Planetary-mass object orbiting the brown dwarf 2M1207
2M1207b
Size comparison of 2M1207b with Jupiter.
Discovery
Discovered by
Chauvin et al.
Discovery site
Paranal Observatory, Chile
Discovery date
April 2004
Detection method
Imaged
Orbital characteristics
Semi-major axis
24–231 AU (3.6×109–3.46×1010 km)[1]
Eccentricity
0.02–0.98[1]
Orbital period (sidereal)
633–20046[1] y
Inclination
13–150[1]
Longitude of ascending node
7–174[1]
Time of periastron
2107.69–12883.36[1]
Argument of periastron
4–176[1]
Star
2M1207
Physical characteristics
Mean radius
1.15 RJ[2]
Mass
5.5±0.5[3]MJ
Temperature
1200 K[3]
Spectral type
mid-to-late L[3]
Atmosphere
Composition by volume
hydrogen, water, carbon monoxide, helium[3][4]
2M1207b is a planetary-mass object orbiting the brown dwarf 2M1207, in the constellation Centaurus, approximately 170 light-years from Earth.[5] 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.[6] It is believed to be from 5 to 6 times the mass of Jupiter[3] and may orbit 2M1207 at a distance roughly as far from the brown dwarf as Pluto is from the Sun.[7]
The object is a very hot gas giant; the estimated surface temperature is roughly 1200 K (930 °C or 1700 °F),[3] mostly due to gravitational contraction.[8] 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).[9] Its infrared spectrum indicates the presence of water molecules in its atmosphere.[10][4] The object is not a likely candidate to support life, either on its surface or on any satellites.
^ abcdefgCite error: The named reference Blunt2017 was invoked but never defined (see the help page).
^ abcdefCite error: The named reference Luhman et al 2023 was invoked but never defined (see the help page).
^ abBarman, Travis S.; Macintosh, Bruce; Konopacky, Quinn M.; Marois, Christian (2011-07-01). "The Young Planet-mass Object 2M1207b: A Cool, Cloudy, and Methane-poor Atmosphere". The Astrophysical Journal. 735 (2): L39. arXiv:1106.1201. Bibcode:2011ApJ...735L..39B. doi:10.1088/2041-8205/735/2/L39. ISSN 0004-637X. S2CID 44225360.
^Mamajek, Eric (November 8, 2007). "The Distance to the 2M1207 System". Archived from the original on 2008-01-24. Retrieved June 15, 2008.
^Chauvin, G.; Lagrange, A.-M.; Dumas, C.; Zuckerman, B.; Mouillet, D.; Song, I.; Beuzit, J.-L.; Lowrance, P. (2004). "A giant planet candidate near a young brown dwarf: Direct VLT/NACO observations using IR wavefront sensing". Astronomy & Astrophysics. 425 (2): L29–L32. arXiv:astro-ph/0409323. Bibcode:2004A&A...425L..29C. doi:10.1051/0004-6361:200400056. ISSN 0004-6361.
^"Star: 2M1207". Extrasolar Planets Encyclopaedia. Archived from the original on 2011-10-06. Retrieved June 15, 2008.
^Mohanty, Subhanjoy; Jayawardhana, Ray; Huelamo, Nuria; Mamajek, Eric (2007-03-10). "The Planetary Mass Companion 2MASS 1207−3932B: Temperature, Mass, and Evidence for an Edge-on Disk". The Astrophysical Journal. 657 (2): 1064–1091. arXiv:astro-ph/0610550. Bibcode:2007ApJ...657.1064M. doi:10.1086/510877. ISSN 0004-637X.
^Estimated observed projected separation from observed angular separation and estimated distance.
^Cite error: The named reference esopr was invoked but never defined (see the help page).
2M1207b is a planetary-mass object orbiting the brown dwarf 2M1207, in the constellation Centaurus, approximately 170 light-years from Earth. It is one...
brown dwarf located in the constellation Centaurus; a companion object, 2M1207b, may be the first extrasolar planetary-mass companion to be directly imaged...
the star GQ Lupi. Its discovery was announced in April 2005. Along with 2M1207b, this was one of the first extrasolar planet candidates to be directly...
allowed astronomers to obtain the first picture of an extrasolar planet (2M1207b) orbiting a brown dwarf 173 light-years away. The High Accuracy Radial...
Infrared image of 2M1207 (bluish) and 2M1207b (reddish). The two objects are separated by less than one arc second in Earth's sky. Image taken using the...
because 2M1207b (or 2M1207B) might be classified as a binary together with 2M1207A and not an exoplanet. This would make the disk around 2M1207b a circumstellar...
There are planetary mass objects known to orbit brown dwarfs, such as 2M1207b, MOA-2007-BLG-192Lb, 2MASS J044144b and Oph 98 B. The 13 Jupiter-mass cutoff...
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Observatory's Very Large Telescope array in Chile to produce an image of 2M1207b, a companion to the brown dwarf 2M1207. In the following year, the planetary...
exoplanet to have a portion of its spectrum directly observed (following 2M1207b and 1RXS J1609b), confirming the feasibility of direct spectrographic studies...
exoplanets have been photographed. The first exoplanet to be photographed, 2M1207b, is in orbit around a star called 2M1207. Astronomers were only able to...
reported a substellar object, GQ Lupi b, orbiting the star. Along with 2M1207b, this was one of the first extrasolar planet candidates to be directly...
approximately 2.5 km, and at a distance of 0.05 AU from the star was announced. 2M1207b Wyatt, M. C.; Smith, R.; Su, K. Y. L.; et al. (July 2007), "Steady State...