Extinct Superheavy Element in Meteorites: Attempted Characterization

Details Extinct Superheavy Element in Meteorites: Attempted Characterization Extinct Superheavy Element in Meteorites: Attempted Characterization

Mar 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972sci...175..981a&link_type=abstract

Science, Volume 175, Issue 4025, pp. 981-983

Computer Science

10

Scientific paper

If the unexplained fission xenon component in meteorites is due to a volatile superheavy element, this element must have had a heat of vaporization of 54 ± 3 kilocalories per mole and a normal boiling point of 2500 degrees ± 400 degrees K. The prime candidates are elements 111 and 115, followed by 113, 114, 112, and 116. Elements 105 to 110 are not volatile enough and can therefore be excluded.

Affiliated with

Also associated with

No associations

Rating

Extinct Superheavy Element in Meteorites: Attempted Characterization 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 Extinct Superheavy Element in Meteorites: Attempted Characterization, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extinct Superheavy Element in Meteorites: Attempted Characterization will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-888668