A 2-3 meter chunk of rock does this on Mars.
posted December 30, 2006 - 10:07pmThis is what happens on Mars when a 2 to 3 meter diameter chunk of rock traverses the thin Martian atmosphere and impacts the surface of Mars.
On Earth it is unlikely that the chunk of rock would have made it through the atmosphere. It would not make a crater, but chunks of it might go through a house roof, if they made it to the surface. On Venus, unless nickel-iron, the rock would be pulverized by impacting the thick, heavy, very dense atmosphere of Venus.
All images courtesy of the American Taxpayer and NASA, JPL and sub-contractors you and I support.
All images: Taxpayer paid for NASA, JPL and sub contractors at taxpayer expense. America, these images belong to YOU.)
The Martian atmosphere is old, unique, and compared to Earth's, atmosphere, very different in composition. It is old, in the sense that it has not changed much in hundreds of millions of years. It is unique, as are the atmospheres of all the Sun's Planets.
Those white circles are 7.5 miles in diameter, and better images will soon be available.
The Earth's atmosphere is composed of:
78% N2 Nitrogen
21% O2 Oxygen
and the rest are trace gases, with Argon having the largest share. But Mars' thin air is different than Earths!
The Martian atmosphere is composed of:
---95.3% - CO2 carbon dioxide
----2.7% - N2 Nitrogen
----1.6% - Ar Argon
99.6%
Trace:
O2 Oxygen
CO Carbon monoxide
H20 Water vapor
Other gases in signature amounts make up the remainder.
That is why, after Viking, it was possible to with certainty find meteorites on Earth that were chips off the Red Planet, ejected by impacts and propelled into space and eventually plummet to Earth.
The pressure of the Martian Air is less than 1/100th of the average surface pressure of Earth's atmosphere. The daily and seasonal temperature changes are dramatic, ranging from roughly 220 K (-64 degrees F) daytime to 145 K (-199 degrees F)at night. At perihelion, on the Martian equator it can near local noon reach 300 K (80 degrees F). That is practically a shirt-sleeve temperature.
That thin signature of Martian air offers little protection from rocks and chips of things from the asteroid belt that collide with Mars. Chips and pieces of asteroids from both major and minor collisions in the asteroid belt along with an ever shifting arrangement of orbits and harmonic orbits make sure the supply of particles to collide with mars is essentially inexhaustible.
This image, on the left, is a basketball-sized nickel-iron meteorite on Mars. It is the first of its kind discovered elsewhere off Earth. These are the dangerous kinds of things that fall from space, but here in this picture from Mars, this one appears to be intact and not much changed from the time it formed when our solar system was being made. It takes a lot of velocity and energy of impact to vaporize a chunk of matter like this. The ones we see making new little craters on Mars, are likely a softer rock. But big ones do fall.
Millions of years of weathering have likely uncovered it, revealing the bubbles of its formation, as well as the gouges maybe polished by a short trip through even an ancient Martian atmosphere. We see these in our museums here on Earth.
The top image shows what a chunk of probably chondritic rock ten times the linear size of this nickel-iron basketball sized chunk of matter can do, striking the nearly naked surface of Mars.
More images and details will emerge as satellite investigators explore the Martian Surface in ever greater detail.

Comments
But only Mars amongst Earth's siblings has close promise.
If they are nickel-iron they are potentially valuable as a new
Mars in my yard?
Lady:P
I found a rock like that in my backyard the other day.
Antonia Dwells
That's interesting..
Michele G.
http://www.youtube.com/user/megwynn4153
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