...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of...

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Transcript of ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of...

Page 1: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 2: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 3: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 4: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 5: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 6: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 7: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 8: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 9: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 10: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 11: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
Page 12: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity
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Ay123 Lecture I:Learning Outcomes

● Overview of how to measure the fundamental properties of stars● Mass● Radius● Temperature● Composition

● Stellar classification schemes● 5-minute overview of stellar evolution

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Parallax

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Spectroscopic binaries

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Eclipsing binary

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Spectral energy distributions of bright stars can be used to derive effective temperatures

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Ay123 Activity 1:Pick the larger star

BlustarusArcturus

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Ay123 Activity 1:Pick the larger star

Let’s pretend Michelson & Pease resolved both stars at ΔΘ = 0.04”.

BlustarusArcturus

0.04” 0.04”

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Ay123 Activity 1:Pick the larger star

Which star has the larger radius?a) Arcturusb) Blustarusc) They’re the same.d) not enough information

BlustarusArcturus

0.04” 0.04”

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Ay123 Activity 1:Pick the larger star

Which star is farther?a) Arcturusb) Blustarusc) They’re the same.d) not enough information

BlustarusArcturus

0.04” 0.04”

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Ay123 Activity 1:Pick the larger star

Which star is intrinsically more luminous?a) Arcturusb) Blustarusc) They’re the same.d) not enough information

BlustarusArcturus

0.04” 0.04”

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Ay123 Activity 1:Pick the larger star

Which star has a higher temperature?a) Arcturusb) Blustarusc) They’re the same.d) not enough information

BlustarusArcturus

0.04” 0.04”

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Ay123 Activity 1:Pick the larger star

Now pretend that the parallaxes are known.

BlustarusArcturus

0.04” 0.04”

π = 9 mas π = 6”

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Ay123 Activity 1:Pick the larger star

BlustarusArcturus

0.04” 0.04”

π = 9 mas π = 6”

Which star is farther?a) Arcturusb) Blustarusc) They’re the same.d) not enough information

Page 27: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity

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Ay123 Activity 1:Pick the larger star

BlustarusArcturus

0.04” 0.04”

π = 9 mas π = 6”

Which star has the larger radius?a) Arcturusb) Blustarusc) They’re the same.d) not enough information

Page 28: ...1 Ay123 Lecture I: Learning Outcomes Overview of how to measure the fundamental properties of stars Mass Radius Temperature Composition Stellar classification schemes 9 Ay123 Activity

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Ay123 Activity 1:Pick the larger star

BlustarusArcturus

0.04” 0.04”

π = 9 mas π = 6”

If both stars have the same apparent brightness, which star is intrinsically more luminous?a) Arcturusb) Blustarusc) They’re the same.d) not enough information

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Stellar Spectral Energy Distributions

Wavelength(Å)

flux

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Spectral Classification

Diagnostic spectral lines act as independent measures of temperature in stellar atmosphere provided surface gravity is known

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Stellar Spectra: Giants vs Dwarfs

G

K

Stars are a 2-D sequence!

Giants are slightly cooler than dwarfs of a similar spectral class with redder continua. This is because line strengths depend on Teff and g

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Luminosity Classes

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The evolution of a single star

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The evolution of a population of stars

Zero Age MS

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Ay123 Activity 1:Pick the larger star

BlustarusArcturus

0.04” 0.04”

π = 9 mas π = 6”

Which star is on the main sequence?a) Arcturusb) Blustarusc) Both

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Ay123 Lecture I:Learning Outcomes

● Overview of how to measure the fundamental properties of stars● Mass● Radius● Temperature● Composition

● Stellar classification schemes● 5-minute overview of stellar evolution

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GRATUITOUS PUPPY PHOTO