Cassiopeia a (Cas A) Is a Relatively Young HOW: the Supernova That Created Cas a Is Supernova Remnant in the Milky Way Galaxy

Total Page:16

File Type:pdf, Size:1020Kb

Cassiopeia a (Cas A) Is a Relatively Young HOW: the Supernova That Created Cas a Is Supernova Remnant in the Milky Way Galaxy CA S S I O P E I A A WHO: Cassiopeia A (Cas A) is a relatively young HOW: The supernova that created Cas A is supernova remnant in the Milky Way galaxy. thought to have occurred when a star about 25 times as massive as the Sun ran out of fuel for WHAT: A supernova remnant is the expanding nuclear power. Its core then collapsed to form an debris field of hot gas and energetic particles cre- ultra-dense object called a neutron star, and the ated when a massive star explodes. outer layers of the star were ejected at enormous speeds (see illustration below). WHERE: Cas A, at a distance of 11,000 light years from Earth, is in the constellation Cassiopeia. This WHY: Supernovas occur about once every 50 years constellation is widely known for its “W” shape in the Galaxy when stars much more massive than that Greek and Roman mythology identified as a our Sun die. They energize their surroundings and queen’s throne. disperse the heavy elements (e.g., green & blue in the image) forged within these stellar interiors. WHEN: Although the exact date is uncertain, this Supernova remnants reveal information about the supernova would have appeared in the night sky grand Galactic drama of life, death and renewal. about 330 years ago. More at: http://chandra.harvard.edu X-RAYS FROM opTICAl dATA InfRAREd EMISSIon NASA’S CHANDRA fRoM nASA’S HubblE FROM NASA’S SpITzER Stellar ILLUSTRATION OF STELLAR EVOLUTION PATH Stellar Nursery Nursery Neutron Star Protostar Blue Supergiant Red Giant Blue Giant Type II Supernova ConSTEllATIon CASSIopEIA .
Recommended publications
  • Cassiopeia A: on the Origin of the Hard X-Ray Continuum and the Implication of the Observed O Vııı Ly-Α/Ly-Β Distribution
    A&A 365, L225–L230 (2001) Astronomy DOI: 10.1051/0004-6361:20000048 & c ESO 2001 Astrophysics Cassiopeia A: On the origin of the hard X-ray continuum and the implication of the observed O vııı Ly-α/Ly-β distribution J. A. M. Bleeker1, R. Willingale2, K. van der Heyden1, K. Dennerl3,J.S.Kaastra1, B. Aschenbach3, and J. Vink4,5,6 1 SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands 2 Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK 3 Max-Planck-Institut f¨ur extraterrestrische Physik, Giessenbachstraße, 85740 Garching, Germany 4 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany 5 Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA 6 Chandra Fellow Received 6 October 2000 / Accepted 24 October 2000 Abstract. We present the first results on the hard X-ray continuum image (up to 15 keV) of the supernova remnant Cas A measured with the EPIC cameras onboard XMM-Newton. The data indicate that the hard X-ray tail, observed previously, that extends to energies above 100 keV does not originate in localised regions, like the bright X-ray knots and filaments or the primary blast wave, but is spread over the whole remnant with a rather flat hardness ratio of the 8–10 and 10–15 keV energy bands. This result does not support an interpretation of the hard X-radiation as synchrotron emission produced in the primary shock, in which case a limb brightened shell of hard X-ray emission close to the primary shock front is expected.
