SPAC Examiner with Roger W
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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. -
Feb BACK BAY 2019
Feb BACK BAY 2019 The official newsletter of the Back Bay Amateur Astronomers CONTENTS COMING UP Gamma Burst 2 Feb 7 BBAA Meeting Eclipse Collage 3 7:30-9PM TCC, Virginia Beach NSN Article 6 Heart Nebula 7 Feb 8 Silent Sky Club meeting 10 10-11PM Little Theatre of VB Winter DSOs 11 Contact info 16 Feb 8 Cornwatch Photo by Chuck Jagow Canon 60Da, various exposures, iOptron mount with an Orion 80ED Calendar 17 dusk-dawn The best 9 out of 3465 images taken from about 10:00 PM on the 20th Cornland Park through 2:20 AM on the 21st. Unprocessed images (only cropped). Feb 14 Garden Stars 7-8:30PM LOOKING UP! a message from the president Norfolk Botanical Gardens This month’s most talked about astronomy event has to be the total lunar Feb 16 Saturday Sun-day eclipse. The BBAA participated by supporting the Watch Party at the 10AM-1PM Chesapeake Planetarium. Anyone in attendance will tell you it was COLD, but Elizabeth River Park manageable if you wore layers, utilized the planetarium where Dr. Robert Hitt seemed to have the thermostat set to 100 degrees, and drank copious amounts Feb 23 Skywatch of the hot coffee that Kent Blackwell brewed in the back office. 6PM-10PM The event had a huge following on Facebook but with the cold Northwest River Park temperatures, we weren’t sure how many would come out. By Kent’s estimate there were between 100–200 people in attendance. Many club members set up telescopes, as well as a few members of the public too. -
Preliminary Catalogue of Isaac Roberts's Collection of Photographs of Celestial Objects
ASTRONOMISCHE NACHRICHTEN. Nr. 4154. Band 174. 2. Preliminary catalogue of Isaac Roberts’s collection of photographs of celestial objects. By Dorotha Isaac-Roberts. The Isaac Roberts collection of celestial photographs The number of the copies of the forthcoming paper comprises 2485 original negatives of stars, star-clusters, being very limited, the observatories and astronomers, official nebulae and other celestial objects together with many posi. or amateur, who are specially interested in photographic tives on glass and on paper, taken by the late Dr. Isaac astronomy will please send in their names to the address Roberts or, under his incessant supervision, by his assistant given below, early in 1907, in order that the various parts W. S. Franks, F. R. A. S., at Dr. Roberts’s Private Obser- of the complete catalogue may be sent to them in course vatory, Kennessee, Maghull, near Liverpool (1885-1 890) and, of time. from 1890 to 1904, at Starfield, Crowborough, Sussex. Positives- on-glass reproduced from the Isaac Roberts Of the above mentioned negatives, negatives will be lent for the purpose of micrometric mea- I) 1412 were taken with the zo-in Reflector (focal surements, if, application be made and provided that the length = 98.0 ins) and with an exposure of the plate of documents be returned after completion of the measurements. ninety minutes in general. In the preliminary catalogue given below, the numbers 2) 648 with the 5-in Cooke lens (f. 1. = 19.22 ins) of Dr. Dreyer’s New General Catalogue of Nebulae and which was mounted on the tube of the zo-in Reflector; or, Clusters of Stars and of Dr. -
Eagle Nebula Star Formation Region
Eagle Nebula Star Formation Region AST 303: Chapter 17 1 The Formation of Stars (2) • A cloud of gas and dust must collapse if stars are to be formed. • The self-gravity of the cloud will tend to cause it to collapse. • Radiation pressure from nearby hot stars may do the same. • The passage of a shock wave from a nearby supernova blast or some other source (such as galactic shock waves) may do the same. – Note: The “sonic boom” of a jet plane is an example of a shock wave. • When two clouds collide, they may cause each other to collapse. AST 303: Chapter 17 2 Trifid Nebula AST 303: Chapter 17 3 Trifid Nebula Stellar Nursery Revealed AST 303: Chapter 17 4 Young Starburst Cluster Emerges from Cloud AST 303: Chapter 17 5 The Formation of Stars (3) • The gas in the collapsing cloud probably becomes turbulent. • This would tend to fragment the collapsing gas, producing condensations that would be the nuclei of new stars. • There is abundant evidence that shows that the stars in a cluster are all about the same age. For a young cluster, many stars have not yet reached the main sequence: ! Isochron Luminosity "Temperature AST 303: Chapter 17 6 The Formation of Stars (4) • The evolutionary paths of young stars on the H-R diagram look like this. Note the T Tauri stars, long thought to be young stars. • Theory says that these stars use convection as the main method of transporting energy to their surfaces. ! T Tauri Stars Luminosity "Temperature AST 303: Chapter 17 7 The Search for Stellar Precursors • Astronomers have long been fascinated by very dark, dense regions seen outlined against bright gas, called globules. -
