Measuring distances by parallax Edexcel International A Level Physics revision

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In plain words

Hold up a finger at arm's length and look at it with one eye and then the other: it seems to jump against the background. Nearby stars do the same thing over six months, as the Earth swings from one side of the Sun to the other. The smaller the jump, the further away the star.

Three things to know

  1. Trigonometric parallax: a nearby star is observed against the background of very distant stars from opposite sides of the Earth's orbit, six months apart. It appears to shift.
  2. The parallax angle p is half of the total angle the star appears to move through. The distance is d = r ÷ tan p, where r is the radius of the Earth's orbit, 1.50 × 10¹¹ m. For such tiny angles, d = r ÷ p with p in radians.
  3. It only works for fairly close stars. For distant ones the angle is too small to measure, and standard candles are used instead.

Worked example

A star has a parallax angle of 3.7 × 10⁻⁶ radians. Find its distance from the Earth.

  1. d = r ÷ p, with p in radians.
  2. = 1.50 × 10¹¹ ÷ 3.7 × 10⁻⁶.
  3. = 4.1 × 10¹⁶ m.

Tips and tricks

  • The parallax angle is half the total shift seen across six months.
  • A smaller angle means a more distant star.
5 questions, about 2 minutes.

It lands in your notebook with its questions as flashcards.

Measuring distances by parallax: 5 questions and answers

These are the quiz’s questions. Do the quiz first, then come back here for the ones that got you.

  1. What is seen when a nearby star is observed six months apart?
    • It appears to shift against the more distant stars. (the answer)
    • It changes colour.
    • It gets brighter.
    • It disappears.

    The Earth has moved to the other side of its orbit.

  2. Why are the two observations made six months apart?
    • so that the Earth is at opposite sides of its orbit (the answer)
    • so that the star has time to move
    • so that the weather is the same
    • so that the Sun is in the same place

    That gives the longest baseline, and so the biggest shift.

  3. Star A has a larger parallax angle than star B. Which is closer to the Earth?
    • star A (the answer)
    • star B
    • they are the same distance away
    • it can't be known

    Nearer stars appear to move more.

  4. How are the distances to very distant galaxies found?
    • with standard candles (the answer)
    • with parallax
    • with a metre rule
    • with radar

    Their parallax angles are too small to measure.

  5. In d = r ÷ p, what must the parallax angle p be measured in?
    • radians (the answer)
    • degrees
    • metres
    • seconds

    The small-angle approximation only works in radians.

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