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Star · M4V

SDSS J092610.28+434322.9

SDSS J092610.28+434322.9 is a main-sequence star of spectral type M4V in the constellation Ursa Major, 257.7 light-years from the Sun.

ConstellationUrsa Major
Distance257.7 light-years (79.0 pc)
Apparent magnitudemagnitude 21.77
Absolute magnitudemagnitude 17.28
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.92 × 10⁻⁴ L☉
Radius0.0522 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)9h 26m 10.3s
Declination (J2000)+43° 43′ 23″
Space velocity (relative to the Sun)24.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.77. Visible from the whole Northern Hemisphere and south to latitude 46° S. North of latitude 46° 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 1768. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.6 million years.

The Sun seen from there

From a planet around SDSS J092610.28+434322.9, the Sun would look like a star of magnitude 9.32, in the direction where our sky has the constellation Microscopium. It would be invisible to the naked eye.

Neighbours

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

  • HIP 46597 13.1 light-years
  • HIP 45627 13.9 light-years
  • SDSS J091206.36+420330.6 15.6 light-years
  • HIP 47124 16.2 light-years
  • HIP 45146 16.4 light-years
  • HIP 44567 17.4 light-years
  • HIP 47046 18.4 light-years
  • HIP 47611 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.