February 2019 These Pages Are Intended to Help You Find Your Way Around the Sky
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Meeting Announcement Upcoming Star Parties And
CVAS Executive Committee Pres – Bruce Horrocks Night Sky Network Coordinator – [email protected] Garrett Smith – [email protected] Vice Pres- James Somers Past President – Dell Vance (435) 938-8328 [email protected] [email protected] Treasurer- Janice Bradshaw Public Relations – Lyle Johnson - [email protected] [email protected] Secretary – Wendell Waters (435) 213-9230 Webmaster, Librarian – Tom Westre [email protected] [email protected] Vol. 7 Number 6 February 2020 www.cvas-utahskies.org The President’s Corner Meeting Announcement By Bruce Horrocks – CVAS President Our next meeting will be held on Wed. I don’t know about most of you, but I for February 26th at 7 pm in the Lake Bonneville Room one would be glad to at least see a bit of sun and of the Logan City Library. Our presenter will be clear skies at least once this winter. I believe there Wendell Waters, and his presentation is called was just a couple of nights in the last 2 months that “Charles Messier and the ‘Not-Comet’ Catalogue”. I was able to get out and do some observing and so I The meeting is free and open to the public. am hoping to see some clear skies this spring. I Light refreshments will be served. COME AND have watched all the documentaries I can stand on JOIN US!! Netflix, so I am running out of other nighttime activities to do and I really want to get out and test my new little 72mm telescope. Upcoming Star Parties and CVAS Events We made a change to our club fees at our last meeting and if you happened to have missed We have four STEM Nights coming up in that I will just quickly explain it to you now. -
Messier Objects
Messier Objects From the Stocker Astroscience Center at Florida International University Miami Florida The Messier Project Main contributors: • Daniel Puentes • Steven Revesz • Bobby Martinez Charles Messier • Gabriel Salazar • Riya Gandhi • Dr. James Webb – Director, Stocker Astroscience center • All images reduced and combined using MIRA image processing software. (Mirametrics) What are Messier Objects? • Messier objects are a list of astronomical sources compiled by Charles Messier, an 18th and early 19th century astronomer. He created a list of distracting objects to avoid while comet hunting. This list now contains over 110 objects, many of which are the most famous astronomical bodies known. The list contains planetary nebula, star clusters, and other galaxies. - Bobby Martinez The Telescope The telescope used to take these images is an Astronomical Consultants and Equipment (ACE) 24- inch (0.61-meter) Ritchey-Chretien reflecting telescope. It has a focal ratio of F6.2 and is supported on a structure independent of the building that houses it. It is equipped with a Finger Lakes 1kx1k CCD camera cooled to -30o C at the Cassegrain focus. It is equipped with dual filter wheels, the first containing UBVRI scientific filters and the second RGBL color filters. Messier 1 Found 6,500 light years away in the constellation of Taurus, the Crab Nebula (known as M1) is a supernova remnant. The original supernova that formed the crab nebula was observed by Chinese, Japanese and Arab astronomers in 1054 AD as an incredibly bright “Guest star” which was visible for over twenty-two months. The supernova that produced the Crab Nebula is thought to have been an evolved star roughly ten times more massive than the Sun. -
Guide Du Ciel Profond
Guide du ciel profond Olivier PETIT 8 mai 2004 2 Introduction hjjdfhgf ghjfghfd fg hdfjgdf gfdhfdk dfkgfd fghfkg fdkg fhdkg fkg kfghfhk Table des mati`eres I Objets par constellation 21 1 Androm`ede (And) Andromeda 23 1.1 Messier 31 (La grande Galaxie d'Androm`ede) . 25 1.2 Messier 32 . 27 1.3 Messier 110 . 29 1.4 NGC 404 . 31 1.5 NGC 752 . 33 1.6 NGC 891 . 35 1.7 NGC 7640 . 37 1.8 NGC 7662 (La boule de neige bleue) . 39 2 La Machine pneumatique (Ant) Antlia 41 2.1 NGC 2997 . 43 3 le Verseau (Aqr) Aquarius 45 3.1 Messier 2 . 47 3.2 Messier 72 . 49 3.3 Messier 73 . 51 3.4 NGC 7009 (La n¶ebuleuse Saturne) . 53 3.5 NGC 7293 (La n¶ebuleuse de l'h¶elice) . 56 3.6 NGC 7492 . 58 3.7 NGC 7606 . 60 3.8 Cederblad 211 (N¶ebuleuse de R Aquarii) . 62 4 l'Aigle (Aql) Aquila 63 4.1 NGC 6709 . 65 4.2 NGC 6741 . 67 4.3 NGC 6751 (La n¶ebuleuse de l’œil flou) . 69 4.4 NGC 6760 . 71 4.5 NGC 6781 (Le nid de l'Aigle ) . 73 TABLE DES MATIERES` 5 4.6 NGC 6790 . 75 4.7 NGC 6804 . 77 4.8 Barnard 142-143 (La tani`ere noire) . 79 5 le B¶elier (Ari) Aries 81 5.1 NGC 772 . 83 6 le Cocher (Aur) Auriga 85 6.1 Messier 36 . 87 6.2 Messier 37 . 89 6.3 Messier 38 . -
