2MASS J11145133-2618235
Coordinates: 11h 14m 51.337s, −26° 18′ 23.56″
Observation data Epoch J2000[1]:{{{3}}} Equinox J2000[1]:{{{3}}} |
|
---|---|
Constellation | Hydra |
Right ascension | 11h 14m 51.337s[1]:{{{3}}} |
Declination | −26° 18′ 23.56″[1]:{{{3}}} |
Characteristics | |
Spectral type | T7.5[2]:{{{3}}}[3]:{{{3}}}[4]:{{{3}}}[5]:{{{3}}}[6]:{{{3}}} |
Apparent magnitude (i (GMOS filter system)) | 23.21 ± 0.09[5]:{{{3}}} |
Apparent magnitude (z (GMOS filter system)) | 19.59 ± 0.04[5]:{{{3}}} |
Apparent magnitude (J (2MASS filter system)) | >15.86 ± 0.08[2]:{{{3}}}[3]:{{{3}}} |
Apparent magnitude (J (MKO filter system)) | 15.52 ± 0.05[6]:{{{3}}} |
Apparent magnitude (H (2MASS filter system)) | >15.73 ± 0.12[3]:{{{3}}} |
Apparent magnitude (H (MKO filter system)) | 15.82 ± 0.05[6]:{{{3}}} |
Apparent magnitude (KS (2MASS filter system)) | >16.1[3]:{{{3}}} |
Apparent magnitude (KS (MKO filter system)) | 16.54 ± 0.05[6]:{{{3}}} |
Astrometry | |
Proper motion (μ) | RA: -3018.8 ± 1.1[7]:{{{3}}} mas/yr Dec.: -384.1 ± 1.4[7]:{{{3}}} mas/yr |
Parallax (π) | 179.2 ± 1.4[7]:{{{3}}} mas |
Distance | 18.2 ± 0.1 ly (5.58 ± 0.04 pc) |
Details | |
Mass | 0.029–0.048[4]:{{{3}}} M☉ |
Mass | 30–50[4]:{{{3}}} MJup |
Surface gravity (log g) | 5.0–5.3[4]:{{{3}}} cgs |
Temperature | 725–775[4]:{{{3}}} K |
Metallicity | -0.3 ± 0.1 [m/H][4]:{{{3}}} |
Age | 3–8[4]:{{{3}}} Gyr |
Other designations | |
Database references | |
SIMBAD | data |
2MASS J11145133-2618235 (designation abbreviated to 2MASS 1114-2618,[3]:{{{3}}} or 2M1114-26,[2]:{{{3}}} or 2M1114-2618,[2]:{{{3}}} or 2MASS 1114-26,[4]:{{{3}}} or 2MASS J1114-2618[6]:{{{3}}}) is nearby brown dwarf of spectral class T7.5,[2]:{{{3}}}[3]:{{{3}}}[4]:{{{3}}}[5]:{{{3}}}[6]:{{{3}}} located in constellation Hydra[note 1] at approximately 18 light-years from Earth.[7]:{{{3}}}
Discovery
2MASS 1114-2618 was discovered in 2005 by C. G. Tinney et al. from the 2MASS Wide-Field T Dwarf Search (WFTS), based on observations obtained at the Anglo-Australian Telescope, Siding Spring, Australia. In 2005 Tinney et al. published a paper in The Astronomical Journal, where they presented discovery of five new brown dwarfs of spectral type T, among which also was 2MASS 1114-2618.[2]:{{{3}}}
Distance
Trigonometric parallax of 2MASS 1114-2618, measured in 2012 by Dupuy & Liu under The Hawaii Infrared Parallax Program, is 0.1792 ± 0.0014 arcsec, corresponding to a distance 5.58 ± 0.04 pc, or 18.20 ± 0.14 ly.[7]:{{{3}}}
Photometric distance estimate of 2MASS 1114-2618, published in its discovery paper in 2005, is 7 pc (22.8 ly).[2]:{{{3}}} Spectrophotometric distance estimate by Kirkpatrick et al. (2012), is 6.6 pc (21.5 ly).[8]:{{{3}}}
Proper motion
2MASS 1114-2618 has quite a large proper motion of 3043.2 mas/yr with position angle 262.75 degrees,[7]:{{{3}}} indicating motion in south-west direction on the sky. At distance 18.20 ly (assuming parallax 179.2 ± 1.4 mas),[7]:{{{3}}} corresponding tangential velocity is 80.56 km/s.[7]:{{{3}}}
See also
The other four discoveries of brown dwarfs, presented in Tinney et al. (2005):[2]:{{{3}}}
- 2MASS 0050-3322 (T7.5)
- 2MASS 0939-2448 (T8, binary brown dwarf)
- 2MASS 0949-1545 (T1)
- 2MASS 1122-3512 (T2)
Notes
- ↑ The nearest known star/brown dwarf in this constellation.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 4.7 4.8 4.9 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 5.0 5.1 5.2 5.3 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 6.0 6.1 6.2 6.3 6.4 6.5 6.6 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 7.0 7.1 7.2 7.3 7.4 7.5 7.6 7.7 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 8.0 8.1 Lua error in package.lua at line 80: module 'strict' not found.