| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus [1] |
| Right ascension | 19h 37m 21.23819s [2] |
| Declination | +50° 20′ 11.5477″ [2] |
| Apparent magnitude (V) | 15.76 [3] |
| Astrometry | |
| Proper motion (μ) |
RA: 2.738
mas/
yr
[2] Dec.: -5.398 mas/ yr [2] |
| Parallax (π) | 0.6597 ± 0.0183 mas [2] |
| Distance | 4,900 ± 100
ly (1,520 ± 40 pc) |
| Details [4] | |
| Mass | 0.99±0.03 M☉ |
| Radius | 1.09±0.05 R☉ |
| Surface gravity (log g) | 4.19±0.10 cgs |
| Temperature | 5835±64 K |
| Metallicity [Fe/H] | 0.010±0.037 dex |
| Other designations | |
| Database references | |
| SIMBAD | data |
Kepler-385 (also designated KOI-2433) is an F-type main-sequence star located about 4,900 light-years (1,500 parsecs) away from Earth in the constellation of Cygnus. The star is 10% larger and 5% hotter than the Sun. The star has at least three, and potentially up to seven, exoplanets discovered orbiting it. [6] [7]
The star has a mass of 1.05 solar masses, a radius of 1.157 solar radii, a temperature of 5829 Kelvin and a luminosity of 1.39 times the solar luminosity. [3]
Planetary system
Kepler-385 was observed by the Kepler space telescope, which initially detected a total of seven planet candidates. Two of these, KOI-2433.01 & .02, were confirmed in 2014 as Kepler-385 b & c, [8] and a third, KOI-2433.03, was confirmed in 2020 as Kepler-385 d. [9] These confirmations were part of studies using statistical validation to confirm large numbers of Kepler candidates. The candidate KOI-2433.05 was shown to be a false positive. [4]
In 2023, a new updated catalog of Kepler candidates was presented, including an eighth candidate around Kepler-385, KOI-2433.08, making it a candidate seven-planet system. [4] [6] Kepler-385 is tied with Kepler-90 - a confirmed eight-planet system - as the Kepler system with the most planet candidates.
| Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| .08 (unconfirmed) | — | — | 3.37376±0.00003 | — | — | 1.206+0.110 −0.101 R🜨 |
| .06 (unconfirmed) | — | 0.067 | 6.06325±0.00006 | — | — | 1.441+0.129 −0.106 R🜨 |
| b | — | 0.097 | 10.04381±0.00008 | — | — | 2.313+0.210 −0.162 R🜨 |
| c | — | 0.127 | 15.16213±0.00014 | — | — | 2.406+0.549 −0.146 R🜨 |
| .04 (unconfirmed) | — | 0.189 | 27.90426±0.00040 | — | — | 1.903+0.184 −0.142 R🜨 |
| d | — | 0.302 | 56.41581±0.00135 | — | — | 2.423+0.210 −0.161 R🜨 |
| .07 (unconfirmed) | — | 0.402 | 86.43086±0.00205 | — | — | 2.252±0.199 R🜨 |
References
- ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
- ^ a b c d 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.
- ^ a b c "Kepler-385 | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 2023-11-07.
- ^ a b c d Lissauer, Jack J.; Rowe, Jason F.; et al. (November 2023). "Updated Catalog of Kepler Planet Candidates: Focus on Accuracy and Orbital Periods". The Planetary Science Journal. arXiv: 2311.00238. Data is available here.
- ^ "Kepler-385". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 November 2023.
- ^ a b "Scorching, Seven-Planet System Revealed by New Kepler Exoplanet List - NASA". 2023-11-02. Retrieved 2023-11-07.
- ^ Anderson, Natali (2023-11-06). "Kepler-385 Hosts Seven Large Exoplanets, Astronomers Say | Sci.News". Sci.News: Breaking Science News. Retrieved 2023-11-07.
- ^ Rowe, Jason F.; Bryson, Stephen T.; et al. (March 2014). "Validation of Kepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-planet Systems". The Astrophysical Journal. 784 (1): 45. arXiv: 1402.6534. Bibcode: 2014ApJ...784...45R. doi: 10.1088/0004-637X/784/1/45.
