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Star · M4V

2MASS J11124910-2044315

2MASS J11124910-2044315 is a main-sequence star of spectral type M4V in the constellation Crater, 159.8 light-years from the Sun.

ConstellationCrater
Distance159.8 light-years (49.0 pc)
Apparent magnitudemagnitude 20.42
Absolute magnitudemagnitude 16.97
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.56 × 10⁻⁴ L☉
Radius0.0602 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)11h 12m 49.1s
Declination (J2000)−20° 44′ 32″
Space velocity (relative to the Sun)4.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 20.42. Visible from the whole Southern Hemisphere and north to latitude 69° N. South of latitude 69° S 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 1866. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.8 million years.

The Sun seen from there

From a planet around 2MASS J11124910-2044315, the Sun would look like a star of magnitude 8.28, in the direction where our sky has the constellation Pegasus. It would be invisible to the naked eye.

Neighbours

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

  • Alkes 11.0 light-years
  • 2MASS J11060459-1907025 11.5 light-years
  • HIP 55487 12.0 light-years
  • HIP 54804 12.9 light-years
  • GJ 9336 14.2 light-years
  • λ Crt 14.6 light-years
  • HIP 52997 15.4 light-years
  • HIP 53172 16.9 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.