astro.wikisort.org - StarGliese 754 is a dim star in the southern constellation of Telescopium. It has an apparent visual magnitude of 12.25,[2] which requires a telescope to view. The star is located at a distance of 19.3 light-years from the Sun based on parallax,[1] and it is drifting further away with a radial velocity of +7 km/s.[3] It is one of the hundred closest stars to the Solar System. Calculations of its orbit around the Milky Way showed that it is eccentric, and indicate that it might be a thick disk object.[8]
High proper motion red dwarf in the constellation of Telescopium
Gliese 754
Observation data Epoch J2000.0 Equinox J2000.0 |
Constellation |
Telescopium |
Right ascension |
19h 20m 47.98349s[1] |
Declination |
−45° 33′ 29.6292″[1] |
Apparent magnitude (V) |
12.25[2] |
Characteristics |
Spectral type |
M4V[2] |
Astrometry |
---|
|
---|
Radial velocity (Rv) | +6.8[3] km/s |
Proper motion (μ) | RA: +659.330[1] mas/yr Dec.: −2,897.035[1] mas/yr |
Parallax (π) | 169.2351 ± 0.0588 mas[4] |
Distance | 19.272 ± 0.007 ly (5.909 ± 0.002 pc) |
|
Details[3] |
---|
|
---|
Mass | 0.173 M☉ |
Radius | 0.205 R☉ |
Luminosity | 0.005[5] L☉ |
Temperature | 3,202±100[6] K |
Metallicity [Fe/H] | −0.169[6] dex |
Rotation | 132.651 days |
|
Other designations |
---|
GJ 754, L 347-14, LHS 60, LTT 7652, 2MASS J19204795-4533283[7] |
Database references |
---|
SIMBAD | data |
Location of Gliese 754 in the constellation Telescopium |
The stellar classification of Gliese 754 is M4V,[2] indicating that this is a small red dwarf star on the core hydrogen fusing main sequence. It has 17% of the mass of the Sun and 21% of the Sun's radius.[3] The star is fully convective and is a source of X-ray emission.[9] It is rotating slowly with a period of about 133 days.[3] The metallicity is sub-solar,[6] indicating it has a lower abundance of heavy elements compared to the Sun. It is radiating just 0.5%[5] of the luminosity of the Sun from its photosphere at an effective temperature of around 3,202 K.[6]
Planetary System
In June 2019 a candidate exoplanet was reported in orbit around Gliese 754. It was detected using the Doppler method and is orbiting at a distance of 0.28 AU with a period of 78 days. The orbit is essentially circular, to within the margin of error.[10] The habitable zone for this star ranges from 0.05 AU to 0.14 AU;[5] inside the orbit of this proposed companion.
The Gliese 754 planetary system
Companion (in order from star) |
Mass |
Semimajor axis (AU) |
Orbital period (days) |
Eccentricity |
Inclination |
Radius |
b (unconfirmed) |
≥9.8+4.6 −5.2 M🜨 |
0.277+0.025 −0.028 |
78.37+0.55 −0.47 |
0.03+0.20 −0.03 |
— |
— |
References
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- Henry, Todd J.; et al. (2018). "The Solar Neighborhood XLIV: RECONS Discoveries within 10 parsecs". The Astronomical Journal. 155 (6): 265. arXiv:1804.07377. Bibcode:2018AJ....155..265H. doi:10.3847/1538-3881/aac262. S2CID 53983430.
- Newton, Elisabeth R.; et al. (November 2018). "New Rotation Period Measurements for M Dwarfs in the Southern Hemisphere: An Abundance of Slowly Rotating, Fully Convective Stars". The Astronomical Journal. 156 (5): 11. arXiv:1807.09365. Bibcode:2018AJ....156..217N. doi:10.3847/1538-3881/aad73b. S2CID 119209638. 217.
- Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- Mayor, M.; et al. (2009). "The HARPS search for southern extra-solar planets. XIII. A planetary system with 3 Super-Earths (4.2, 6.9, & 9.2 Earth masses)". Astronomy and Astrophysics. 493 (2): 639–644. arXiv:0806.4587. Bibcode:2009A&A...493..639M. doi:10.1051/0004-6361:200810451. S2CID 116365802.
- Houdebine, E. R.; et al. (May 2016). "Rotation-Activity Correlations in K and M Dwarfs. I. Stellar Parameters and Compilations of v sin I and P/sin I for a Large Sample of Late-K and M Dwarfs". The Astrophysical Journal. 822 (2): 38. arXiv:1604.07920. Bibcode:2016ApJ...822...97H. doi:10.3847/0004-637X/822/2/97. S2CID 119118088. 97.
- "L 347-14". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-12-12.
- Innanen, K.A.; Flynn, C. (2010). "The Radial Velocity, Space Motion, and Galactic Orbit of GJ 754". Journal of the Royal Astronomical Society of Canada. 104 (6): 223–24. Bibcode:2010JRASC.104..223I.
- Wright, Nicholas J.; et al. (September 2018). "The stellar rotation-activity relationship in fully convective M dwarfs". Monthly Notices of the Royal Astronomical Society. 479 (2): 2351–2360. arXiv:1807.03304. Bibcode:2018MNRAS.479.2351W. doi:10.1093/mnras/sty1670.
- Barnes, J. R.; et al. (June 2019). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644. Bibcode:2019arXiv190604644T.
← Celestial objects within 15–20 light-years |
---|
Primary member type | Celestial objects by systems. |
|
---|
|
|
|
|
Brown dwarfs | L-type |
- DEN 0255-4700 (15.877±0.014 ly)
|
---|
T-type | |
---|
Y-type | |
---|
|
---|
|
Sub-brown dwarfs and rogue planets | |
---|
|
Constellation of Telescopium |
---|
|
Stars | |
---|
|
|
Galaxies | |
---|
 Category |
На других языках
- [en] Gliese 754
[es] Gliese 754
Gliese 754 (GJ 754 / LHS 60 / L 347-14)[1] es una estrella en la constelación de Telescopium situada cerca del límite con Sagitario, visualmente a menos de 1º de Arkab Posterior (β2 Sagittarii). Medidas precisas de su paralaje (169,03 mas)[2] sitúan a Gliese 754 a una distancia de 19,4 años luz, siendo la más estrella más cercana dentro de su constelación y una de las 100 estrellas más próximas al sistema solar.[3] De magnitud aparente +12,23,[1] no es observable a simple vista.
Текст в блоке "Читать" взят с сайта "Википедия" и доступен по лицензии Creative Commons Attribution-ShareAlike; в отдельных случаях могут действовать дополнительные условия.
Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
2019-2025
WikiSort.org - проект по пересортировке и дополнению контента Википедии