Gliese 832 (Gl 832 or GJ 832) is a red dwarf (spectrum M1.5V) in the constellation Grus. It is located relatively close to the Sun, at a distance of 16.1 light years. Gliese 832 has about half the mass and radius of the Sun.
Planetary system
In September 2008, it was announced that a Jupiter-like planet had been detected in a long-period, near-circular orbit around this star (false alarm probability thus far: a negligible 0.05%). It would induce an astrometric perturbation on its star of at least 0.95 milliarcseconds and is thus a good candidate for being detected by astrometric observations. Among currently-known exoplanets, it would have an angular distance from its star second only to Epsilon Eridani b, although direct imaging is problematic due to the star–planet contrast.[2]
If this system has a comet disc, it is undetectable "brighter than the fractional dust luminosity 10−5" of a recent Herschel study.[5]
X-ray source
Gliese 832 emits X-rays.[6]
See also
Notes
- ↑ From L = 4πR2σTeff4, where L is the luminosity, R is the radius, Teff is the effective surface temperature and σ is the Stefan–Boltzmann constant.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Bailey, J.; Butler, R. P.; Tinney, C. G.; Jones, H. R. A.; O'Toole, S.; Carter, B. D.; Marcy, G. W. (2008). "A Jupiter-like Planet Orbiting the Nearby M Dwarf GJ832". The Astrophysical Journal 690 (1): 743–747. arXiv:0809.0172. Bibcode:2009ApJ...690..743B. doi:10.1088/0004-637X/690/1/743.
- ↑ Johnson, H. M.; Wright, C. D. (1983). "Predicted infrared brightness of stars within 25 parsecs of the sun". The Astrophysical Journal Supplement Series 53: 643–771. Bibcode:1983ApJS...53..643J. doi:10.1086/190905.
- ↑ Interpolated value from NASA Exoplanet Archive, per: Bessell, M. S. (1995). "The Temperature Scale for Cool Dwarfs". In Tinney, C. G. The Bottom of the Main Sequence - and Beyond, Proceedings of the ESO Workshop. Springer-Verlag. p. 123. Bibcode:1995bmsb.conf..123B.
- ↑ B. C. Matthews; forthcoming study promised in Lestrade, J.-F.; et al. (2012). "A DEBRIS Disk Around The Planet Hosting M-star GJ581 Spatially Resolved with Herschel". Astronomy and Astrophysics 548: A86. arXiv:1211.4898. Bibcode:2012A&A...548A..86L. doi:10.1051/0004-6361/201220325.
- ↑ Schmitt, J. H. M. M.; Fleming, T. A.; Giampapa, M. S. (1995). "The X-ray view of the low-mass stars in the solar neighborhood". The Astrophysical Journal 450 (9): 392–400. Bibcode:1995ApJ...450..392S. doi:10.1086/176149.
