Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Carina [1] |
Right ascension | 09h 21m 37.60154s [2] |
Declination | −60° 16′ 55.0300″ [2] |
Apparent magnitude (V) | 9.465 [3] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | M0.0 [3] |
Apparent magnitude (B) | 10.955 [3] |
Apparent magnitude (V) | 9.465 [3] |
Apparent magnitude (G) | 8.681±0.003 [2] |
Apparent magnitude (J) | 6.442±0.023 [3] |
Apparent magnitude (H) | 5.793±0.033 [3] |
Apparent magnitude (K) | 5.587±0.021 [3] |
Astrometry | |
Radial velocity (Rv) | 39.59±0.14 [2] km/s |
Proper motion (μ) |
RA: -840.185
mas/
yr
[2] Dec.: 182.056 mas/ yr [2] |
Parallax (π) | 95.6982 ± 0.0145 mas [2] |
Distance | 34.082 ± 0.005
ly (10.450 ± 0.002 pc) |
Details [4] | |
Mass | 0.522 [5] M☉ |
Radius | 0.506 R☉ |
Surface gravity (log g) | 4.72±0.02 cgs |
Temperature | 3770±40 K |
Other designations | |
Database references | |
SIMBAD | data |
Gliese 341 is a red dwarf star located 34.1 light-years (10.5 parsecs) away in the constellation Carina. It hosts one known exoplanet.
Evidence of a transiting exoplanet, Gliese 341 b, was found in data from TESS, [5] and was confirmed in January 2024 along with a spectrum from JWST. The spectrum is consistent with the planet having no atmosphere, a hazy atmosphere, or an atmosphere mainly composed of certain molecules such as water vapor, while ruling out other types of atmospheres. [4]
Gliese 341 b is slightly smaller than Earth, at 92% of its radius. Its mass is known to be less than 4.5 times that of Earth, and is predicted to be about 0.72±0.14 M🜨 based on its radius. It orbits close to its star, completing an orbit every 7.6 days, and has an equilibrium temperature of 540 K (267 °C; 512 °F). [4]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | <4.5 M🜨 | 0.0577 [note 1] | 7.576863 | — | 89.22+0.54 −0.96 ° |
0.92±0.05 R🜨 |
{{
cite journal}}
: CS1 maint: unflagged free DOI (
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Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pictor [1] |
Right ascension | 05h 05m 14.42843s [2] |
Declination | −47° 56′ 15.5263″ [2] |
Apparent magnitude (V) | 14.365 [3] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | M [4] |
Apparent magnitude (B) | 15.960±0.07 [3] |
Apparent magnitude (V) | 14.365±0.04 [3] |
Apparent magnitude (G) | 12.874±0.003 [2] |
Apparent magnitude (J) | 9.755±0.022 [3] |
Apparent magnitude (H) | 9.170±0.022 [3] |
Apparent magnitude (K) | 8.900±0.021 [3] |
Astrometry | |
Radial velocity (Rv) | 17.33±1.03 [2] km/s |
Proper motion (μ) |
RA: -65.901
mas/
yr
[2] Dec.: 24.895 mas/ yr [2] |
Parallax (π) | 71.5134 ± 0.0215 mas [2] |
Distance | 45.61 ± 0.01
ly (13.983 ± 0.004 pc) |
Details [4] | |
Mass | 0.159±0.014 M☉ |
Radius | 0.1895±0.0079 R☉ |
Luminosity (bolometric) | 0.00346±0.00021 L☉ |
Temperature | 3216±83 K |
Rotation | 0.72610±0.00039 d |
Rotational velocity (v sin i) | 13.5±1.5 km/s |
Age | 0.1-2 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
TOI-540 is a red dwarf star located 45.6 light-years (14.0 parsecs) away in the constellation Pictor. It has about 16% the mass and 19% the radius of the Sun, and a temperature of about 3,216 K (2,943 °C; 5,329 °F). This is a rapidly-rotating star, with a rotation period of only 17 hours. TOI-540 hosts one known exoplanet.
