DH Tauri

Star in the constellation Taurus From Wikipedia, the free encyclopedia

DH Tauri

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.

Quick Facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
DH Tauri
Thumb
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]
Distance441 ± 4 ly
(135 ± 1 pc)
Details
Mass0.41[5] M
Radius1.26[5] R
Luminosity0.22[5] L
Temperature3,751[4] K
Age3.16[5] Myr
Other designations
DH Tau, WDS J04297+2633B, IRAS 04267+2626, 2MASS J04294155+2632582
Database references
SIMBADdata
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Characteristics

Summarize
Perspective

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, which is unusually large for a red dwarf.

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 has detected water vapor and carbon monoxide in its atmosphere and has a rotational velocity of 9.6 ± 0.7 km/s. This is between 9 and 15% of the breakup speed of DH Tau B. This low rotation is in agreement with magnetic coupling to a circumplanetary disk in the late stages of accretion, which reduces angular momentum of the companion.[11] 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).[12] 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.[13]

More information Companion (in order from star), Mass ...
The DH Tauri planetary system[14]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 11±3 MJ 330 120.450 2.7±0.8 RJ
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References

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