Parallax

The parallax method of measuring a star's distance
The parallax method of measuring a star's distance

Distances in the Universe are unimaginably vast: even the nearest star is 40 trillion kilometres away. This is too far to send a spacecraft, but astronomers use a mathematical trick, called parallax, to calculate such faraway distances.

You can discover the concept of parallax right now by holding your finger out in front of your face and closing one eye. Look at where your finger is in relation to objects in the background. Now open the other eye, and close the first. Your finger appears to move against the more distant objects, even though you haven’t moved it. This is parallax!

You can experiment further by moving your finger to different distances in front of your face and blinking from eye to eye. You will see that your finger appears to move a greater distance when it is closer to your face than when it is further away.

Let’s use the orbit of Earth around the Sun as an example in astronomy. Every 6 months, Earth moves halfway around its orbit and presents a different vantage point for observing a star, the equivalent of blinking between two eyes. In this case the star appears to move from side to side against the backdrop of more distant stars.

By measuring the amount of displacement – the parallax angle – and knowing the distance between the Sun and the Earth, astronomers can determine the star’s distance using simple trigonometry.

Even for the nearest stars the amount of apparent movement is tiny: less than one arcsecond. Yet Gaia will measure the positions of one billion stars to microarcsecond accuracies.

Last update: 14 June 2013

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