Gliese 221

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Gliese 221
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Orion
Right ascension 05h 53m 00.285s[1]
Declination −05° 59′ 41.44″[1]
Apparent magnitude (V) 9.70[2]
Characteristics
Spectral type K7V/M0V[3]
B−V color index 1.321±0.001[2]
Distance
66.23 ± 0.02 ly
(20.305 ± 0.008 pc)
Absolute magnitude (MV)8.154±0.077[4]
Details
Gyr
Gaia EDR3
3022099969137163904
Database references
Exoplanet Archive
data

Gliese 221 (GJ 221), also known as BD-06 1339, is a

″·yr−1.[7]

This is a

active star and the level of chromospheric activity has been found to vary significantly over time.[3] The star is radiating 10%[5] of the luminosity of the Sun from its photosphere at an effective temperature of 4,324 K.[5]

Planetary system

From 2003 to 2012, the star was under observance from the High Accuracy Radial Velocity Planet Searcher (

HARPS
). It is becoming less active and this reduced activity allowed for lower-mass planetary measurements to be made.

A super-Venus

d was proposed.[10]

The planet Gliese 221b (BD-06 1339 b) is not transiting the disk of the parent star,[11] and its existence was disputed in 2022.[12]

The Gliese 221 planetary system[13][8]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b (disputed[12]) >8.5806 ± 1.2712 M🜨 0.0428 ± 0.0007 3.8728 ± 0.0004
c >54.026 ± 9.534 M🜨 0.435 ± 0.007 125.94 ± 0.44 0.31 ± 0.11
d (unconfirmed) 22.246 M🜨 1.0947 500

References