    [Show full text]
  • Events: General Meeting : No General Meeting This Month
    The monthly newsletter of the Temecula Valley Astronomers July 2016 Events: General Meeting : No general meeting this month. Join us for our annual Anza Star-B-Q. Watch your email for details. For the latest on Star Parties, check the web page. Juno spacecraft and its science instruments. Image credit: NASA/JPL General information: Subscription to the TVA is included in the annual $25 WHAT’S INSIDE THIS MONTH: membership (regular members) donation ($9 student; $35 family). Cosmic Comments by President Mark Baker President: Mark Baker 951-691-0101 Looking Up <[email protected]> Vice President: Chuck Dyson <[email protected]> by Curtis Croulet Past President: John Garrett <[email protected]> Random thoughts Treasurer: Curtis Croulet <[email protected]> by Chuck Dyson Secretary: Deborah Cheong <[email protected]> Hubble's bubble lights up the Club Librarian: Bob Leffler <[email protected]> interstellar rubble Facebook: Tim Deardorff <[email protected]> Star Party Coordinator and Outreach: Deborah Cheong by Ethan Siegel <[email protected]> Send newsletter submissions to Mark DiVecchio Address renewals or other correspondence to: <[email protected]> by the 20th of the month for Temecula Valley Astronomers the next month's issue. PO Box 1292 Murrieta, CA 92564 Like us on Facebook Member’s Mailing List: [email protected] Website: http://www.temeculavalleyastronomers.com/ Page 1 of 10 The monthly newsletter of the Temecula Valley Astronomers July 2016 Cosmic Comments – July/2016 by President Mark Baker As some of you may notice, I will often despair at the current state of the US Space program, to the point of disparagement.
    [Show full text]
  • A Csillagképek Története És Látnivalói, 2019. Március 13
    Az északi pólus környéke 2. A csillagképek története és látnivalói, 2019. március 13. Sárkány • Latin: Draco, birtokos: Draconis, rövidítés: Dra • Méretbeli rangsor: 8. (1083°2, a teljes égbolt 2,63%-a) 2m 3m 4m 5m 6m • Eredet: görög (Δράκων (Drakón)) 1 5 10 57 144 Cefeusz Kis Medve Kultúrtörténet Görögök: kígyó (korábban) v. sárkány • ő Ladón, a Heszperiszek Kertjének őre: itt található Héra nászajándéka, egy örök ifjúságot és halhatatlanságot adó aranyalmákat érlelő fa • Héraklész 10+1-edik feladatként ellopott három almát • vagy ő maga, mérgezett nyilakkal elpusztítva Ladónt • vagy megkérte erre Atlaszt, és addig tartotta helyette az eget Héraklész rálép a sárkány • Héra emlékül az égre helyezte fejére (Dürer) Arabok • a sárkányfej-négyszöget (, , , ) 4 anyatevének látták • akik egy teveborjút védelmeznek (?) • mert azt két hiéna (, ) támadja • a tevék gazdái (, , ) a közelben táboroznak Kína • a Központi Palotát közrefogó két „fal” nagy része itt futott • Csillagok: semmi nagyon extra • Az É-i ekliptikai pólus ide esik • Az É-i pólus -3000 környékén az Dra (Thuban) közelébe esett • Mélyég: Macskaszem-köd (NGC 6543): planetáris köd: haldokló óriáscsillag által ledobott anyagfelhő A Kéfeusz-Kassziopeia-Androméda • Kéfeusz Etiópia királya, Zeusz leszármazottja (egyik szeretője, Io jóvoltából) mondakör • felesége, Kassziopeia annyira hiú volt a saját vagy a lánya szépségére („szebb, mint a nereidák”), hogy Poszeidón egy tengeri szörnyet (Cet) küldött büntetésből a királyság pusztítására • hogy elhárítsák a veszedelmet, egy jós tanácsára
    [Show full text]
  • Blasts from the Past Historic Supernovas
    BLASTS from the PAST: Historic Supernovas 185 386 393 1006 1054 1181 1572 1604 1680 RCW 86 G11.2-0.3 G347.3-0.5 SN 1006 Crab Nebula 3C58 Tycho’s SNR Kepler’s SNR Cassiopeia A Historical Observers: Chinese Historical Observers: Chinese Historical Observers: Chinese Historical Observers: Chinese, Japanese, Historical Observers: Chinese, Japanese, Historical Observers: Chinese, Japanese Historical Observers: European, Chinese, Korean Historical Observers: European, Chinese, Korean Historical Observers: European? Arabic, European Arabic, Native American? Likelihood of Identification: Possible Likelihood of Identification: Probable Likelihood of Identification: Possible Likelihood of Identification: Possible Likelihood of Identification: Definite Likelihood of Identification: Definite Likelihood of Identification: Possible Likelihood of Identification: Definite Likelihood of Identification: Definite Distance Estimate: 8,200 light years Distance Estimate: 16,000 light years Distance Estimate: 3,000 light years Distance Estimate: 10,000 light years Distance Estimate: 7,500 light years Distance Estimate: 13,000 light years Distance Estimate: 10,000 light years Distance Estimate: 7,000 light years Distance Estimate: 6,000 light years Type: Core collapse of massive star Type: Core collapse of massive star Type: Core collapse of massive star? Type: Core collapse of massive star Type: Thermonuclear explosion of white dwarf Type: Thermonuclear explosion of white dwarf? Type: Core collapse of massive star Type: Thermonuclear explosion of white dwarf Type: Core collapse of massive star NASA’s ChANdrA X-rAy ObServAtOry historic supernovas chandra x-ray observatory Every 50 years or so, a star in our Since supernovas are relatively rare events in the Milky historic supernovas that occurred in our galaxy. Eight of the trine of the incorruptibility of the stars, and set the stage for observed around 1671 AD.
