Chemical and Biological Studies of Mars Meteorites

Mathematics – Logic

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Mars (Planet), Mars Atmosphere, Planetary Surfaces, Snc Meteorites, Mars Surface, Mars Sample Return Missions, Containment, Mars Surface Samples

Scientific paper

Twelve meteorites, with a total mass of 80 kg, are accepted as having come to Earth from the planet Mars. The meteorites are tied to a common parent body by the ratios of oxygen isotopes in their silicate minerals. These ratios are concordant as well as distinct from those of terrestrial and lunar rocks, and other meteorites. All twelve of the meteorites are igneous rocks, and eleven are geologically young, which indicates that they originated on a planet-sized body. Several of the meteorites contain trapped gas that closely match the composition of the martian atmosphere. Models of hypervelocity impacts on planetary surfaces indicate that a small percentage of the near-surface target material can be ejected into space. These data combine to provide extremely strong support for a martian origin of the meteorite suite. These unsterilized, random samples of Mars have been on Earth for at least 100,000 years and in contact with people for nearly 200 years. However, none of this obviates the statutory requirements for containment and testing of returned martian samples.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Chemical and Biological Studies of Mars Meteorites does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Chemical and Biological Studies of Mars Meteorites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical and Biological Studies of Mars Meteorites will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-893308

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.