DX Cancri

DX Cancri is a variable star in the northern zodiac constellation of Cancer. With an apparent visual magnitude of 14.81, it is much too faint to be seen with the naked eye. Visually viewing this star requires a telescope with a minimum aperture of 16 in (41 cm). Based upon parallax measurements, DX Cancri is located at a distance of 11.8 light-years (3.6 parsecs) from Earth. This makes it the 18th closest star (or star system) to the Sun.

DX Cancri

An ultraviolet band light curve for a flare on DX Cancri, adapted from Pettersen (1981)
Observation data
Epoch J2000      Equinox J2000
Constellation Cancer
Right ascension 08h 29m 49.345s
Declination +26° 46 33.74
Apparent magnitude (V) 14.81
Characteristics
Spectral type M6.5V
Apparent magnitude (J) 8.2
U−B color index +2.11
B−V color index +2.08
Variable type Flare star
Astrometry
Radial velocity (Rv)+9.0 km/s
Proper motion (μ) RA: −1,140 mas/yr
Dec.: −602 mas/yr
Parallax (π)279.2496 ± 0.0637 mas
Distance11.680 ± 0.003 ly
(3.5810 ± 0.0008 pc)
Absolute magnitude (MV)16.98
Details
Mass0.09 M
Radius0.11 R
Luminosity0.00065 L
Temperature2,840 K
Rotation0.46 days
Rotational velocity (v sin i)11.0 km/s
Age200 Myr
Other designations
G 051-015, GCTP 2016.01, GJ 1111, LHS 248
Database references
SIMBADdata
DX
Location of DX Cancri in the constellation Cancer

The star has a stellar classification of M6.5V, identifying it as a type of main sequence star known as a red dwarf. It has about 9% of the mass of the Sun, and 11% of the Sun's radius. The outer envelope of the star has an effective temperature of 2,840 K, making it an M-type star. It is a flare star that has random, intermittent increases in brightness by up to a factor of five. It is a proposed member of the Castor Moving Group of stars that share a common trajectory through space. This group has an estimated age of 200 million years.

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