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Star · M1V

SDSS J123112.97+405027.9

SDSS J123112.97+405027.9 is a main-sequence star of spectral type M1V in the constellation Canes Venatici, 199.0 light-years from the Sun.

ConstellationCanes Venatici
Distance199.0 light-years (61.0 pc)
Apparent magnitudemagnitude 21.36
Absolute magnitudemagnitude 17.43
Spectral typeM1V
Surface temperature3,410 K
Luminosity6.13 × 10⁻⁵ L☉
Radius0.0224 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)12h 31m 12.8s
Declination (J2000)+40° 50′ 28″
Space velocity (relative to the Sun)53.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.36. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° N it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1827. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.5 million years.

The Sun seen from there

From a planet around SDSS J123112.97+405027.9, the Sun would look like a star of magnitude 8.76, in the direction where our sky has the constellation Phoenix. It would be invisible to the naked eye.

Neighbours

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

  • HIP 61880 6.51 light-years
  • HIP 61010 11.8 light-years
  • 2MASS J12352675+4124310 13.5 light-years
  • HIP 62201 14.6 light-years
  • HIP 61854 14.7 light-years
  • HIP 61674 16.0 light-years
  • HIP 60286 19.2 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.