Kepler-1229 b is located 769.7 light years (236 parsecs) from our solar system, and was discovered in 2016 orbiting its host star Kepler-1229. The apparent magnitude of the host star is 13.2 and the absolute magnitude is 6.4. Kepler-1229 is about 0.5 the mass of our sun and has about 0.5 the radius. It’s surface temperature is 3784 K and is a spectral M0 type star. The planet Kepler-1229 b orbits the star every 86.8 days, it’s orbital radius is 0.31 SEAU.
Kepler-1410 b is located 1197.0 light-years (367 parsecs) from our solar system and was discovered in 2016 orbiting its host star Kepler-1410. The apparent magnitude of the host star is 13.6 and the absolute magnitude is 5.8. Kepler-1410 is about 0.6 the mass of our sun and has about 0.6 the radius. Its surface temperature is 4092 K and is a spectral K7 type star. The planet Kepler-1410 b orbits the star every 60.9 days, it’s orbital radius is 0.26 SEAU.
Kepler-1455 b is located 1278.5 light-years (392 parsecs) from our solar system and was discovered in 2016 orbiting its host star Kepler-1455. The apparent magnitude of the host star is 13.8 and the absolute magnitude is 5.8. Kepler-1455 is about 0.6 the mass of our sun and has about 0.6 the radius. Its surface temperature is 4075 K and is a spectral K7 type star. The planet Kepler-1455 b orbits the star every 49.3 days, it’s orbital radius is 0.22 SEAU.
For more information about Kepler-1455 b please visit the ExoKyoto database:
<Imaginary Picture of Kepler-1544 b, © 2018 ExoplanetKyoto- Chise Hatsuoka, SGH Moriyama High School>
[Imaginary Picture of Kepler-1544 b, Fuka Takagi & Yosuke A. Yamashiki ]
Kepler 1544 b is located 1138.3 light-years (349 parsecs) from our solar system and was discovered in 2016 orbiting its host star Kepler 1544. The apparent magnitude of the host star is 12.5 and the absolute magnitude is 4.8. Kepler 1544 is about 0.8 the mass of our sun and has about 0.7 the radius. Its surface temperature is 4886 K and is a spectral K2 type star. The planet Kepler 1544 b orbits the star every 168.8 days, it’s orbital radius is 0.56 SEAU.
Kepler 1544 b has a radius that is thought to be about 1.8 times that of the Earth, and its black body temperature (248 K), which was calculated assuming an albedo of 0.3, is almost that of the Earth (255 K). This might suggest the presence of continents and water. The following imaginary video was posted by PlanetExplorer and details the surface of this planet, but what is it really like?
For more information about Kepler-1544 b, please visit the ExoKyoto Database:
Kepler-1593 b is located 2462.5 light-years (755 parsecs) from our solar system and was discovered in 2016 orbiting its host star Kepler-1593. The apparent magnitude of the host star is 14.2 and the absolute magnitude is 4.8. Kepler-1593 is about 0.8 the mass of our sun and has about 0.8 the radius. Its surface temperature is 4995 K and is a spectral K2 type star. The planet Kepler-1593 b orbits the star every 174.5 days, it’s orbital radius is 0.57 SEAU.
For more information about Kepler-1593 b, visit the ExoKyoto Database:
(Imaginary Picture of Kepler-1606 b by Mr. Daichi Ogawa, SGH Moriyama High School)
Kepler-1606 b is located 2870.2 light-years (880 parsecs) from our solar system and was discovered in 2016 orbiting its host star Kepler-1606. The apparent magnitude of the host star is 13.9 and the absolute magnitude is 4.2. Kepler-1606 is about 0.9 the mass of our sun and has about 0.9 the radius. Its surface temperature is 5422 K and is a spectral G7 type star. The planet Kepler-1606 b orbits the star every 196.4 days, it’s orbital radius is 0.64 SEAU.
Kepler 1606 b has an estimated radius of 2.073 times the Earth (0.185 that of Jupiter). Although the actual weight is unknown, if it is a rocky planet, it should be more than 10 times that of the Earth, but due to its size, it is considered to be a Neptune-type planet. ExoKyoto estimates that it weighs 5.1985 times the Earth. It is located in the habitable zone, but it is slightly inside the runaway greenhouse limit, so there is a possibility that if it has a sea, it might have evaporated.
If you would like to know more about Kepler-1606 b, please see Exokyoto’s database page below.
