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Star · M4V

ULAS J141710.01+131737.1

ULAS J141710.01+131737.1 is a main-sequence star of spectral type M4V in the constellation Boötes, 163.1 light-years from the Sun.

ConstellationBoötes
Distance163.1 light-years (50.0 pc)
Apparent magnitudemagnitude 22.51
Absolute magnitudemagnitude 19.02
Spectral typeM4V
Surface temperature2,980 K
Luminosity3.89 × 10⁻⁵ L☉
Radius0.0235 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)14h 17m 10.1s
Declination (J2000)+13° 17′ 37″
Space velocity (relative to the Sun)27.6 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.51. Visible from the whole Northern Hemisphere and south to latitude 77° S. North of latitude 77° N it never sets. It stands highest at midnight in April, 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 ULAS J141710.01+131737.1, the Sun would look like a star of magnitude 8.32, in the direction where our sky has the constellation Cetus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 69391 9.80 light-years
  • HIP 68801 13.5 light-years
  • HIP 70181 14.2 light-years
  • HIP 71247 14.4 light-years
  • HIP 71572 14.9 light-years
  • ULAS J141203.85+121609.9 17.0 light-years
  • HIP 71759 17.5 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.