TOI-755

TOI-755, also known as HD 110113, is a Sun-like star with a distance from the Solar System of about and located in the Centaurus constellation. The discovery by Osborn et al. was published at the Monthly Notices of the Royal Astronomical Society in 2021.
Characteristics.
TOI-755 has been classified as a G-type main-sequence star (yellow dwarf). It has a temperature of , and a solar mass of almost 1, similar to the Sun.
Planetary system.
The two planets that are orbiting TOI-755, TOI-755b and TOI-755c, were suspected since 2021. TOI-755b's temperature is over and TOI-755c's temperature is cooler at around , which means they are Hot Neptunes.