Gliese 221

Gliese 221 is an orange-red dwarf star 66 light years from Earth. It is depleted in heavy elements, containing just 46% of solar abundance of iron.[2]

Gliese 221
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Orion
Right ascension 05h 53m 00.0s
Declination −05° 59 41
Apparent magnitude (V) 9.69 ± 0.01
Characteristics
Spectral type K7V/M0V
Astrometry
Radial velocity (Rv)22.9±0.4[1] km/s
Proper motion (μ) RA: -1.170[1] mas/yr
Dec.: -346.762[1] mas/yr
Parallax (π)49.2485 ± 0.0185[1] mas
Distance66.23 ± 0.02 ly
(20.305 ± 0.008 pc)
Details[2]
Mass0.72±0.21 M
Radius? R
Luminosity0.095 ± 0.01 L
Surface gravity (log g)4.74 ± 0.02 cgs
Temperature4324 ± 100 K
Metallicity-0.34±0.08
Age4.4±4 Gyr
Other designations
BD-061339, HIP 27803, LTT 2396, 2MASS J05530028-0559410, Gaia EDR3 3022099969137163904
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia
data

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 planet, and an eccentric Neptune / Saturn in the habitable zone, were deduced by radial velocity in January 2013.[3] They were confirmed in May 2013.[4] In January 2014, a candidate planet d was proposed.[5]

The planet Gliese 221b is not transiting the disk of the parent star.[6]

The Gliese 221 planetary system[7][3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b >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

  1. Brown, A. G. A.; et al. (Gaia collaboration). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics (in press). arXiv:2012.01533. doi:10.1051/0004-6361/202039657. S2CID 227254300. Gaia EDR3 record for this source at VizieR.
  2. SWEET-Cat updated New homogenous spectroscopic parameters, 2018, arXiv:1810.08108
  3. G. Lo Curto; et al. (2013). "The HARPS search for southern extrasolar planets: XXXVI. New multi-planet systems in the HARPS volume limited sample: a super-Earth and a Neptune in the habitable zone". Astronomy & Astrophysics. 551: A59. arXiv:1301.2741. Bibcode:2013A&A...551A..59L. doi:10.1051/0004-6361/201220415.
  4. Two planetary companions around the K7 dwarf GJ 221 : a hot super-Earth and a candidate in the sub-Saturn desert range, 2013, arXiv:1305.2203
  5. A new cold sub-Saturnian candidate planet orbiting GJ 221, 2014, arXiv:1401.4000
  6. The Spitzer search for the transits of HARPS low-mass planets -II. Null results for 19 planets, 2017, arXiv:1701.01303
  7. "Planet BD-061339b".
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