AT Microscopii

AT Microscopii is a binary star system located at a distance of 35 ly (11 pc) from the Sun in the constellation of Microscopium. Both members are flare stars, meaning they are red dwarf stars that undergo random eruptions that increase their brightness. This pair lies physically near the red dwarf star AU Microscopii, which may mean they form a wide triple star system.

AT Microscopii

An ultraviolet band light curve for AT Microscopii, adapted from Andrews (1990)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Microscopium
Right ascension 20h 41m 51.15925s
Declination −32° 26 06.8283
Apparent magnitude (V) 11.0/11.1
Characteristics
Spectral type M4 Ve + M4.5e
U−B color index +0.91
B−V color index +1.58
Variable type Flare star
Astrometry
Radial velocity (Rv)4.5 km/s
Proper motion (μ) RA: +270.45 mas/yr
Dec.: –365.60 mas/yr
Parallax (π)93.50 ± 3.67 mas
Distance35 ± 1 ly
(10.7 ± 0.4 pc)
Orbit
Period (P)141.39 yr
Semi-major axis (a)2.616″
Eccentricity (e)0.607
Inclination (i)148.4°
Longitude of the node (Ω)82.6°
Periastron epoch (T)2035.10
Argument of periastron (ω)
(secondary)
54.6°
Details
AT Mic A
Mass0.27+0.04
−0.09
 M
Radius0.41 R
Luminosity0.036 L
Temperature3,150 K
Age12+8
−4
 Myr
AT Mic B
Mass0.25+0.04
−0.09
 M
Radius0.37 R
Luminosity0.033 L
Temperature3150 K
Other designations
AT Mic, CD−32°16135, GJ 799, HD 196982, HIP 102141, SAO 212355, WDS J20452-3120BC
Database references
SIMBADdata
ARICNSA
B
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