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Starlight and What it Tells Us

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Absolute Magnitude. Altair and Deneb are about equally bright as seen from Earth ... Absolute Magnitude. How bright a star would be at a distance of 32.6 l.y. ... – PowerPoint PPT presentation

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Title: Starlight and What it Tells Us


1
Starlight and What it Tells Us
2
Brightness of Stars
  • Variations in distance and intrinsic brightness
  • Scale based on one by Hipparcos 500 B.C.
  • Magnitude Large Numbers Fainter
  • One magnitude 2.5 x
  • Five magnitudes 100 x

3
Magnitudes
  • Planet around nearby star 30
  • Pluto 13
  • Faintest Naked-Eye Star 6
  • Big Dipper Stars 2
  • Sirius (Brightest Star) -1.6
  • Venus -4
  • Full Moon -12
  • Sun -27

4
Absolute Magnitude
  • Altair and Deneb are about equally bright as seen
    from Earth
  • Altair is 16 l.y. away, Deneb 1600
  • Hence Deneb must be about 10,000 times brighter

5
Absolute Magnitude
  • How bright a star would be at a distance of 32.6
    l.y. (10 parsecs)
  • Sun 4.5 (inconspicuous naked-eye star)
  • Altair 2.2
  • Deneb -7.1 (bright as crescent moon)
  • Note Deneb - Altair about 10 magnitudes 100 x
    100 10,000 times

6
Black-Body Radiation
  • Objects Emit Radiation Because They Are Hot
  • Why Black? Because None of the Radiation is
    Reflected from Some Other Source
  • The Sun Emits Black-Body Radiation, the Moon Does
    Not

7
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8
Why Black-Body Radiation is so Important
  • Color is directly related to temperature
  • Temperature is the only determinant of color
  • Energy per unit area is the same if temperature
    is the same
  • If two stars have the same color and distance,
    difference in brightness is due to difference in
    size
  • Dwarf and giant stars are literally dwarfs or
    giants

9
Spectroscopy
  • Different atoms absorb or emit specific
    wavelengths of light
  • When light spread into a spectrum, the absorbed
    wavelengths show up as dark (missing) bands
  • These spectral lines are indicators of
  • Chemical composition
  • Physical conditions

10
The Solar Spectrum
11
Spectral Lines are Affected By
  • Electrical and Magnetic Fields
  • Number of Electrons Atoms Have Lost (Indicates
    Temperature and Pressure)
  • Motion (Doppler Effect)
  • Blue-shifted if Motion Toward Observer
  • Red-shifted if Motion Away From Observer

12
The Doppler Effect
13
What the Doppler Effect Tells Us
  • Radial Motion
  • Rotation of Stars
  • Approaching side of star blue-shifted, receding
    side red-shifted
  • Unseen Companions (Stars or Planets)
  • Star oscillates around center of mass
  • Surface and Interior Motions
  • Changes in Size
  • Interior Oscillations
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