Learn / Light, and how we know anything

Telescopes in space

The air blocks most kinds of light and blurs the rest. Lifting a telescope above it costs a fortune, and has changed what is known about almost everything.

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First look

The idea, in plain words

  1. Why would anyone put a telescope in space, where nobody can reach it to mend it? Because of the air. The air that keeps you alive is a poor window. It stops most kinds of light from ever reaching the ground: gamma rays, X-rays, most ultraviolet and most infrared. What does get through is shaken about on the way down, which is why stars twinkle. A telescope above the air sees every kind of light, and sees it steady.

  2. The best known is the Hubble Space Telescope. It was carried up by a space shuttle on 24 April 1990 and is still working. It is the size of a bus, 13 metres long, with a mirror 2.4 metres across. It circles the Earth a little under 500 km up, at about 27,000 km an hour, and goes round once every 95 minutes.

  3. Hubble began with a disaster. Its first pictures were blurred. The mirror had been ground to the wrong shape: too flat at the edge by 2.2 thousandths of a millimetre, about a fiftieth of the width of a hair. Hubble had been built to be visited, and in December 1993 seven astronauts flew up and fitted it with what were, in effect, glasses. The pictures have been sharp ever since.

  4. Hubble’s successor is the James Webb Space Telescope, launched on 25 December 2021. Its mirror is 6.5 metres across, too wide for any rocket, so it is made of 18 six-sided pieces that were folded for launch and opened out in space. Each piece is coated in a film of real gold, because gold is very good at reflecting infrared light, the kind Webb is built to see.

  5. Infrared matters for two reasons. It passes through dust, so Webb can see into the clouds where stars are being born. And the light of the earliest galaxies has been stretched on its long journey until it is infrared and nothing else. But everything warm glows in infrared, the telescope included. So Webb sits 1.5 million km from the Earth, behind a sunshield the size of a tennis court, and stays colder than 223 degrees below freezing.

  6. Webb’s first deep picture was shown on 11 July 2022. It covers a patch of sky the size of a grain of sand held at arm’s length, and it holds thousands of galaxies. Some of their light set out more than 13 billion years ago. There are dozens of other telescopes in space, for X-rays, gamma rays and more, and every one of them is there for the same reason: to get above the air.

Go deeper

That was the idea. The same subject is written again below for readers who want more, each on a page of its own.

  1. How it worksCause and effect, with real numbersAbout 5 minutes

Words used here

Aperture
The width of a telescope's main lens or mirror. It sets how much light the telescope collects and how fine a detail it can show.
Wavelength
The distance from one crest of a wave to the next.
Infrared
Light with wavelengths a little longer than red, which we feel as heat.
Ultraviolet
Light with wavelengths a little shorter than violet, given off by very hot things.
X-rays
Light of very short wavelength, given off by gas at millions of degrees.
Gamma rays
Light with the shortest wavelengths and the most energy of all, made by the most violent events in the universe.
Lagrange point
One of five places where a small object can keep step with two larger ones.
Look-back time
How long ago the light you are seeing set out.

Where this comes from

The words are written for this site. The pictures are drawn by the page from the figures in the lesson, and each one says underneath what it is based on.