Published June 1983 | Version v1
Journal article

The ancient Sun and biogenesis

Description

In this paper evidence is presented that there is a large drop in the surface activity of G-dwarf stars at an age of about 109 years. There are at least five indications that this was also the case for the sun, itself a G-type star. It is suggested that at a critical period in the past the then accentuated UV radiation may have generated HCN in the atmosphere, which, as a result of rain, would fall on the Earth's surface, leading in turn to biogenesis. Before the transition period of approx. 109 years the solar X-ray flux would have been high and the HCN photo-dissociated. (author)

Additional details

Publishing Information

Journal Title
Observatory
Journal Volume
103
Journal Issue
1054
Series
Observatory.
Journal Page Range
160-162
ISSN
0029-7704

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
15000581
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BIOSYNTHESIS; DWARF STARS; EARTH ATMOSPHERE; HYDROCYANIC ACID; SOLAR ACTIVITY; SOLAR RADIATION; STAR EVOLUTION; SUN
Descriptors DEC
HYDROGEN COMPOUNDS; INORGANIC ACIDS; MAIN SEQUENCE STARS; RADIATIONS; STARS; STELLAR RADIATION; SYNTHESIS