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==Distance== | ==Distance== | ||
{| class="wikitable" | |||
{{πt}} | |||
|+ Gliese 832 distance estimates | |||
|- | |||
! Source !! Parallax, ] !! Distance, ] !! Distance, ] !! Distance, ] !! Ref. | |||
{{πp|wo|214|7|<ref name="Woolley1970">{{plxref|wo=832|accessdate=2014-11-22}}</ref>}} | {{πp|wo|214|7|<ref name="Woolley1970">{{plxref|wo=832|accessdate=2014-11-22}}</ref>}} | ||
{{πp|gj|215.0|6.1|<ref name="Gliese1991">{{plxref|gj=832|accessdate=2014-11-22}}</ref>}} | {{πp|gj|215.0|6.1|<ref name="Gliese1991">{{plxref|gj=832|accessdate=2014-11-22}}</ref>}} | ||
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{{πp|hip2|201.87|1.01|<ref name="van Leeuwen2007">{{plxref|hip=106440|hipsource=hip2|accessdate=2014-11-22}}</ref>|b=}} | {{πp|hip2|201.87|1.01|<ref name="van Leeuwen2007">{{plxref|hip=106440|hipsource=hip2|accessdate=2014-11-22}}</ref>|b=}} | ||
{{πp|recons2012|202.03|1.00|<ref name="RECONS TOP100">{{plxref|recons2012|accessdate=2014-11-22}}</ref>|c1=<ref group=note>Weighted parallax based on parallaxes from van Altena et al. (1995) and van Leeuwen (2007).</ref>}} | {{πp|recons2012|202.03|1.00|<ref name="RECONS TOP100">{{plxref|recons2012|accessdate=2014-11-22}}</ref>|c1=<ref group=note>Weighted parallax based on parallaxes from van Altena et al. (1995) and van Leeuwen (2007).</ref>}} | ||
|} | |||
{{πe}} | |||
<small>Non-trigonometric distance estimates are marked in ''italic''. The {{abbr|most precise|Distance estimates from preliminary versions of e-prints or published only on web pages are not taken into account.}} estimate is marked in '''bold'''.</small> | |||
==Planetary system== | ==Planetary system== |
Revision as of 22:16, 19 September 2015
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Grus |
Right ascension | 21 33 33.975 |
Declination | −49° 00′ 32.42″ |
Apparent magnitude (V) | 8.66 |
Characteristics | |
Spectral type | M1.5V |
B−V color index | 1.52 |
Astrometry | |
Radial velocity (Rv) | 18.0 km/s |
Proper motion (μ) | RA: −46.05 ± 0.95 mas/yr Dec.: −817.63 ± 0.59 mas/yr |
Parallax (π) | 201.87 ± 1.01 mas |
Distance | 16.16 ± 0.08 ly (4.95 ± 0.02 pc) |
Absolute magnitude (MV) | 10.19 |
Details | |
Mass | 0.45 ± 0.05 M☉ |
Radius | 0.48 R☉ |
Luminosity (bolometric) | 0.035 L☉ |
Luminosity (visual, LV) | 0.007 L☉ |
Surface gravity (log g) | 4.7 cgs |
Temperature | 3,620 K |
Metallicity | −0.31 ± 0.2 |
Other designations | |
HD 204961, HIP 106440, LHS 3865, PLX 5190 | |
Database references | |
SIMBAD | The star |
planet c | |
planet b | |
Exoplanet Archive | data |
Data sources: | |
Hipparcos Catalogue, HD |
Gliese 832 (Gl 832 or GJ 832) is a red dwarf of spectral type 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.
In 2014, Gliese 832 was announced to be hosting the closest potentially habitable Earth-mass-range exoplanet to the Solar System.
Distance
Source | Parallax, mas | Distance, pc | Distance, ly | Distance, Pm | Ref.
Template:Πp Template:Πp Template:Πp Template:Πp Template:Πp Template:Πp Template:Πp |
---|
Non-trigonometric distance estimates are marked in italic. The most precise estimate is marked in bold.
