GSTDTAP  > 地球科学
DOI10.1126/science.aal2879
Relativistic deflection of background starlight measures the mass of a nearby white dwarf star
Sahu, Kailash C.1; Anderson, Jay1; Casertano, Stefano1; Bond, Howard E.2; Bergeron, Pierre3; Nelan, Edmund P.1; Pueyo, Laurent1; Brown, Thomas M.1; Bellini, Andrea1; Levay, Zoltan G.1; Sokol, Joshua1; Dominik, Martin4; Calamida, Annalisa1; Kains, Noe1; Livio, Mario5
2017-06-09
发表期刊SCIENCE
ISSN0036-8075
EISSN1095-9203
出版年2017
卷号356期号:6342页码:1046-1050
文章类型Article
语种英语
国家USA; Canada; Scotland
英文摘要

Gravitational deflection of starlight around the Sun during the 1919 total solar eclipse provided measurements that confirmed Einstein's general theory of relativity. We have used the Hubble Space Telescope to measure the analogous process of astrometric microlensing caused by a nearby star, the white dwarf Stein 2051 B. As Stein 2051 B passed closely in front of a background star, the background star's position was deflected. Measurement of this deflection at multiple epochs allowed us to determine the mass of Stein 2051 B-the sixth-nearest white dwarf to the Sun-as 0.675 +/- 0.051 solar masses. This mass determination provides confirmation of the physics of degenerate matter and lends support to white dwarf evolutionary theory.


领域地球科学 ; 气候变化 ; 资源环境
收录类别SCI-E
WOS记录号WOS:000402871700047
WOS关键词HUBBLE-SPACE-TELESCOPE ; RADIUS RELATION ; MICROLENSING EVENTS ; PROPER MOTIONS ; GALACTIC HALO ; ASTROMETRY ; CATALOG ; SYSTEM ; CONSTRAINTS ; ISOCHRONES
WOS类目Multidisciplinary Sciences
WOS研究方向Science & Technology - Other Topics
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文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/196217
专题地球科学
资源环境科学
气候变化
作者单位1.Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA;
2.Penn State Univ, Dept Astron & Astrophys, 525 Davey Lab, University Pk, PA 16802 USA;
3.Univ Montreal, Dept Phys, CP 6128,Succ Ctr Ville, Montreal, PQ H3C 3J7, Canada;
4.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland;
5.Univ Nevada, Dept Phys & Astron, 4505 South Maryland Pkwy, Las Vegas, NV 89154 USA
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Sahu, Kailash C.,Anderson, Jay,Casertano, Stefano,et al. Relativistic deflection of background starlight measures the mass of a nearby white dwarf star[J]. SCIENCE,2017,356(6342):1046-1050.
APA Sahu, Kailash C..,Anderson, Jay.,Casertano, Stefano.,Bond, Howard E..,Bergeron, Pierre.,...&Livio, Mario.(2017).Relativistic deflection of background starlight measures the mass of a nearby white dwarf star.SCIENCE,356(6342),1046-1050.
MLA Sahu, Kailash C.,et al."Relativistic deflection of background starlight measures the mass of a nearby white dwarf star".SCIENCE 356.6342(2017):1046-1050.
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