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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
Stars

Arcturus

Arcturus is the brightest star in the northern hemisphere. Even though it gives off 180 times more power than the Sun, it only looks 110 times brighter because a lot of the light it emits is infra-red and invisible to the human eye.

Arcturus is about 37 light years away from us and could be a binary star, but its companion is 20 times dimmer and very difficult to see.

Arcturus takes its name from the Ancient Greek, ‘Arktouros’, which means ‘bear guard’, because it is the brightest star next to Ursa Major and Minor – the Big and Little Bears.

Photos: Science Photo Library
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