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2M1207
EntityQ222075· pop 26· linked from 263 articles

Also known as 2M1207 A

2M1207, 2M1207A or 2MASS J12073346−3932539 is a brown dwarf located in the constellation Centaurus; a companion object, 2M1207b, may be the first extrasolar planetary-mass companion to be directly imaged, and is the first discovered orbiting a brown dwarf.

Wikidata facts

Constellation
Centaurus
Child body
2M1207b
Distance from Earth
64.308
Radius
0.21887
Mass
0.024
Image
Primera foto planeta extrasolar ESO.jpg
Show 19 more facts
topic's main category
Category:2M1207
right ascension
181.88944813534997
declination
-39.54833795144000
effective temperature
2825
radial velocity
7.50
apparent magnitude
17.388071
catalog code
TIC 102076870
spectral class
M8pec
epoch
J2000.0
parallax
18.51
luminosity
0.015
absolute magnitude
9.38
age estimated by a dating method
0.008
right ascension component of proper motion
-64.083
declination component of proper motion
-23.72
surface gravity
300000
Commons category
2M1207
time of discovery or invention
2005-00-00
semi-major axis of an orbit
42
Sources (3)

via Wikidata · CC0

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Encyclopedic overview

5 sections
Contents
  • Planetary system
  • See also
  • Notes
  • References
  • External links

2M1207, 2M1207A or 2MASS J12073346−3932539 is a brown dwarf located in the constellation Centaurus; a companion object, 2M1207b, may be the first extrasolar planetary-mass companion to be directly imaged, and is the first discovered orbiting a brown dwarf.

2M1207 was discovered during the course of the 2MASS infrared sky survey: hence the "2M" in its name, followed by its celestial coordinates. With a fairly early (for a brown dwarf) spectral type of M8, it is very young, and probably a member of the TW Hydrae association. Its estimated mass is around 25 Jupiter masses. The companion, 2M1207b, is estimated to have a mass of 5–6 Jupiter masses. Still glowing red hot, it will shrink to a size slightly smaller than Jupiter as it cools over the next few billion years.

Excerpted from Wikipedia’s “2M1207” article, available under the CC BY-SA 4.0 licence.

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