Forthcoming meetings
| Friday, June 07, 2013 |
| 19:30 |
| Strange Weather! Exploring the Giant Planets of our Solar System |
| Dr Leigh Fletcher
(University of Oxford)
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| United Reformed Church Hall, Newbury |
| Note: |
The speaker will be followed by the Society's AGM. |
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| No beginners meetings currently scheduled in the diary. |
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| No observing sessions currently scheduled in the diary. |
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| Society visit to the national space centre |
| Saturday, June 08, 2013 |
| 08:30 |
| National Space Centre, Leicester |
| Note: |
See the home page for details. Contact Ann Davies for more imformation. |
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Planetary information
Click a planet in the list below and the information will be displayed.
Planetary information for Mars
The red planet Mars has inspired wild flights of imagination over the centuries, as well as intense scientific interest. Whether fancied to be the source of hostile invaders of Earth, the home of a dying civilization, or a rough-and-tumble mining colony of the future, Mars provides fertile ground for science fiction writers, based on seeds planted by centuries of scientific observations.
We know that Mars is a small rocky body once thought to be very Earth-like. Like the other "terrestrial" planets - Mercury, Venus, and Earth - its surface has been changed by volcanism, impacts from other bodies, movements of its crust, and atmospheric effects such as dust storms. It has polar ice caps that grow and recede with the change of seasons; areas of layered soils near the Martian poles suggest that the planet's climate has changed more than once, perhaps caused by a regular change in the planet's orbit. Martian tectonism - the formation and change of a planet's crust - differs from Earth's. Where Earth tectonics involve sliding plates that grind against each other or spread apart in the seafloors, Martian tectonics seem to be vertical, with hot lava pushing upwards through the crust to the surface. Periodically, great dust storms engulf the entire planet. The effects of these storms are dramatic, including giant dunes, wind streaks, and wind-carved features.
The planet is named for the Roman God of War. |
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| Known by the Ancients |
| 4th |
88,006,827 miles
141,633,260 kilometres |
128,400,000miles
206,600,000 kilometres
1.40 x Earth by comparison |
154,900,000 miles
249,200,000 kilometres
1.64 x Earth by comparison |
2,111 miles
3,397 kilometres
0.53 x Earth by comparison |
13,263 miles
21,344 kilometres |
39,139,300,000 miles3
163,140,000,000 kilometres3
0.15 x Earth by comparison |
641,850,000,000,000,000,000,000 Kilogrammes
0.11 x Earth by comparison |
3.94 gm3
0.71 x Earth by comparison |
89,500,000 miles2
144,100,000 kilometres2
0.28 x Earth by comparison |
12.12 feet/second2
3.69 metres/second2
If you weighed 100 pounds on Earth, you would weigh 38 pounds on Mars |
11,229 miles per hour
18,072 kilometres per hour
0.45 x Earth by comparison |
| 24.62 hours |
| 686.93 Earth days |
53,979 miles per hour
86,871.00 kilomtetres per hour
0.81 x Earth by comparison |
849,400,000 miles
1,366,900,000 kilometres
1.48 x Earth by comparison |
0.09°
5.59 x Earth by comparison |
1.8°
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| 25.19°
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Max: -5°C ( 23°F)
Min: -87°C (-125 °F)
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| Carbon Dioxide, Nitrogen, Argon |
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