HD 140283: A Star in the Solar Neighborhood that Formed Shortly After the Big Bang
Howard E. Bond (1, 2), Edmund P. Nelan (2), Don A. VandenBerg (3),, Gail H. Schaefer (4), and Dianne Harmer (5) ((1) Pennsylvania State, University, (2) Space Telescope Science Institute, (3) University of, Victoria, (4) CHARA Array, Georgia State University, (5) NOAO)

TL;DR
HD 140283 is an ancient, metal-poor star whose precisely measured age of approximately 14.5 billion years suggests it formed shortly after the Big Bang, providing insights into early stellar evolution.
Contribution
This study provides a highly precise age estimate of HD 140283 using advanced parallax measurements and modern stellar models, refining our understanding of early star formation.
Findings
Age of HD 140283 is 14.46 +/- 0.31 Gyr.
The star's age aligns with the Universe's age within uncertainties.
Uncertainties in chemical composition now dominate the age error budget.
Abstract
HD 140283 is an extremely metal-deficient and high-velocity subgiant in the solar neighborhood, having a location in the HR diagram where absolute magnitude is most sensitive to stellar age. Because it is bright, nearby, unreddened, and has a well-determined chemical composition, this star avoids most of the issues involved in age determinations for globular clusters. Using the Fine Guidance Sensors on the Hubble Space Telescope, we have measured a trigonometric parallax of 17.15 +/- 0.14 mas for HD 140283, with an error one-fifth of that determined by the Hipparcos mission. Employing modern theoretical isochrones, which include effects of helium diffusion, revised nuclear reaction rates, and enhanced oxygen abundance, we use the precise distance to infer an age of 14.46 +/- 0.31 Gyr. The quoted error includes only the uncertainty in the parallax, and is for adopted surface oxygen and…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Geophysics and Gravity Measurements · Solar and Space Plasma Dynamics
