2b supernovae summary

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  • 8/9/2019 2b Supernovae Summary

    1/2

    Supernovae

    History

    The first supernova sighting ever

    recorded was in 185 A.D. Chinese

    astronomers were star gazing, and

    witnessed a bright light emerging

    from the white-specked blackness

    above. These astronomers were the

    first known spectators of a giant

    exploding star.

    Basics

    Type I Supernova occur in

    binary stars. Binary staare made up of a white dwa

    and another star orbiting

    closely together. The whi

    dwarf stars gravitationa

    pull gradually draws mass

    mass from the larger star

    When it is 1.4 times that

    the sun it collapses and

    explodes.

    Type II supernovae usuall

    occur when a single star

    burns out and its core

    quickly collapses and the

    explodes. This star is

    usually a lot more massiv

    than the sun. When it

    explodes it releases

    tremendous energy and

    electromagnetic radiation

    The Results/Importance of Supernovae

    A small, dense neutron star;

    A black hole;

    All of the heavier elements such as

    iron, gold, and uranium, on Earth and

    in objects out side of the solar

    system;

    High-energy cosmic waves, which most

    likely get their energy from the

    Supernovas vast, powerful magnetic

    field;

    Neutrinos;

    Electromagnetic Radiation; or

    Nothing at all

  • 8/9/2019 2b Supernovae Summary

    2/2

    Current Events

    On November 14, 2006, the

    largest supernova ever

    recorded (SN 2006gy) was

    detected by NASAs orbiting

    Chandra X-Ray Observatory and

    as well as ground-based

    telescopes.

    In November, 2008, 14-year-

    old Caroline Moore of upstate

    New York became the youngest

    person ever recorded to

    discover a supernova.Additional Information

    There are many interesting aspects to

    pernovae, despite the fact that they are

    ormous exploding stars. For instance, it is

    lieved that some supernovae create many of theavier elements, such as iron, gold, and

    anium, that are found both on Earth and in

    jects outside the solar system. Also, high-

    ergy cosmic waves originate from supernovae.

    is thought that these waves get their energy

    om vast, powerful magnetic fields surrounding

    e remnants of the explosions.

    tp://chandra.harvard.edu/photo/2007/sn2006gy/

    tp://imagine.gsfc.nasa.gov/docs/science/know_l2/

    pernovae.html

    tp://www.bbc.co.uk/schools/gcsebitesize/science/edexcel/space/

    eoriginsoftheuniverserev3.shtml

    tp://www.cnn.com/2006/TECH/space/09/26/supernova/

    dex.html

    tp://www.gemini.edu/node/11226

    tps://www.llnl.gov/str/Guidestr.html

    tp://www.msnbc.msn.com/id/18523377

    tp://www.nasa.gov/worldbook/supernova_worldbook.html

    tp://www.sciencedaily.com/releases/2009/06/090610154505.htm

    tp://www2.slac.stanford.edu/vvc/cosmicrays/crsuper.html

    http://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpg

    http://media.smithsonianmag.com/images/505*506/black-hole-Hubble-telescope-52

    http://scienceblogs.com/startswithabang/upload/2010/02/the_greatest_story_ever_

    p2673_467b467cc3e7ac9d44e6282b5446f302supernova.jpg

    http://science.nationalgeographic.com/science/photos/supernovae-gallery/#cynus-

    loop_911_600x450.jpg

    Information Bibliography

    Picture Bibliography

    Caroline MacLeod

    and

    Emma Pidden

    http://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://www2.slac.stanford.edu/vvc/cosmicrays/crsuper.htmlhttp://www.sciencedaily.com/releases/2009/06/090610154505.htmhttp://www.nasa.gov/worldbook/supernova_worldbook.htmlhttp://www.msnbc.msn.com/id/18523377https://www.llnl.gov/str/Guidestr.htmlhttp://www.gemini.edu/node/11226http://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://www2.slac.stanford.edu/vvc/cosmicrays/crsuper.htmlhttp://www.sciencedaily.com/releases/2009/06/090610154505.htmhttp://www.sciencedaily.com/releases/2009/06/090610154505.htmhttp://www.nasa.gov/worldbook/supernova_worldbook.htmlhttp://www.msnbc.msn.com/id/18523377http://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://www2.slac.stanford.edu/vvc/cosmicrays/crsuper.htmlhttp://www.sciencedaily.com/releases/2009/06/090610154505.htmhttp://www.nasa.gov/worldbook/supernova_worldbook.htmlhttp://www.msnbc.msn.com/id/18523377https://www.llnl.gov/str/Guidestr.htmlhttp://www.gemini.edu/node/11226http://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://chandra.harvard.edu/photo/2005/tycho/tycho_hand.jpghttp://www2.slac.stanford.edu/vvc/cosmicrays/crsuper.htmlhttp://www2.slac.stanford.edu/vvc/cosmicrays/crsuper.htmlhttp://www.sciencedaily.com/releases/2009/06/090610154505.htmhttp://www.sciencedaily.com/releases/2009/06/090610154505.htmhttp://www.nasa.gov/worldbook/supernova_worldbook.htmlhttp://www.nasa.gov/worldbook/supernova_worldbook.htmlhttp://www.msnbc.msn.com/id/18523377http://www.msnbc.msn.com/id/18523377https://www.llnl.gov/str/Guidestr.htmlhttps://www.llnl.gov/str/Guidestr.htmlhttp://www.gemini.edu/node/11226http://www.gemini.edu/node/11226http://www.cnn.com/2006/TECH/space/09/26/supernova/index.htmlhttp://www.cnn.com/2006/TECH/space/09/26/supernova/index.htmlhttp://www.cnn.com/2006/TECH/space/09/26/supernova/index.htmlhttp://www.cnn.com/2006/TECH/space/09/26/supernova/index.htmlhttp://www.bbc.co.uk/schools/gcsebitesize/science/edexcel/space/theoriginsoftheuniverserev3.shtmlhttp://www.bbc.co.uk/schools/gcsebitesize/science/edexcel/space/theoriginsoftheuniverserev3.shtmlhttp://www.bbc.co.uk/schools/gcsebitesize/science/edexcel/space/theoriginsoftheuniverserev3.shtmlhttp://www.bbc.co.uk/schools/gcsebitesize/science/edexcel/space/theoriginsoftheuniverserev3.shtmlhttp://imagine.gsfc.nasa.gov/docs/science/know_l2/supernovae.htmlhttp://imagine.gsfc.nasa.gov/docs/science/know_l2/supernovae.htmlhttp://imagine.gsfc.nasa.gov/docs/science/know_l2/supernovae.htmlhttp://imagine.gsfc.nasa.gov/docs/science/know_l2/supernovae.htmlhttp://chandra.harvard.edu/photo/2007/sn2006gy/http://chandra.harvard.edu/photo/2007/sn2006gy/