Injunction Sought to Delay J.C. Penney
Injunction sought to delay J.C. Penney and meaningful consideration of en the town’s Economic Development original complaint but not in the By Scot French Manchester law firm of Beck & new,” since it has been part of the vironmental factors.” Commission, said this morning he complaint for a new trial. He Herald Reporter Pagano, said the coalition has coalition’s plans for several years. ’The environmentalists, organized The justices ruled that the lower had not yet seen a copy of the injunc speculated that the motion was filed already proved that the lack of a tion motion and therefore could not to correct that oversight. A Manchester enviromnmeiital mass transit system to serve the by local pharmacist Michael court had followed improper Dworkin, won a major victory last procedures in rejecting the en comment. The J.C. Penney vvarehouse, a coalition fighting for a mass transit site will dangerously increase air regional distribution center for system to serve the Buckiand In- May when the state Supreme Court vironmentalists case and ordered a Bourke G. Spellacy, an attorney pollution in the area. who has represented J.C. Penney catalogue sales in the northeast, dustriai Park has formally asked He said the injunction is the “only struck down a lower court ruling new trial. against the coalition and ordered a since the originai suit was filed in began accepting applications for 1,- the courts to block the J.C. Penney relief avaiiable” while the coalition I’AGANO SAID PROCEDURAL 500 full-time jobs last month. warehouse from opening this fall. new trial. -
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). -
March 2021 These Pages Are Intended to Help You Find Your Way Around the Sky
WHAT'S UP THIS MONTH – MARCH 2021 THESE PAGES ARE INTENDED TO HELP YOU FIND YOUR WAY AROUND THE SKY The chart above shows the whole night sky as it appears on 15th March at 21:00 (9 o’clock) Greenwich Mean Time (GMT). As the Earth orbits the Sun and we look out into space each night the stars will appear to have moved across the sky by a small amount. Every month Earth moves one twelfth of its circuit around the Sun, this amounts to 30 degrees each month. There are about 30 days in each month so each night the stars appear to move about 1 degree. The sky will therefore appear the same as shown on the chart above at 8 o’clock GMT at the beginning of the month and at 10 o’clock GMT at the end of the month. The stars also appear to move 15º (360º divided by 24) each hour from east to west, due to the Earth rotating once every 24 hours. The centre of the chart will be the position in the sky directly overhead, called the Zenith. First we need to find some familiar objects so we can get our bearings. The Pole Star Polaris can be easily found by first finding the familiar shape of the Great Bear ‘Ursa Major’ that is also sometimes called the Plough or even the Big Dipper by the Americans. Ursa Major is visible throughout the year from Britain and is always quite easy to find. This month it is high in the North East. -
OBSERVING BASICS by GUY MACKIE
OBSERVING BASICS by GUY MACKIE Observing Reports The colorful and detailed photographs we see of celestial objects are not at all like the ubiquitous "fuzzy blobs" we see at the eyepiece. Nevertheless, you are freezing your buns off and loosing much needed sleep for work, the next day so why not make a description of your observations that will make the hunt worthwhile. Here are some suggestions to fill the empty spaces in your logbook and to imprint the observing experience more deeply in your memory. The Basics Your website www.m51.ca has a downloadable log sheet template that is just super, but you can also make up one for yourself or customize the website version to your own needs. The main things to start your report should be the circumstances under which you observed: Observing Location Time (of observing session and of the observation of each object) Optics (type of instrument, eyepiece, filters, power of magnification) Transparency (page 56 of the Observers Handbook) Seeing (for me this is a subjective rating of the atmospheric stability based on Planet features and double star observations) It is good to know the field of view (FOV) of each of your eyepieces in minutes of degree, then you can estimate the approximate size of the object. The sketchpad I use has the FOV for every eyepiece I use taped to the back, a handy reference. To calculate your field of view there are websites that will punch out the both the magnification and the FOV for most eyepieces. You can do it yourself: With any motor drives turned off, place a star near the celestial equator just outside the field of view in the eyepiece so that it will drift across the middle of the field of view. -
