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Star · M4V

SDSS J104842.70+300650.5

SDSS J104842.70+300650.5 is a main-sequence star of spectral type M4V in the constellation Leo Minor, 179.4 light-years from the Sun.

ConstellationLeo Minor
Distance179.4 light-years (55.0 pc)
Apparent magnitudemagnitude 21.40
Absolute magnitudemagnitude 17.70
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.31 × 10⁻⁴ L☉
Radius0.0431 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)10h 48m 42.7s
Declination (J2000)+30° 06′ 50″
Space velocity (relative to the Sun)35.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.40. Visible from the whole Northern Hemisphere and south to latitude 60° S. North of latitude 60° 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 1847. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.2 million years.

The Sun seen from there

From a planet around SDSS J104842.70+300650.5, the Sun would look like a star of magnitude 8.53, in the direction where our sky has the constellation Piscis Austrinus. It would be invisible to the naked eye.

Neighbours

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

  • SDSS J105814.54+303159.8 9.76 light-years
  • TOI-1806 10.8 light-years
  • HIP 51999 11.8 light-years
  • HIP 53324 12.2 light-years
  • HIP 51487 12.8 light-years
  • HIP 54056 13.2 light-years
  • HIP 53452 16.4 light-years
  • HIP 54619 16.5 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.