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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. -
Celebrating the Wonder of the Night Sky
Celebrating the Wonder of the Night Sky The heavens proclaim the glory of God. The skies display his craftsmanship. Psalm 19:1 NLT Celebrating the Wonder of the Night Sky Light Year Calculation: Simple! [Speed] 300 000 km/s [Time] x 60 s x 60 m x 24 h x 365.25 d [Distance] ≈ 10 000 000 000 000 km ≈ 63 000 AU Celebrating the Wonder of the Night Sky Milkyway Galaxy Hyades Star Cluster = 151 ly Barnard 68 Nebula = 400 ly Pleiades Star Cluster = 444 ly Coalsack Nebula = 600 ly Betelgeuse Star = 643 ly Helix Nebula = 700 ly Helix Nebula = 700 ly Witch Head Nebula = 900 ly Spirograph Nebula = 1 100 ly Orion Nebula = 1 344 ly Dumbbell Nebula = 1 360 ly Dumbbell Nebula = 1 360 ly Flame Nebula = 1 400 ly Flame Nebula = 1 400 ly Veil Nebula = 1 470 ly Horsehead Nebula = 1 500 ly Horsehead Nebula = 1 500 ly Sh2-106 Nebula = 2 000 ly Twin Jet Nebula = 2 100 ly Ring Nebula = 2 300 ly Ring Nebula = 2 300 ly NGC 2264 Nebula = 2 700 ly Cone Nebula = 2 700 ly Eskimo Nebula = 2 870 ly Sh2-71 Nebula = 3 200 ly Cat’s Eye Nebula = 3 300 ly Cat’s Eye Nebula = 3 300 ly IRAS 23166+1655 Nebula = 3 400 ly IRAS 23166+1655 Nebula = 3 400 ly Butterfly Nebula = 3 800 ly Lagoon Nebula = 4 100 ly Rotten Egg Nebula = 4 200 ly Trifid Nebula = 5 200 ly Monkey Head Nebula = 5 200 ly Lobster Nebula = 5 500 ly Pismis 24 Star Cluster = 5 500 ly Omega Nebula = 6 000 ly Crab Nebula = 6 500 ly RS Puppis Variable Star = 6 500 ly Eagle Nebula = 7 000 ly Eagle Nebula ‘Pillars of Creation’ = 7 000 ly SN1006 Supernova = 7 200 ly Red Spider Nebula = 8 000 ly Engraved Hourglass Nebula -
New Type of Black Hole Detected in Massive Collision That Sent Gravitational Waves with a 'Bang'
New type of black hole detected in massive collision that sent gravitational waves with a 'bang' By Ashley Strickland, CNN Updated 1200 GMT (2000 HKT) September 2, 2020 <img alt="Galaxy NGC 4485 collided with its larger galactic neighbor NGC 4490 millions of years ago, leading to the creation of new stars seen in the right side of the image." class="media__image" src="//cdn.cnn.com/cnnnext/dam/assets/190516104725-ngc-4485-nasa-super-169.jpg"> Photos: Wonders of the universe Galaxy NGC 4485 collided with its larger galactic neighbor NGC 4490 millions of years ago, leading to the creation of new stars seen in the right side of the image. Hide Caption 98 of 195 <img alt="Astronomers developed a mosaic of the distant universe, called the Hubble Legacy Field, that documents 16 years of observations from the Hubble Space Telescope. The image contains 200,000 galaxies that stretch back through 13.3 billion years of time to just 500 million years after the Big Bang. " class="media__image" src="//cdn.cnn.com/cnnnext/dam/assets/190502151952-0502-wonders-of-the-universe-super-169.jpg"> Photos: Wonders of the universe Astronomers developed a mosaic of the distant universe, called the Hubble Legacy Field, that documents 16 years of observations from the Hubble Space Telescope. The image contains 200,000 galaxies that stretch back through 13.3 billion years of time to just 500 million years after the Big Bang. Hide Caption 99 of 195 <img alt="A ground-based telescope&amp;#39;s view of the Large Magellanic Cloud, a neighboring galaxy of our Milky Way. -
Spatially Resolved Star Formation Image and the Ultraluminous X-Ray Source Population in Ngc 2207/Ic 2163
