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Star · M4V

WISEPA J041022.71+150248.5

WISEPA J041022.71+150248.5 is a main-sequence star of spectral type M4V in the constellation Taurus, 21.3 light-years from the Sun.

ConstellationTaurus
Distance21.3 light-years (6.54 pc)
Apparent magnitudemagnitude 26.94
Absolute magnitudemagnitude 27.86
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.13 × 10⁻⁸ L☉
Radius3.99 × 10⁻⁴ R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)4h 10m 22.1s
Declination (J2000)+15° 03′ 12″
Space velocity (relative to the Sun)74.9 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 26.94. Visible from the whole Northern Hemisphere and south to latitude 75° S. North of latitude 75° N it never sets. It stands highest at midnight in November, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 2005. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 378 thousand years.

The Sun seen from there

From a planet around WISEPA J041022.71+150248.5, the Sun would look like a star of magnitude 3.91, in the direction where our sky has the constellation Scorpius. It would be visible 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.