Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 41m 43.04008s [1] |
Declination | +39° 53′ 11.4990″ [1] |
Characteristics | |
Apparent magnitude (K) | 13.916 [2] |
Astrometry | |
Proper motion (μ) |
RA: −2.088(32)
mas/
yr
[1] Dec.: −4.804(32) mas/ yr [1] |
Parallax (π) | 0.4548 ± 0.0289 mas [1] |
Distance | 7,200 ± 500
ly (2,200 ± 100 pc) |
Details | |
Mass | 1.04±0.08 [3] M☉ |
Radius | 1.73±0.24 [3] R☉ |
Luminosity (bolometric) | 2.57±0.68 [3] L☉ |
Surface gravity (log g) | 3.99±0.10 [3] cgs |
Temperature | 5563±86 [3] K |
Metallicity [Fe/H] | 0.06±0.13 [3] dex |
Age | 8.7±2.1 [3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Kepler-1625 is a 14th- magnitude solar-mass star located in the constellation of Cygnus approximately 7,200 light-years (2,200 parsecs) away. Its mass is within 5% of that of the Sun, but its radius is approximately 70% larger reflecting its more evolved state. A candidate gas giant exoplanet was detected by the Kepler Mission around the star in 2015, [5] which was later validated as a real planet to >99% confidence in 2016. [6] In 2018, the Hunt for Exomoons with Kepler project reported evidence for a Neptune-sized exomoon around this planet, based on observations from NASA’s Kepler mission and the Hubble Space Telescope. [7] [3] Subsequently, the evidence for and reality of this exomoon candidate has been subject to debate. [8] [9] [10] [11]
Kepler-1625 is an approximately solar-mass star and yet is 1.7 times larger in diameter. [3] Its effective temperature is around 5,550 K, slightly lower than that of the Sun. [12] [3] These parameters suggest that Kepler-1625 may be a yellow subgiant nearing the end of its life, with an age of approximately 8.7 billion years. [3] The star has been observed to be photometrically quiet, with periodic variability below 0.02%. [10] Kepler-1625 is located approximately 7,200 light-years away [1] in the constellation Cygnus. [12]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≤11.6 [13] MJ | 0.98±0.14 | 287.3727±0.0022 | — | 89.97±0.02 ° | 11.4±1.6 R🜨 |
The star is known to have one validated planet. Designated Kepler-1625b, it is a Jovian-sized planet orbiting its star every 287.3 Earth days. No other candidate transiting planets have been found around the star. [10]
The Kepler Mission recorded three planetary transits of Kepler-1625b from 2009 to 2013. [5] From these, anomalous out-of-transit flux decrements indicated the possible existence of a Neptune-sized exomoon, as first reported by the Hunt for Exomoons with Kepler project in 2018. [7] The Kepler data were inconclusive and so the planetary transit was re-observed by the Hubble Space Telescope in October 2018. The light curve from Hubble exhibited evidence for both a moon-like transit and a transit timing variation, both of which were consistent as being caused by the same Neptune-sized moon in orbit of Kepler-1625b. [3] The transit timing variation has been independently recovered by two teams analyzing the same data. [8] [9] One of these teams also independently recovered the moon-like transit, but suggest that radial velocity measurements are needed to exclude the possibility of a close-in masquerading planet. [8] The other team are unable to recover the moon-like transit and suggested it may be an artifact of the data reduction. [9] This conclusion was challenged by the original team soon after, who showed that the other analysis exhibits larger systematics that may explain their differing conclusion. [10]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 41m 43.04008s [1] |
Declination | +39° 53′ 11.4990″ [1] |
Characteristics | |
Apparent magnitude (K) | 13.916 [2] |
Astrometry | |
Proper motion (μ) |
RA: −2.088(32)
mas/
yr
[1] Dec.: −4.804(32) mas/ yr [1] |
Parallax (π) | 0.4548 ± 0.0289 mas [1] |
Distance | 7,200 ± 500
ly (2,200 ± 100 pc) |
Details | |
Mass | 1.04±0.08 [3] M☉ |
Radius | 1.73±0.24 [3] R☉ |
Luminosity (bolometric) | 2.57±0.68 [3] L☉ |
Surface gravity (log g) | 3.99±0.10 [3] cgs |
Temperature | 5563±86 [3] K |
Metallicity [Fe/H] | 0.06±0.13 [3] dex |
Age | 8.7±2.1 [3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Kepler-1625 is a 14th- magnitude solar-mass star located in the constellation of Cygnus approximately 7,200 light-years (2,200 parsecs) away. Its mass is within 5% of that of the Sun, but its radius is approximately 70% larger reflecting its more evolved state. A candidate gas giant exoplanet was detected by the Kepler Mission around the star in 2015, [5] which was later validated as a real planet to >99% confidence in 2016. [6] In 2018, the Hunt for Exomoons with Kepler project reported evidence for a Neptune-sized exomoon around this planet, based on observations from NASA’s Kepler mission and the Hubble Space Telescope. [7] [3] Subsequently, the evidence for and reality of this exomoon candidate has been subject to debate. [8] [9] [10] [11]
Kepler-1625 is an approximately solar-mass star and yet is 1.7 times larger in diameter. [3] Its effective temperature is around 5,550 K, slightly lower than that of the Sun. [12] [3] These parameters suggest that Kepler-1625 may be a yellow subgiant nearing the end of its life, with an age of approximately 8.7 billion years. [3] The star has been observed to be photometrically quiet, with periodic variability below 0.02%. [10] Kepler-1625 is located approximately 7,200 light-years away [1] in the constellation Cygnus. [12]
Companion (in order from star) |
Mass |
Semimajor axis ( AU) |
Orbital period ( days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≤11.6 [13] MJ | 0.98±0.14 | 287.3727±0.0022 | — | 89.97±0.02 ° | 11.4±1.6 R🜨 |
The star is known to have one validated planet. Designated Kepler-1625b, it is a Jovian-sized planet orbiting its star every 287.3 Earth days. No other candidate transiting planets have been found around the star. [10]
The Kepler Mission recorded three planetary transits of Kepler-1625b from 2009 to 2013. [5] From these, anomalous out-of-transit flux decrements indicated the possible existence of a Neptune-sized exomoon, as first reported by the Hunt for Exomoons with Kepler project in 2018. [7] The Kepler data were inconclusive and so the planetary transit was re-observed by the Hubble Space Telescope in October 2018. The light curve from Hubble exhibited evidence for both a moon-like transit and a transit timing variation, both of which were consistent as being caused by the same Neptune-sized moon in orbit of Kepler-1625b. [3] The transit timing variation has been independently recovered by two teams analyzing the same data. [8] [9] One of these teams also independently recovered the moon-like transit, but suggest that radial velocity measurements are needed to exclude the possibility of a close-in masquerading planet. [8] The other team are unable to recover the moon-like transit and suggested it may be an artifact of the data reduction. [9] This conclusion was challenged by the original team soon after, who showed that the other analysis exhibits larger systematics that may explain their differing conclusion. [10]