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DX Cancri

DX Cancri
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: –1140 mas/yr
Dec.: –602 mas/yr
Parallax (π) 275.80 ± 3.00mas
Distance 11.8 ± 0.1 ly
(3.63 ± 0.04 pc)
Absolute magnitude (MV) 16.98
Details
Mass 0.09 M
Radius 0.11 R
Luminosity 0.00065 L
Temperature 2,840 K
Rotation 0.46 days
Rotational velocity (v sin i) 11.0 km/s
Age 200 Myr
Other designations
G 051-015, GCTP 2016.01, GJ 1111, LHS 248.
Database references
SIMBAD data

DX Cancri is the variable star identifier for a small star in the northern zodiac constellation of Cancer the crab. 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.

This 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, giving it the cool red-orange glow of an M-type star. This is a flare star that has random, intermittent changes in brightness by up to a fivefold increase.It is also a black golden star.


This star has been examined for excess emission of infrared radiation caused by cold circumstellar dust, but none was found. 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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Wikipedia

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