HD 156411 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 156411 | |
Constellation | Ara | |
Right ascension | (α) | 17h 19m 51.401s[1] |
Declination | (δ) | –48° 32′ 57.54″[1] |
Apparent magnitude | (mV) | 6.67 |
Distance | 179 ± 5[1] ly (55 ± 1[1] pc) | |
Spectral type | G1Vw | |
Orbital elements | ||
Semi-major axis | (a) | 1.81 AU (270 Gm) |
32.8 mas | ||
Orbital period | (P) | 842 d (2.31 y) |
Physical characteristics | ||
Minimum mass | (m sin i) | 0.75 MJ |
Discovery information | ||
Discovery date | October 19, 2009 | |
Discoverer(s) | Naef et al. | |
Discovery method | radial velocity (HARPS) | |
Discovery site | La Silla Observatory | |
Discovery status | Published[2] | |
Other designations | ||
HIP 84787 b | ||
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 156411 b (also known as HIP 84787 b) is an extrasolar planet which orbits the G-type main sequence star HD 156411, located approximately 179 light years away in the constellation Ara. This planet has at least three-fourths the mass of Jupiter and takes eight-thirds years to orbit the star at a semimajor axis of 1.81 AU.[2] However unlike most other known exoplanets, its eccentricity is not known, but it is typical that its inclination is not known. This planet was detected by HARPS on October 19, 2009, together with 29 other planets.
References
- 1 2 3 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
- 1 2 Naef, D.; et al. (2010). "The HARPS search for southern extrasolar planets XXIII. 8 planetary companions to low-activity solar-type stars". Astronomy and Astrophysics 523. A15. arXiv:1008.4600. Bibcode:2010A&A...523A..15N. doi:10.1051/0004-6361/200913616.
Coordinates: 17h 19m 51.3992s, −48° 32′ 57.548″
This article is issued from Wikipedia - version of the Thursday, May 21, 2015. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.