The Age of the Universe
Astrophysics
2009-10-30 v1
Abstract
A minimum age of the universe can be estimated directly by determining the age of the oldest objects in the our Galaxy. These objects are the metal-poor stars in the halo of the Milky Way. Recent work on nucleochronology finds that the oldest stars are 15.2+/-3.7 Gyr old. White dwarf cooling curves have found a minimum age for the oldest stars of 8 Gyr. Currently, the best estimate for the age of the oldest stars is based upon the absolute magnitude of the main sequence turn-off in globular clusters. The oldest globular clusters are 11.5+/-1.3 Gyr old, implying a minimum age of the universe of t_universe > 9.5 Gyr (95% confidence level).
Cite
@article{arxiv.astro-ph/9808200,
title = {The Age of the Universe},
author = {Brian Chaboyer},
journal= {arXiv preprint arXiv:astro-ph/9808200},
year = {2009}
}
Comments
invited review to appear in Physics Reports