Coordinates: 21h 33m 33.9752s, −49° 00′ 32.422″
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- Sirius (8.60 ± 0.04 ly; 2 stars)
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- Tau Ceti (11.905 ± 0.007 ly; 1 star, 5? planets: b
- c
- d
- e
- f)
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- Altair (16.73 ± 0.05 ly; 1 star)
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- Gliese 876 (15.21 ± 0.04 ly; 1 star, 4 planets: d
- c
- b
- e)
- GJ 1002 (15.31 ± 0.26 ly; 1 star)
- LHS 288 (15.55 ± 0.20 ly; 1 star)
- Gliese 412 (15.81 ± 0.08 ly; 2 stars)
- AD Leonis (15.94 ± 0.22 ly; 1 star)
- Gliese 832 (16.16 ± 0.08 ly; 1 star, 1 planet: b)
- EV Lacertae (16.46 ± 0.07 ly; 1 star)
- Gliese 682 (16.60 ± 0.20 ly; 1 star)
- GJ 1116 (17.06 ± 0.23 ly; 2 stars)
- GJ 3379 (17.10 ± 0.17 ly; 1 star)
- LHS 1723 (17.36 ± 0.12 ly; 1 star)
- Gliese 445 (17.42 ± 0.15 ly; 1 star)
- Wolf 498 (17.66 ± 0.07 ly; 1 star)
- Stein 2051 (18.07 ± 0.08 ly; 2 stars)
- Gliese 251 (18.31 ± 0.15 ly; 1 star)
- Gliese 205 (18.53 ± 0.11 ly; 1 star)
- L 449-1 (18.6 ± 3.9 ly; 1 star)
- LP 816-060 (18.63 ± 0.37 ly; 1 star)
- Gliese 229 (18.77 ± 0.11 ly; 1 star, 1 brown dwarf)
- Ross 47 (19.02 ± 0.11 ly; 1 star)
- Gliese 693 (19.06 ± 0.25 ly; 1 star)
- Gliese 752 (19.08 ± 0.06 ly; 2 stars: A
- B (vB 10))
- Gliese 754 (19.28 ± 0.18 ly; 1 star)
- Gliese 588 (19.35 ± 0.15 ly; 1 star)
- GJ 1005 (19.37 ± 0.10 ly; 2 stars)
- Gliese 908 (19.41 ± 0.14 ly; 1 star)
- YZ Canis Minoris (19.51 ± 0.24 ly; 1 star)
- 2MASS J05332802-4257205 (~19.6 ly; 1 star)
- 2MASS J18450079-1409036 (~19.6 ly; 2 stars)
- Gliese 338 (19.92 ± 0.31 ly; 2 stars)
- Gliese 268 (19.96 ± 0.22 ly; 2 stars)
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- Gliese 784 (20.22 ± 0.13 ly; 1 star)
- HN Librae (20.29 ± 0.25 ly; 1 star)
- Gliese 581 (20.38 ± 0.21 ly; 1 star, 4 (6?) planets: e
- b
- c
- g?
- d
- f?)
- EQ Pegasi (20.40 ± 0.20 ly; 2 stars)
- LHS 2090 (20.8 ± 0.4 ly; 1 star)
- LHS 337 (20.8 ± 0.3 ly; 1 star)
- Furuhjelm 46 (20.9 ± 0.2 ly; 2 stars)
- G 180-060 (20.9 ± 0.6 ly; 1 star)
- V1054 Ophiuchi (21.05 ± 0.07 ly; 5 stars: Ba
- Bb
- A
- Gl 643
- C (vB 8))
- LP 71-82 (~21.2 ly; 1 star)
- G 161-71 (~21.3 ly; 1 star)
- Gliese 625 (21.3 ± 0.2 ly; 1 star)
- GJ 1128 (21.3 ± 0.4 ly; 1 star)
- GL Virginis (21.3 ± 0.4 ly; 1 star)
- LHS 3003 (21.4 ± 0.3 ly; 1 star)
- Gliese 408 (21.8 ± 0.3 ly; 1 star)
- SCR J1546−5534 (~21.9 ly; 1 star)
- Gliese 829 (21.9 ± 0.3 ly; 2 stars)
- G 41-14 (22.1 ± 0.3 ly; 3 stars)
- EE Leonis (22.2 ± 0.5 ly; 1 star)
- Gliese 880 (22.3 ± 0.2 ly; 2 stars)
- Gliese 299 (22.3 ± 0.5 ly; 1 star)
- LP 771-095 (22.7 ± 0.4 ly; 3 stars)
- GJ 1068 (22.7 ± 0.3 ly; 1 star)
- 2MASS J20360829-3607115 (~22.8 ly; 1 star)
