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Stellar Nurseries Karena Fiore
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What is a Stellar Nursery? Also known as molecular clouds, a stellar nursery is a dense region in space where new stars are made. A stellar nursery is located within a nebula These interstellar clouds have high concentrations of molecular hydrogen and helium. Temperatures range from 10 to 30 K
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History Nebulas were first recorded around 150 AD by Ptolemy The first true nebula was mentioned in 954 by Abd al-Rahman al- Sufi in his Book of Fixed Stars. The nebula was distinct from surrounding star clusters Al-Sufi also catalogued other nebulas such as the Omicron Velorum Cluster and Brocchi’s Cluster
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History In the late 1700s, the Herschels published three catalogs that listed thousands of nebulas and star clusters they had found An updated version of the Herschels catalog was published in 1888 by J.L.E. Dreyer The New General Catalogue (NGC) is a compilation of clusters, nebulas, and galaxies
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Ways a Stellar Nursery is Formed A cloud of gas becomes so dense that it collapses under its own gravity A shockwave from a supernova (ex. The Crab Nebula) When a low-mass star has lost most of its material, its temperature increases and it emits UV radiation that will ionize the surrounding gas This is a planetary nebula The Crab Nebula (NGC 1952 )
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Structure of a Stellar Nursery It is composed of mainly hydrogen and helium There are trace amounts of the other elements (under 1%) There is also plasma (ionized gas) within the nebula Width of millions of miles to hundreds of light years across Planetary nebulas have a central star
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Star Formation Interstellar clouds are at a state of hydrostatic equilibrium gas pressure and the internal gravitational forces balance each other Certain events will happen to trigger star formation Molecular clouds collide Shockwaves of a supernova explosion Galactic collisions This will trigger a gravitational collapse within the nebula
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Star Formation As a molecular cloud fragment collapses under gravity, it becomes a protostar This is the early stage of a forming star When a protostar reaches 10 million K in its core, it becomes a main-sequence star It is now able to undergo hydrogen fusion
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Stars Stars are born in clusters because the cloud in which they are formed is thousands of times more massive than each star Brand new stars are main-sequence stars High mass stars expand to become giants and supergiants These stars fuse hydrogen, helium, carbon, oxygen, etc. Low mass stars eventually become white dwarfs Outer layers of star have been ejected and nuclear fusion has ceased
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Life Span of a Stellar Nursery Nebulas exist for a few million years The radiation pressure from new stars drive away the gas of a nebula The dissipated nebula cannot be considered a stellar nursery anymore There is not enough concentrated hydrogen and helium gas to form new stars
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Cat’s Paw Nebula (NGC 6334) In September of 2013, a newly discovered stellar nursery was found approximately 5,500 light years from Earth It was found with ArTeMiS, a wide-field sub-millimeter- wavelength camera It can sense interstellar dust grains that can be found inside a nebula
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Cat’s Paw Nebula (NGC 6334)
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Bibliography http://en.wikipedia.org/wiki/Star_formation http://en.wikipedia.org/wiki/Star_formation http://en.wikipedia.org/wiki/Molecular_cloud http://en.wikipedia.org/wiki/Molecular_cloud http://en.wikipedia.org/wiki/Nebula http://en.wikipedia.org/wiki/Nebula http://www.universetoday.com/65067/newly-discovered-stellar-nurseries-in-the- milky-way/ http://www.universetoday.com/65067/newly-discovered-stellar-nurseries-in-the- milky-way/ http://www.kidsastronomy.com/nebulae.htm http://www.kidsastronomy.com/nebulae.htm www.nasa.gov www.nasa.gov Bennett, Jeffrey O. The Essential Cosmic Perspective. 5th ed. San Francisco: Addison-Wesley, 2009. Print. http://news.discovery.com/space/astronomy/cats-paw-nebula-star-forming- region-vista-eso-130925.htm http://news.discovery.com/space/astronomy/cats-paw-nebula-star-forming- region-vista-eso-130925.htm http://en.wikipedia.org/wiki/Star http://en.wikipedia.org/wiki/Star
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