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Star · M4V

SDSS J073922.26+661503.5

SDSS J073922.26+661503.5 is a main-sequence star of spectral type M4V in the constellation Camelopardalis, 107.6 light-years from the Sun.

ConstellationCamelopardalis
Distance107.6 light-years (33.0 pc)
Apparent magnitudemagnitude 24.32
Absolute magnitudemagnitude 21.73
Spectral typeM4V
Surface temperature2,980 K
Luminosity3.20 × 10⁻⁶ L☉
Radius0.00673 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)7h 39m 22.1s
Declination (J2000)+66° 15′ 04″
Space velocity (relative to the Sun)38.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 24.32. Visible from the whole Northern Hemisphere and south to latitude 24° S. North of latitude 24° N it never sets. It stands highest at midnight in January, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1918. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.9 million years.

The Sun seen from there

From a planet around SDSS J073922.26+661503.5, the Sun would look like a star of magnitude 7.42, in the direction where our sky has the constellation Pavo. It would be invisible to the naked eye.

Neighbours

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

  • SDSS J065405.63+652805.4 8.80 light-years
  • HIP 41308 11.5 light-years
  • Gl 296.2 13.0 light-years
  • HIP 40882 13.6 light-years
  • Gl 285.1 14.5 light-years
  • HIP 40918 15.0 light-years
  • HIP 40848 15.9 light-years
  • HIP 43745 16.4 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.