HD 212301 is a yellow-white main sequence star located approximately 172 light years away in the south circumpolar constellation Octans. The magnitudes are m=7.77 and M=4.16. It has spectral type of F8V. The temperature of the photosphere is 5998 kelvins and have mass 5% more than our Sun. Its age is older than our local star by 1.3 billion years or by the factor of 1.3 times. It is a metal-rich star with 50% more metals than the Sun has. This star is also called HIP 110852.
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- HD 212301 ist ein etwa 180 Lichtjahre entferntes Sternsystem im Sternbild Octans. Es besteht aus zwei Sternen sowie einem Exoplaneten. Hauptkomponente des Systems ist ein Hauptreihenstern der Spektralklasse F8 mit einer scheinbaren visuellen Helligkeit von 7,8 mag, der die 1,3-fache Masse der Sonne aufweist. In einer Winkeldistanz von 4",4 wurde ein Roter Zwerg der Spektralklasse M3 detektiert.
- HD 212301 is a yellow-white main sequence star located approximately 172 light years away in the south circumpolar constellation Octans. The magnitudes are m=7.77 and M=4.16. It has spectral type of F8V. The temperature of the photosphere is 5998 kelvins and have mass 5% more than our Sun. Its age is older than our local star by 1.3 billion years or by the factor of 1.3 times. It is a metal-rich star with 50% more metals than the Sun has. This star is also called HIP 110852.
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- CD−78 1011, GC 31330, HIP 110852, SAO 258040
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- HD 212301 ist ein etwa 180 Lichtjahre entferntes Sternsystem im Sternbild Octans. Es besteht aus zwei Sternen sowie einem Exoplaneten. Hauptkomponente des Systems ist ein Hauptreihenstern der Spektralklasse F8 mit einer scheinbaren visuellen Helligkeit von 7,8 mag, der die 1,3-fache Masse der Sonne aufweist. In einer Winkeldistanz von 4",4 wurde ein Roter Zwerg der Spektralklasse M3 detektiert.
- HD 212301 is a yellow-white main sequence star located approximately 172 light years away in the south circumpolar constellation Octans. The magnitudes are m=7.77 and M=4.16. It has spectral type of F8V. The temperature of the photosphere is 5998 kelvins and have mass 5% more than our Sun. Its age is older than our local star by 1.3 billion years or by the factor of 1.3 times. It is a metal-rich star with 50% more metals than the Sun has. This star is also called HIP 110852.
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