Gliese 849
From Wikipedia, the free encyclopedia
| Observation data Epoch J2000.0 |
|
|---|---|
| Constellation (pronunciation) |
Aquarius |
| Right ascension | 22h 9m 40.346s |
| Declination | –4° 38′ 26.624″ |
| Apparent magnitude (V) | 10.42 |
| Characteristics | |
| Spectral type | M3.5V |
| U-B color index | 1.13 |
| B-V color index | 1.51 |
| V-R color index | 1.11 |
| R-I color index | 1.41 |
| Variable type | suspected |
| Astrometry | |
| Radial velocity (Rv) | −12 km/s |
| Proper motion (μ) | RA: 1134.93 mas/yr Dec.: −19.71 mas/yr |
| Parallax (π) | 113.97 ± 2.10 mas |
| Distance | 28.618 ± 0.7 ly (8.774 ± 0.2 pc) |
| Absolute magnitude (MV) | 10.70 |
| Details | |
| Mass | 0.36 M☉ |
| Radius | 0.52 ± 0.07 R☉ |
| Surface gravity (log g) | 4.66 |
| Luminosity | 0.0045 L☉ |
| Temperature | ? K |
| Metallicity | ? |
| Rotation | ? |
| Age | ? years |
| Other designations | |
|
BD-05° 5715, LHS 517, LFT 1689, LPM 814, LTT 8889, Wolf 1329, Vys 73, HIP 109388
|
|
| Database references | |
| SIMBAD | data |
| Planet | |
| Gliese 849b | Data |
Gliese 849 is a red dwarf star in the constellation of Aquarius.
[edit] Gliese 849 b
| Extrasolar planet | List of extrasolar planets | |
|---|---|---|
| Orbital elements | ||
| Semimajor axis | (a) | 2.35 AU |
| Eccentricity | (e) | 0.06 ± 0.09 |
| Orbital period | (P) | 1890 ± 130 d |
| Angular distance | (θ) | 267.039 mas |
| Longitude of periastron |
(ω) | 351 ± 60° |
| Time of periastron | (T0) | 2411462 ± 550 JD |
| Semi-amplitude | (K) | 22 ± 4 m/s |
| Physical characteristics | ||
| Mass | (m) | >0.82 MJ |
| Radius | (r) | (Estimated) 1.0 RJ |
| Discovery information | ||
| Discovery date | Aug 2006 | |
| Discoverer(s) | Buccino et al. | |
| Detection method | radial velocity | |
| Discovery status | Published | |
| Database references | ||
| exoplanet | [data] | |
Gliese 849 b is a first long-period Jupiter-like planet discovered around the red dwarf star, announced in August 2006 by Buccino that used a radial velocity technique. The previously longest-period Jupiter-like planet around the red dwarf star was Gliese 876 b. However, there are two disproven longer period Jupiter-like planets around Lalande 21185. There are indication of a possible second companion. The planet's mass is less than that of Jupiter, though only the minimum mass is known. The distance of the planet is 2.35 AU and it takes 1890 days to revolve. The orbit is circular.

