Astronomy:Stein 2051

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Short description: Star in the constellation Camelopardalis

Coordinates: Sky map 04h 31m 11.52059s, +58° 58′ 37.4806″

Stein 2051
Einstein revisited.jpg
Image of Stein 2051 B and a background star taken by the Hubble Space Telescope.[1]
Credit: NASA, ESA, and K. Sahu (STScI)
Observation data
{{#ifeq:J2000|J2000.0 (ICRS)|Epoch J2000.0      Equinox J2000.0 (ICRS)| [[History:Epoch|Epoch J2000]]      [[Astronomy:Equinox (celestial coordinates)|Equinox J2000}}
Constellation Camelopardalis
Stein 2051 A
Right ascension  04h 31m 11.5181s[2]
Declination +58° 58′ 37.461″[2]
Apparent magnitude (V) 10.977[2]
Stein 2051 B
Right ascension  04h 31m 12.570s[3]
Declination +58° 58′ 41.15″[3]
Apparent magnitude (V) 11.19[3]
Characteristics
Stein 2051 A
Spectral type M4.0Ve[2]
U−B color index +1.21[4]
B−V color index +1.65[4]
Stein 2051 B
Spectral type DC5[3]
U−B color index -0.53[4]
B−V color index +0.31[4]
Astrometry
Stein 2051 A
Radial velocity (Rv)29 km/s
Proper motion (μ) RA: 1300.365[5] mas/yr
Dec.: -2046.106[5] mas/yr
Parallax (π)181.2438 ± 0.0499[5] mas
Distance17.995 ± 0.005 ly
(5.517 ± 0.002 pc)
Stein 2051 B
Radial velocity (Rv)2.0 km/s
Proper motion (μ) RA: 1334.780±0.021[6] mas/yr
Dec.: −1947.638±0.019[6] mas/yr
Parallax (π)181.2730 ± 0.0203[6] mas
Distance17.993 ± 0.002 ly
(5.5165 ± 0.0006 pc)
Details[7]
Stein 2051 A
Mass0.252±0.013[8] M
Radius0.292±0.031[8] R
Luminosity0.0081[8] L
Surface gravity (log g)4.80+0.13−0.10 cgs
Temperature3277+42−75 K
Metallicity [Fe/H]0.26+0.06−0.22 dex
Rotational velocity (v sin i)5.2+1.7−2.7 km/s
Stein 2051 B
Mass0.675±0.051[9] M
Radius0.0114±0.0004[9] R
Temperature7122±181[9] K
Other designations
Stein 2051, G 175-34, HIP 21088,[10] WDS J04312+5858AB, GJ 169.1,[11] PLX 986.01[12]
Stein 2051 A: LHS 26, NLTT 13373, TYC 3744-412-1, 2MASS J04311147+585837, WISE J043113.20+585816.7[2]
Stein 2051 B: EGGR 180, LHS 27, NLTT 13375, TYC 3744-2062-1, 2MASS J04311201+5858476, WD 0426+58, WD2 0426+585, WD3 0426+588[3]
Database references
SIMBADThe system
A
B
Stein 2051 is located in the constellation Camelopardalis
Stein 2051 is located in the constellation Camelopardalis
Stein 2051
Location of Stein 2051 in the constellation Camelopardalis

Stein 2051 (Gliese 169.1, G 175-034, LHS 26/27) is a nearby binary star system, containing a red dwarf (component A) and a degenerate star (white dwarf) (component B), located in constellation Camelopardalis at about 18 ly from Earth.[12]

Stein 2051 is the nearest (red dwarf + white dwarf) separate binary system (40 Eridani BC is located closer at 16.26 light-years,[13] but it is a part of a triple star system).

Stein 2051 B is the 6th nearest white dwarf after Sirius B, Procyon B, van Maanen's star, LP 145-141 and 40 Eridani B.

Properties

The brighter of this two stars is A (a red dwarf), but the more massive is component B (a white dwarf).

In 2017, Stein 2051 B was observed passing in front of a more distant star. The bending of starlight by the gravitational field of the nearer star allowed its mass to be directly measured. The estimated mass of Stein 2051 B is 0.675±0.051 M, which fits the expected range of a white dwarf with a carbon-oxygen core.[9]

References

  1. "Einstein revisited". https://www.spacetelescope.org/images/potw1724a/. 
  2. 2.0 2.1 2.2 2.3 2.4 "NAME Stein 2051 A". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NAME+Stein+2051+A. 
  3. 3.0 3.1 3.2 3.3 3.4 "NAME Stein 2051 B". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NAME+Stein+2051+B. 
  4. 4.0 4.1 4.2 4.3 Hardie, R. H. (1966). "UBV Photometry of the Lowell Proper Motion Object G175-34". Publications of the Astronomical Society of the Pacific 78 (462): 171. doi:10.1086/128321. Bibcode1966PASP...78..171H. 
  5. 5.0 5.1 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.
  6. 6.0 6.1 6.2 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.
  7. Passegger, V. M.; Bello-García, A.; Ordieres-Meré, J.; Caballero, J. A.; Schweitzer, A.; González-Marcos, A.; Ribas, I.; Reiners, A. et al. (2020), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics 642: A22, doi:10.1051/0004-6361/202038787 
  8. 8.0 8.1 8.2 Ghosh, Samrat; Ghosh, Supriyo; Das, Ramkrishna; Mondal, Soumen; Khata, Dhrimadri (2020), "Understanding the physical properties of young M dwarfs: NIR spectroscopic studies", Monthly Notices of the Royal Astronomical Society 493 (3): 4533–4550, doi:10.1093/mnras/staa427, Bibcode2020MNRAS.493.4533K 
  9. 9.0 9.1 9.2 9.3 Sahu, Kailash C. et al. (June 2017), "Relativistic deflection of background starlight measures the mass of a nearby white dwarf star", Science 356 (6342): 1046–1050, doi:10.1126/science.aal2879, PMID 28592430, Bibcode2017Sci...356.1046S. 
  10. Perryman (1997). "HIP 21088". The Hipparcos and Tycho Catalogues. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=I/239/hip_main&HIP=21088. 
  11. "Gl 169.1". Preliminary Version of the Third Catalogue of Nearby Stars. 1991. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=V/70A&Name=Gl%20169.1. 
  12. 12.0 12.1 "GCTP 986.01". The General Catalogue of Trigonometric Stellar Parallaxes. 1995. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=I/238A/picat&GCTP=986.01. 
  13. Perryman (1997). "HIP 19849". The Hipparcos and Tycho Catalogues. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=I/239/hip_main&HIP=19849. 

External links