SPATIALLY RESOLVED STAR FORMATION IMAGE AND THE ULTRALUMINOUS X-RAY SOURCE POPULATION IN NGC 2207/IC 2163 The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Mineo, S., S. Rappaport, B. Steinhorn, A. Levine, M. Gilfanov, and D. Pooley. “SPATIALLY RESOLVED STAR FORMATION IMAGE AND THE ULTRALUMINOUS X-RAY SOURCE POPULATION IN NGC 2207/IC 2163.” The Astrophysical Journal 771, no. 2 (June 25, 2013): 133. © 2013 American Astronomical Society. As Published http://dx.doi.org/10.1088/0004-637X/771/2/133 Publisher Institute of Physics/American Astronomical Society Version Final published version Citable link http://hdl.handle.net/1721.1/93903 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The Astrophysical Journal, 771:133 (12pp), 2013 July 10 doi:10.1088/0004-637X/771/2/133 C 2013. The American Astronomical Society. All rights reserved. Printed in the U.S.A. SPATIALLY RESOLVED STAR FORMATION IMAGE AND THE ULTRALUMINOUS X-RAY SOURCE POPULATION IN NGC 2207/IC 2163 S. Mineo1, S. Rappaport2,3, B. Steinhorn4, A. Levine5, M. Gilfanov6,7, and D. Pooley3 1 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street Cambridge, MA 02138, USA; [email protected] 2 37-602B, M.I.T. Department of Physics and Kavli Institute for Astrophysics and Space Research, 70 Vassar Street, Cambridge, MA 02139, USA; [email protected] 3 Eureka Scientific, 5248 Valley View Road, El Sobrante, CA 94803-3435, USA; [email protected] 4 Harvard-MIT Division of Health Sciences and Technology, Harvard Medical School, 260 Longwood Avenue, Boston, MA 02115, USA; [email protected] 5 M.I.T. -
September 2017 BRAS Newsletter
September 2017 Issue September 2017 Next Meeting: Monday, September 11th at 7PM at HRPO nd (2 Mondays, Highland Road Park Observatory) September Program: GAE (Great American. Eclipse) Membership Reports. Club members are invited to “approach the mike. ” and share their experiences travelling hither and thither to observe the August total eclipse. What's In This Issue? HRPO’s Great American Eclipse Event Summary (Page 2) President’s Message Secretary's Summary Outreach Report - FAE Light Pollution Committee Report Recent Forum Entries 20/20 Vision Campaign Messages from the HRPO Spooky Spectrum Observe The Moon Night Observing Notes – Draco The Dragon, & Mythology Like this newsletter? See past issues back to 2009 at http://brastro.org/newsletters.html Newsletter of the Baton Rouge Astronomical Society September 2017 The Great American Eclipse is now a fond memory for our Baton Rouge community. No ornery clouds or“washout”; virtually the entire three-hour duration had an unobstructed view of the Sun. Over an hour before the start of the event, we sold 196 solar viewers in thirty-five minutes. Several families and children used cereal box viewers; many, many people were here for the first time. We utilized the Coronado Solar Max II solar telescope and several nighttime telescopes, each outfitted with either a standard eyepiece or a “sun funnel”—a modified oil funnel that projects light sent through the scope tube to fabric stretched across the front of the funnel. We provided live feeds on the main floor from NASA and then, ABC News. The official count at 1089 patrons makes this the best- attended event in HRPO’s twenty years save for the historic Mars Opposition of 2003. -
A Galaxy Classification Grid That Better Recognises Early-Type Galaxy
MNRAS 000,1– ?? (2019) Preprint 24 July 2019 Compiled using MNRAS LATEX style file v3.0 A galaxy classification grid that better recognises early-type galaxy morphology Alister W. Graham? Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia. Accepted 2019 June 7. Received 2019 June 7; in original form 2019 April 26 ABSTRACT A modified galaxy classification scheme for local galaxies is presented. It builds upon the Aitken-Jeans nebula sequence, by expanding the Jeans-Hubble tuning fork diagram, which it- self contained key ingredients from Curtis and Reynolds. The two-dimensional grid of galaxy morphological types presented here, with elements from de Vaucouleurs’ three-dimensional classification volume, has an increased emphasis on the often overlooked bars and continua of disc sizes in early-type galaxies — features not