From Wikipedia, the free encyclopedia

Gliese 341 Information

Gliese 341
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]
Distance34.082 ± 0.005  ly
(10.450 ± 0.002  pc)
Details [4]
Mass0.522 [5]  M
Radius0.506  R
Surface gravity (log g)4.72±0.02  cgs
Temperature3770±40  K
Other designations
CD−59 2351, CPD−59 1362, GJ 341, HD 304636, HIP 45908, L 140-9, LFT 643, LHS 2128, LTT 3453, NLTT 21618, TOI-741, TIC 359271092, TYC 8940-2067-1 [3]
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.

Planetary system

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]

The Gliese 341 planetary system [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🜨

See also

Notes

  1. ^ Calculated from a/R*

References

  1. ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
  2. ^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211. Bibcode: 2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940. S2CID  244398875. Gaia DR3 record for this source at VizieR.
  3. ^ a b c d e f g h "GJ 341". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 15 January 2024.
  4. ^ a b c d Kirk, James; Stevenson, Kevin B.; et al. (March 2024). "JWST/NIRCam Transmission Spectroscopy of the Nearby Sub-Earth GJ 341b". The Astronomical Journal. 167 (3): 90. arXiv: 2401.06043. Bibcode: 2024AJ....167...90K. doi: 10.3847/1538-3881/ad19df.{{ cite journal}}: CS1 maint: unflagged free DOI ( link)
  5. ^ a b "ExoFOP TIC 359271092". exofop.ipac.caltech.edu. Retrieved 15 January 2024.

TOI-540 Information

TOI-540
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]
Distance45.61 ± 0.01  ly
(13.983 ± 0.004  pc)
Details [4]
Mass0.159±0.014  M
Radius0.1895±0.0079  R
Luminosity (bolometric)0.00346±0.00021  L
Temperature3216±83  K
Rotation0.72610±0.00039  d
Rotational velocity (v sin i)13.5±1.5 km/s
Age0.1-2  Gyr
Other designations
TOI-540, TIC 200322593, 2MASS J05051443-4756154, UPM J0505-4756 [3]
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.

Planetary system

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]

The TOI-540 planetary system [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🜨

References

  1. ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
  2. ^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211. Bibcode: 2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940. S2CID  244398875. Gaia DR3 record for this source at VizieR.
  3. ^ a b c d e f g "TOI-540". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 15 January 2024.
  4. ^ a b c d Ment, Kristo; Irwin, Jonathan; et al. (January 2021). "TOI 540 b: A Planet Smaller than Earth Orbiting a Nearby Rapidly Rotating Low-mass Star". The Astronomical Journal. 161 (1): 23. arXiv: 2009.13623. Bibcode: 2021AJ....161...23M. doi: 10.3847/1538-3881/abbd91.{{ cite journal}}: CS1 maint: unflagged free DOI ( link)


From Wikipedia, the free encyclopedia

Gliese 341 Information

Gliese 341
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]
Distance34.082 ± 0.005  ly
(10.450 ± 0.002  pc)
Details [4]
Mass0.522 [5]  M
Radius0.506  R
Surface gravity (log g)4.72±0.02  cgs
Temperature3770±40  K
Other designations
CD−59 2351, CPD−59 1362, GJ 341, HD 304636, HIP 45908, L 140-9, LFT 643, LHS 2128, LTT 3453, NLTT 21618, TOI-741, TIC 359271092, TYC 8940-2067-1 [3]
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.

Planetary system

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]

The Gliese 341 planetary system [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🜨

See also

Notes

  1. ^ Calculated from a/R*

References

  1. ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
  2. ^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211. Bibcode: 2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940. S2CID  244398875. Gaia DR3 record for this source at VizieR.
  3. ^ a b c d e f g h "GJ 341". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 15 January 2024.
  4. ^ a b c d Kirk, James; Stevenson, Kevin B.; et al. (March 2024). "JWST/NIRCam Transmission Spectroscopy of the Nearby Sub-Earth GJ 341b". The Astronomical Journal. 167 (3): 90. arXiv: 2401.06043. Bibcode: 2024AJ....167...90K. doi: 10.3847/1538-3881/ad19df.{{ cite journal}}: CS1 maint: unflagged free DOI ( link)
  5. ^ a b "ExoFOP TIC 359271092". exofop.ipac.caltech.edu. Retrieved 15 January 2024.

TOI-540 Information

TOI-540
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]
Distance45.61 ± 0.01  ly
(13.983 ± 0.004  pc)
Details [4]
Mass0.159±0.014  M
Radius0.1895±0.0079  R
Luminosity (bolometric)0.00346±0.00021  L
Temperature3216±83  K
Rotation0.72610±0.00039  d
Rotational velocity (v sin i)13.5±1.5 km/s
Age0.1-2  Gyr
Other designations
TOI-540, TIC 200322593, 2MASS J05051443-4756154, UPM J0505-4756 [3]
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.

Planetary system

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]

The TOI-540 planetary system [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🜨

References

  1. ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
  2. ^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211. Bibcode: 2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940. S2CID  244398875. Gaia DR3 record for this source at VizieR.
  3. ^ a b c d e f g "TOI-540". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 15 January 2024.
  4. ^ a b c d Ment, Kristo; Irwin, Jonathan; et al. (January 2021). "TOI 540 b: A Planet Smaller than Earth Orbiting a Nearby Rapidly Rotating Low-mass Star". The Astronomical Journal. 161 (1): 23. arXiv: 2009.13623. Bibcode: 2021AJ....161...23M. doi: 10.3847/1538-3881/abbd91.{{ cite journal}}: CS1 maint: unflagged free DOI ( link)



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