Discovery [1] | |
---|---|
Discovery date | 2023 |
Transit | |
Orbital characteristics [1] | |
0.02709±0.00046 AU | |
Eccentricity | 0.029+0.0 −0.29 |
2.6 days | |
Inclination | 88.14±0.046 ° |
Star | TOI-3235 |
Physical characteristics [1] | |
1.017±0.04 RJ | |
Mass | 0.665±0.025 MJ |
Temperature | 604±19 K |
TOI-3235 b is a gas giant exoplanet found 237 light-years away from Earth. [2] It was discovered in 2023 by the transit method. [2]
TOI-3235 b was discovered by the transit method. The exoplanet's mass is 0.665±0.025 MJ and has a radius of 1.017±0.04 MJ. It's semi-major axis is 0.02709±0.00046 AU and has a temperature of 604±19 Kelvin. [3]
TOI-3235 b has a smaller orbit than Mercury. The exoplanet's orbit is 2.6 days, which is similar to the orbital period of Gliese 436 b and has an inclination of 88.14±0.046 Degree (angle).
The host star of the exoplanet is TOI-3235, a M-type main sequence star (red dwarf) that is not visible to the naked eye from Earth with a apparent magnitude of 14.5. [4] The star has a mass of 0.394±0.003 M☉, a radius of 0.3697±0.0018 R☉ and a temperature of 3388±68 Kelvin. [3] It is located 237 light-years away in the constellation Centaurus. [4] [a]
Discovery [1] | |
---|---|
Discovery date | 2023 |
Transit | |
Orbital characteristics [1] | |
0.02709±0.00046 AU | |
Eccentricity | 0.029+0.0 −0.29 |
2.6 days | |
Inclination | 88.14±0.046 ° |
Star | TOI-3235 |
Physical characteristics [1] | |
1.017±0.04 RJ | |
Mass | 0.665±0.025 MJ |
Temperature | 604±19 K |
TOI-3235 b is a gas giant exoplanet found 237 light-years away from Earth. [2] It was discovered in 2023 by the transit method. [2]
TOI-3235 b was discovered by the transit method. The exoplanet's mass is 0.665±0.025 MJ and has a radius of 1.017±0.04 MJ. It's semi-major axis is 0.02709±0.00046 AU and has a temperature of 604±19 Kelvin. [3]
TOI-3235 b has a smaller orbit than Mercury. The exoplanet's orbit is 2.6 days, which is similar to the orbital period of Gliese 436 b and has an inclination of 88.14±0.046 Degree (angle).
The host star of the exoplanet is TOI-3235, a M-type main sequence star (red dwarf) that is not visible to the naked eye from Earth with a apparent magnitude of 14.5. [4] The star has a mass of 0.394±0.003 M☉, a radius of 0.3697±0.0018 R☉ and a temperature of 3388±68 Kelvin. [3] It is located 237 light-years away in the constellation Centaurus. [4] [a]