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Star · M4V

SDSS J123034.66+324534.5

SDSS J123034.66+324534.5 is a main-sequence star of spectral type M4V in the constellation Canes Venatici, 296.8 light-years from the Sun.

ConstellationCanes Venatici
Distance296.8 light-years (91.0 pc)
Apparent magnitudemagnitude 21.92
Absolute magnitudemagnitude 17.12
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.22 × 10⁻⁴ L☉
Radius0.0561 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)12h 30m 34.7s
Declination (J2000)+32° 45′ 35″
Space velocity (relative to the Sun)84.0 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.92. Visible from the whole Northern Hemisphere and south to latitude 57° S. North of latitude 57° 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 1729. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.3 million years.

The Sun seen from there

From a planet around SDSS J123034.66+324534.5, the Sun would look like a star of magnitude 9.63, in the direction where our sky has the constellation Sculptor. It would be invisible to the naked eye.

Neighbours

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

  • HIP 61309 4.91 light-years
  • HIP 61114 8.10 light-years
  • HIP 60927 12.3 light-years
  • HIP 60242 14.3 light-years
  • HIP 60530 15.9 light-years
  • HIP 60955 16.0 light-years
  • HIP 61589 17.4 light-years
  • HIP 61779 19.6 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.