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Star · M1V

SDSS J160743.08+345947.4

SDSS J160743.08+345947.4 is a main-sequence star of spectral type M1V in the constellation Corona Borealis, 207.5 light-years from the Sun.

ConstellationCorona Borealis
Distance207.5 light-years (63.6 pc)
Apparent magnitudemagnitude 21.91
Absolute magnitudemagnitude 17.89
Spectral typeM1V
Surface temperature3,420 K
Luminosity3.94 × 10⁻⁵ L☉
Radius0.0179 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)16h 07m 43.1s
Declination (J2000)+34° 59′ 48″
Space velocity (relative to the Sun)52.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.91. Visible from the whole Northern Hemisphere and south to latitude 55° S. North of latitude 55° N it never sets. It stands highest at midnight in May, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1819. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.7 million years.

The Sun seen from there

From a planet around SDSS J160743.08+345947.4, the Sun would look like a star of magnitude 8.85, in the direction where our sky has the constellation Eridanus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 79677 7.23 light-years
  • HIP 80279 12.7 light-years
  • HIP 78161 13.6 light-years
  • 2MASS J16123860+3126489 14.3 light-years
  • HIP 78700 17.0 light-years
  • HIP 78859 18.1 light-years
  • HIP 78028 18.5 light-years
  • HIP 78222 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.