WISE 0350−5658
Coordinates: 03h 50m 00.32s, −56° 58′ 30.2″
Observation data Epoch J2000[1] Equinox J2000[1]:{{{3}}} |
|
---|---|
Constellation | Reticulum |
Right ascension | 03h 50m 00.32s[1]:{{{3}}} |
Declination | −56° 58′ 30.2″[1]:{{{3}}} |
Characteristics | |
Spectral type | Y1[1]:{{{3}}} |
Apparent magnitude (J (MKO-NIR filter system)) | >22.8[1]:{{{3}}} |
Apparent magnitude (H (MKO-NIR filter system)) | >21.5[1]:{{{3}}} |
Astrometry | |
Proper motion (μ) | RA: −125±97[2] mas/yr Dec.: −865±76[2]:{{{3}}} mas/yr |
Parallax (π) | 291 ± 50[2]:{{{3}}} mas |
Distance | 11.2+2.3 −1.6[3]:{{{3}}} ly (3.44+0.71 −0.50[3] pc) |
Other designations | |
Database references | |
SIMBAD | data |
WISE J035000.32−565830.2 (designation abbreviated to WISE 0350−5658) is a brown dwarf of spectral class Y1,[1]:{{{3}}} located in constellation Reticulum, the nearest known star/brown dwarf in this constellation. Being approximately 11.2 light-years from Earth,[3]:{{{3}}} it is one of the Sun's nearest neighbors.
Contents
Discovery
WISE 0350−5658 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 the discovery of seven new brown dwarfs of spectral type Y that had been found by WISE, among which was WISE 0350−5658.[1]:{{{3}}}
Distance
WISE 0350−5658 is one of the nearest known brown dwarfs: its trigonometric parallax is 0.291 ± 0.050 arcsecond[2]:{{{3}}}, corresponding to a direct inversion distance[3]:{{{3}}} of 3.44+0.71
−0.5 pc (11.2+2.3
−1.6 ly).
See also
The other six discoveries of brown dwarfs, published in Kirkpatrick et al. (2012):[1]:{{{3}}}
- WISE 0146+4234 (Y0)
- WISE 0359−5401 (Y0)
- WISE 0535−7500 (≥Y1)
- WISE 0713−2917 (Y0)
- WISE 0734−7157 (Y0)
- WISE 2220−3628 (Y0)
References
- ↑ 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.
- ↑ 2.0 2.1 2.2 2.3 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 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.