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Stellar Astrophysics

emmalmillar Physics Masters Inglés 4,0Valoración media 4,0 de 5 (1 valoración) 15 fichas

Stellar Astrophysics

Fichas del conjunto (15)

  1. 1What is Luminosity?The power emitted by the star. The amount of energy emitted over time.
    L=-dE/dt
    The total light emitted over a specified wavelength intensity
  2. 2What is Bolometric Luminosity?The total power emitted.
    The integral of the luminosity with respect to the wavelength.
  3. 3What is the effective temperature?The temperature the star would have if it was a perfect black body. The temperature of a star is different all over.
    "The temperature a BB would have if it was a sphere with the same radius and luminosity of the star"
  4. 4What equation relates luminosity and temperature?The surface area * the Stefan BoltzmanWhat equation relates luminosity and temperature?
  5. 5What is the mass of the sun?2E30 kg
  6. 6What is the range of mass of a star0.08 SM - 100 SM
    Stars with core less than 0.08 SM never get hot enough for nuclear reaction.
    stars greater than 30 SM are unstable
  7. 7How do you directly measure the mass of a star?By observing the star in a binary system.
    Measure the orbital velocity from Doppler Shift and use Kepler's laws.
  8. 8How to you calculate the mass of a single star?Measure the effective temperature and luminosity and fit to the stellar model.
  9. 9How is the radii of a star defined?As the radius at which most photons escape (the photosphere), which is wavelength dependent. It is not normally used as the photosphere can appear very fuzzy.
  10. 10What is the Sun's radius?7E8m
  11. 11What is a WD and RG radius?10E-2 SR and 10E3 SR.
  12. 12How are radii measured?Very few stars are spatially resolvable.
    Can measure L&T but this is model dependent.
    For direct measurements use lunar occulations, binary eclipses or inetrferometry.
  13. 13What is spectroscopy?As stars are not perfect BBs, the cooler layers of their atmospheres imprint absorption lines onto their spectra.
  14. 14What is spectral classification? Included hottest, coolest and the Sun.OBAFGKM
    O is hottest
    M is coolest
    The Sun is G
  15. 15What is Wein's displacement law?A way to calculate the max wavelength.
    Max Wavelength=2..9E-3/Effective Temp

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Descripción
Masters Physics Fichas sobre Stellar Astrophysics, creado por emmalmillar el 06/12/2015.
Creado por
emmalmillar
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Valoración media 4,0 de 5 (1 valoración)

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