Minimum Times to Form Clay in Martian Surface and Near-Surface Environments

Details Minimum Times to Form Clay in Martian Surface and Near-Surface Environments Minimum Times to Form Clay in Martian Surface and Near-Surface Environments

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1708b&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1708

Computer Science

1

Scientific paper

We estimate the minimum time required to produce detectable amounts of
clay by aqueous alteration of volcanic glasses under different sets of
idealized Martian conditions. The effects of glass composition,
alteration temperature, pH, and grain size on reaction rates are
considered.

Affiliated with

Also associated with

No associations

Rating

Minimum Times to Form Clay in Martian Surface and Near-Surface Environments 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 Minimum Times to Form Clay in Martian Surface and Near-Surface Environments, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Minimum Times to Form Clay in Martian Surface and Near-Surface Environments will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1856710