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How%20Far?

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How Far? Measuring Distance in the Universe How? Gian Domenico Cassini, in 1672, used a technique called parallax to measure the distance to Mars. – PowerPoint PPT presentation

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Title: How%20Far?


1
How Far?
  • Measuring Distance in the Universe

2
How?
  • Gian Domenico Cassini, in 1672, used a technique
    called parallax to measure the distance to Mars.

3
Cassini figured it out!
  • The Sun is about 93 million miles from
  • Earth. As Earth and Mars never come closer than
    35 million miles to each other.
  • Saturn, the most distant planet known when
    Cassini was alive, is around 900 million miles
    away.

4
How?
  • Parallax!

5
What is Parallax?
  • Try this out
  • Hold 1 finger out at arms length
  • Close one eye, and then the other
  • Notice how your finger jumps?

6
Measuring Stars
  • Stars are billions of light years away winking
    wont help
  • Our orbit is 186 million miles wide (93 million
    93 million)
  • Star A and B are the same star, as they appear 6
    months apart

7
How to
  • The parallax angle p is illustrated in the above
    figure.
  • We can determine they adjacent (d) using
    trigonometry.

8
Trigonometry
  • Our adjacent line (d in the prior picture) is the
    distance from Earths Orbit (BC) to the star (A)
  • Adjacent length opposite length tangent angle A

9
Trigonometry
  • Measure the angle of the star to our central
    point of orbit
  • Simple calculation
  • Even the Hubble Telescope limited to 1000 LY

Earths Orbit
10
Parsec
  • The method of parallax gives rise to a natural
    distance unit that astronomers call the parsec.
  • defined as the distance at which a star would
    have a parallax angle p equal to one second of
    arc.
  • using trigonometry distance equal to 206,265
    astronomical units or 3.26 LY
  • AU is the average distance of Earth to Sun

11
Further away?
  • The universe is expanding
  • Galaxies furthest away are moving away faster
    than galaxies closer to us
  • We can us Doppler Effect

12
Visible Spectrum
13
Doppler
  • Doppler

14
What is Red Shift?
  • As light moves away, the waves stretch out
  • Longer waves are shifted towards the red
  • As light moves towards us, the waves condense
  • Shorter waves are shifted towards the blue

15
Spectral Signature
  • Each element has a unique spectral signature
  • Two elements combine

16
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