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Home
Observing Space
Introduction
Telescopes
Invisible Astronomy
Section 1.4
Section 1.5
Section 1.6
Section 1.7
Section 1.8
Section 1.9
Section 1.10
Section 1.11
Section 1.12
Section 1.13
Section 1.14
Section 1.15
Exploring Space
Introduction
Pioneers
Shuttles
Launchers
ISS
USA in Space
UK in Space
China in Space
France in Space
Russia in Space
The X-Prize
Section 2.12
Section 2.13
Section 2.14
Section 2.15
Planets
Introduction
Mercury
Venus
Earth
Mars
Jupiter
Saturn
Uranus
Neptune
Pluto
Section 3.11
Section 3.12
Section 3.13
Section 3.14
Section 3.15
Moons
Section 4.1
Section 4.2
Section 4.3
Section 4.4
Section 4.5
Section 4.6
Section 4.7
Section 4.8
Section 4.9
Section 4.10
Section 4.11
Section 4.12
Section 4.13
Section 4.14
Section 4.15
Stars
Introduction
The Sun
Sirius
Canopus
Alpha Centauri
Arcturus
Others
Section 5.8
Section 5.9
Section 5.10
Section 5.11
Section 5.12
Section 5.13
Section 5.14
Section 5.15
Comets, Meteors & Asteroids
Deep Impact Mission
Section 6.2
Section 6.3
Section 6.4
Section 6.5
Section 6.6
Section 6.7
Section 6.8
Section 6.9
Section 6.10
Section 6.11
Section 6.12
Section 6.13
Section 6.14
Section 6.15
Galaxies
Section 7.1
Section 7.2
Section 7.3
Section 7.4
Section 7.5
Section 7.6
Section 7.7
Section 7.8
Section 7.9
Section 7.10
Section 7.11
Section 7.12
Section 7.13
Section 7.14
Section 7.15
The Universe
Section 8.1
Section 8.2
Section 8.3
Section 8.4
Section 8.5
Section 8.6
Section 8.7
Section 8.8
Section 8.9
Section 8.10
Section 8.11
Section 8.12
Section 8.13
Section 8.14
Section 8.15
Eclipses
Solar Eclipse
Lunar Eclipse
Lunar Eclipse 2008
What Eclipses Have Taught Us
Significant Eclipses in History
The Blood Red Moon
Section 9.7
Section 9.8
Section 9.9
Section 9.10
Section 9.11
Section 9.12
Section 9.13
Section 9.14
Section 9.15
Amazing Facts
Section 10.1
Section 10.2
Section 10.3
Section 10.4
Section 10.5
Section 10.6
Section 10.7
Section 10.8
Section 10.9
Section 10.10
Section 10.11
Section 10.12
Section 10.13
Section 10.14
Section 10.15
Play: Comet Impact
Section 11.1
Section 11.2
Section 11.3
Section 11.4
Section 11.5
Section 11.6
Section 11.7
Section 11.8
Section 11.9
Section 11.10
Section 11.11
Section 11.12
Section 11.13
Section 11.14
Section 11.15
Space Blog
Section 12.1
Section 12.2
Section 12.3
Section 12.4
Section 12.5
Section 12.6
Section 12.7
Section 12.8
Section 12.9
Section 12.10
Section 12.11
Section 12.12
Section 12.13
Section 12.14
Section 12.15
Section 13
Section 13.1
Section 13.2
Section 13.3
Section 13.4
Section 13.5
Section 13.6
Section 13.7
Section 13.8
Section 13.9
Section 13.10
Section 13.11
Section 13.12
Section 13.13
Section 13.14
Section 13.15
Section 14
Section 14.1
Section 14.2
Section 14.3
Section 14.4
Section 14.5
Section 14.6
Section 14.7
Section 14.8
Section 14.9
Section 14.10
Section 14.11
Section 14.12
Section 14.13
Section 14.14
Section 14.15
Section 15
Section 15.1
Section 15.2
Section 15.3
Section 15.4
Section 15.5
Section 15.6
Section 15.7
Section 15.8
Section 15.9
Section 15.10
Section 15.11
Section 15.12
Section 15.13
Section 15.14
Section 15.15
Observing Space
Invisible Space

The universe is talking to us – the only problem is we can’t always hear what it has to say, because it speaks in a variety of wavelengths that we can’t see or listen to without special technology.

The sounds coming from space cover the whole range of the electromagnetic spectrum, from very energetic gamma rays to lower energy radio waves. We can only see a small part of this spectrum (visible light), so astronomers have developed special equipment to allow us to observe other wavelengths. On Earth, radio telescopes - like the 250ft ‘dish’ at Jodrell Bank - bring radio waves into focus from beyond the Solar System.

Cosmic microwave background radiation is the last echo of the ‘big bang’, which happened 13.8 thousand million years ago when our universe was created. Much of the electromagnetic spectrum is absorbed by the Earth’s atmosphere, so instruments on orbiting satellites collect information on infra-red, gamma rays and x-rays.

Photos: Hubble
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