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Curiosity - Mars Science Laboratory
* Mission goal is to determine whether Mars has ever had the conditions to support life
* Project costed at $2.5bn; will see initial surface operations lasting two Earth years
* Onboard plutonium generators will deliver heat and electricity for at least 14 years
* 75kg science payload more than 10 times as massive as those of earlier US Mars rovers
* Equipped with tools to brush and drill into rocks, to scoop up, sort and sieve samples
* Variety of analytical techniques to discern chemistry in rocks, soil and atmosphere
* Will try to make first definitive identification of organic (carbon rich) compounds
* Even carries a laser to zap rocks; beam will identify atomic elements in rocks
* Discover more about the planets
Mars
Mars is the fourth planet from the Sun in the Solar System. Named after the Roman
god of war , Mars , it is often described as the "Red Planet" as the iron oxide prevalent on its surface gives it
a reddish appearance Mars is a terrestrial planet with a thin atmosphere having surface features reminiscent both of the impact craters of the Moon and the
volcanoes, valleys, deserts, and polar ice caps of Earth . The rotational period and
seasonal cycles of Mars are likewise similar to those of Earth, as is
the tilt that produces the seasons. Mars can easily be seen from Earth with the naked eye. Its apparent magnitude, which is only surpassed by Jupiter, Venus , the Moon, and the Sun. Optical
ground-based telescopes are typically limited to resolving features about 300 km (186 miles) across when Earth and Mars are
closest
Mars has two moons, Phobos and Deimos, which are small and irregularly shaped. These may
be captured asteroids , similar to 5261 Eureka, a Martian trojan asteroid.
The composition of Mars: 95.32% carbon dioxide , 2.7% nitrogen, 1.6% argon, 0.13% oxygen, 0.08% carbon monoxide,
210 ppm water vapor, 100 ppm nitric oxide,15 ppm molecular hydrogen
Until the first successful flyby of Mars occurred in 1965, by Mariner 4, many speculated about the presence of liquid water on the planet's surface.
In 2005, radar data revealed the presence of large quantities of water ice at the poles,
and at mid-latitudes. The Mars rover Spirit sampled chemical compounds
containing water molecules in March 2007. The Phoenix lander sampled water ice in shallow Martian soil on July 31, 2008. |
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