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Star · M4V

PSO J103.0927+41.4601

PSO J103.0927+41.4601 is a main-sequence star of spectral type M4V in the constellation Auriga, 56.1 light-years from the Sun.

ConstellationAuriga
Distance56.1 light-years (17.2 pc)
Apparent magnitudemagnitude 22.98
Absolute magnitudemagnitude 21.80
Spectral typeM4V
Surface temperature2,980 K
Luminosity2.99 × 10⁻⁶ L☉
Radius0.0065 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)6h 52m 22.2s
Declination (J2000)+41° 27′ 36″
Space velocity (relative to the Sun)3.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 22.98. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° N it never sets. It stands highest at midnight in January, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1970. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 995 thousand years.

The Sun seen from there

From a planet around PSO J103.0927+41.4601, the Sun would look like a star of magnitude 6.01, in the direction where our sky has the constellation Corona Australis. 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.