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The top documents tagged [main sequence slide]
1st Step: –Stars form from nebulas Regions of concentrated dust and gas –Gas and dust begin to collide, contract and heat up All due to gravity
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Ch. 9 – The Lives of Stars from Birth through Middle Age Second part The evolution of stars on the main sequence
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Hour 2: Stars, Stellar Evolution, and Creation of Chemical Elements The Sun & Nuclear Fusion - Energy for Life The Sun Compared With Other Stars Stellar
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Astronomy Unit Test Jeopardy Review Game. The SunLife Cycle of Stars GalaxiesMeasuring Matter Gravity and the Big Bang 100 200 300 400 500
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Astronomy Unit Review 1. Read the question 2. Write your answer on the white board 3. Write ONLY the answer
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The Magnitude Scale A measure of the apparent brightness Logarithmic scale Notation: 1 m.4 (smaller brighter) Originally six groupings –1 st magnitude
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The Lives of Stars Chapter 12. Life on Main-Sequence Zero-Age Main Sequence (ZAMS) –main sequence location where stars are born Bottom/left edge of main
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Ch. 9 The Lives of Stars from Birth through Middle Age The Cone Nebula
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Internal motions in star clusters Gordon Drukier Dept. of Astronomy, Yale University Yale Astrometry Workshop — 21 July 2005 Gordon Drukier Dept. of Astronomy,
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Structure of the Universe Astronomy 315 Professor Lee Carkner Lecture 23
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Evolution of the Solar System Matt Rogers AT350 9 September 2003
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Properties of Stars II The Hurtzprung-Russell Diagram How long do stars live? Star clusters
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