Planetary system
Gliese 832 hosts two known planets.
Discovery of Jupiter mass planet
In September 2008, it was announced that a Jupiter-like planet, now designated as Gliese 832 b, 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. Despite its relatively large angular distance, direct imaging is problematic due to the star–planet contrast.
Discovery of Gliese 832 c (super-Earth mass planet) in habitable zone
In 2014, a second planet was discovered by astronomers at the University of New South Wales. This one is believed to be of super-Earth mass and has since been given the scientific name Gliese 832 c. It was announced to orbit in the optimistic habitable zone but outside the conservative habitable zone of its parent star.
The planet is believed to be in, or very close to, the right distance from its sun to allow liquid water to exist on its surface.
Search for cometary disc
If this system has a comet disc, it is undetectable "brighter than the fractional dust luminosity 10" of a recent Herschel study.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
c | ≥5.4±1 M🜨 | 0.162±0-017 | 35.68±0.03 | 0.18 ± 0.13 | — | — |
b | ≥0.64 ± 0.06 MJ | 3.4 ± 0.4 | 3416 ± 131 | 0.12 ± 0.11 | — | — |
X-ray source
Gliese 832 emits X-rays.
See also
Notes
- Using the absolute visual magnitude of Gliese 832 with a bolometric correction of the bolometric magnitude can be calculated as , the bolometric magnitude of the Sun , and so therefore the bolometric luminosity can be calculated by
- Using the absolute visual magnitude of Gliese 832 and the absolute visual magnitude of the Sun , the visual luminosity can be calculated by
References
- ^ van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction" (PDF). Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
- ^ 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.
- Flower, Phillip J. (September 1996). "Transformations from Theoretical Hertzsprung-Russell Diagrams to Color-Magnitude Diagrams: Effective Temperatures, B-V Colors, and Bolometric Corrections". The Astrophysical Journal. 469: 355. Bibcode:1996ApJ...469..355F. doi:10.1086/177785.
-
Torres, Guillermo (November 2010). "On the Use of Empirical Bolometric Corrections for Stars". The Astronomical Journal. 140 (5): 1158–1162. arXiv:1008.3913. Bibcode:2010AJ....140.1158T. doi:10.1088/0004-6256/140/5/1158.
{{cite journal}}
: Unknown parameter|layurl=
ignored (help) - Interpolated value from NASA Exoplanet Archive, per: Bessell, M. S. (1995). "The Temperature Scale for Cool Dwarfs". In Tinney, C. G. (ed.). The Bottom of the Main Sequence - and Beyond, Proceedings of the ESO Workshop. Springer-Verlag. p. 123. Bibcode:1995bmsb.conf..123B.
{{cite conference}}
: Unknown parameter|booktitle=
ignored (|book-title=
suggested) (help) - ^ "Nearby Alien Planet May Be Capable of Supporting Life", Mike Wall, Space.com, June 25, 2014, http://www.space.com/26357-exoplanet-habitable-zone-gliese-832c.html
-
Wittenmyer, R.A.; Tuomi, M.; Butler, R.P.; Jones, H. R. A.; O'Anglada-Escude, G.; Horner, J.; Tinney, C.G.; Marshall, J.P.; Carter, B.D.; et al. (2014). "GJ 832c: A super-earth in the habitable zone". 1406: 5587. arXiv:1406.5587. Bibcode:2014ApJ...791..114W. doi:10.1088/0004-637X/791/2/114.
{{cite journal}}
: Cite journal requires|journal=
(help) - B. C. Matthews; forthcoming study promised in Lestrade, J.-F.; Matthews, B. C.; Sibthorpe, B.; Kennedy, G. M.; Wyatt, M. C.; Bryden, G.; Greaves, J. S.; Thilliez, E.; Moro-Martín, A.; Booth, M.; Dent, W. R. F.; Duchêne, G.; Harvey, P. M.; Horner, J.; Kalas, P.; Kavelaars, J. J.; Phillips, N. M.; Rodriguez, D. R.; Su, K. Y. L.; Wilner, D. J. (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.
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