Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cancer |
Right ascension | 09h 00m 23.594s [1] |
Declination | +21° 50′ 05.43″ [1] |
Apparent magnitude (V) | 16.11 [2] |
Characteristics | |
Evolutionary stage | Main-sequence star [2] |
Spectral type | M6.5 V [3] |
Apparent magnitude (J) | 9.44 [2] |
Astrometry | |
Radial velocity (Rv) | 23.3 [2] km/s |
Proper motion (μ) | RA: -514.942 mas/yr [4] Dec.: -592.253 mas/yr [4] |
Parallax (π) | 157.2686 ± 0.0535 mas [4] |
Distance | 20.739 ± 0.007 ly (6.359 ± 0.002 pc) |
Details | |
Mass | 0.09 [5] M☉ |
Radius | 0.12 [6] R☉ |
Luminosity | 0.00082 [7] L☉ |
Temperature | 2680±24 [7] K |
Metallicity [Fe/H] | -0.06±0.17 [8] dex |
Rotation | 0.439 d [6] |
Rotational velocity (v sin i) | 15.0±1.0 [6] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Location of LHS 2090 in the constellation Cancer |
LHS 2090 is a red dwarf star of spectral type M6.5V, located in constellation Cancer at 20.8 light-years from Earth. [10]
The star was identified to be a red dwarf at short distance (6 parsecs from Sun) in 2001. [11] As typical for very cool red dwarfs, its spectrum is dominated by molecular water absorption. Stellar metallicity is similar to that of Sun`s. [8]
Radial velocity measurements did not yield any detection of stellar companion or giant planet on orbit around LHS 2090, as in 2018. [2]
BD−10°3166 is a K-type main sequence star approximately 268 light-years away in the constellation of Crater. It was inconspicuous enough not be included in the Draper catalog (HD). The Hipparcos satellite also did not study it, so its true distance is poorly known. The distance measured by the Gaia spacecraft of 268 light years rules out a suggested companion star, LP 731-076, being its true binary star companion.
SCR 1845−6357 is a binary system, about 13 light-years away in the constellation Pavo. The primary is a faint red dwarf. It has a brown dwarf companion. The primary red dwarf was discovered in 2004 by Hambly et al., while the secondary brown dwarf was later discovered in 2006.
DENIS J1048−3956 is an exceptionally small, dim ultra-cool red dwarf star about 13.2 light years from Earth in the southern constellation of Antlia, among the closest stars to Earth. This star is very dim with an apparent magnitude of about 17, and will require a telescope with a camera to be seen. It was discovered in 2000 by Xavier Delfosse and Thierry Forveille, with the assistance of nine other astronomers.
LHS 288 is a red dwarf around 15.8 light years from the Sun, the closest in the constellation Carina. It is far too faint to be seen with the unaided eye, with an apparent magnitude of 13.92.
LP 658-2 is a degenerate star in the constellation of Orion, the single known object in its system. It has an apparent visual magnitude of approximately 14.488.
L 97-12 is a nearby degenerate star, located in the constellation Volans, the single known component of the system.
WD 2359-434 is a nearby degenerate star of spectral class DAP5.8, the single known component of the system, located in the constellation Phoenix, the nearest star in this constellation.
2MASS J15404341−5101357 is a red dwarf of spectral type M7, located in Norma at approximately 17 light-years from Earth. It is the nearest known M7 dwarf.
LP 816-60 is a single red dwarf star of spectral type M4, located in constellation Capricornus at 18.6 light-years from Earth.
Gliese 555 is a red dwarf star of spectral type M4.0V, located in constellation Libra at 20.2 light-years from Earth.
GJ 1128 is a red dwarf star of spectral type M4.0V, located in constellation Carina 21 light-years away from Earth. It is one of the closer stars to the Sun.
Gliese 54 is a star near the Solar System located at 25.7 light years away. It is located in the constellation of Tucana, close to the edge, almost in the neighboring Hydrus. It is below the threshold brightness to be observable eye with an apparent magnitude of +9.80,.
SIPS 1259-4336 is a red dwarf star first documented in 2005, in the constellation Centaurus. It is located around 25 light-years from Earth.
LTT 1445 is a triple M-dwarf system about 22 light-years distant in the constellation Eridanus. The primary LTT 1445 A hosts two exoplanets- one discovered in 2019 that transits the star every 5.36 days, and another found in 2021 that transits the star every 3.12 days, close to a 12:7 resonance. As of August 2019 it is the second closest transiting exoplanet system discovered, with the closest being HD 219134 bc.
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