HD 25295

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HD 25295, also known as TOI-4602, is a single G-type main-sequence star about 205 light-years away in the constellation Perseus. In 2026, a hot sub-Neptune with a 3.98-day orbital period was discovered via the transit method, whose planet has a mass of approximately 5.5 times that of Earth and a radius of 2.5 times that of Earth.

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