OGLE-TR-122
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Carina |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Characteristics | |
| Spectral type | ? (primary)/M (b)[2] |
| Apparent magnitude (I) | 15.61 (system)[1] |
| Variable type | Eclipsing binary |
| Orbit[2] | |
| Period (P) | 7.26867 d |
| Eccentricity (e) | 0.205 ± 0.008 |
| Inclination (i) | 88–90° |
| Periastron epoch (T) | JD 2452342.41 ± 0.02 |
| Argument of periastron (ω) (secondary) | 99.2 ± 0.8° |
| Semi-amplitude (K1) (primary) | 9.642 ± 0.088 km/s |
| Details[2] | |
| OGLE-TR-122A | |
| Mass | 0.98 ± 0.14 Template:Solar mass |
| Radius | Script error: No such module "val". Template:Solar radius |
| Surface gravity (log g) | 3.9 ± 0.5 cgs |
| Temperature | 5700 ± 300 K |
| Metallicity [Fe/H] | 0.15 ± 0.36 dex |
| Rotational velocity (v sin i) | 5.7 ± 0.6 km/s |
| OGLE-TR-122B | |
| Mass | 0.092 ± 0.009 Template:Solar mass |
| Radius | Script error: No such module "val". Template:Solar radius |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| V817 Car | |
| Database references | |
| SIMBAD | data |
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OGLE-TR-122 is a binary stellar system containing one of the smallest main-sequence stars whose radius has been measured. It was discovered when the Optical Gravitational Lensing Experiment (OGLE) survey observed the smaller star eclipsing the larger primary. The orbital period is approximately 7.3 days. The system's primary is thought to resemble the Sun.[2]
OGLE-TR-122B
The smaller star, OGLE-TR-122B, is estimated to have a radius around 0.12 solar radii, or around 20% larger than Jupiter's, and a mass of around 0.1 solar masses, or approximately 100 times Jupiter's. This makes its average density approximately 50 times the Sun's[2][3] or over 80 times the density of water. OGLE-TR-122b's mass is close to the lowest possible mass for a hydrogen-fusing star, estimated to be around 0.07 or 0.08 solar masses.[4] The observed transit provides the first direct evidence for a star with a radius comparable to Jupiter's.[2]
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Brightness «Dip» and Velocity Variations of OGLE-TR-122.
See also
References
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