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 -
March 2021 PDF Newsletter
1 The Los Angeles Astronomical Society March, 2021 The Bulletin Volume 95, Issue 03 In This Issue NSN Webinar: James Webb Telescope…….Page 2 Seven Minutes of Terror ………………………..Page 3 Mars Perseverance Rover Watch Party…...Page 4 Taking The Dog Stars ……….………………..Pages 5-6 The Jellyfish Nebula - IC443 ……….…………..Page 7 The Soul Nebula - Sh2-199 ……………. …..….Page 8 The Heart Nebula—Sh2-190 ……....………….Page 9 Monthly Star Report ……………..…..………. Page 10 Almanac ………………………….…..…….………..Page 11 Calendar of Events ..…...……..……….….…...Page 12 Image credit: NASA/JPL-Caltech Meet the New Members .............…...……Page 13 The LAAS Outreach & Club Swag ..…...…..Page 14 February 18, 2021 Amazon Smiles & Astro Magazines ..…....Page 15 Members of NASA’s Mars 2020 Perseverance rover mission were jubi- Club Contacts & Social Media Link ……… .Page 16 lant on Feb. 18, 2021, after the spacecraft successfully touched down on Mars. They are in Mission Control at the Jet Propulsion Laboratory All members are encouraged to contribute arti- in Southern California. cles of interest for publication in The Bulletin. Please send your articles and images to: Learn more about the mission by following one of the links below: [email protected] mars.nasa.gov/mars2020/ nasa.gov/perseverance https://mars.nasa.gov/# New Contact Info For 2021? If you have recently moved, changed your Upcoming Virtual Club Events email address or phone number, please contact our club secretary at Board Meeting; Mar. 3, 2021 [email protected]. General Meeting; Mar. 8, 2021 2 NSN Webinar Series: What to Expect from the James Webb Space Telescope Join the NASA Night Sky Network on Tuesday, March 23 at 6pm Pacific (9pm Eastern) to hear Dr. -
Stars and Their Purpose
Stars & Their Purpose.indd 3 8/17/06 8:19:54 AM First Master Books printing: August 2006 Copyright © 2006 by Werner Gitt. All rights reserved. No part of this book may be used or reproduced in any manner whatsoever without written permission of the publisher except in the case of brief quotations in articles and reviews. For information write: Master Books, P.O. Box 726, Green Forest, AR 72638. ISBN-13: 978-0-89051-482-5 ISBN-10: 0-89051-482-8 Library of Congress Number: 2006929548 Cover by Bryan Miller Unless otherwise noted, all Scripture is from the New International Version of the Bible. References to apocryphal books have been taken from The Jerusalem Bible (London: Darton, Longman & Todd, 1966 edition). Printed in the United States of America. Please visit our website for other great titles: www.masterbooks.net. For information regarding author interviews, please contact the publicity department at (870) 528-5288. Stars & Their Purpose.indd 4 8/17/06 8:19:54 AM INDEX Preface............................................................................. 7 Preface to the English Edition ....................................... 13 Introduction.................................................................. 15 1. Can the Stars Be Counted?............................................ 17 2. In What Respects Do the Stars Differ?........................... 27 3. How Big Is the Universe? .............................................. 39 4. Four Characteristics of Space......................................... 43 5. Why Were the Stars Created? ........................................ 49 5.1 The Stars Were Made to Shine on Earth................. 50 5.2 The Stars Were Made to Determine Times and Seasons ................................................. 53 6. How Do the Stars Transmit Their Messages? ................. 57 6.1 Their Messages Are Silent....................................... 57 6.2 God’s Message Can Be Understood by Anybody ... -
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 -
Open Clusters
