Discovery | |
---|---|
Discovered by | Paul A. Dalba et al. [1] |
Discovery date | 2021 |
Designations | |
KOI-375.01 | |
Orbital characteristics | |
Periastron | 0.16 |
Apoastron | 3.9 |
2.026+0.024 −0.031 AU | |
Eccentricity | 0.921+0.010 −0.015 |
988.8811177±0.0009114 [2] | |
Inclination | 89.01+0.59 −0.27° |
Physical characteristics | |
10.81 R🜨 [2] | |
Mass | 4.15 ± 0.29 MJ |
Temperature | 253.8+3.7 −4.1 K [1] |
Kepler-1704b is a super-Jupiter on a highly eccentric orbit around the star Kepler-1704. It has a mass of 4.51 MJ. The planet's distance from its star varies from 0.16 to 3.9 AU. It is a failed hot Jupiter, having been scattered from its birth orbit to orbit with a periastron just above the tidal circularization distance. [1]
Kepler-1704b is much more massive than Jupiter, at 4.51 MJ. [1] The high planetary mass makes Kepler-1704b a super-Jupiter. Kepler-1704b goes on a highly eccentric 2.7 year-long (988.88 days) orbit around its star as well as transiting. [1] The extreme eccentricity yields a temperature difference of up to 700 K. [1]
The star, Kepler-1704, is a G2, 5745-kelvin star 825 parsecs (2,690 ly) from Earth and the sun. It has a mass of 1.131 M☉, a radius of 1.697 R☉, and a luminosity of 2.83 L☉. The high radius for the star's mass hints that Kepler-1704 is not a main-sequence star. [3]