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Star · M6 V

TOI-2267 B

TOI-2267 B is a main-sequence star of spectral type M6 V in the constellation Cepheus, 73.5 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationCepheus
Distance73.5 light-years (22.6 pc)
Apparent magnitudemagnitude 18.74
Absolute magnitudemagnitude 16.97
Spectral typeM6 V
Surface temperature3,020 K
Luminosity0.0011 L☉
Radius0.13 R☉
Mass0.0989 M☉
Age1.0 billion years
Metallicity [Fe/H]0.16
Right ascension (J2000)4h 20m 14.8s
Declination (J2000)+84° 54′ 03″
Space velocity (relative to the Sun)31.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 18.74. Visible from the whole Northern Hemisphere and south to latitude 5° S. North of latitude 5° N it never sets.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1952. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.3 million years.

The Sun seen from there

From a planet around TOI-2267 B, the Sun would look like a star of magnitude 6.60, in the direction where our sky has the constellation Octans. It would be invisible to the naked eye.

Planets

Neighbours

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

Open in the simulation

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