and Associated Topics Outreach 303 – Outer Limits of the Milky Way III: 104 – University of Arizona Astronomy Club 202 – Bridging Laboratory and Astrophysics: Mapping Galactic Structure in Stars and Dust 105 – WIYN Observatory - Building on the Dust and Ices 304 – Stars, Cool Dwarfs, and Brown Dwarfs Past, Looking to the Future: Groundbreaking 203 – Outer Limits of the Milky Way I: 305 – Recent Advances in Our Understanding Science and Education Overview and Theories of Galactic Structure of Star Formation 106 – SPD Hale Prize Lecture: Twisting and 204 – WIYN Observatory - Building on the 308 – Bridging Laboratory and Astrophysics: Writhing with George Ellery Hale Past, Looking to the Future: Partnerships Nuclear 108 – Astronomy Education: Where Are We 205 – The Atacama Large 309 – Galaxies and AGN II Now and Where Are We Going? Millimeter/submillimeter Array: A New 310 – Young Stellar Objects, Star Formation 109 – Bridging Laboratory and Astrophysics: Window on the Universe and Star Clusters Molecules 208 – Galaxies and AGN I 311 – Curiosity on Mars: The Latest Results 110 – Interstellar Medium, Dust, Etc. 209 – Supernovae and Neutron -
How Far Away One Can Penetrate with Gaia in Star Cluster Studies?
How far away we can penetrate with Gaia in star clusters study? D.A.Kovaleva, INASAN, Moscow, Russia N.V.Kharchenko, MAO, Kiev, Ukraine A.E.Piskunov, INASAN, Moscow, Russia S. Röser, LSW-ARI, Heidelberg, Germany E. Schilbach, LSW-ARI, Heidelberg, Germany S.Yen, LSW, Heidelberg, Germany SFB 881 Workshop Heidelberg 15-17 Aug 2018 Clusters: MWSC Globular (logt>9.8) Young (logt≤7.3) in the Other (logt>7.3) Milky Way MWSC includes 3210 clusters of different types among them: associations 51 globular clusters 147 moving groups 19 embedded/with nebula 132 remnant clusters 401 members 0.8 mln All having ages, masses, distances and other parameters d <10 kpc dmod 2.4 kpc εd/d ~11% R.Hurt, Spitzer Science Center SFB 881 Workshop Heidelberg 15-17 Aug 2018 2 R.Hurt, Spitzer Science Center Gaia DR1 (TGAS) stars with trigonometric parallaxes 휛 2 mln. ε휛 0.3-0.7 mas G_lim 12 mag available since Sept 2016 Kovaleva, Dana A.; Piskunov, Anatoly E.; Kharchenko, Nina V.; Röser, Siegfried; Schilbach, Elena; Scholz, Ralf- Dieter; Reffert, Sabine; Yen, Steffi X. “Open star clusters in the Milky Way. Comparison of photometric and trigonometric distance scales based on Gaia TGAS data” 2017A&A...606L...8K 66 clusters with 16+ MWSC 60%-members in TGAS SFB 881 Workshop Heidelberg 15-17 Aug 2018 3 Gaia DR2 stars with trigonometric parallaxes 휛 1.3 bln. ε휛 0.007-0.6 mas G_lim >20 mag (not in all area) available since Apr 2018 + proper motions + two-color photometry G_BP, G_RP + radial velocities for 7.2 mln. -
SAC's 110 Best of the NGC
SAC's 110 Best of the NGC by Paul Dickson Version: 1.4 | March 26, 1997 Copyright °c 1996, by Paul Dickson. All rights reserved If you purchased this book from Paul Dickson directly, please ignore this form. I already have most of this information. Why Should You Register This Book? Please register your copy of this book. I have done two book, SAC's 110 Best of the NGC and the Messier Logbook. In the works for late 1997 is a four volume set for the Herschel 400. q I am a beginner and I bought this book to get start with deep-sky observing. q I am an intermediate observer. I bought this book to observe these objects again. q I am an advance observer. I bought this book to add to my collect and/or re-observe these objects again. The book I'm registering is: q SAC's 110 Best of the NGC q Messier Logbook q I would like to purchase a copy of Herschel 400 book when it becomes available. Club Name: __________________________________________ Your Name: __________________________________________ Address: ____________________________________________ City: __________________ State: ____ Zip Code: _________ Mail this to: or E-mail it to: Paul Dickson 7714 N 36th Ave [email protected] Phoenix, AZ 85051-6401 After Observing the Messier Catalog, Try this Observing List: SAC's 110 Best of the NGC [email protected] http://www.seds.org/pub/info/newsletters/sacnews/html/sac.110.best.ngc.html SAC's 110 Best of the NGC is an observing list of some of the best objects after those in the Messier Catalog.