Log in | Contact us | About us | Site map
What's up home page | The Planets |          

Forthcoming meetings

Speaker Meeting
Date: Friday, June 07, 2013
Time: 19:30
Subject: Strange Weather! Exploring the Giant Planets of our Solar System
Speaker: Dr Leigh Fletcher  (University of Oxford)
Location: United Reformed Church Hall, Newbury
Note: The speaker will be followed by the Society's AGM.
 
Beginners Meeting
No beginners meetings currently scheduled in the diary.
 
Observing Session
No observing sessions currently scheduled in the diary.
 
Special Meeting
Society visit to the national space centre
Date: Saturday, June 08, 2013
Time: 08:30
Location: National Space Centre, Leicester
Note: See the home page for details. Contact Ann Davies for more imformation.
 

 
 


Follow us on Twitter at
@NewburyAstro

Planetary information

Click a planet in the list below and the information will be displayed.

Mercury Venus Mars Jupiter Saturn Uranus Neptune Pluto


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.

 
Discovery: Known by the Ancients
Position from the sun: 4th
Average distance from the Sun: 88,006,827 miles
141,633,260 kilometres
Perihelion:
(Closest point to the sun in orbital path)
128,400,000miles
206,600,000 kilometres
1.40 x Earth by comparison
Aphelion:
(Furthest point from the sun in orbital path)
154,900,000 miles
249,200,000 kilometres
1.64 x Earth by comparison
Equatorial radius of the planet: 2,111 miles
3,397 kilometres
0.53 x Earth by comparison
Plaentary circumference at the equator: 13,263 miles
21,344 kilometres
Volume: 39,139,300,000 miles3
163,140,000,000 kilometres3
0.15 x Earth by comparison
Mass of the planet: 641,850,000,000,000,000,000,000 Kilogrammes
0.11 x Earth by comparison
Density of the planet: 3.94 gm3
0.71 x Earth by comparison
Surface area: 89,500,000 miles2
144,100,000 kilometres2
0.28 x Earth by comparison
Equatorial surface gravity:

12.12 feet/second2
3.69 metres/second2
If you weighed 100 pounds on Earth, you would weigh 38 pounds on Mars

Escape velocity:
(The speed required to achieve orbit)
11,229 miles per hour
18,072 kilometres per hour
0.45 x Earth by comparison
Sidereal Rotation Period:
(Length of Day)
24.62 hours
Sidereal Orbit Period:
(Length of Year)
686.93 Earth days
Orbital velocity:
(The speed at which Mars goes around the Sun)
53,979 miles per hour
86,871.00 kilomtetres per hour
0.81 x Earth by comparison
Orbital Circumference:
(The distance that Mars travels to complete one orbit)
849,400,000 miles
1,366,900,000 kilometres
1.48 x Earth by comparison
Orbital eccentricity:
(How elliptical is Mars's orbit around the Sun)
0.09°
5.59 x Earth by comparison
Orbital inclination:
(How tilted is the orbit of Mars from the plane of the solar system)
1.8°
Equatorial inclination:
(How tilted is Mars itself from a vertical axis)
25.19°
Surface temperature: Max: -5°C ( 23°F)
Min: -87°C (-125 °F)
Contents of the Atmosphere: Carbon Dioxide, Nitrogen, Argon

 

 

 

Website designed by Paul Thompson.
Graphics based on designs by Adrian West.

The site is maintained by Paul Thompson and members of the Society committee.
The Society is a member of the Federation of Astronomical Societies and a registered charity.

Streamline.Net - 100,000 sites hosted, join the revolution! - The home of good value web hosting