fully captured by past tuning forks, tridents, or combs. The grid encompasses nuclear discs in elliptical (E) galaxies, intermediate-scale discs in ellicular (ES) galaxies, and large-scale discs in lenticular (S0) galaxies, while the E4-E7 class is made redundant given that these galaxies are lenticular galaxies. Today, these struc- tures continue to be neglected, or surprise researchers, perhaps partly due to our indoctrination to galaxy morphology through the tuning fork diagram. To better understand the current and proposed classification schemes — whose origins reside in solar/planetary formation models — a holistic overview is given. This provides due credit to some of the lesser known pioneers, presents some rationale for the grid, and reveals the incremental nature of, and some of the lesser known connections in, the field of galaxy morphology. -
ISSUE No. 12 February 2012
THE BOLTON ISSUE No. 12 ASTRONOMER February 2012 Next Meeting A BUMPER EDITION Attending a Star WITH SOME AMAZING Party IMAGES FROM BAS 7th February 2012 MEMBERS The monthly journal of the Bolton Astronomical Society In this Issue Setting up for Astro-imaging Image Processing Secrets 2 January Supernova Discoveries Part 5 by Ross Wilkinson David Ratledge DECONVOLUTION 22 Supernovae Featured Constellation Images from BAS Members DRACO ARTICLES AND OBSERVATIONS ALWAYS NEEDED FOR THE BOLTON ASTRONOMER Ross Wilkinson February Objects of Interest Crossword Number 12 BAS Calendar Carl Stone Jupiter Mike Schaffel Jupiter Have you spotted it yet? Please send magazine articles & MEETINGS: Ladybridge Community Centre Beaumont Drive Bolton BL3 4RZ contributions to the Editor Non-members invited to drop in to meetings which are held every other Tuesday evening at 7.30 p.m. £2 charge per Len Adam. meeting or £20 annual membership. [email protected] Go to http:www.boltonastro.org/calendar to find the next meeting. There are plenty of parking spaces at the centre. SETTING UP FOR ASTRO-IMAGING PART 5 ROSS WILKINSON IMAGES FROM BAS MEMBERS DavidGerald Ratledge Bramall David Ratledge David Ratledge Gerald Bramall David Ratledge Gerald Bramall Gerald Bramall David Ratledge Carl Stone M82 Len Adam 30s Exposure Just watched Stargazing Live on TV – the image of NGC 1365 from South Africa reminded me of the shape of galaxy NGC 2535 that I took the other night. It was good Carl Stone to see the clear skies at Jodrell Bank – it has been raining here in Spain since this morning!! Mars First attempt at taking Mars. -
Making a Sky Atlas
Appendix A Making a Sky Atlas Although a number of very advanced sky atlases are now available in print, none is likely to be ideal for any given task. Published atlases will probably have too few or too many guide stars, too few or too many deep-sky objects plotted in them, wrong- size charts, etc. I found that with MegaStar I could design and make, specifically for my survey, a “just right” personalized atlas. My atlas consists of 108 charts, each about twenty square degrees in size, with guide stars down to magnitude 8.9. I used only the northernmost 78 charts, since I observed the sky only down to –35°. On the charts I plotted only the objects I wanted to observe. In addition I made enlargements of small, overcrowded areas (“quad charts”) as well as separate large-scale charts for the Virgo Galaxy Cluster, the latter with guide stars down to magnitude 11.4. I put the charts in plastic sheet protectors in a three-ring binder, taking them out and plac- ing them on my telescope mount’s clipboard as needed. To find an object I would use the 35 mm finder (except in the Virgo Cluster, where I used the 60 mm as the finder) to point the ensemble of telescopes at the indicated spot among the guide stars. If the object was not seen in the 35 mm, as it usually was not, I would then look in the larger telescopes. If the object was not immediately visible even in the primary telescope – a not uncommon occur- rence due to inexact initial pointing – I would then scan around for it. -
