IRAS 04125+2902

IRAS 04125+2902

IRAS 04125+2902 (green star in the middle) and its companion (yellow star below)
Credit: Pan-STARRS & Meli thev
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 04h 15m 42.7871s
Declination +29° 09′ 59.832″
Apparent magnitude (V) 15.487±0.003
Characteristics
Evolutionary stage pre main sequence
Spectral type M1.25±0.25 + M6.5
Variable type T Tauri
Astrometry
Radial velocity (Rv)13.35±0.39 km/s
Proper motion (μ) RA: +21.811 mas/yr
Dec.: −18.145 mas/yr
Parallax (π)6.2474±0.0270 mas
Distance522 ± 2 ly
(160.1 ± 0.7 pc)
Details
Primary
Mass0.70±0.04 M
Radius1.45±0.1 R
Luminosity0.466±0.041 L
Temperature4,080±95 K
Rotation11.31±0.06 d
Rotational velocity (v sin i)7.1±0.5 km/s
Age3.3+0.6
−0.5
 Myr
Companion
Mass0.17±0.04 M
Radius0.96±0.12 R
Luminosity0.050±0.004 L
Temperature2,830±90 K
Other designations
TIC 56658270, IRAS 04125+2902, 2MASS J04154278+2909597, WISE J041542.77+290959.5
Database references
SIMBADdata

IRAS 04125+2902 is an M-type star and a T Tauri variable located in the Taurus Molecular Cloud, 160 parsecs (520 light-years) from Earth. This young protostar has 70% of the Sun's mass, 1.45 times the Sun's radius and an effective temperature of 4,080 K (3,810 °C; 6,880 °F). It has a very young age of three million years. It is surrounded by a transitional disk, inclined at 30° relative to Earth, and has one known exoplanet.

It is part of a binary system with 2MASS J04154269+2909558, the two being separated by a projected distance of 635 astronomical units, or 4 arcseconds in the sky. The companion was discovered in 2009, has a spectral type of M6.5, and does not show any infrared excess.