HD 231701
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| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Sagitta |
| Right ascension | 19h 32m 04.1611s |
| Declination | +16° 28′ 27.444″ |
| Apparent magnitude (V) | +8.97 |
| Distance | 353.6 ly (108.4 pc) |
| Spectral type | F8V |
| Other designations | |
HIP 96078, NSV 7680, SAO 104946 | |
| Database references | |
| SIMBAD | data |
HD 231701 is a yellow-white dwarf star approximately 354 light years away in the constellation of Sagitta. It is a 9th magnitude star, meaning the star is not visible to the naked eye, but powerful binoculars or a small telescope is needed to view the star. It is an F-type main-sequence star, a type of hydrogen-fusing star that is hotter, more massive, and brighter than our Sun.
Planetary system
In 2007, the N2K Consortium used the radial velocity technique to discover a Jupiter-like planet orbiting at 0.55 AU around the star.[1]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | >1.08 MJ | 0.55 | 142 ± 2.8 | 0.19 ± 0.05 | — | — |
See also
- List of extrasolar planets
References
- ↑ 1.0 1.1 Fischer, Debra A. et al. (2007). "Five Intermediate-Period Planets from the N2K Sample". The Astrophysical Journal 669 (2): 1336–1344. arXiv:0704.1191. Bibcode:2007ApJ...669.1336F. doi:10.1086/521869.
External links
- "HD 231701". The Extrasolar Planets Encyclopedia.
Coordinates: 
19h 32m 04.1611s, +16° 28′ 27.444″
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