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The Impact of Stellar Abundance Variations on Stellar Habitable Zone Evolution
- Publication Year :
- 2012
-
Abstract
- The high quality spectra required for radial velocity planet searches are well-suited to providing abundances for a wide array of elements in large samples of stars. Abundance ratios of the most common elements relative to Fe are observed to vary by more than a factor of two in planet host candidates. This level of variation has a substantial impact on the evolution of the host star and the extent of its habitable zone. We present stellar models of 1 solar mass stars with custom compositions representing the full range of these non-solar abundance ratios. We find that the effects derived from variation over the observed range of [O/Fe] are particularly dramatic. Habitability lifetimes for some classes of orbits can vary by gigayears for the observed range in [O/Fe].<br />Comment: 3 figures, accepted for publication in the Astrophysical Journal Letters
Details
- Database :
- arXiv
- Publication Type :
- Report
- Accession number :
- edsarx.1207.4755
- Document Type :
- Working Paper
- Full Text :
- https://doi.org/10.1088/2041-8205/755/2/L31