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Star · M4V

SDSS J095850.68+200150.6

SDSS J095850.68+200150.6 is a main-sequence star of spectral type M4V in the constellation Leo, 192.4 light-years from the Sun.

ConstellationLeo
Distance192.4 light-years (59.0 pc)
Apparent magnitudemagnitude 21.58
Absolute magnitudemagnitude 17.73
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.28 × 10⁻⁴ L☉
Radius0.0425 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)9h 58m 50.8s
Declination (J2000)+20° 01′ 52″
Space velocity (relative to the Sun)103.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.58. Visible from the whole Northern Hemisphere and south to latitude 70° S. North of latitude 70° N it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1834. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.4 million years.

The Sun seen from there

From a planet around SDSS J095850.68+200150.6, the Sun would look like a star of magnitude 8.68, in the direction where our sky has the constellation Capricornus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 48837 1.89 light-years
  • HIP 48504 11.4 light-years
  • HIP 49942 18.2 light-years
  • HIP 49623 18.4 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.