Canvas and Cosmos: Visual Art Techniques Applied to Astronomy Data
March 14, 2017 0:27 WSPC/INSTRUCTION FILE EnglishJCanvasCos- mos International Journal of Modern Physics D c World Scientific Publishing Company Canvas and Cosmos: Visual Art Techniques Applied to Astronomy Data. JAYANNE ENGLISH∗ Department of Physics and Astronomy, University of Manitoba, Winnipeg, Manitoba, R3T 2N2, Canada. Jayanne [email protected] Received Day Month Year Revised Day Month Year Bold colour images from telescopes act as extraordinary ambassadors for research astronomers because they pique the public's curiosity. But are they snapshots docu- menting physical reality? Or are we looking at artistic spacescapes created by digitally manipulating astronomy images? This paper provides a tour of how original black and white data, from all regimes of the electromagnetic spectrum, are converted into the colour images gracing popular magazines, numerous websites, and even clothing. The history and method of the technical construction of these images is outlined. However, the paper focuses on introducing the scientific reader to visual literacy (e.g. human per- ception) and techniques from art (e.g. composition, colour theory) since these techniques can produce not only striking but politically powerful public outreach images. When cre- ated by research astronomers, the cultures of science and visual art can be balanced and the image can illuminate scientific results sufficiently strongly that the images are also used in research publications. Included are reflections on how they could feedback into astronomy research endeavours and future forms of visualization as well as on the rele- vance of outreach images to visual art. (See the colour online version, in which figures can be enlarged, at http://xxxxxxx.) Keywords: astronomy; astrophysics; public outreach; image-making; visualization; colour theory; art arXiv:1703.04183v1 [astro-ph.IM] 12 Mar 2017 PACS numbers: 1. -
M-102 (NGC-5866) Spindle Galaxy in Draco Introduction the Purpose of the Observer’S Challenge Is to Encourage the Pursuit of Visual Observing
MONTHLY OBSERVER’S CHALLENGE Las Vegas Astronomical Society Compiled by: Roger Ivester, Boiling Springs, North Carolina & Fred Rayworth, Las Vegas, Nevada With special assistance from: Rob Lambert, Las Vegas, Nevada June 2011 M-102 (NGC-5866) Spindle Galaxy in Draco Introduction The purpose of the observer’s challenge is to encourage the pursuit of visual observing. It is open to everyone that is interested, and if you are able to contribute notes, drawings, or photographs, we will be happy to include them in our monthly summary. Observing is not only a pleasure, but an art. With the main focus of amateur astronomy on astrophotography, many times people tend to forget how it was in the days before cameras, clock drives, and GOTO. Astronomy depended on what was seen through the eyepiece. Not only did it satisfy an innate curiosity, but it allowed the first astronomers to discover the beauty and the wonderment of the night sky. Before photography, all observations depended on what the astronomer saw in the eyepiece, and how they recorded their observations. This was done through notes and drawings and that is the tradition we are stressing in the observers challenge. By combining our visual observations with our drawings, and sometimes, astrophotography (from those with the equipment and talent to do so), we get a unique understanding of what it is like to look through an eyepiece, and to see what is really there. The hope is that you will read through these notes and become inspired to take more time at the eyepiece studying each object, and looking for those subtle details that you might never have noticed before. -
