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Star · M0V

TOI-6662

TOI-6662 is a main-sequence star of spectral type M0V in the constellation Camelopardalis, 69.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationCamelopardalis
Distance69.0 light-years (21.2 pc)
Apparent magnitudemagnitude 13.34
Absolute magnitudemagnitude 11.71
Spectral typeM0V
Surface temperature3,360 K
Luminosity0.0126 L☉
Radius0.332 R☉
Mass0.313 M☉
Right ascension (J2000)5h 39m 25.4s
Declination (J2000)+74° 46′ 03″
Space velocity (relative to the Sun)14.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.34. Visible from the whole Northern Hemisphere and south to latitude 15° S. North of latitude 15° N it never sets. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1957. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.2 million years.

The Sun seen from there

From a planet around TOI-6662, the Sun would look like a star of magnitude 6.46, in the direction where our sky has the constellation Apus. It would be visible 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.