Observation data Epoch J2000 [1] Equinox J2000 [1] | |
---|---|
Constellation | Camelopardalis |
Right ascension | 05h 32m 53.46s [1] |
Declination | +82° 46′ 46.5″ [1] |
Characteristics | |
Spectral type | L7 [1] |
Astrometry | |
Parallax (π) | 40.2369 ± 0.6389 mas [1] |
Distance | 81 ± 1
ly (24.9 ± 0.4 pc) |
Details | |
Mass | 0.077–0.085 [2] M☉ |
Temperature | 1600 [3] K |
Metallicity [Fe/H] | -1.6 [3] dex |
Age | ~10 [3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
2MASS J05325346+8246465 (abbreviated 2MASS J0532+8246) is possibly the first brown dwarf observed in the galactic halo of the Milky Way, and the first known substellar subdwarf star. [4] [5] It was discovered from Two Micron All-Sky Survey data, and verified by observations at Palomar Observatory and W. M. Keck Observatory. [5] It has a low metallicity, which indicates it is an old star. [5]
The mass and temperature of 2MASS 0532+8246 makes it a rare object in stellar-substellar gap between conventional stars and brown dwarfs. [6] It produces roughly half of its luminosity from hydrogen fusion. [3] Such "gap" objects, covering a narrow range of masses but a wide range of temperatures, and powered by unsteady hydrogen fusion, are exotic but expected to be more common among low-metallicity objects like 2MASS J05325346+8246465. [7]
Observation data Epoch J2000 [1] Equinox J2000 [1] | |
---|---|
Constellation | Camelopardalis |
Right ascension | 05h 32m 53.46s [1] |
Declination | +82° 46′ 46.5″ [1] |
Characteristics | |
Spectral type | L7 [1] |
Astrometry | |
Parallax (π) | 40.2369 ± 0.6389 mas [1] |
Distance | 81 ± 1
ly (24.9 ± 0.4 pc) |
Details | |
Mass | 0.077–0.085 [2] M☉ |
Temperature | 1600 [3] K |
Metallicity [Fe/H] | -1.6 [3] dex |
Age | ~10 [3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
2MASS J05325346+8246465 (abbreviated 2MASS J0532+8246) is possibly the first brown dwarf observed in the galactic halo of the Milky Way, and the first known substellar subdwarf star. [4] [5] It was discovered from Two Micron All-Sky Survey data, and verified by observations at Palomar Observatory and W. M. Keck Observatory. [5] It has a low metallicity, which indicates it is an old star. [5]
The mass and temperature of 2MASS 0532+8246 makes it a rare object in stellar-substellar gap between conventional stars and brown dwarfs. [6] It produces roughly half of its luminosity from hydrogen fusion. [3] Such "gap" objects, covering a narrow range of masses but a wide range of temperatures, and powered by unsteady hydrogen fusion, are exotic but expected to be more common among low-metallicity objects like 2MASS J05325346+8246465. [7]