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Age of the sun

The Astrophysical JournalPublished 1 April 1989
D. B. Guenther
Citations45
SJR quartileQ1
SJR score2.04
SNIP1.25

Abstract

view Abstract Citations (78) References (9) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Age of the Sun Guenther, D. B. Abstract The age of the sun is deduced to be 4.49 + or - 0.04 Gyr. This determination is based on the ages of the oldest meteorites, current models of solar system formation, and the premain-sequence evolution of a 1-solar-mass star from T Tauri phase to the ZAMS. Prior to this it was common to use an age of 4.7 Gyr for the sun. Comparing a solar model evolved to 4.5 Gyr with a model evolved to 4.7 Gyr shows that the 200 Myr difference in their ages has very little effect on the helium abundance and mixing-length parameters of the solar models. Publication: The Astrophysical Journal Pub Date: April 1989 DOI: 10.1086/167370 Bibcode: 1989ApJ...339.1156G Keywords: Meteorites; Solar Interior; Stellar Evolution; Helium; Solar Oscillations; Stellar Models; Solar Physics; METEORS AND METEORITES; STARS: EVOLUTION; SUN: INTERIOR; SUN: OSCILLATIONS full text sources ADS |

Keywords

Physics and Astronomy