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Star · M4.0 V

G 264-012

G 264-012 is a main-sequence star of spectral type M4.0 V in the constellation Cepheus, 52.1 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

ConstellationCepheus
Distance52.1 light-years (16.0 pc)
Apparent magnitudemagnitude 13.12
Absolute magnitudemagnitude 12.10
Spectral typeM4.0 V
Surface temperature3,330 K
Luminosity0.0107 L☉
Radius0.305 R☉
Mass0.297 M☉
Metallicity [Fe/H]0.10
Right ascension (J2000)21h 46m 41.3s
Declination (J2000)+66° 48′ 14″
Space velocity (relative to the Sun)34.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.12. Visible from the whole Northern Hemisphere and south to latitude 23° S. North of latitude 23° N it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1974. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 925 thousand years.

The Sun seen from there

From a planet around G 264-012, the Sun would look like a star of magnitude 5.85, in the direction where our sky has the constellation Carina. It would be visible to the naked eye.

Planets

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

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Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.