    [Show full text]
  • Jul 2016 Ephemeris
    JULY 2016 UPCOMING EVENTS Wednesday, July 6 - Regular PAC meeting @ 6:30 PM in Rm 107, Bldg 74, Embry-Riddle Aeronautical University. Club member Marilyn Unruh will present on ‘Star Hopping’, describing how to navigate through the sky and find objects without a GOTO telescope/mount. In addition, if time allows, there will be an open discussion about happenings and experiences at the recent Grand Canyon Star Party. Wednesday, July 13 - METASIG @ 5:00 PM at a local restaurant. Sign up at meeting on July 6. Wednesday, July 20 - Board Meeting @ 6:30 PM. Tuesday, July 26 - Friendly Pines @ 8:15 PM star party for children with heart disease. Sign up at meeting on July 6. OBSERVING MINI-MARATHONS The first mini-marathon, focusing on double stars and scheduled for July, has been postponed until September when weather will be cooler and the event can start earlier in the evening. The event would be held at Jeff Stillman's home in Chino Valley, pending organizing and agreement of interested individuals. Details will be described and discussed at the July 6 general club meeting. ASTRONOMICAL LEAGUE OBSERVING AWARDS PAC member Rob Esson has become the 281st to be awarded for completing the Astronomical League’s Globular Cluster Observing Program. 1 HUBBLE'S BUBBLE LIGHTS UP THE INTERSTELLAR RUBBLE By Ethan Siegel When isolated stars like our Sun reach the end of their lives, they're expected to blow off their outer layers in a roughly spherical configuration: a planetary nebula. But the most spectacular bubbles don't come from gas-and-plasma getting expelled into otherwise empty space, but from young, hot stars whose radiation pushes against the gaseous nebulae in which they were born.
    [Show full text]
  • Today's Topics A. Supernova Remnants. B. Neutron Stars. C
    Today’s Topics Wednesday, November 3, 2020 (Week 11, lecture 31) – Chapter 23. A. Supernova remnants. B. Neutron stars. C. Pulsars. Cassiopeia A: Supernova Remnant Supernova in the late 1600’s Cassiopeia A supernova remnant (type II) False color composite image from Hubble (optical = gold), Spitzer (IR = red),and Chandra (X-ray = green & blue) [source: Wikipedia, Oliver Krause (Steward Observatory) and co-workers] Cassiopeia A: Supernova Remnant neutron star Cassiopeia A supernova remnant (type II) False color composite image from Hubble (optical = gold), Spitzer (IR = red),and Chandra (X-ray = green & blue) [source: Wikipedia, Oliver Krause (Steward Observatory) and co-workers] Cassiopeia A: Supernova Remnant neutron star 10 light years Cassiopeia A supernova remnant (type II) False color composite image from Hubble (optical = gold), Spitzer (IR = red),and Chandra (X-ray = green & blue) [source: Wikipedia, Oliver Krause (Steward Observatory) and co-workers] Crab Nebula: Supernova Remnant Supernova in 1054 AD (type II) constellation: Taurus [NASA/ESA/Hubble, 1999-2000] Crab Nebula: Supernova Remnant Supernova in 1054 AD (type II) constellation: Taurus 11 light years [NASA/ESA/Hubble, 1999-2000] Tycho’s Supernova Remnant SN 1572 (type I = white dwarf + red giant binary explosion) Constellation: Cassiopeia Composite image: blue = hard x-rays, red = soft x-rays, background stars = optical [NASA/Chandra (2009)] Tycho’s Supernova Remnant SN 1572 (type I = white dwarf + red giant binary explosion) Constellation: Cassiopeia 10 light years Composite image: blue = hard x-rays, red = soft x-rays, background stars = optical [NASA/Chandra (2009)] Where do heavy elements come from ? ▪ Supernovae are a major source of heavy elements ▪ Most of the iron core of a massive star is “dissolves” into protons in the core collapse.
