Kepler-1625
Star Kepler-1625 |
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AladinLite | |||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | swan | ||||
Right ascension | 19 h 41 m 43.04 s | ||||
declination | + 39 ° 53 ′ 11.5 ″ | ||||
Typing | |||||
Known exoplanets | 1 | ||||
Astrometry | |||||
parallax | 0.41 ± 0.04 mas | ||||
distance | (8,000) ly (2,400) pc |
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Proper movement | |||||
Rec. Share: | (−2.14 ± 0.06) mas / a | ||||
Dec. portion: | (−4.80 ± 0.07) mas / a | ||||
Physical Properties | |||||
Dimensions | 0.96 M ☉ | ||||
radius | 0.94 R ☉ | ||||
Effective temperature | 5700 K | ||||
Metallicity [Fe / H] | 0.0 | ||||
Age | 4 billion a | ||||
Other names and catalog entries |
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Kepler-1625 is a star in the constellation Swan , of about 8,000 light-years from the sun away. It is orbited by at least one exoplanet , which in turn may be accompanied by an exomoon . Kepler-1625 has an apparent magnitude of only around 14 mag (K-band) and can therefore not be observed with the naked eye.
Planetary system
Based on observations of the star by the Kepler space telescope using the transit method , the discovery of a planet around Kepler-1625, called Kepler-1625b , was announced in 2016 . According to studies published in 2017, the approximately Jupiter-sized planet may be orbited by a Neptune-sized moon .
Individual evidence
- ↑ a b c SIMBAD : Kepler-1625. Retrieved October 8, 2018 .
- ↑ a b T. Morton et al .: False positive probabilties for all Kepler Objects of Interest: 1284 newly validated planets and 428 likely false positives . arxiv : 1605.02825 .
- ↑ a b c d Kepler-1625b. In: NASA Exoplanet Archive . Retrieved October 8, 2018 .
- ^ S. Mathur et al .: Revised Stellar Properties of Kepler Targets for the Q1-17 (DR25) Transit Detection Run . arxiv : 1609.04128 .
- ↑ A. Teachey include: HEK VI: On the Dearth of Galilean analogue in Kepler and the Exomoon Candidate Kepler 1625b I . arxiv : 1707.08563 .