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Life Cycle of a Star. Stage 1 Protostars Protostars Huge clouds of gas (hydrogen) in which stars are made. Many thousands of times bigger than our
Life Cycle of a Star. Stage 1 Protostars Protostars Huge clouds of gas (hydrogen) in which stars are made. Many thousands of times bigger than our
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P 7 20 Questions Traffic Light Quiz. Rules Everyone should reveal their answer at the same time Count down: 3, 2, 1, show!
P 7 20 Questions Traffic Light Quiz. Rules Everyone should reveal their answer at the same time Count down: 3, 2, 1, show!
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Life Cycle of a Star Waves, Atoms and Space. Stage 1 Protostars
Life Cycle of a Star Waves, Atoms and Space. Stage 1 Protostars
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A JOURNEY TO THE STARS. WHAT IS A STAR? The star shines due to a process called … A star is a hot ball of plasma (electrically charged gases, mainly hydrogen
A JOURNEY TO THE STARS. WHAT IS A STAR? The star shines due to a process called … A star is a hot ball of plasma (electrically charged gases, mainly hydrogen
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Announcements Homework 10 due Monday: Make your own H-R diagram!
Announcements Homework 10 due Monday: Make your own H-R diagram!
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Summary of Post-Main-Sequence Evolution of Sun-Like Stars M < 4 M sun Fusion stops at formation of C,O core. C,O core becomes degenerate Core collapses;
Summary of Post-Main-Sequence Evolution of Sun-Like Stars M < 4 M sun Fusion stops at formation of C,O core. C,O core becomes degenerate Core collapses;
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1 Endpoints of stellar evolution The end of stellar evolution is an inert core of spent fuel that cannot maintain gas pressure to balance gravity Chandrasekhar
1 Endpoints of stellar evolution The end of stellar evolution is an inert core of spent fuel that cannot maintain gas pressure to balance gravity Chandrasekhar
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Lives of Stars. A star is born… All stars begin their lives as NEBULAS, large clouds of gas and dust spread out in an immense volume. A STAR, on the
Lives of Stars. A star is born… All stars begin their lives as NEBULAS, large clouds of gas and dust spread out in an immense volume. A STAR, on the
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Gamow conference, Odessa, 20.08.2009 Ivan L. Andronov Odessa National Maritime University Space Laboratory to Study Accretion in Magnetic Cataclysmic Variables:
Gamow conference, Odessa, 20.08.2009 Ivan L. Andronov Odessa National Maritime University Space Laboratory to Study Accretion in Magnetic Cataclysmic Variables:
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YELLOW DWARFS Color: Appear yellow Gases Burned: Fuse H, He to generate into light Size : Small 80-100% mass of the sun Surface Temperature: 5300-6000
YELLOW DWARFS Color: Appear yellow Gases Burned: Fuse H, He to generate into light Size : Small 80-100% mass of the sun Surface Temperature: 5300-6000
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Announcements Quiz 4 - March 4 –Stellar evolution Low-mass stars Binaries High-mass stars –Supernovae –Synthesis of the elements WWW lab is available
Announcements Quiz 4 - March 4 –Stellar evolution Low-mass stars Binaries High-mass stars –Supernovae –Synthesis of the elements WWW lab is available
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1 The structure and evolution of stars Lecture13: Supernovae - deaths of massive stars Complete notes available online: sjs/teaching.html
1 The structure and evolution of stars Lecture13: Supernovae - deaths of massive stars Complete notes available online: sjs/teaching.html
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