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Star · M4V

SDSS J000250.98+245413.8

SDSS J000250.98+245413.8 is a main-sequence star of spectral type M4V in the constellation Pegasus, 163.1 light-years from the Sun.

ConstellationPegasus
Distance163.1 light-years (50.0 pc)
Apparent magnitudemagnitude 22.67
Absolute magnitudemagnitude 19.18
Spectral typeM4V
Surface temperature2,980 K
Luminosity3.36 × 10⁻⁵ L☉
Radius0.0218 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)0h 02m 51.0s
Declination (J2000)+24° 54′ 14″
Space velocity (relative to the Sun)15.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.67. Visible from the whole Northern Hemisphere and south to latitude 65° S. North of latitude 65° N it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1863. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.9 million years.

The Sun seen from there

From a planet around SDSS J000250.98+245413.8, the Sun would look like a star of magnitude 8.32, in the direction where our sky has the constellation Corvus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 117972 7.28 light-years
  • HIP 460 12.3 light-years
  • HIP 84 12.8 light-years
  • HIP 1334 14.7 light-years
  • HIP 117918 16.8 light-years
  • HIP 920 17.9 light-years
  • HIP 117870 18.6 light-years
  • HIP 116740 18.7 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.