Relativistic deflection of background starlight measures the mass of a nearby white dwarf star

Author:

Sahu Kailash C.1ORCID,Anderson Jay1ORCID,Casertano Stefano1,Bond Howard E.2ORCID,Bergeron Pierre3,Nelan Edmund P.1ORCID,Pueyo Laurent1,Brown Thomas M.1ORCID,Bellini Andrea1ORCID,Levay Zoltan G.1ORCID,Sokol Joshua1,Dominik Martin4ORCID,Calamida Annalisa1ORCID,Kains Noé1ORCID,Livio Mario5

Affiliation:

1. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA.

2. Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802, USA.

3. Département de Physique, Université de Montréal, C.P. 6128, Succ. Centre-Ville, Montréal, QC H3C 3J7, Canada.

4. University of St Andrews, School of Physics and Astronomy, North Haugh, St Andrews, KY16 9SS, UK.

5. Department of Physics and Astronomy, University of Nevada, Las Vegas, 4505 South Maryland Parkway, Las Vegas, NV 89154, USA.

Abstract

General relativity weighs a white dwarf Light from a background star is deflected by the gravitational field of the Sun. This effect was used in 1919 to provide some of the first evidence for general relativity. Sahu et al. applied the concept to another star: a nearby white dwarf called Stein 2051 B, which passed close in front of a more distant normal star (see the Perspective by Oswalt). The authors measured the tiny shifts in the apparent position of the background star, an effect called astrometric microlensing. The apparent motion matched the predictions of general relativity, which allowed the authors to determine the mass of the white dwarf. Science , this issue p. 1046 ; see also p. 1015

Funder

National Aeronautics and Space Administration

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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