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Star · M3V

SDSS J145057.34+392045.2

SDSS J145057.34+392045.2 is a main-sequence star of spectral type M3V in the constellation Boötes, 117.7 light-years from the Sun.

ConstellationBoötes
Distance117.7 light-years (36.1 pc)
Apparent magnitudemagnitude 21.52
Absolute magnitudemagnitude 18.73
Spectral typeM3V
Surface temperature3,180 K
Luminosity2.97 × 10⁻⁵ L☉
Radius0.0179 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)14h 50m 57.3s
Declination (J2000)+39° 20′ 45″
Space velocity (relative to the Sun)7.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 21.52. Visible from the whole Northern Hemisphere and south to latitude 51° S. North of latitude 51° 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 1908. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.1 million years.

The Sun seen from there

From a planet around SDSS J145057.34+392045.2, the Sun would look like a star of magnitude 7.62, in the direction where our sky has the constellation Fornax. It would be invisible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 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.