    [Show full text]
  • Observer Report 5 Telescope for Sale 6 July 2016 “Quick and Easy Observing Pad”, by John Land 7 Iota Meeting Announcement by Byron Labadie 8
    INSIDE THIS ISSUE: ASTRONOMY CLUB OF TULSA CALENDAR & EVENTS 2 PRESIDENT’S MESSAGE 3 TREASURER’S AND MEMBERSHIP OBSERVER REPORT 5 TELESCOPE FOR SALE 6 JULY 2016 “QUICK AND EASY OBSERVING PAD”, BY JOHN LAND 7 IOTA MEETING ANNOUNCEMENT BY BYRON LABADIE 8 PHOTOS OF THE OBSERVATORY BY BYRON LABADIE 9 IMAGE OF THE MONTH: MARS AND ANTARES “HUBBLE’S BUBBLE LIGHTS UP THE INTERSTELLAR RUBBLE”, BY DR. ETHAN SIEGEL 10 TAKEN AT THE ACT OBSERVATORY JUNE 6, 2016 WHERE WE MEET 12 BY BYRON LABADIE OFFICERS, BOARD & STAFF 13 PERMISION TO REPRINT ANYTHING FROM THIS NEWSLETTER IS GRANTED, PROVIDED THAT CREDIT IS GIVEN TO THE ORIGINAL AUTHOR AND THAT THE ASTRONOMY CLUB OF TULSA “OBSERVER” IS LISTED AS THE ORIGINAL SOURCE. FOR ORIGINAL CONTENT CREDITED TO OTHERS AND SO NOTED IN THIS PUBLICATION, YOU SHOULD OBTAIN PERMISSION FROM THAT RESPECTIVE SOURCE PRIOR TO REPRINTING. THANK YOU VERY MUCH FOR YOUR COOPERATION. PLEASE ENJOY THIS EDITION OF THE OBSERVER. THE ASTRONOMY CLUB TULSA IS A PROUD MEMBER OF View is of Mars shining over the constellation Scorpius, taken at the ACT Observatory, looking Southeast. Thank you Byron for such a stunning image! THE ASTRONOMICAL LEAGUE JULY 2016 MOON PHASES AND HOLIDAYS: SUN MON TUE WED THU FRI SAT NEW MOON MON JUL 4 1 2 INDEPENDENCE DAY MON JUL 4 3 4 5 6 7 8 9 FIRST QUARTER MON JUL 11 10 11 12 13 14 15 16 FULL (Buck) MOON TUES JUL 19 LAST QUARTER TUES JUL 26 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 UPCOMING EVENTS: MEMBERS’ NIGHT** FRI, JUL 1 8:45 PM ACT OBSERVATORY MEMBERS’ NIGHT BACKUP** SAT, JUL 2 8:45 PM ACT OBSERVATORY SIDEWALK ASTRONOMY SAT, JUL 9 8:00 PM BASS PRO PUBLIC STAR PARTY SAT, JUL 23 8:30 PM ACT OBSERVATORY MEMBERS’ NIGHT POTLUCK** FRI, JUL 29 TBA ACT OBSERVATORY MEMBERS’ NIGHT BACKUP** SAT, JUL 30 8:30 PM ACT OBSERVATORY SIDEWALK ASTRONOMY SAT, AUG 13 7:15 PM BASS PRO PUBLIC STAR PARTY SAT AUG 27 8:00 PM ACT OBSERVATORY **MEMBERS AND FAMILY ONLY PLEASE.
