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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
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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
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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
Planets

Venus

Venus is named after the Roman goddess of love and is the hottest planet in the Solar System.

It’s about the same size as Earth, but it rotates in a retrograde (backwards) direction and has a much thicker atmosphere; standing on the surface of Venus would feel like standing 1km down under the sea on Earth!

Until 1962, when Mariner 2 passed by, it was thought that there were oceans on this most brilliant of planets. We now know that Venus is far too hot to have water on the surface; it’s covered in deadly volcanoes and was probably shaped by the movement of tectonic plates.

Average distance from the Sun:  108,200,000km 
                                                (67,230,000miles)

Length of year:                          225 Earth days

Diameter:                                 12,102km (7520miles)

Average temperature:                896°F (480°C)

Photos: NASA

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