LTT 9779
LTT 9779 is a G-type main-sequence star located 264 light-years (81 pc) away from the Solar System in the constellation of Sculptor. The star is about 95% the radius and about the same mass as the Sun. It has a temperature of 5,443 K (5,170 °C; 9,338 °F) and a rotation period of 45 days.[3] LTT 9779 is orbited by one known exoplanet.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Sculptor[1] |
Right ascension | 23h 54m 40.20731s[2] |
Declination | −37° 37′ 40.5244″[2] |
Apparent magnitude (V) | 9.76±0.03[3] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | G7V[3] |
Apparent magnitude (B) | 10.55±0.04[3] |
Apparent magnitude (V) | 9.76±0.03[3] |
Apparent magnitude (G) | 9.606±0.003[2] |
Apparent magnitude (J) | 8.45±0.02[3] |
Apparent magnitude (H) | 8.15±0.02[3] |
Apparent magnitude (K) | 8.02±0.03[3] |
Astrometry | |
Radial velocity (Rv) | −10.72±0.22[2] km/s |
Proper motion (μ) | RA: 247.634 mas/yr[2] Dec.: −69.752 mas/yr[2] |
Parallax (π) | 12.3381 ± 0.0166 mas[2] |
Distance | 264.3 ± 0.4 ly (81.0 ± 0.1 pc) |
Absolute magnitude (MV) | 5.30±0.07[3] |
Details[3] | |
Mass | 1.00+0.02 −0.03 M☉ |
Radius | 0.949±0.006 R☉ |
Luminosity (bolometric) | 0.71±0.01 L☉ |
Surface gravity (log g) | 4.51±0.01 cgs |
Temperature | 5443+14 −13 K |
Metallicity [Fe/H] | 0.27±0.03 dex |
Rotation | 45 d |
Rotational velocity (v sin i) | 1.06±0.37 km/s |
Age | 1.9+1.7 −1.2 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Planetary system
The discovery of the exoplanet LTT 9779 b using TESS was published in 2020. It is an ultra-hot Neptune with about 29 times the mass and 4.7 times the radius of Earth and an orbital period of less than a day. These parameters make it one of the very few known planets in the Neptunian desert.[3] Observations using the Spitzer Space Telescope have measured the planet's dayside temperature at 2,305 K (2,032 °C; 3,689 °F).[5][6] A study published in 2019, prior to the confirmation of planet b, proposed a second candidate planet in the system based on transit timing variations, but this has not been confirmed.[7]
In August 2022, this planetary system was included among 20 systems to be named by the third NameExoWorlds project.[8]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 29.32+0.78 −0.81 M🜨 |
0.01679+0.00014 −0.00012 |
0.7920520±0.0000093 | <0.01 | 76.39±0.43° | 4.72±0.23 R🜨 |
References
- "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008. Retrieved 30 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.
- Jenkins, James S.; Díaz, Matías R.; et al. (September 2020). "An Ultra-Hot Neptune in the Neptune desert". Nature Astronomy. 4 (12): 1148–1157. arXiv:2009.12832. Bibcode:2020NatAs...4.1148J. doi:10.1038/s41550-020-1142-z. S2CID 256707813.
- "LTT 9779". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 30 August 2022.
- Dragomir, Diana; Crossfield, Ian J. M.; et al. (November 2020). "Spitzer Reveals Evidence of Molecular Absorption in the Atmosphere of the Hot Neptune LTT 9779b". The Astrophysical Journal Letters. 903 (1): L6. arXiv:2010.12744. Bibcode:2020ApJ...903L...6D. doi:10.3847/2041-8213/abbc70. S2CID 225067568.
- Crossfield, Ian J. M.; Dragomir, Diana; et al. (November 2020). "Phase Curves of Hot Neptune LTT 9779b Suggest a High-metallicity Atmosphere". The Astrophysical Journal Letters. 903 (1): L7. arXiv:2010.12745. Bibcode:2020ApJ...903L...7C. doi:10.3847/2041-8213/abbc71. S2CID 225067727.
- Pearson, Kyle A. (December 2019). "A Search for Multiplanet Systems with TESS Using a Bayesian N-body Retrieval and Machine Learning". The Astronomical Journal. 158 (6): 243. arXiv:1907.03377. Bibcode:2019AJ....158..243P. doi:10.3847/1538-3881/ab4e1c. S2CID 195833716.
- "List of ExoWorlds 2022". nameexoworlds.iau.org. IAU. 8 August 2022. Retrieved 27 August 2022.