Messier 102 in Constellation Draco NGC 5866 (Also Called the Spindle
Messier 102 in Constellation Draco NGC 5866 (also called the Spindle Galaxy or Messier 102) is a relatively bright lenticular or spiral galaxy in the constellation Draco. NGC 5866 was most likely discovered by Pierre Méchain or Charles Messier in 1781, and independently found by William Herschel in 1788. Measured orbital velocities of its globular cluster system imply that dark matter makes up only 34±45% of the mass within 5 effective radii; a notable paucity. OBSERVATION DATA (J2000 EPOCH) Constellation Draco Right ascension 15h 06m 29.5s Declination +55° 45' 48" Redshift 0.002518±0.000017 Distance 50 ± 3 Mly (15.3 ± 0.7 Mpc) Apparent magnitude (V) 10.7 Notable features - The galaxy is viewed edge on Other designations - Spindle Galaxy, UGC 9723, PGC NGC 5866, as observed by the Hubble Space 53933 Telescope One of the most outstanding features of NGC 5866 is the extended dust disk, which is seen almost exactly edge-on. This dust disk is highly unusual for a lenticular galaxy. The dust in most lenticular galaxies is generally found only near the nucleus and generally follows the light profile of the galaxies' bulges. This dust disk may contain a ring-like structure, although the shape of this structure is difficult to determine given the edge-on orientation of the galaxy. It is also possible that the galaxy is a spiral galaxy that was misclassified as a lenticular galaxy because of its edge-on orientation, in which case the dust disk would not be too unusual. NGC 5866 is one of the brightest galaxies in the NGC 5866 Group, a small galaxy group that also includes the spiral galaxies NGC 5879 and NGC 5907. -
194 9 Ce Le B Rating 65 Ye Ars O F Br Inging As Tr on Omy T O No Rth Te X
1949 Celebrating 65 Years of Bringing Astronomy to North Texas 2014 Contact information: Inside this issue: Info Officer (General Info) – [email protected]@fortworthastro.com Website Administrator – [email protected] Postal Address: Page Fort Worth Astronomical Society Club Event Calendar 3 3812 Fenton Avenue Fort Worth, TX 76133 This Month’s Celestial Events 4 Web Site: http://www.fortworthastro.org Lunar Ephemeris 4 Facebook: http://tinyurl.com/3eutb22 Twitter: http://twitter.com/ftwastro Moon Phase Calendar 5 Yahoo! eGroup (members only): http://tinyurl.com/7qu5vkn 6 Officers (2013-2014): Mars/Venus Data Sheet President – Jim Murray, [email protected] – Jupiter Data Sheet 7 Vice President – Matt Reed, [email protected] Sec/Tres – Lewis Westerfield, [email protected] Space Place—”Saturn’s Moon 8 Board Members: Iapetus” 2012-2014 Phil Stage Cloudy Night Library 9 Bruce Cowles AL Observing Club of the Month 11 2013-2015 Bill Nichols Constellation of the Month 12 Jim Craft Constellation Mythology 13 Young Astronomer News 14 Cover Photo: 15 The Messier Catalog Credit: SEDS That’s A Fact November’s Full Moon Name 15 General Club Information 15 Observing Site Reminders: Be careful with fire, mind all local burn bans! Prior Club Meeting Minutes 16 Dark Site Usage Requirements (ALL MEMBERS): Maintain Dark-Sky Etiquette (http://tinyurl.com/75hjajy) FWAS Foto Files 17 Turn out your headlights at the gate! Sign the logbook (in camo-painted storage shed. Inside the door on the left- hand side) E d i t o r : Log club equipment problems (please contact a FWAS board member to in- form them of any problems) Shawn Kirchdorfer Put equipment back neatly when finished Last person out: FW Check all doors – secured, but NOT locked M o n t h l y Make sure nothing is left out Contributors: Matt McCullar The Fort Worth Astronomical Society (FWAS) was founded in 1949 and is a non-profit scientific Jerry Keith educational organization incorporated in the state of Texas.