Mars - The Red Planet, Physical Properties Of Mars, The History Of Mars, A Requiem For Percival Lowell
surface fascinating nasa life
Mars is the fourth planet from the center of the solar system, orbiting the Sun once every 687 (Earth) days at a mean distance of 141 million mi (227 million km). Called the "red planet" for its distinct orange-red color, Mars has been the object of intense interest for over a century. Popularly regarded as a possible source of life, Mars was thought to be barren after the Viking spacecraft landed on it in 1976 and found no evidence of living organisms. But interest in Mars as at least an ancient host of life resurged in the 1990s with the claim of fossilized microbes in meteorites from Mars, and pictures from the 1997 Pathfinder mission that suggested water once swept across the Martian surface.
Mars has numerous earthlike features. There are large, extinct volcanoes dotting its surface, eroded channels where water once flowed freely, and ice caps covering its poles that look very much like Earth's polar regions. But, the thin Martian atmosphere is made mainly of carbon dioxide. Although Mars may now be a cold, dead world, the variety of features on its surface suggests a complex and fascinating past.
Perhaps we will learn more about this fascinating planet when the new NASA Odyssey mission and the two planned NASA Mars Exploration Rover missions launch and reach Mars in the next few years.
Additional Topics
There are three planets other than Earth in the inner solar system. The innermost is Mercury: tiny, barren, and hard to observe as it is located near the Sun. Next comes Venus, the planet nearest in size and mass to Earth, but swathed in clouds; a bland, featureless ball through the small telescope. Mars, half again as far from the Sun as Earth, is different. Features are distinguishable on its su…
The "red planet" is so named because of the color of its surface, which indeed is strikingly red. Simply put, Mars has rusted—iron oxides are responsible for its orange hue. Mars is smaller than Earth. Its diameter of about 2,111 mi (3,397 km) is a little over half that of Earth, and it is only 10% as massive as our planet. Mars has seasons because the tilt of its axis relativ…
The surface features of Mars show that the planet has had an exciting history. Long ago, the surface was volcanically active. Early in the planet's history, it probably had crustal plates moving about as is the case on Earth, but as Mars cooled and its crust thickened, the tectonic activity ceased. The enormous size of Olympus Mons supports this idea. The crust slides over a hot spot, and l…
Until very recently it appeared that Percival Lowell was wrong about the existence of life on Mars. However, in August 1996, a team of scientists at the National Aeronautics and Space Administration's (NASA) Johnson Space Center and at Stanford University announced the discovery of evidence that strongly suggests primitive life may have existed on Mars over 3.6 billion years ago. This evide…
Mars has two tiny satellites, Phobos (27 x 19 km) and Deimos (15 x 11 km). Studies of both show that they are chondritic asteroids that have been captured by Mars gravity (but were originally formed in the main belt of asteroids located beyond Mars). Both are in 1:1 spin orbit couples with Mars, meaning that the same face of these small moons faces Mars all the time. Both satellites have densities…
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