    [Show full text]
  • Cassiopeia A
    National Aeronautics and Space Administration Cassiopeia A www.nasa.gov Cassiopeia A: Exploring the Third Dimension of Cassiopeia A The Chandra X-ray Observatory has observed the Cassiopeia A supernova remnant many times since its launch in 1999. Cassiopeia A (Cas A) is the debris left behind after a massive star exploded. Chandra images have been instrumental in unlocking the mysteries of this stellar explosion. The Cassiopeia A supernova remnant is one of the most In 2004, Chandra observed Cas A for over a million famous objects in the sky. Chandra’s spectacular first seconds, yielding an extremely detailed image of the image of Cas A in 1999 showed a hot point-like source supernova remnant. In the years since then, astronomers close to the center of the remnant. This extremely compact have continued to observe Cas A with Chandra, making object, thought to be a neutron star or black hole, had additional important discoveries. never been seen in any wavelength. In addition, the shell of material surrounding the central source was in clearer For example, astronomers found evidence for a bizarre focus than ever before, displaying dense knots, complex state of matter—known as a superfluid—in the neutron filamentary structures, and a jet of material protruding out star at the center of Cas A. Other researchers analyzed of the shell. Chandra data of Cas A to discover that the supernova remnant acts as a relativistic pinball machine by The next year, astronomers used Chandra to map the accelerating electrons to enormous energies. Scientists heavy elements that were ejected in the supernova blast.
    [Show full text]
  • Spitzer Spectral Mapping of Supernova Remnant Cassiopeia A
    SPITZER SPECTRAL MAPPING OF SUPERNOVA REMNANT CASSIOPEIA A The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Smith, J. D. T., Lawrence Rudnick, Tracey Delaney, Jeonghee Rho, Haley Gomez, Takashi Kozasa, William Reach, and Karl Isensee. “ SPITZER SPECTRAL MAPPING OF SUPERNOVA REMNANT CASSIOPEIA A .” The Astrophysical Journal 693, no. 1 (March 1, 2009): 713–721. © 2009 American Astronomical Society. As Published http://dx.doi.org/10.1088/0004-637x/693/1/713 Publisher Institute of Physics/American Astronomical Society Version Final published version Citable link http://hdl.handle.net/1721.1/96252 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, 693:713–721, 2009 March 1 doi:10.1088/0004-637X/693/1/713 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. SPITZER SPECTRAL MAPPING OF SUPERNOVA REMNANT CASSIOPEIA A J. D. T. Smith1,2, Lawrence Rudnick3, Tracey Delaney4, Jeonghee Rho5, Haley Gomez6, Takashi Kozasa7, William Reach5, and Karl Isensee3 1 Ritter Astrophysical Observatory, University of Toledo, Toledo, OH 43606, USA; [email protected] 2 Steward Observatory, University of Arizona, Tucson, AZ 85721, USA 3 Astronomy Department, University of Minnesota, Minneapolis, MN 55455, USA 4 Massachusetts Institute of Technology, Kavli Institute for Astrophysics and Space Research,
    [Show full text]
  • Binocular Universe: Hail the Queen November 2010
    Binocular Universe: Hail the Queen November 2010 Phil Harrington hope you're dressed appropriately, because this month we have an audience with the Queen…Queen Cassiopeia, that is. Cassiopeia reigns over the autumn I sky as she rides high in the north, sitting on her royal throne. You have probably heard the story of Queen Cassiopeia, of how she and King Cepheus ruled ancient Ethiopia. Cassiopeia was well known for two things: her great beauty and her shameless arrogance. One day, she bragged of being more beautiful than the sea nymphs, who were well-known for their exquisite loveliness. Above: Autumn star map from Star Watch by Phil Harrington Above: Finder chart for this month's Binocular Universe. Chart adapted from Touring the Universe through Binoculars Atlas (TUBA), www.philharrington.net/tuba.htm The sea nymphs overheard this boasting and complained to their father, Poseidon, the king of the seas. Poseidon became so infuriated that he created Cetus the Sea Monster. Cetus was sent to Ethiopia to devour the citizens of the land. King Cepheus was told that his people could be saved only if he were to sacrifice his daughter Andromeda to the sea monster. As king, he had no alternative but to lead his daughter to the water's edge and chain her to a rock. There, she was left to the mercy of Cetus. Just then, our hero, Perseus, appeared on the scene. Perseus, the son of Zeus, had been ordered to kill a gorgon called Medusa. Medusa was a very ugly creature whose hair was made of snakes.
