Your Eyes In Space Open the simulation

Star · M3V

2MASS J06320617+8305014

2MASS J06320617+8305014 is a main-sequence star of spectral type M3V in the constellation Camelopardalis, 74.4 light-years from the Sun.

ConstellationCamelopardalis
Distance74.4 light-years (22.8 pc)
Apparent magnitudemagnitude 21.18
Absolute magnitudemagnitude 19.39
Spectral typeM3V
Surface temperature3,120 K
Luminosity1.88 × 10⁻⁵ L☉
Radius0.0148 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)6h 32m 06.3s
Declination (J2000)+83° 05′ 00″
Space velocity (relative to the Sun)26.7 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.18. Visible from the whole Northern Hemisphere and south to latitude 7° S. North of latitude 7° 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 2MASS J06320617+8305014, the Sun would look like a star of magnitude 6.62, in the direction where our sky has the constellation Octans. It would be invisible to the naked eye.

Neighbours

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

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.