- ^ Armstrong, David J.; Gamper, Jevgenij; Damoulas, Theodoros (July 2021). "Exoplanet validation with machine learning: 50 new validated Kepler planets". Monthly Notices of the Royal Astronomical Society. 504 (4): 5327–5344. arXiv: 2008.10516. Bibcode: 2021MNRAS.504.5327A. doi: 10.1093/mnras/staa2498.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus [1] |
| Right ascension | 19h 37m 21.23819s [2] |
| Declination | +50° 20′ 11.5477″ [2] |
| Apparent magnitude (V) | 15.76 [3] |
| Astrometry | |
| Proper motion (μ) |
RA: 2.738
mas/
yr
[2] Dec.: -5.398 mas/ yr [2] |
| Parallax (π) | 0.6597 ± 0.0183 mas [2] |
| Distance | 4,900 ± 100
ly (1,520 ± 40 pc) |
| Details [4] | |
| Mass | 0.99±0.03 M☉ |
| Radius | 1.09±0.05 R☉ |
| Surface gravity (log g) | 4.19±0.10 cgs |
| Temperature | 5835±64 K |
| Metallicity [Fe/H] | 0.010±0.037 dex |
| Other designations | |
| Database references | |
| SIMBAD | data |
Kepler-385 (also designated KOI-2433) is an F-type main-sequence star located about 4,900 light-years (1,500 parsecs) away from Earth in the constellation of Cygnus. The star is 10% larger and 5% hotter than the Sun. The star has at least three, and potentially up to seven, exoplanets discovered orbiting it. [6] [7]
The star has a mass of 1.05 solar masses, a radius of 1.157 solar radii, a temperature of 5829 Kelvin and a luminosity of 1.39 times the solar luminosity. [3]
Planetary system
Kepler-385 was observed by the Kepler space telescope, which initially detected a total of seven planet candidates. Two of these, KOI-2433.01 & .02, were confirmed in 2014 as Kepler-385 b & c, [8] and a third, KOI-2433.03, was confirmed in 2020 as Kepler-385 d. [9] These confirmations were part of studies using statistical validation to confirm large numbers of Kepler candidates. The candidate KOI-2433.05 was shown to be a false positive. [4]
In 2023, a new updated catalog of Kepler candidates was presented, including an eighth candidate around Kepler-385, KOI-2433.08, making it a candidate seven-planet system. [4] [6] Kepler-385 is tied with Kepler-90 - a confirmed eight-planet system - as the Kepler system with the most planet candidates.
| Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| .08 (unconfirmed) | — | — | 3.37376±0.00003 | — | — | 1.206+0.110 −0.101 R🜨 |
| .06 (unconfirmed) | — | 0.067 | 6.06325±0.00006 | — | — | 1.441+0.129 −0.106 R🜨 |
| b | — | 0.097 | 10.04381±0.00008 | — | — | 2.313+0.210 −0.162 R🜨 |
| c | — | 0.127 | 15.16213±0.00014 | — | — | 2.406+0.549 −0.146 R🜨 |
| .04 (unconfirmed) | — | 0.189 | 27.90426±0.00040 | — | — | 1.903+0.184 −0.142 R🜨 |
| d | — | 0.302 | 56.41581±0.00135 | — | — | 2.423+0.210 −0.161 R🜨 |
| .07 (unconfirmed) | — | 0.402 | 86.43086±0.00205 | — | — | 2.252±0.199 R🜨 |
References
- ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
- ^ a b c d 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.
- ^ a b c "Kepler-385 | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 2023-11-07.
- ^ a b c d Lissauer, Jack J.; Rowe, Jason F.; et al. (November 2023). "Updated Catalog of Kepler Planet Candidates: Focus on Accuracy and Orbital Periods". The Planetary Science Journal. arXiv: 2311.00238. Data is available here.
- ^ "Kepler-385". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 November 2023.
- ^ a b "Scorching, Seven-Planet System Revealed by New Kepler Exoplanet List - NASA". 2023-11-02. Retrieved 2023-11-07.
- ^ Anderson, Natali (2023-11-06). "Kepler-385 Hosts Seven Large Exoplanets, Astronomers Say | Sci.News". Sci.News: Breaking Science News. Retrieved 2023-11-07.
- ^ Rowe, Jason F.; Bryson, Stephen T.; et al. (March 2014). "Validation of Kepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-planet Systems". The Astrophysical Journal. 784 (1): 45. arXiv: 1402.6534. Bibcode: 2014ApJ...784...45R. doi: 10.1088/0004-637X/784/1/45.
- ^ Armstrong, David J.; Gamper, Jevgenij; Damoulas, Theodoros (July 2021). "Exoplanet validation with machine learning: 50 new validated Kepler planets". Monthly Notices of the Royal Astronomical Society. 504 (4): 5327–5344. arXiv: 2008.10516. Bibcode: 2021MNRAS.504.5327A. doi: 10.1093/mnras/staa2498.