The exoplanet TOI-540 b is a transiting planet smaller than Earth, discovered in 2020 by TESS. It orbits very close to its star, completing an orbit in just over a day, and has an equilibrium temperature of 611 K (338 °C; 640 °F). [4]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | — | 0.01223±0.00036 | 1.2391491(17) | 0 | 86.80±0.28 ° | 0.903±0.052 R🜨 |
{{
cite journal}}
: CS1 maint: unflagged free DOI (
link)
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Carina [1] |
Right ascension | 09h 21m 37.60154s [2] |
Declination | −60° 16′ 55.0300″ [2] |
Apparent magnitude (V) | 9.465 [3] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | M0.0 [3] |
Apparent magnitude (B) | 10.955 [3] |
Apparent magnitude (V) | 9.465 [3] |
Apparent magnitude (G) | 8.681±0.003 [2] |
Apparent magnitude (J) | 6.442±0.023 [3] |
Apparent magnitude (H) | 5.793±0.033 [3] |
Apparent magnitude (K) | 5.587±0.021 [3] |
Astrometry | |
Radial velocity (Rv) | 39.59±0.14 [2] km/s |
Proper motion (μ) |
RA: -840.185
mas/
yr
[2] Dec.: 182.056 mas/ yr [2] |
Parallax (π) | 95.6982 ± 0.0145 mas [2] |
Distance | 34.082 ± 0.005
ly (10.450 ± 0.002 pc) |
Details [4] | |
Mass | 0.522 [5] M☉ |
Radius | 0.506 R☉ |
Surface gravity (log g) | 4.72±0.02 cgs |
Temperature | 3770±40 K |
Other designations | |
Database references | |
SIMBAD | data |
Gliese 341 is a red dwarf star located 34.1 light-years (10.5 parsecs) away in the constellation Carina. It hosts one known exoplanet.
Evidence of a transiting exoplanet, Gliese 341 b, was found in data from TESS, [5] and was confirmed in January 2024 along with a spectrum from JWST. The spectrum is consistent with the planet having no atmosphere, a hazy atmosphere, or an atmosphere mainly composed of certain molecules such as water vapor, while ruling out other types of atmospheres. [4]
Gliese 341 b is slightly smaller than Earth, at 92% of its radius. Its mass is known to be less than 4.5 times that of Earth, and is predicted to be about 0.72±0.14 M🜨 based on its radius. It orbits close to its star, completing an orbit every 7.6 days, and has an equilibrium temperature of 540 K (267 °C; 512 °F). [4]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | <4.5 M🜨 | 0.0577 [note 1] | 7.576863 | — | 89.22+0.54 −0.96 ° |
0.92±0.05 R🜨 |
{{
cite journal}}
: CS1 maint: unflagged free DOI (
link)
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pictor [1] |
Right ascension | 05h 05m 14.42843s [2] |
Declination | −47° 56′ 15.5263″ [2] |
Apparent magnitude (V) | 14.365 [3] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | M [4] |
Apparent magnitude (B) | 15.960±0.07 [3] |
Apparent magnitude (V) | 14.365±0.04 [3] |
Apparent magnitude (G) | 12.874±0.003 [2] |
Apparent magnitude (J) | 9.755±0.022 [3] |
Apparent magnitude (H) | 9.170±0.022 [3] |
Apparent magnitude (K) | 8.900±0.021 [3] |
Astrometry | |
Radial velocity (Rv) | 17.33±1.03 [2] km/s |
Proper motion (μ) |
RA: -65.901
mas/
yr
[2] Dec.: 24.895 mas/ yr [2] |
Parallax (π) | 71.5134 ± 0.0215 mas [2] |
Distance | 45.61 ± 0.01
ly (13.983 ± 0.004 pc) |
Details [4] | |
Mass | 0.159±0.014 M☉ |
Radius | 0.1895±0.0079 R☉ |
Luminosity (bolometric) | 0.00346±0.00021 L☉ |
Temperature | 3216±83 K |
Rotation | 0.72610±0.00039 d |
Rotational velocity (v sin i) | 13.5±1.5 km/s |
Age | 0.1-2 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
TOI-540 is a red dwarf star located 45.6 light-years (14.0 parsecs) away in the constellation Pictor. It has about 16% the mass and 19% the radius of the Sun, and a temperature of about 3,216 K (2,943 °C; 5,329 °F). This is a rapidly-rotating star, with a rotation period of only 17 hours. TOI-540 hosts one known exoplanet.
The exoplanet TOI-540 b is a transiting planet smaller than Earth, discovered in 2020 by TESS. It orbits very close to its star, completing an orbit in just over a day, and has an equilibrium temperature of 611 K (338 °C; 640 °F). [4]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | — | 0.01223±0.00036 | 1.2391491(17) | 0 | 86.80±0.28 ° | 0.903±0.052 R🜨 |
{{
cite journal}}
: CS1 maint: unflagged free DOI (
link)