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Star · M4V

SDSS J110454.25+554841.4

SDSS J110454.25+554841.4 is a main-sequence star of spectral type M4V in the constellation Ursa Major, 156.6 light-years from the Sun.

ConstellationUrsa Major
Distance156.6 light-years (48.0 pc)
Apparent magnitudemagnitude 25.15
Absolute magnitudemagnitude 21.74
Spectral typeM4V
Surface temperature2,980 K
Luminosity3.15 × 10⁻⁶ L☉
Radius0.00668 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)11h 04m 54.2s
Declination (J2000)+55° 48′ 41″
Space velocity (relative to the Sun)33.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 25.15. Visible from the whole Northern Hemisphere and south to latitude 34° S. North of latitude 34° 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 1869. 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 SDSS J110454.25+554841.4, the Sun would look like a star of magnitude 8.24, in the direction where our sky has the constellation Grus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 54094 8.16 light-years
  • HIP 53042 9.08 light-years
  • HIP 56622 12.3 light-years
  • HIP 53634 14.6 light-years
  • HIP 52278 14.9 light-years
  • HIP 55840 15.4 light-years
  • HIP 56337 15.6 light-years
  • HIP 56092 16.7 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.