- L 369-44 (~22.8 ly; 2 stars)
- 2MASS J18522528-3730363 (~22.8 ly; 1 star)
- G 161-7 (~22.8 ly; 2 stars)
- Gliese 809 (23.0 ± 0.1 ly; 2 stars)
- Gliese 393 (23.0 ± 0.4 ly; 1 star)
- Gliese 54 (23.1 ± 0.6 ly; 2 stars)
- SCR J0740−4257 (~23.5 ly; 1 star)
- L 43-72 (23.5 ± 4.9 ly; 1 star)
- GJ 1286 (23.6 ± 0.6 ly; 1 star)
- GJ 4063 (23.6+9.6
−5.3 ly; 1 star)
- GJ 4053 (23.7 ± 0.9 ly; 1 star)
- GJ 4274 (24.3 ± 0.9 ly; 1 star)
- GJ 3991 (24.28 ± 0.36 ly; 2 stars)
- GJ 4248 (24.29 ± 0.24 ly; 1 star)
- Gliese 109 (24.5 ± 0.4 ly; 1 star)
- GJ 1224 (24.6 ± 0.7 ly; 1 star)
- GJ 3378 (24.7 ± 0.5 ly; 1 star)
- Gliese 514 (24.97 ± 0.20 ly; 1 star)
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K (Orange) |
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| V |
- Gliese 673 (25.12 ± 0.14 ly; 1 star)
- Gliese 884 (26.6 ± 0.3 ly; 1 star)
- p Eridani (26.57 ± 0.31 ly; 2 stars)
- Gliese 250 (28.4 ± 0.3 ly; 2 stars)
- HR 1614 (28.8 ± 0.3 ly; 1 star)
- HR 7722 (28.8 ± 0.3 ly; 1 star, 2 planets: b
- c)
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- LHS 1070 (25.2 ± 0.5 ly; 3 stars)
- Gliese 701 (25.3 ± 0.3 ly; 1 star)
- GJ 1093 (25.3 ± 0.7 ly; 1 star)
- Gliese 480.1 (25.4 ± 0.8 ly; 1 star)
- SIPS 1259-4336 (25.4 ± 0.2 ly; 1 star)
- Gliese 382 (25.48 ± 0.30 ly; 1 star)
- DG Canum Venaticorum (25.9+5.5
−3.8 ly; 1 star)
- Wolf 922 (25.9 ± 0.5 ly; 2 stars)
- Gliese 300 (25.97 ± 0.20 ly; 1 star)
- SSSPM J1138-7722 (26 ± 3 ly; 1 star)
- Gliese 793 (26.08 ly; 1 star)
- 2MASS J12140866-2345172 (~26.1 ly; 1 star)
- 2MASS J19513587-3510375 (~26.1 ly; 1 star)
- SCR 0838-5855 (~26.1 ly; 1 star)
- Gliese 257 (26.2 ± 0.6 ly; 2 stars)
- Gliese 623 (26.2 ± 0.3 ly; 2 stars)
- GJ 1289 (26.4 ± 0.6 ly; 1 star)
- GJ 1105 (26.4 ± 0.7 ly; 1 star)
- Gliese 686 (26.5 ± 0.4 ly; 1 star)
- Gliese 493.1 (26.6 ± 1.0 ly; 1 star)
- Gliese 48 (26.6 ± 0.3 ly; 1 star)
- Gliese 747 (26.6 ± 0.4 ly; 2 stars)
- SCR 1138-7721 (26.7 ± 0.7 ly; 1 star)
- Gliese 486 (26.8 ± 0.6 ly; 1 star)
- GJ 1151 (26.8 ± 0.7 ly; 1 star)
- GJ 1227 (26.9 ± 0.4 ly; 1 star)
- GJ 1230 (27.0+1.7
−1.5 ly; 3 stars)
- Gliese 232 (27.2 ± 0.4 ly; 1 star)
- AP Columbae (27.4 ± 0.2 ly; 1 star)
- GJ 3146 (27.6 ± 1.7 ly; 1 star)
- GJ 1154 (27.6 ± 0.9 ly; 1 star)
- GJ 1057 (27.6 ± 0.9 ly; 1 star)
- Gliese 618 (27.6 ± 0.6 ly; 2 stars)
- GJ 3076 (27.6+6.0
−4.2 ly; 1 star)
- SCR 0640-0552 (~27.7 ly; 1 star)
- HD 32450 (27.8 ± 0.4 ly; 2 stars)
- Gliese 450 (27.9 ± 0.3 ly; 1 star)
- Gliese 877 (28.1 ± 0.3 ly; 1 star)
- Gliese 745 (28.1 ± 0.6 ly; 2 stars)
- Gliese 867 (28.2 ± 0.4 ly; 2 stars)
- GJ 3454 (28.2 ± 0.2 ly; 2 stars)
- SCR 0630-7643 (28.6 ± 0.5 ly; 2 stars)
- HU Delphini (28.6 ± 0.5 ly; 2 stars)
- LDS 169 (28.6 ± 0.8 ly; 2 stars)
