2M1207b
Sign in to saveAlso known as 2M1207 b, TIC 102076870b
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 European Southern Observatory led by Gaël Chauvin. It is believed to be from 5 to 6 times the mass of Jupiter and may orbit 2M1207 at a distance roughly as far from the brown dwarf as Pluto is from the Sun.
Astronomical data · SIMBAD
- Object type
- BD*
- Spectral type
- L3
- Distance
- 171 light-years
- Coordinates
- RA 181.8896° · Dec -39.5484°
via SIMBAD · CDS Strasbourg
Key facts
- Planet.extrasolarplanet
- yes
- Planet.name
- 2M1207b
- Planet.image
- Exoplanet Comparison 2M1207 b.png
- Planet.caption
- Size comparison of 2M1207b with Jupiter.
- Planet.discoverer
- Chauvin et al.
- Planet.discovery_site
- Paranal Observatory, Chile
- Planet.discovered
- April 2004
- Planet.discovery_method
- Imaged
- Planet.apsis
- astron
- Planet.period
- y
- Planet.star
- 2M1207
- Planet.mean_radius
- 1.399
- Planet.single_temperature
- 1200 K
- Planet.spectral_type
- mid-to-late L
- Planet.atmosphere_composition
- hydrogen, water, carbon monoxide, helium
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 64.673
- Mass
- 5.5
- Image
- Primera foto planeta extrasolar ESO.jpg
Show 11 more facts
- spectral class
- L3gammapec
- Commons category
- 2M1207 b
- time of discovery or invention
- 2004-10-00
- apparent magnitude
- 16.93
- catalog code
- TIC 102076870b
- parallax
- 19.10
- declination component of proper motion
- -23
- semi-major axis of an orbit
- 42
- right ascension
- 181.889583
- declination
- -39.548444
- right ascension component of proper motion
- -63
Sources (1)
via Wikidata · CC0
~5 min read
Article
7 sectionsContents
- Discovery and identification
- Properties
- Status as an exoplanet
- See also
- References
- External links
- Catalog views: Aladin Lite
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 European Southern Observatory led by Gaël Chauvin. It is believed to be from 5 to 6 times the mass of Jupiter and may orbit 2M1207 at a distance roughly as far from the brown dwarf as Pluto is from the Sun.
The object is a very hot gas giant; the estimated surface temperature is roughly 1200 K (930 °C or 1700 °F), mostly due to gravitational contraction. Its mass is well below the calculated limit for deuterium fusion in brown dwarfs, which is 13 Jupiter masses. The projected distance between 2M1207b and its primary is around 40 AU (similar to the mean distance between Pluto and the Sun). Its infrared spectrum indicates the presence of water molecules in its atmosphere. The object is not a likely candidate to support life, either on its surface or on any satellites.