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2M1207b is a planetary-mass object orbiting the brown dwarf 2M1207, in the constellation Centaurus, approximately 170 light-years from Earth. It is one of the first candidate exoplanets to be directly observed (by infrared imaging). It was discovered in April 2004 by the Very Large Telescope (VLT) at the Paranal Observatory in Chile by a team from the…
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| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| 2M1207b | Argument of periastron | 4–176 | 1.00 | infobox |
| 2M1207b | Composition by volume | hydrogen, water, carbon monoxide, helium | 1.00 | infobox |
| 2M1207b | Detection method | Imaged | 1.00 | infobox |
| 2M1207b | Discovered by | Chauvin et al. | 1.00 | infobox |
| 2M1207b | Discovery date | April 2004 | 1.00 | infobox |
| 2M1207b | Discovery site | Paranal Observatory, Chile | 1.00 | infobox |
| 2M1207b | Eccentricity | 0.02–0.98 | 1.00 | infobox |
| 2M1207b | Inclination | 13–150 | 1.00 | infobox |
| 2M1207b | Longitude of ascending node | 7–174 | 1.00 | infobox |
| 2M1207b | Mass | 5.5±0.5 MJ | 1.00 | infobox |
| 2M1207b | Mean radius | 1.399 +0.008 −0.010 RJ | 1.00 | infobox |
| 2M1207b | Orbital period (sidereal) | 633–20046 y | 1.00 | infobox |
| 2M1207b | Semi-major axis | 24–231 AU (3.6×109–3.46×1010 km) | 1.00 | infobox |
| 2M1207b | Spectral type | mid-to-late L | 1.00 | infobox |
| 2M1207b | Star | 2M1207 | 1.00 | infobox |
| 2M1207b | Temperature | 1200 K | 1.00 | infobox |
| 2M1207b | Time of periastron | 2107.69–12883.36 | 1.00 | infobox |
| 2M1207b | is a | planetary-mass object orbiting the brown dwarf 2M1207 | 0.90 | text |
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