HD 56414

Yazar(lar): Karistus

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HD 56414, aka TOI-1228, is a young binary composed of an A-type main sequence star and a K-type main sequence star located about 873.24 lightyears from the solar system. A single hot Neptune-sized planet on a roughly 30-day orbit around the primary was discovered by TESS. Given the system's young age and the planet's size, Parts of the planet's original atmosphere remain.

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