Open Clusters Open clusters (also known as galactic clusters) are of tremendous importance to the science of astronomy, if not to astrophysics and cosmology generally. Star clusters serve as the "laboratories" of astronomy, with stars now all at nearly the same distance and all created at essentially the same time. Each cluster thus is a running experiment, where we can observe the effects of composition, age, and environment. We are hobbled by seeing only a snapshot in time of each cluster, but taken collectively we can understand their evolution, and that of their included stars. These clusters are also important tracers of the Milky Way and other parent galaxies. They help us to understand their current structure and derive theories of the creation and evolution of galaxies. Just as importantly, starting from just the Hyades and the Pleiades, and then going to more distance clusters, open clusters serve to define the distance scale of the Milky Way, and from there all other galaxies and the entire universe. However, there is far more to the study of star clusters than that. Anyone who has looked at a cluster through a telescope or binoculars has realized that these are objects of immense beauty and symmetry. Whether a cluster like the Pleiades seen with delicate beauty with the unaided eye or in a small telescope or binoculars, or a cluster like NGC 7789 whose thousands of stars are seen with overpowering wonder in a large telescope, open clusters can only bring awe and amazement to the viewer. These sights are available to all. -
Atlas Menor Was Objects to Slowly Change Over Time
C h a r t Atlas Charts s O b by j Objects e c t Constellation s Objects by Number 64 Objects by Type 71 Objects by Name 76 Messier Objects 78 Caldwell Objects 81 Orion & Stars by Name 84 Lepus, circa , Brightest Stars 86 1720 , Closest Stars 87 Mythology 88 Bimonthly Sky Charts 92 Meteor Showers 105 Sun, Moon and Planets 106 Observing Considerations 113 Expanded Glossary 115 Th e 88 Constellations, plus 126 Chart Reference BACK PAGE Introduction he night sky was charted by western civilization a few thou - N 1,370 deep sky objects and 360 double stars (two stars—one sands years ago to bring order to the random splatter of stars, often orbits the other) plotted with observing information for T and in the hopes, as a piece of the puzzle, to help “understand” every object. the forces of nature. The stars and their constellations were imbued with N Inclusion of many “famous” celestial objects, even though the beliefs of those times, which have become mythology. they are beyond the reach of a 6 to 8-inch diameter telescope. The oldest known celestial atlas is in the book, Almagest , by N Expanded glossary to define and/or explain terms and Claudius Ptolemy, a Greco-Egyptian with Roman citizenship who lived concepts. in Alexandria from 90 to 160 AD. The Almagest is the earliest surviving astronomical treatise—a 600-page tome. The star charts are in tabular N Black stars on a white background, a preferred format for star form, by constellation, and the locations of the stars are described by charts. -
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 -
Just What Are Those Sky Chart "M" and "NGC" Numbers? by Barry D
Just what are those Sky Chart "M" and "NGC" Numbers? By Barry D. Malpas – Special to the Williams-Grand Canyon News – 2014 November One of the pastimes for some early sky observers was to locate new comets. Charles Messier (1730-1817) was a French comet hunter during the late 1700s, and discovered 13 new comets between 1760 and 1785. His interest in astronomy, and comets in particular, was influenced by seeing the great comet of 1744, and the comet of 1759 (of which Edmond Halley had believed the comets of 1531, 1607, and 1682 were the same and had predicted the comet’s 1759 apparition which is now known as Halley's Comet.) At this time telescopes were relatively small. The understanding of supernovae, or galaxies, was not yet in the current knowledge, as such objects only appeared as blurry smudges that did not move across the sky. In order not to waste time and become frustrated with viewing fuzzy objects that resembled, but were not, comets, Messier compiled a list of 110 of these celestial blurs which we now refer to as Messier, or "M Objects." The Messier Catalog has become a very popular list of "Deep Sky Objects" among amateur astronomers around the world because it consists of most of the galaxies, nebulae and star clusters easily observable with binoculars or small telescopes in the northern skies. Now, however, the objects in the list are the source of interest, as opposed to the reason the compilation was originally intended by Messier. At large astronomical get-togethers, known as "star parties", there is often a "Messier Marathon" competition to view the most Messier Objects during one observing night.