Core-Collapse Supernovae Overview with Swift Collaboration
Publications Spring 2015 Core-Collapse Supernovae Overview with Swift Collaboration Kiranjyot Gill Embry-Riddle Aeronautical University, [email protected] Michele Zanolin Embry-Riddle Aeronautical University, [email protected] Marek Szczepańczyk Embry-Riddle Aeronautical University, [email protected] Follow this and additional works at: https://commons.erau.edu/publication Part of the Astrophysics and Astronomy Commons, and the Physics Commons Scholarly Commons Citation Gill, K., Zanolin, M., & Szczepańczyk, M. (2015). Core-Collapse Supernovae Overview with Swift Collaboration. , (). Retrieved from https://commons.erau.edu/publication/3 This Report is brought to you for free and open access by Scholarly Commons. It has been accepted for inclusion in Publications by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. Core-Collapse Supernovae Overview with Swift Collaboration∗ Kiranjyot Gill,y Dr. Michele Zanolin,z and Marek Szczepanczykx Physics Department, Embry Riddle Aeronautical University (Dated: June 30, 2015) The Core-Collapse supernovae (CCSNe) mark the dynamic and explosive end of the lives of massive stars. The mysterious mechanism, primarily focused with the shock revival phase, behind CCSNe explosions could be explained by detecting the corresponding gravitational wave (GW) emissions by the laser interferometer gravitational wave observatory, LIGO. GWs are extremely hard to detect because they are weak signals in a floor of instrument noise. Optical observations of CCSNe are already used in coincidence with LIGO data, as a hint of the times where to search for the emission of GWs. More of these hints would be very helpful. For the first time in history a Harvard group has observed X-ray transients in coincidence with optical CCSNe. -
Rules & Requirements for an SBAS Observing Certificate 1. You Must
Rules & Requirements for an SBAS Observing Certificate 1. You must be a member of the SBAS in good standing to receive a certificate. 2. No Go To or Push To aided attempts will be accepted. Reading charts and star hopping are essential skills in our hobby. (You may use these methods to confirm your findings.) 3. Honor system is in full effect. These lists benefit your knowledge of the sky. Cheating only cheats yourself and the SBAS membership. Observations will be verified against digital planetarium charts. You may be required to answer questions about the objects you observed to verify your work. You may also be asked to show one of these objects at a star party. Once a list is completed, it is assumed you are familiar with every object on that list to the point where you can find it again and describe it to another person. 4. Upon completion of a list, submit the original paper version in person to Coy Wagoner at an SBAS meeting, public star party, or informal observing at the Worley. No digital submissions will be accepted at this time. 5. No observations may overlap. If one object is on two lists, your observations must be done on separate dates/times for credit. Copies of your observing logs will be saved and later compared to additional lists to make sure nothing overlaps. No observations prior to January 1, 2015 will be accepted for credit. 6. Observations should be done on your own. If you observe an object in someone else’s telescope or binoculars, the observation does not count unless you did the work to find it. -
A Guide to Smartphone Astrophotography National Aeronautics and Space Administration
