Praesepe and the Solar Neutrino Problem

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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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