WISE 0359−5401

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Coordinates: Sky map 03h 59m 34.06s, −54° 01′ 54.6″

WISE J035934.06−540154.6
Observation data
Epoch J2000[1]:{{{3}}}      Equinox J2000[1]:{{{3}}}
Constellation Reticulum
Right ascension 03h 59m 34.06s[1]:{{{3}}}
Declination −54° 01′ 54.6″[1]:{{{3}}}
Characteristics
Spectral type Y0[1]:{{{3}}}
Apparent magnitude (J (MKO-NIR filter system)) 21.56±0.24[1]:{{{3}}}
Apparent magnitude (H (MKO-NIR filter system)) 22.20±0.43[1]:{{{3}}}
Astrometry
Proper motion (μ) RA: −177±53[2]:{{{3}}} mas/yr
Dec.: −930±62[2]:{{{3}}} mas/yr
Parallax (π) 145 ± 39[2]:{{{3}}} mas
Distance 22.5+8.3
−4.8
[3]:{{{3}}} ly
(6.9+2.5
−1.5
[3]:{{{3}}} pc)
Other designations
WISE J035934.06−540154.6,[1]:{{{3}}}
WISE 0359−5401[1]:{{{3}}}
Database references
SIMBAD data

WISE J035934.06−540154.6 (designation abbreviated to WISE 0359−5401) is a brown dwarf of spectral class Y0,[1]:{{{3}}} located in constellation Reticulum. Estimated to be approximately 22.5 light-years from Earth[3]:{{{3}}}, it is one of the Sun's nearest neighbors.

Discovery

WISE 0359−5401 was discovered in 2012 by J. Davy Kirkpatrick and colleagues from data collected by the Wide-field Infrared Survey Explorer (WISE) in the infrared at a wavelength of 40 cm (16 in), whose mission lasted from December 2009 to February 2011. In 2012 Kirkpatrick et al. published a paper in The Astrophysical Journal, where they presented discovery of seven new found by WISE brown dwarfs of spectral type Y, among which also was WISE 0359−5401.[1]:{{{3}}}

Distance

The trigonometric parallax of WISE 0359−5401 is 0.145±0.039 arcsec[2]:{{{3}}}, corresponding to a direct inversion distance[3]:{{{3}}} of 6.9+2.5
−1.5
 pc
, or 22.5+8.3
−4.8
 ly
.

See also

The other six discoveries of brown dwarfs, published in Kirkpatrick et al. (2012):[1]:{{{3}}}

References

  1. 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 Lua error in package.lua at line 80: module 'strict' not found.
  2. 2.0 2.1 2.2 2.3 Lua error in package.lua at line 80: module 'strict' not found.
  3. 3.0 3.1 3.2 3.3 Paterson, David.A. "Topics in Astronomy: Topic 8. Inappropriateness of the Lutz-Kelker equation for brown dwarfs". Retrieved on 24 September 2015.


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