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Star · M4V

2MASS J16005759+3021571

2MASS J16005759+3021571 is a main-sequence star of spectral type M4V in the constellation Corona Borealis, 163.1 light-years from the Sun.

ConstellationCorona Borealis
Distance163.1 light-years (50.0 pc)
Apparent magnitudemagnitude 22.83
Absolute magnitudemagnitude 19.34
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.90 × 10⁻⁵ L☉
Radius0.0203 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)16h 00m 57.6s
Declination (J2000)+30° 21′ 57″
Space velocity (relative to the Sun)320.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.83. Visible from the whole Northern Hemisphere and south to latitude 60° S. North of latitude 60° 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 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 2MASS J16005759+3021571, the Sun would look like a star of magnitude 8.32, 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 78923 11.5 light-years
  • HIP 77152 11.7 light-years
  • HIP 76941 12.4 light-years
  • HIP 79068 13.3 light-years
  • ULAS J154914.45+262145.6 13.8 light-years
  • TOI-2266 14.3 light-years
  • δ CrB 14.9 light-years
  • HIP 78680 15.8 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.