    [Show full text]
  • Observer's Handbook 1980
    OBSERVER’S HANDBOOK 1980 EDITOR: JOHN R. PERCY ROYAL ASTRONOMICAL SOCIETY OF CANADA CONTRIBUTORS AND ADVISORS A l a n H. B a t t e n , Dominion Astrophysical Observatory, Victoria, B.C., Canada V 8 X 3X3 (The Nearest Stars). Terence Dickinson, R.R. 3, Odessa, Ont., Canada K0H 2H0 (The Planets). M arie Fidler, Royal Astronomical Society of Canada, 124 Merton St., Toronto, Ont., Canada M4S 2Z2 (Observatories and Planetariums). V ictor Gaizauskas, Herzberg Institute of Astrophysics, National Research Council, Ottawa, Ont., Canada K1A 0R6 (Sunspots). J o h n A. G a l t , Dominion Radio Astrophysical Observatory, Penticton, B.C., Canada V2A 6K3 (Radio Sources). Ian Halliday, Herzberg Institute of Astrophysics, National Research Council, Ottawa, Ont., Canada K1A 0R6 (Miscellaneous Astronomical Data). H e le n S. H o g g , David Dunlap Observatory, University of Toronto, Richmond Hill, Ont., Canada L4C 4Y6 (Foreword). D o n a l d A. M a c R a e , David Dunlap Observatory, University of Toronto, Richmond Hill, Ont., Canada L4C 4Y6 (The Brightest Stars). B r ia n G. M a r s d e n , Smithsonian Astrophysical Observatory, Cambridge, Mass., U.S.A. 02138 (Comets). Janet A. M attei, American Association o f Variable Star Observers, 187 Concord Ave., Cambridge, Mass. U.S.A. 02138 (Variable Stars). P e t e r M. M illm a n , Herzberg Institute o f Astrophysics, National Research Council, Ottawa, Ont., Canada K1A 0R6 (Meteors, Fireballs and Meteorites). A n t h o n y F. J. M o f f a t , D épartement de Physique, Université de Montréal, Montréal, P.Q., Canada H3C 3J7 (Star Clusters).
    [Show full text]
  • Cassiopeia a the Death of a Star
    Cassiopeia A The Death of a Star Ten thousand, three hundred and twenty years ago and sixty trillion miles away, a giant star was dying. More than ten times more massive than our Sun, the star had existed for more than ten million years. Now the star was running out of hydrogen, the fuel necessary to keep its nuclear fires burning. The radiation pressure pushing outwards from the nuclear fires in the core of the star stopped. Without the radiation pressure, there was nothing to balance the relentless inward pull of gravity and the star began to collapse. The star, which had existed since the evolution of mammals on Earth, finally lost its battle with gravity. The complete and total destruction of the star followed in a catastrophic explosion. On Earth, the year was 8320 BC and the glaciers had finally finished receding, ending the last great Ice Age. Small bands of hunter- gatherers had crossed the Bering Strait and were spreading throughout North and South America. A paleo-Indian culture was flourishing in the region of the Rio Grand Valley in New Mexico. Prehistoric cultures had already turned their eyes to the sky above them. The repeating patterns of the motions of the Sun, Moon and stars had become a calendar, clock, and compass. The sky told them when the game herds would migrate, the direction in which to travel, and eventually when to plant and harvest their crops. They believed that human events and cycles were part of larger cosmic events and cycles, and that the night sky was part of that cycle.
    [Show full text]