HD 99109
From Wikipedia, the free encyclopedia
| Observation data Epoch J2000.0 |
|
|---|---|
| Constellation (pronunciation) |
Leo |
| Right ascension | 11h 24m 17.358s |
| Declination | -01° 31′ 44.674″ |
| Apparent magnitude (V) | +9.10 |
| Characteristics | |
| Spectral type | K0V |
| U-B color index | ? |
| B-V color index | +0.87 |
| Variable type | suspected |
| Astrometry | |
| Radial velocity (Rv) | ? km/s |
| Proper motion (μ) | RA: -179.71 mas/yr Dec.: -160.61 mas/yr |
| Parallax (π) | 16.54 ± 1.31 mas |
| Distance | 197.19 ± 15.7 ly (60.46 ± 4.8 pc) |
| Absolute magnitude (MV) | +5.19 |
| Details | |
| Mass | 0.93 M☉ |
| Radius | ? R☉ |
| Luminosity | 0.724 L☉ |
| Temperature | 5272 K |
| Metallicity | 2.07 × Sun |
| Rotation | ? |
| Age | >12.2 years |
| Other designations | |
|
BD-00º2437, HIP 55664, SAO 138182
|
|
HD 99109 is a K-type main-sequence star in the constellation Leo. It is one and half degree away from the celestial equator to the south. It is an orange dwarf, meaning that it is 93% as massive, probably smaller, and 72.4% the luminosity of our Sun. It is over twice the abundance of iron relative to hydrogen than the Sun in which the planets are common around such stars. There is one known planet in this star system found in 2006.
[edit] HD 99109 b
| Orbital elements | ||
|---|---|---|
| Semi-major axis a: | 1.105 ± 0.065 AU | |
| Eccentricity e: | 0.09 ± 0.16 | |
| Orbital period P: | 439.3 ± 5.6 d | |
| Inclination i: | ?° | |
| Angular distance θ: | 18.264 mas | |
| Longitude of periastron ω: |
256° | |
| Time of periastron τ: | 2,411,310 ± 80 JD | |
| Semi-amplitude K: | 14.1 ± 2.2 m/s | |
| Physical characteristics | ||
| Mass: | >0.502 ± 0.07 MJ | |
| Radius: | ? RJ | |
| Density: | ? kg/m³ | |
| Gravity: | ? g | |
| Temperature: | ~225 K | |
| Discovery | ||
| Discovery date: | July 15, 2006 | |
| Discovery site: | ||
| Detection method(s): | Radial velocity | |
| Discoverer(s): | Butler et al. | |
| Other catalogue | ||
HD 99109 b is a W-type planet one half the mass of Jupiter and orbits slightly further from the star than Earth to the Sun. The orbital eccentricity is about the same as planet Mars.
[edit] References
- Butler et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505 – 522. doi:. (web Preprint)

