Water On, Water Off
Posted: September 28, 2010 Filed under: astronomers, Astronomical Societies, astronomy, Brian Hynek, Cassini Orbiter, Earth, entertainment, Gaetano Di Achille, John Carter, Mars, NASA, NASA's Mars Reconnaissance Orbiter, Nature Geoscience, Shallow Radar (SHARAD) instrument, Sol, Spirit Mars Rover, the planets, the Red Planet, the solar system, the Universe | Tags: astronomers, astronomy, carbonate, Mars, NASA's Spirit Mars Rover, space scientists, the solar system, water on Mars Leave a comment »
More evidence for the case for the presence of water on the Red Planet
Planetary scientists taking a second look at a Mars outcropping first examined by NASA’s Spirit Mars Rover back in 2005 think there could be additional evidence for water on large areas of Mars. In specific, planetary scientists have found high concentrations of carbonate, a mineral that scientists have previously shown to originate in wet conditions that dissolves in acid. This leads planet scientists to the conclusion that ancient oceans on Mars couldn’t be acidic and could therefore have been favorable environments for the evolution of life forms.
This is hardly news as planet scientists have noted the presence of carbonates on the surface of Mars previously, and there could be all sorts of natural ways to produce the carbonates that we humans haven’t experienced, yet. Reports indicate that scientists are finding rock outcroppings with as much as 25 percent carbonate by weight. This is a far higher percentage of carbonate than previously recorded, though, and this data could indicate the presence of vast oceans on the surface of the Red Planet in the past, according to some scientists.
One group of planet scientists in Boulder, Colorado has been studying the possibility that oceans of water once existed on the Red Planet. Gaetano Di Achille and Brian Hynek have been taking a close look at 52 martian deltas and about 40,000 river valleys on Mars, using the combined data from a series of orbiting Mars missions, conducted over years. Their studies lead them to speculate that broad and deep expanses of water once covered up to one-third of the surface of Mars, 3.5 billion years ago.
This team of astronomers concluded that at least half the deltas and river valleys they studied likely marked the boundaries of an ancient sea. The geological features in question are all at the same relative elevation, which implies they were possibly connected to martian seas or large bodies of water, according to this team of scientists.
The volume of water scientist are talking about once existing on the Red Planet is around 30 million cubic kilometers of water, about 10 times less than the volume of water contained in Earth’s oceans. This study appeared online on June 13 in Nature Geoscience.
John Carter and a team of scientists at the University of Paris, on the other hand, claim that the Red Planet certainly once had vast quantities of water, only not in the form of vast seas and oceans. This team found hydrated silicate minerals within craters on the northern lowlands of the Red Planet, a place where these minerals hadn’t previously been found. This fact, combined with previous indications of hydrated silicate minerals in Mars Southern Hemisphere, leads this team of scientists to conclude that Mars was changed on a global scale by liquid water around 4 billion years in the past. This group of astronomers used NASA’s Mars Reconnaissance Orbiter to look inside 91 impact craters where asteroids have exposed ancient marine material several kilometers beneath the surface of Mars. They found nine contained phyllosilicates or other hydrated silicates, minerals that scientists know form in wet environments.
The real question now is, where did all this water go? Future missions to the Red Planet will be looking for facts to help determine where all the water went or if it might still might exist on Mars, in another form. They’ll also be taking a close look at river deltas, which could be excellent regions to search for evidence of past Martian life.
The Windswept Northern Polar Cap of Mars
Posted: September 12, 2010 Filed under: Chasma Boreale, Earth, Mars, NASA, NASA's Mars Reconnaissance Orbiter, north polar cap, Shallow Radar (SHARAD) instrument, Sol, the Milky Way galaxy, the planets, the solar system, the Universe | Tags: Chasma Boreale, Mars, NASA, NASA;s Mars Reconnaissance Orbiter, north polar cap, SHADAR, Shallow Radar instrument, spiral troughs Leave a comment »Astronomical News –
Scientists using the Shallow Radar (SHARAD) instrument on NASA’s Mars Reconnaissance Orbiter to look beneath Mar’s north polar ice cap and get an idea of the lay of the ground think they know how Chasma Boreale and the much discussed series of spiral troughs were formed. The formation of Chasma Boreale and enigmatic spiral troughs have been talked about for four decades by space scientists and amateur astronomers. Mar’s north polar region is really just a stack of ice and dust layers up to 2 miles thick and encompassing an area equivalent to Texas. Chasma Boreale is a distinctive land feature as long as the Grand Canyon, only wider and deeper, while the troughs spiral outward from their centers like huge pinwheels.
What did astronomers and planet scientists using SHARAD to look beneath Mar’s north polar cap reveal about the formation of Chasma Boreale and associated spiral troughs? The view beneath Mar’s north polar cap suggests strong winds were the main force of geological change involved in the formation of the Chasma Boreale and spiral troughs over millions of years. The geological processes involved would have formed Chasma Boreale and spiral troughs as Mar’s north polar ice cap was formed, according to space scientists.


