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Star in the constellation Taurus From Wikipedia, the free encyclopedia
DH Tauri, also known as DH Tau, is a type M star, located 140 parsecs (456.619 light years) away. It forms a binary system with DI Tauri 15″ away, and has a substellar companion, either a brown dwarf or massive exoplanet.
DH Tauri and the b companion (lower left) with the Very Large Telescope Credit: ESO VLT SPHERE; Van Holstein et al.; Processing: Meli_thev | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Taurus |
Right ascension | 04h 29m 41.558s[1] |
Declination | +26° 32′ 58.27″[1] |
Apparent magnitude (V) | 13.1[2] |
Characteristics | |
Spectral type | M0-M1Ve(T)[3] |
Variable type | T Tau[3] |
Astrometry | |
Proper motion (μ) | RA: +7.065[4] mas/yr Dec.: -20.699[4] mas/yr |
Parallax (π) | 7.3880 ± .0593 mas[4] |
Distance | 441 ± 4 ly (135 ± 1 pc) |
Details | |
Mass | 0.41[5] M☉ |
Radius | 1.26[5] R☉ |
Luminosity | 0.22[5] L☉ |
Temperature | 3,751[4] K |
Age | 3.16[5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
DH Tauri is a type M, or red dwarf star, one of the most common types of star in the Milky Way.[6] It has an apparent magnitude of 13.71 and temperature of 3,751 K. DH Tauri has a mass of 0.41 M☉ and an estimated radius of 1.26 R☉.
The companion DH Tauri B or b has a mass estimated to be between eight MJ and 50 MJ, making it either a super-Jupiter or brown dwarf.[7][8] Other sources give a mass as high as 0.03 M☉, with a bolometric luminosity of 0.01 L☉.[9] The spectral type has been classified as M7.5[9] or M9.25.[10] The companion, while its host star still having a protoplanetary disk, is still accreting material, being surrounded by a circumsubstellar disk (possibly a circumplanetary disk, depending on its formation history).[11] It is potentially orbited by a smaller candidate companion DH Tauri Bb (possibly an exomoon) with 1 MJ, and a mass ratio with respect to the brown dwarf of one-tenth.[12]
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