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Intensity and Distance

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Intensity and Distance. Intensity depends. on luminosity and. distance. Inverse-square law ... Cameron Reed in 'The Composite Observational-Theoretical HR Diagram' ... – PowerPoint PPT presentation

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Title: Intensity and Distance


1
Intensity and Distance
  • Intensity dependson luminosity anddistance
  • Inverse-square lawdiscovered by Newton
  • Magnitude systemused in astronomy

2
Parallax
  • Parallax is usedto measure thedistance to
    thenearest stars
  • d (parsec) 1 / p (arcsec)
  • Parsec is 3.26light years

3
Stellar Spectra
4
Color Related to Temperature
5
Temperature Affects Absorption
6
Taking a Temperature
7
Careful Study of Absorption
8
Taking the Temperature of Stars
9
Color vs. Temperature
  • Cameron Reed in "The Composite Observational-Theor
    etical HR Diagram"The Journal of the Royal
    Astronomical Society of CanadaFebruary/March
    1998 Volume 92 Number 1
  • B-V -3.684 log(T) 14.551for log(T) lt 3.961
  • B-V 0.344 log(T)2 -3.402 log(T) 8.037for
    log(T) gt3.961

10
H-R Diagram
  • 90 of the stars appear on the main sequence when
    plotted on the H-R diagram
  • Giants have appear to have larger radii
  • Supergiants appear to have largest radii
  • White dwarfs have peculiar spectra

11
Stellar Masses with Binaries
  • Binary stars have elliptical orbits about the
    center of mass.
  • These orbits obey Newtons form of Keplers 3rd
    law M1 M2 4p2/G (a3/p2)
  • The ratio of masses can also be determined
    M1 / M2 a2 / a1
  • Three values must be measured to determine
    individual masses

12
Visual Binaries
  • Visual binary star systems supply all the
    necessary data to compute masses (inclination and
    3 values)

13
Spectroscopic Binary
14
Eclipsing Binary
15
Stellar Masses
  • Masses from binary star data
  • A sizeable fraction of stars have mass data
  • Supergiants have higher average mass than Giants
  • White Dwarfs not shown on this plot

16
Main Sequence Masses
  • There is a relation between mass and luminosity
    for main sequence stars
  • This relation holds only for the main sequence
    (plotted with filled circles)
  • Simple power-law fit gives L M3.5
  • Break in fit at M 0.43
  • M gt 0.43, L M 4.0M lt 0.43, L 0.23 M 2.3

17
Predicted Radii
  • According to the theory of thermal radiationL
    s T4 A 4ps T4 R2
  • The luminosity of a star is related to the
    surface temperature and radius
  • The observed radii in eclipsing binaries are
    consistent with theory

18











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