'Low mass stars' diaporamas de présentation

Announcements

Announcements. Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14 Angel Quiz. Questions:. Black Holes Star-Gas-Star cycle Halo, halo stars, halo vs. bulge, halo vs disk Spiral arms Do dying stars come back as the same star? superbubbles. Halo Stars:

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Endpoints of stellar evolution

Endpoints of stellar evolution. The end of stellar evolution is an inert core of spent fuel that cannot maintain gas pressure to balance gravity .

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The interstellar medium (ISM ) (Section 18.2, bits of 18.7,18.8)

The interstellar medium (ISM ) (Section 18.2, bits of 18.7,18.8). Space between stars is not a vacuum but is filled with gas. Why is the ISM important? Stars form out of it Stars end their lives by returning gas to it Evolution of gas in ISM and stars is crucial

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WELCOME to the SAASTA AstroQuiz 2017 NATIONAL FINALS 5 OCTOBER 2017

WELCOME to the SAASTA AstroQuiz 2017 NATIONAL FINALS 5 OCTOBER 2017. RULES OF THE QUIZ. The audience must be silent throughout the quiz and NOT whisper to anyone. No resource material can be taken into the quiz venue.

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Dimensions of Stars

Dimensions of Stars. Having determined that stars are at large distances, high temperatures and very luminous, the next question to ask is how large they are. An Example:. Dimensions of Stars. The star Betelgeuse ( a Orionis) has the following parameters: Distance 150 pc

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Stellar Death High Mass Stars

Stellar Death High Mass Stars. Nucleosynthesis. Evolutionary Time Scales for a 15 M ? Star. Fe. C. H. He. Used energy. Released energy. Energy Budget. Energy. Fusion Stages. Animation. The Final Second. Fe fusion begins Energy debt results Core contracts - temperature increases.

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Chapter 12

Chapter 12. We can use space exploration to learn about stars, nebulae, and galaxies outside our solar system. Learning about Space. Our current understanding of the solar system has changed with improved technologies Theories are based on evidence that are collected remotely. Early ideas.

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Chapter 15: Star Formation and the Interstellar Medium

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Stellar Evolution: Low Mass Stars

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Stellar Evolution: The Live and Death of a Star

Stellar Evolution: The Live and Death of a Star. Star ch. 20. Standards. Understand the scale and contents of the universe, including stars

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A New Technique to Measure ? Y/ ? Z

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Death of Low Mass Stars 8 Solar Masses or less

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Lecture 17

Lecture 17. Post-ms evolution II. Review. Review. Review. Second dredge-up: He-shell burning. A Helium-burning shell ignites around a C,O core. Similar to the H-shell burning phase Again, the envelope expands and cools, becoming convective and causing a second dredge-up.

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The Life Cycles of Stars

The Life Cycles of Stars. In a group, create a theory that explains: The origin of stars Where do they come from? The death of stars Why do stars die? What happens to a star when it dies?. What is a Star?. Stars are massive, glowing balls of hot gases, mostly hydrogen and helium.

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The Death of High Mass Stars: 8 Solar Masses and up.

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Components of the Universe

Components of the Universe. Chapter 11 . 11.1 STARS . Stars are spherical objects in space that radiate energy from their hot cores like a thermonuclear reactor. They outnumber all other celestial bodies. Stars have a life span like all living things on earth.

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PART 1 CLUES TO THE FORMATION AND EVOLUTION OF THE MILKY WAY

PART 1 CLUES TO THE FORMATION AND EVOLUTION OF THE MILKY WAY. This scenario is based upon observations of the motions , ages , metalicities of stars as a function of their locations in the galaxy. There are very clear trends in these observables .

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The Aging of High Mass Stars is Completely Different

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20.3 The lives of stars

20.3 The lives of stars. Key concepts: how does a star form? What determines how long a star will exist? What happens to a star when it runs out of fuel? Key terms: nebula, protostar , white dwarf, supernova, neutron star, pulsar, black hole. A star is born.

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