GJ 758 B
GJ 758 B is a brown dwarf orbiting the G-type main sequence star GJ 758, located approximately 50 light years away, in the constellation Lyra.
GJ 758 B was detected by direct imaging using the HiCIAO instrument of the Subaru Telescope.[2][3][4] The parameters have subsequently been revised in a follow-up study which also revealed that a putative second substellar object in the system was in fact an unrelated background star.[1]
References
- ^ a b c d e Janson, M.; Carson, J.; Thalmann, C.; McElwain, M. W.; Goto, M.; Crepp, J.; Wisniewski, J.; Abe, L.; Brandner, W.; Burrows, A.; Egner, S.; Feldt, M.; Grady, C. A.; Golota, T.; Guyon, O.; Hashimoto, J.; Hayano, Y.; Hayashi, M.; Hayashi, S.; Henning, T.; Hodapp, K. W.; Ishii, M.; Iye, M.; Kandori, R.; Knapp, G. R.; Kudo, T.; Kusakabe, N.; Kuzuhara, M.; Matsuo, T.; Mayama, S.; Miyama, S.; Morino, J.-I.; Moro-Martín, A.; Nishimura, T.; Pyo, T.-S.; Serabyn, E.; Suto, H.; Suzuki, R.; Takami, M.; Takato, N.; Terada, H.; Tofflemire, B.; Tomono, D.; Turner, E. L.; Watanabe, M.; Yamada, T.; Takami, H.; Usuda, T.; Tamura, M. (2011). "Near-infrared Multi-band Photometry of the Substellar Companion GJ 758 B". The Astrophysical Journal 728 (2). arXiv:1011.5505. Bibcode 2011ApJ...728...85J. doi:10.1088/0004-637X/728/2/85.
- ^ Thalmann, Christian (2009). "Discovery of the Coldest Imaged Companion of a Sun-Like Star". arXiv:0911.1127v1 [astro-ph.EP].
- ^ "Possible Planet Around a G-class Star". Centauri Dreams. 2009-12-04. http://www.centauri-dreams.org/?p=10517. Retrieved 2009-12-04.
- ^ "Discovery of an Exoplanet Candidate Orbiting a Sun-Like Star: Inaugural Observations with Subaru's New Instrument HiCIAO". Subaru Telescope. 2009-12-03. http://subarutelescope.org/Pressrelease/2009/12/03/index.html. Retrieved 2009-12-04.
External links
Animation of GJ 758 B's orbit compared to outer Solar System
Coordinates: 19h 23m 34.0s, +33° 13′ 19.1″
|
|
Stars |
|
|
Brown dwarf |
GJ 758 B
|
|
← «Bright» star systems within 50–60 light-years →
|
|
|
|
|
|
|
|
|
|
Chi Eridani (57.0 ± 0.6 ly; 2 stars)
|
|
|
Mu Arae (49.8 ± 0.6 ly; 1 star, 4 planets: planet d • planet e • planet b • planet c)‡ • 51 Pegasi ( 50.1 ± 0.6 ly; 1 star, 1 planet: planet b «Bellerophon»)‡ • HR 7368 ( 50.5 ± 0.5 ly; 1 star, 2 brown dwarfs: brown dwarf C • brown dwarf B) • HR 2007 ( 50.8 ± 0.9 ly; 1 star, 1 planet: planet b)‡ • HR 8323 ( 51.0 ± 0.6 ly; 1 star) • HR 7670 ( 51.8 ± 0.5 ly; 3 stars, 2 planets: planet c • planet b) • Psi⁵ Aurigae ( 53.9 ± 0.6 ly; 1 star) • HR 3538 ( 55.8 ± 0.8 ly; 1 star) • Iota Horologii ( 56.2 ± 0.5 ly; 1 star, 1 planet: planet b) • 37 Geminorum ( 56.3 ± 0.9 ly; 1 star) • Rho Coronae Borealis ( 56.8 ± 0.7 ly; 1 star, 1 planet: planet b) • GJ 3021 ( 57.5 ± 0.5 ly; 1 star, 1 planet: planet b) • 15 Sagittae ( 57.6 ± 0.6 ly; 1 star, 1 brown dwarf) • HR 7644 ( 57.8 ± 0.8 ly; 1 star, 1 planet: planet b) • HR 5534 ( 58.5 ± 0.9 ly; 1 star, 2 brown dwarfs) • Gliese 651 ( 58.9 ± 0.6 ly; 1 star, 1 planet: planet b) • 70 Virginis ( 59.1 ± 0.8 ly; 1 star, 1 planet: planet b) • Pi Mensae ( 59.4 ± 0.5 ly; 1 star, 1 planet: planet b)
|
|
|
|
|
|
In left column are stellar classes of primary members of star systems. ‡Distance error margin extends out of declared distance interval. Italic are systems possibly located within declared distance interval, but probably not.
|
|