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Star · M4V

CFBDS J203737.07-192202.9

CFBDS J203737.07-192202.9 is a main-sequence star of spectral type M4V in the constellation Capricornus, 166.3 light-years from the Sun.

ConstellationCapricornus
Distance166.3 light-years (51.0 pc)
Apparent magnitudemagnitude 26.22
Absolute magnitudemagnitude 22.68
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.33 × 10⁻⁶ L☉
Radius0.00434 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)20h 37m 37.1s
Declination (J2000)−19° 22′ 03″
Space velocity (relative to the Sun)12.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 26.22. Visible from the whole Southern Hemisphere and north to latitude 71° N. South of latitude 71° S it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1860. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.0 million years.

The Sun seen from there

From a planet around CFBDS J203737.07-192202.9, the Sun would look like a star of magnitude 8.37, in the direction where our sky has the constellation Cancer. It would be invisible to the naked eye.

Neighbours

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

  • HIP 101651 1.53 light-years
  • HIP 100685 8.87 light-years
  • HIP 101443 12.2 light-years
  • HIP 102675 12.2 light-years
  • HIP 101942 13.2 light-years
  • HIP 101785 13.8 light-years
  • HIP 100568 14.7 light-years
  • HIP 101906 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.