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Astronomy

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... are perpendicular. Entire pattern races along at c = 2.99 x 108 m/s ... RAY - 'geometrical optics' reflection and refraction in mirrors, lenses, telescopes ... – PowerPoint PPT presentation

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Title: Astronomy


1
  • Electric and Magnetic Fields are perpendicular
  • Entire pattern races along at c 2.99 x 108 m/s
  • Optical wavelengths l ? 400 (violet) 700
    (red) nm

2
The REAL rainbow
3
Four Ways of Thinking about EM radiation
  • RAY - geometrical optics reflection and
    refraction in mirrors, lenses, telescopes
  • WAVE - diffraction optics interference and
    diffraction, amounts reflected, transmitted
  • from VIS, to IR, to radio
  • PHOTON - absorption and emission spectra of hot
    gases from VIS, to UV, to x-ray, to g-ray
  • PHOTON GAS - diffusion, cosmic background

4
The atmosphere is mostly opaque except in the
visible, some IR and radio
The Doppler Effect works for light too
  • if object moves AWAY viewer light is
    red-shifted
  • if object moves TOWARD viewer light is
    blue-shifted
  • speed must be pretty large to see significant
    shift
  • Dl/l vo/c is the formula (we wont use it)

5
The Photon Idea
  • Einsteins conception in 1905
  • Think of EM radiation as a PARTICLE, not a wave
  • Absorbed, Emitted All at Once
  • Packet of Energy E hf
  • E energy in electron-volts (eV)
  • f frequency in Hz
  • h Plancks constant 4.14 x 10-15 eV/Hz
  • Optical E ? 1.5 eV 2.5 eV (LEDs)
  • Typical chemical energy

6
Energy, Power, Flux and All That
  • Energy the total amount present, like a candy
    bar (units Joules or eV electron-Volts)
  • Power the time rate at which energy is
    consumed, or produced P E/t (units J/s
    Watts), like a light bulb
  • Flux the power divided by the area over which
    it is smeared F P/A (units W/m2)
  • Note book is goofy on this point
  • If power is emitted in all directions equally
    (like a star), then the flux drops off with
    distance d like 1/d2 inverse-square law

7
Power emitted from a point-like source spreads
over larger and larger areas
8
Law of Reflection
Angle of Incidence Angle of Reflection
9
Law of Refraction
Rays bend toward (away) from the normal as they
pass from one medium to a more (less) optically
dense medium
10
Fig.06.18
11
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12
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13
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14
For a telescope on the moon
15
Fig.06.23
CCD detectors and x-ray optics
16
How the Eye Sees the diverging cone of rays
  • Two cones here one from top, one from bottom
  • Image is REAL (there IS light there) and
    INVERTED

17
The object is so close to the lens that a
magnified VIRTUAL (there is no light there) image
is formed Looks diverging
MORAL Convex lenses are not always converging
The object is sufficiently far from the lens that
a shrunken REAL (there is light there) image is
formed Looks converging
18
How a telescope ANGULARLY MAGNIFIES
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