Carbonic Acid Stability In Solar System Ices

Biology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Scientific paper

Carbonic acid (H2CO3) is a major product of energetically processed ices containing H2O and CO2. It is thermally stable at 200 K, higher than the sublimation temperature of H2O. Ices containing both H2O and CO2 have been found on a variety of surfaces such as those of Europa, Callisto, Iapetus, and Mars, where processing by magnetospheric ions or the solar wind may lead to the formation of H2CO3. We have investigated the stability of carbonic acid at 14 K, 100 K, and 200 K upon irradiation with 0.8 MeV protons. The energy deposited into the ice by the incident proton beam not only destroys H2CO3, but also amorphizes the crystalline phase of the solid. The radiation destruction and amorphization processes will be discussed along with an estimate for the expected lifetimes of H2CO3 on the surfaces of different solar system bodies.
This research is funded through NASA's Mars Fundamental Research Program and the Goddard Center for Astrobiology.

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

Carbonic Acid Stability In Solar System Ices 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 Carbonic Acid Stability In Solar System Ices, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Carbonic Acid Stability In Solar System Ices will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1439446

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