Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus[1] |
Right ascension | 20h 49m 27.44052s[2] |
Declination | +33° 36′ 50.9686″[2] |
Apparent magnitude (V) | 17.8 (estimate)[3] |
Characteristics | |
Evolutionary stage | Red dwarf |
Spectral type | M6.5±0.5[4] |
Apparent magnitude (B) | 19[5] |
Apparent magnitude (R) | 16.4[5] |
Apparent magnitude (G) | 15.379[2] |
Apparent magnitude (J) | 11.5[6] |
Apparent magnitude (H) | 10.867±0.021[5] |
Apparent magnitude (K) | 10.54[6] |
Astrometry | |
Proper motion (μ) | RA: –207.809 mas/yr[2] Dec.: –412.215 mas/yr[2] |
Parallax (π) | 59.7005 ± 0.0434 mas[2] |
Distance | 54.63 ± 0.04 ly (16.75 ± 0.01 pc)[2] |
Details[4] | |
Mass | 0.1009±0.0024 M☉ |
Radius | 0.123±0.0022 R☉ |
Luminosity | 0.000835±0.000019 L☉ |
Surface gravity (log g) | 5.265±0.014 cgs |
Temperature | 2800±29 K |
Metallicity [Fe/H] | 0.07±0.1 dex |
Rotation | 1.34±0.14 d |
Rotational velocity (v sin i) | 4.8±0.5 km/s |
Age | 6.6+1.8 −2.4 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
SPECULOOS-3, also known as LSPM J2049+3336, is a red dwarf star (spectral type M6.5) located 54.6 light-years from Earth[4] in the constellation Cygnus. It is one of the smallest known stars, and is much cooler, dimmer and smaller than the Sun, having 0.1 times the mass, 0.08% the Sun's luminosity, and an effective temperature of 2,800 K (2,530 °C), which is less than half of the Sun's temperature (5,772 K).[4] It is orbited by one known exoplanet, and is the second ultra-cool dwarf discovered to have a planetary system, after TRAPPIST-1.[7][8]
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