RP112005

RP112005 is a planet located in the habitable zone of the outer rim planetary system RP112005. It was discovered in 2020 as part of a larger observational survey. The planet is situated approximately 1,000 light-years from Earth in the constellation of Vulpecula.

Characterization of RP112005 has been conducted primarily through transit spectroscopy and follow-up radial velocity measurements. Initial studies indicated that the planet orbits a K-type main-sequence star, with estimated parameters of an orbital period of 130 Earth days, a close-in semi-major axis of 0.25 astronomical units (AU), and an eccentricity of 0. One of the defining characteristics of RP112005 is its prospective habitability, suggested by its orbit within the star's habitable zone. This does not guarantee the existence of liquid water, but suggests regions might meet conditions necessary to sustain it.

Continued observations of RP112005 have furthered our understanding of its atmosphere. The world is considered a super-Earth, with a mass several times that of Earth and possibly an atmosphere composed primarily of hydrogen gas. Ground-based follow-up observations may reveal the charge of clouds of gas floating in the celestial body's atmosphere.

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