Ross 176

Autor(zy): SolaraSystem

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Ross 176, also known as TOI‑4491 and TIC 193336820, is a single K7‑type main‑sequence star about 152 light‑years away in the constellation Cygnus. A hot sub‑Neptune with a 5.01‑day orbital period was discovered via the transit method, whose planet has a mass of approximately 4.57 times that of Earth and a radius of 1.84 times that of Earth.

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