Further progress on solar age calibration

Details Further progress on solar age calibration Further progress on solar age calibration

2008-12-30

arxiv.org/abs/0812.5044v1

Astronomy and Astrophysics

Astrophysics

Accepted for publication in Comm. Asteroseis., 2 pages, 1 figure

Scientific paper

We recalibrate a standard solar model seismologically to estimate the
main-sequence age of the Sun. Our procedure differs from what we have done in
the past by removing from the observed frequencies the effect of hydrogen
ionization and the superadiabatic convective boundary layer. Our preliminary
result is $t_\odot=4.63 \pm 0.02$ Gy.

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