- Gliese 849 (28.6 ± 0.5 ly; 1 star, 2 planets: b
- c)
- GJ 1103 (28.7 ± 0.8 ly; 2 stars)
- GJ 1207 (28.8 ± 0.4 ly; 1 star)
- Gliese 465 (29.0 ± 0.7 ly; 1 star)
- GJ 1277 (29.0 ± 4.6 ly; 1 star)
- GJ 3128 (29.1 ± 0.5 ly; 1 star)
- V374 Pegasi (29.1 ± 0.9 ly; 1 star)
- Gliese 357 (29.3 ± 0.5 ly; 1 star)
- Gliese 595 (29.4 ± 3.5 ly; 1 star)
- Gliese 433 (29.5 ± 0.5 ly; 1 star, 2 planets: b
- c)
- Gliese 424 (29.7 ± 0.3 ly; 1 star)
- GJ 3801 (29.7 ± 0.9 ly; 1 star)
- GJ 2066 (29.9 ± 0.5 ly; 1 star)
- LHS 224 (29.9 ± 0.8 ly; 2 stars)
- SCR 1826-6542 (~30 ly; 1 star)
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DA |
- G 99-47 (26.1 ± 0.8 ly; 1 star)
- WD 2359-434 (26.7 ± 0.3 ly; 1 star)
- Gliese 318 (28.7 ± 0.5 ly; 1 star)
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| DC | |
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| DQ |
- LHS 1126 (29.5 ± 0.3 ly; 1 star)
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| DZ |
- Wolf 489 (26.9 ± 0.8 ly; 1 star)
- LP 701-29 (27.9 ± 0.2 ly; 1 star)
- L 745-46 (29.7 ± 0.2 ly; 2 stars)
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M |
- DENIS 0334-49 (27.04 ± 0.83 ly; 1 brown dwarf)
- GJ 3517 (27.8 ± 0.4 ly; 1 brown dwarf)
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| L | |
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| T |
- 2MASS 0348-6022 (~25.4 ly; 1 brown dwarf)
- 2MASS 0729-39 (25.8 ± 1.8 ly; 1 brown dwarf)
- UGPS J0521+3640 (26.7+3.9
−3.2 ly; 1 brown dwarf)
- WISE 0313+7807 (~28.0 ly; 1 brown dwarf)
- 2MASS 0727+1710 (29.0 ± 0.2 ly; 1 brown dwarf)
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| Y |
- WISE 1405+5534 (25.3+4.4
−3.2 ly; 1 brown dwarf)
- WISE 2220-3628 (~26.4 ly; 1 brown dwarf)
- WISE 0647-6232 (28.4+3.3
−2.7 ly; 1 brown dwarf)
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In left column are stellar classes of primary members of star systems. Bold are systems containing at least one component with absolute magnitude of +8.5 or brighter. Italic are systems without known trigonometric parallax. |
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| Bayer | |
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| Variable |
- U
- W
- RS
- RZ
- BC
- BP
- BZ
- CE
- DL
- DQ
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| HR |
- 8236
- 8241
- 8299
- 8323
- 8366
- 8379
- 8440
- 8477
- 8484
- 8501
- 8635
- 8639
- 8657
- 8658
- 8659
- 8685
- 8713
- 8749
- 8760
- 8771
- 8791
- 8793
- 8814
- 8835
- 8846
- 8847
- 8877
- 8896
- 8898
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| HD | |
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| Gliese | |
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| Other | |
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