Titan's Atmosphere and Evolution thru Disk Resolved Spectroscopy

Details Titan's Atmosphere and Evolution thru Disk Resolved Spectroscopy Titan's Atmosphere and Evolution thru Disk Resolved Spectroscopy

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4790l&link_type=abstract

HST Proposal ID #4790

Physics

Hst Proposal Id #4790

Scientific paper

By using disk resolved spectroscopy with HST's HRS, a search for
formaldehyde (CH2O) will be performed on Titan. Formaldehyde is known to
serve as an oligomer to Hydrogen Cyan- ide resulting ultimately in
simple precursors, purines and pyrimidines (e.g., adenine, uracils)
necessary for DNA.

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