5.6 - Observing the Universe
Optical telescopes
- Telescopes let us see distant objects in space more clearly.
- An optical telescope detects visible light.
- Optical telescopes use refraction and reflection to gather light from a distant object and form an image.
Improving the image
Image quality can be improved in two ways:
- Increase the aperture - The aperture is the diameter of the objective lens (the large lens where light enters). A larger aperture collects more light, so fainter objects can be seen.
- Use a higher quality objective lens - This produces a sharper, clearer image.
Observing from above the atmosphere
- Earth's atmosphere absorbs a lot of the electromagnetic radiation coming from space, so some wavelengths never reach telescopes on the ground, as the graph below shows.
- Placing a telescope on a satellite in space avoids the atmosphere entirely.
- Telescopes in space receive radiation that would otherwise be absorbed, giving a clearer view and more accurate measurements of distant astronomical objects.

Grey shows the wavelengths the atmosphere absorbs; the coloured gaps reach the ground.
Light pollution, air pollution and siting
Ground-based telescopes are limited by two main factors:
- Light pollution - Artificial light from street lamps and buildings makes faint objects hard to see.
- Air pollution - Pollutants reflect and absorb light coming from space.
Getting the best view from the ground
- Place the telescope on top of a mountain, where there's less atmosphere above it.
- Place it in a dark location far from cities to minimise light pollution.
Observing across the whole spectrum
- Visible light is only one part of the electromagnetic spectrum.
- Different astronomical objects emit and reflect radiation in different parts of the spectrum, and many can't be detected in visible light at all.
- To build a complete picture of the Universe, astronomers use a range of telescopes that cover the entire electromagnetic spectrum.
Telescopes across the spectrum
- The earliest telescopes were all optical telescopes.
- Telescopes have since been developed for every part of the electromagnetic spectrum, revealing details about the Universe that can't be seen in visible light.
Different telescopes reveal different things
- X-ray telescopes - Detect violent, high-temperature events, such as exploding stars.
- Radio telescopes - Detected cosmic microwave background radiation, which helped scientists learn about the origins of the Universe.
How telescopes keep improving
- Larger telescopes give better resolution and gather more light, so fainter and more distant objects can be detected.
- Modern telescopes work alongside computers, which process data to produce sharper images and analyse huge amounts of information continuously.
TermDefinition
ApertureThe opening that lets light into a telescope or camera. For a telescope it is the diameter of the objective lens, which sets how much light it collects.
Objective lensThe large lens in an optical telescope where light enters to form an image.
Key points to remember
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