G 9-38

GJ 1116

An ultraviolet band light curve showing several flares on EI Cancri, adapted from Pettersen (1985)
Observation data
Epoch J2000      Equinox J2000
Constellation Cancer
Right ascension 08h 58m 15.194s
Declination +19° 45 47.08
Apparent magnitude (V) 13.720
Characteristics
Spectral type M8Ve+M7V
Astrometry
G 9-38 A
Radial velocity (Rv)13 ± 5 km/s
Proper motion (μ) RA: −767.060±0.122 mas/yr
Dec.: −100.176±0.083 mas/yr
Parallax (π)194.1443±0.1228 mas
Distance16.80 ± 0.01 ly
(5.151 ± 0.003 pc)
G 9-38 B
Proper motion (μ) RA: −937.133±0.190 mas/yr
Dec.: −34.559±0.138 mas/yr
Parallax (π)196.2619 ± 0.1976 mas
Distance16.62 ± 0.02 ly
(5.095 ± 0.005 pc)
Orbit
PrimaryG 9-38A
CompanionG 9-38B
Period (P)360 yr
Semi-major axis (a)33 AU
Details
G 9-38A
Mass0.127±0.043 M
Radius0.136±0.020 R
Luminosity (bolometric)0.000965 L
Temperature2896±18 K
Metallicity [Fe/H]+0.08 dex
G 9-38B
Mass0.111±0.045 M
Radius0.119±0.021 R
Luminosity (bolometric)0.000992 L
Metallicity [Fe/H]+0.14 dex
Other designations
EI Cnc, GJ 1116, WDS J08582+1945AB, G 9-38, G 47-14, G 41-11, LP 426-40, LTT 12343, PLX 2144.03, GSC 01397-01138, 2MASS J08581519+1945470
A: Gaia DR2 660597997696173440, LHS 2076, NLTT 20638
B: Gaia DR2 660597997697274752, LHS 2077, NLTT 20637
Database references
SIMBADThe system
A
B
G 9-38
Location of G 9-38 in the constellation Cancer

G 9-38, also known as EI Cancri and GJ 1116, is a binary star system consisting of two M-type stars. Located at a distance of 16.7 light-years, it is among the nearest star systems.

In 1985, Bjørn Ragnvald Pettersen announced his discovery that the star shows very high stellar flare activity, with an average of five flares per hour. It was given its variable star designation, EI Cancri, in 1987.

In 2015, the search for third star in the system has yielded inconclusive results.