LHS 3844
LHS 3844 is a red dwarf star located 48.5 light-years (14.9 pc) away from the Solar System in the constellation of Indus. The star has about 15% the mass and 19% the radius of the Sun.[3] It is a relatively inactive red dwarf with a slow rotation period of about 128 days, though UV flares have been observed.[6] LHS 3844 is orbited by one known exoplanet.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Indus[1] |
Right ascension | 22h 41m 58.11718s[2] |
Declination | −69° 10′ 08.3207″[2] |
Apparent magnitude (V) | 15.26±0.03[3] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | M4.5-M5[3] |
Apparent magnitude (V) | 15.26±0.03[3] |
Apparent magnitude (G) | 13.365±0.003[2] |
Apparent magnitude (J) | 10.046±0.023[3] |
Apparent magnitude (H) | 9.477±0.023[3] |
Apparent magnitude (K) | 9.145±0.023[3] |
Astrometry | |
Radial velocity (Rv) | −9.90±0.76[2] km/s |
Proper motion (μ) | RA: 334.419 mas/yr[2] Dec.: −726.986 mas/yr[2] |
Parallax (π) | 67.2123 ± 0.0187 mas[2] |
Distance | 48.53 ± 0.01 ly (14.878 ± 0.004 pc) |
Absolute magnitude (MV) | 14.39±0.02[3] |
Details[3] | |
Mass | 0.151±0.014 M☉ |
Radius | 0.189±0.006 R☉ |
Luminosity (bolometric) | 0.00272±0.0004 L☉ |
Surface gravity (log g) | 5.06±0.01 cgs |
Temperature | 3036±77 K |
Rotation | 128±24 d |
Age | 7.8±1.6[4] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Planetary system
The exoplanet LHS 3844 b was discovered in 2018 using TESS.[3] It is a terrestrial planet larger than Earth with an orbital period of less than a day, and likely does not have an atmosphere. Its low albedo suggests that its surface may resemble that of the Moon or Mercury.[7][8]
In August 2022, this planetary system was included among 20 systems to be named by the third NameExoWorlds project.[9]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ~2.25 M🜨 | 0.00622±0.00017 | 0.46292913±0.0000019 | — | 88.50±0.51° | 1.303±0.022 R🜨 |
References
- "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008. Retrieved 27 August 2022.
- Vallenari, A.; et al. (Gaia Collaboration) (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. arXiv:2208.00211. doi:10.1051/0004-6361/202243940. Gaia DR3 record for this source at VizieR.
- Vanderspek, Roland; et al. (February 2019). "TESS Discovery of an Ultra-short-period Planet around the Nearby M Dwarf LHS 3844". The Astrophysical Journal Letters. 871 (2): L24. arXiv:1809.07242. Bibcode:2019ApJ...871L..24V. doi:10.3847/2041-8213/aafb7a. S2CID 119009146.
- Kane, Stephen R.; et al. (September 2020). "A Volatile-poor Formation of LHS 3844b Based on Its Lack of Significant Atmosphere". The Planetary Science Journal. 1 (2): 36. arXiv:2007.14493. Bibcode:2020PSJ.....1...36K. doi:10.3847/PSJ/abaab5. S2CID 220845575.
- "LHS 3844". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 27 August 2022.
- Diamond-Lowe, Hannah; et al. (July 2021). "The High-energy Spectrum of the Nearby Planet-hosting Inactive Mid-M Dwarf LHS 3844". The Astronomical Journal. 162 (1): 10. arXiv:2104.10522. Bibcode:2021AJ....162...10D. doi:10.3847/1538-3881/abfa1c.
- Kreidburg, Laura; et al. (August 2019). "Absence of a thick atmosphere on the terrestrial exoplanet LHS 3844b". Nature. 573 (7772): 87–90. arXiv:1908.06834. Bibcode:2019Natur.573...87K. doi:10.1038/s41586-019-1497-4. PMID 31427764. S2CID 256819677.
- Diamond-Lowe, Hannah; et al. (October 2020). "Optical Transmission Spectroscopy of the Terrestrial Exoplanet LHS 3844b from 13 Ground-based Transit Observations". The Astronomical Journal. 160 (4): 188. arXiv:2008.05444. Bibcode:2020AJ....160..188D. doi:10.3847/1538-3881/abaf4f. S2CID 221103928.
- "List of ExoWorlds 2022". nameexoworlds.iau.org. IAU. 8 August 2022. Retrieved 27 August 2022.