National Aeronautics and Space Administration A Guide to Smartphone Astrophotography National Aeronautics and Space Administration A Guide to Smartphone Astrophotography A Guide to Smartphone Astrophotography Dr. Sten Odenwald NASA Space Science Education Consortium Goddard Space Flight Center Greenbelt, Maryland Cover designs and editing by Abbey Interrante Cover illustrations Front: Aurora (Elizabeth Macdonald), moon (Spencer Collins), star trails (Donald Noor), Orion nebula (Christian Harris), solar eclipse (Christopher Jones), Milky Way (Shun-Chia Yang), satellite streaks (Stanislav Kaniansky),sunspot (Michael Seeboerger-Weichselbaum),sun dogs (Billy Heather). Back: Milky Way (Gabriel Clark) Two front cover designs are provided with this book. To conserve toner, begin document printing with the second cover. This product is supported by NASA under cooperative agreement number NNH15ZDA004C. [1] Table of Contents Introduction.................................................................................................................................................... 5 How to use this book ..................................................................................................................................... 9 1.0 Light Pollution ....................................................................................................................................... 12 2.0 Cameras ................................................................................................................................................ -
MESSIER 15 RA(2000) : 21H 29M 58S DEC(2000): +12° 10'
MESSIER 15 RA(2000) : 21h 29m 58s DEC(2000): +12° 10’ 01” BASIC INFORMATION OBJECT TYPE: Globular Cluster CONSTELLATION: Pegasus BEST VIEW: Late October DISCOVERY: Jean-Dominique Maraldi, 1746 DISTANCE: 33,600 ly DIAMETER: 175 ly APPARENT MAGNITUDE: +6.2 APPARENT DIMENSIONS: 18’ FOV:Starry 1.00Night FOV: 60.00 Vulpecula Sagitta Pegasus NGC 7009 (THE SATURN NEBULA) Delphinus NGC 7009 RA(2000) : 21h 04m 10.8s DEC(2000): -11° 21’ 48.6” Equuleus Pisces Aquila NGC 7009 FOV: 5.00 Aquarius Telrad Capricornus Sagittarius Cetus Piscis Austrinus NGC 7009 Microscopium BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Aquarius Sculptor BEST VIEW: Early November DISCOVERY: William Herschel, 1782 DISTANCE: 2000 - 4000 ly DIAMETER: 0.4 - 0.8 ly Grus APPARENT MAGNITUDE: +8.0 APPARENT DIMENSIONS: 41” x 35” Telescopium Telrad Indus NGC 7662 (THE BLUE SNOWBALL) RA(2000) : 23h 25m 53.6s DEC(2000): +42° 32’ 06” BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Andromeda BEST VIEW: Late November DISCOVERY: William Herschel, 1784 DISTANCE: 1800 – 6400 ly DIAMETER: 0.3 – 1.1 ly APPARENT MAGNITUDE: +8.6 APPARENT DIMENSIONS: 37” MESSIER 52 RA(2000) : 23h 24m 48s DEC(2000): +61° 35’ 36” BASIC INFORMATION OBJECT TYPE: Open Cluster CONSTELLATION: Cassiopeia BEST VIEW: December DISCOVERY: Charles Messier, 1774 DISTANCE: ~5000 ly DIAMETER: 19 ly APPARENT MAGNITUDE: +7.3 APPARENT DIMENSIONS: 13’ AGE: 50 million years FOV:Starry 1.00Night FOV: 60.00 Auriga Cepheus Andromeda MESSIER 31 (THE ANDROMEDA GALAXY) M 31 RA(2000) : 00h 42m 44.3Cassiopeias DEC(2000): +41° 16’ 07.5” Perseus Lacerta AndromedaM 31 FOV: 5.00 Telrad Triangulum Taurus Orion Aries Andromeda M 31 Pegasus Pisces BASIC INFORMATION OBJECT TYPE: Galaxy CONSTELLATION: Andromeda Telrad BEST VIEW: December DISCOVERY: Abd al-Rahman al-Sufi, 964 Eridanus CetusDISTANCE: 2.5 million ly DIAMETER: ~250,000 ly* APPARENT MAGNITUDE: +3.4 APPARENT DIMENSIONS: 178’ x 63’ (3° x 1°) *This value represents the total diameter of the disk, based on multi-wavelength measurements. -
The Messier Catalog
The Messier Catalog Messier 1 Messier 2 Messier 3 Messier 4 Messier 5 Crab Nebula globular cluster globular cluster globular cluster globular cluster Messier 6 Messier 7 Messier 8 Messier 9 Messier 10 open cluster open cluster Lagoon Nebula globular cluster globular cluster Butterfly Cluster Ptolemy's Cluster Messier 11 Messier 12 Messier 13 Messier 14 Messier 15 Wild Duck Cluster globular cluster Hercules glob luster globular cluster globular cluster Messier 16 Messier 17 Messier 18 Messier 19 Messier 20 Eagle Nebula The Omega, Swan, open cluster globular cluster Trifid Nebula or Horseshoe Nebula Messier 21 Messier 22 Messier 23 Messier 24 Messier 25 open cluster globular cluster open cluster Milky Way Patch open cluster Messier 26 Messier 27 Messier 28 Messier 29 Messier 30 open cluster Dumbbell Nebula globular cluster open cluster globular cluster Messier 31 Messier 32 Messier 33 Messier 34 Messier 35 Andromeda dwarf Andromeda Galaxy Triangulum Galaxy open cluster open cluster elliptical galaxy Messier 36 Messier 37 Messier 38 Messier 39 Messier 40 open cluster open cluster open cluster open cluster double star Winecke 4 Messier 41 Messier 42/43 Messier 44 Messier 45 Messier 46 open cluster Orion Nebula Praesepe Pleiades open cluster Beehive Cluster Suburu Messier 47 Messier 48 Messier 49 Messier 50 Messier 51 open cluster open cluster elliptical galaxy open cluster Whirlpool Galaxy Messier 52 Messier 53 Messier 54 Messier 55 Messier 56 open cluster globular cluster globular cluster globular cluster globular cluster Messier 57 Messier