AstronomyLight and Telescopes

Looking Back in Time

Light takes time to reach us (8.3 minutes from the Sun), so the farther we look, the older the view.

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In Light-Years, Stars and Galaxies you met the light-year as a distance. Here is the other side of that idea: because light needs time to reach us, every look into space is a look into the past. Light is part of the electromagnetic spectrum, and all of it, from radio to gamma rays, travels through space at the same speed, $c = 3.00 \times 10^{5}$ km/s.

Why it works

Light is fast but not instant. In 1676 Ole Rømer noticed that the eclipses of Jupiter's moon Io came several minutes late when Jupiter was far from Earth and early when it was near: the light carrying the news needed extra time to cross the wider gap. Travel time is distance divided by speed, $t = \dfrac{d}{c}$. A light-year is how far light goes in one year: $3.00 \times 10^{5}\ \text{km/s} \times 3.156 \times 10^{7}\ \text{s} = 9.46 \times 10^{12}$ km. So light from an object $N$ light-years away left it $N$ years ago. The numbers are huge, so operations in scientific notation do most of the work.

Key idea

Light takes time $t = d/c$ to reach us, so we see every object as it was when its light left: the Sun as it was $8.3$ minutes ago, the nearest star $4.2$ years ago, the Andromeda Galaxy about $2.5$ million years ago.
Distances from Earth on a scale where each step is ten times farther, with how long light takes to cross each one.

Worked examples

Worked example: Sunlight

The Sun is $1.496 \times 10^{8}$ km away. How long does its light take to reach us?
  1. $t = \frac{1.496 \times 10^{8}\ \text{km}}{3.00 \times 10^{5}\ \text{km/s}} = 4.99 \times 10^{2}$ s.
  2. $499 \div 60 = 8.3$ min.
  3. If the Sun vanished, we would keep seeing it, and Earth would keep orbiting, for about 8 minutes.

Answer: About $8.3$ minutes.

Worked example: Driving on Mars

Mars is $2.25 \times 10^{8}$ km away. How long must a rover driver wait for a reply to a command?
  1. The signal goes there and back: $4.50 \times 10^{8}$ km.
  2. $t = \frac{4.50 \times 10^{8}}{3.00 \times 10^{5}} = 1.50 \times 10^{3}$ s $= 25$ min.
  3. With a 25-minute delay, nobody can steer a rover live, so rovers carry software to drive themselves between commands.

Answer: $25$ minutes.

Common mistake

It is natural to think we see the stars as they are now. We never do. The light from Betelgeuse left it centuries ago; if it exploded tonight, nobody on Earth would know for hundreds of years. Check the units: a light-year is a distance, and the travel time in years equals the distance in light-years. The farther away we look, the older the view, which is how astronomers study the young universe: they look very far.
How far back in time we look.
ObjectDistanceLight travel time
Moon$3.84 \times 10^{5}$ km$1.3$ s
Sun$1.50 \times 10^{8}$ km$8.3$ min
Neptune$4.5 \times 10^{9}$ km$4.2$ h
Proxima Centauri$4.2$ ly$4.2$ yr
Center of the Milky Way$26{,}000$ ly$26{,}000$ yr
Andromeda Galaxy$2.5$ million ly$2.5$ million yr

Practice

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Sources and further reading

  • OpenStax, Astronomy 2e, section 1.5, Consequences of Light Travel Time
  • OpenStax, Astronomy 2e, section 5.1, The Behavior of Light
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