Other
Scientific paper
Aug 1973
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.244..560s&link_type=abstract
Nature, Volume 244, Issue 5418, pp. 560 (1973).
Other
Scientific paper
Sagan and Young1 have suggested that the solar neutrino problem and the apparent presence of river channels on Mars may both be resolved by variations of 10% to 20% in the solar luminosity, and they have cited the observed width of the main sequence in Praesepe as evidence that such luminosity excursions have occurred in other solar-type stars. But the main sequence width has previously been interpreted2,3 as due to the observed spread in rotational velocity of the stars. Are these interpretations mutually exclusive or could they be compatible?
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