Pre-biotic molecules in Martian dust clouds

Details Pre-biotic molecules in Martian dust clouds Pre-biotic molecules in Martian dust clouds

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.267..687a&link_type=abstract

Nature, vol. 267, June 23, 1977, p. 687, 688.

Computer Science

1

Abiogenesis, Dust Storms, Extraterrestrial Life, Mars Surface, Organic Compounds, Interstellar Matter, Titanium Compounds, Ultraviolet Absorption

Scientific paper

The possibility is considered that a broad absorption feature centered on a wavelength close to 2200 A, derived from scattering studies of dust clouds observed during the storm at the Martian surface in 1971, may be a signature of highly complex organic or prebiotic molecules. Attention is given to considerations reported by Hoyle and Wickramasinghe (1977) concerning the evolution of a primitive life form in the interstellar medium and studies conducted by Pank and Ajello (1977).

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