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WISE 1049-5319

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Also known as WISE J104915.57-531906.1, WISE J104915.57-531906, Luhman 16, LUH 16

binary brown dwarf, third closest star system.

Key facts

Constellation
Vela
Right ascension
10 49 18.771
Declination
−53 ° 19 ′ 09.88 ″
Spectral type
A: L7.5 , B: T0.5 ± 1
Apparent magnitude i denis filter system
14.94 ± 0.03
Apparent magnitude j 2mass filter system
10.73 ± 0.03
Apparent magnitude j denis filter system
10.68 ± 0.05
Apparent magnitude h 2mass filter system
9.56 ± 0.03
Apparent magnitude k s 2mass filter syst
8.84 ± 0.02
Apparent magnitude k s denis filter syst
8.87 ± 0.08

via Wikipedia infobox

Wikidata facts

Constellation
Vela
Distance from Earth
2
Image
Wise1049-5319 Multi-Color (No Marker).png
Show 11 more facts
catalog code
TIC 119862115
Commons category
Luhman 16
time of discovery or invention
2013-00-00
parallax
496
spectral class
L6-7.5+T0
right ascension
162.3288125
declination
-53.3194667
apparent magnitude
16.919827
declination component of proper motion
354
epoch
J2000.0
right ascension component of proper motion
-2759
Sources (2)

via Wikidata · CC0

~20 min read

Encyclopedic overview

Luhman 16 (also designated WISE 1049−5319 or WISE J104915.57−531906.1) is a binary system of two brown dwarfs, located in the southern constellation Vela at a distance of 6.51 light-years (2.00 parsecs) from the Sun. These are the closest-known brown dwarfs and the closest system found since the measurement of the proper motion of Barnard's Star in 1916, and the third-closest-known system to the Sun (after the Alpha Centauri system and Barnard's Star). The primary is of spectral type L7.5 and the secondary of type T0.5±1 (and is hence near the L–T transition). The masses of Luhman 16 A and B are 35.4 and 29.4 Jupiter masses, respectively, and their ages are estimated to be 400–800 million years. Luhman 16 A and B orbit each other at a distance of about 3.5 astronomical units with an orbital period of approximately 26.6 years.

Discovery

Excerpted from Wikipedia’s “WISE 1049-5319” article, available under the CC BY-SA 4.0 licence.