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Star · M4V

UGPS J03553200+4743588

UGPS J03553200+4743588 is a main-sequence star of spectral type M4V in the constellation Perseus, 49.6 light-years from the Sun.

ConstellationPerseus
Distance49.6 light-years (15.2 pc)
Apparent magnitudemagnitude 23.70
Absolute magnitudemagnitude 22.79
Spectral typeM4V
Surface temperature2,980 K
Luminosity1.20 × 10⁻⁶ L☉
Radius0.00413 R☉
Mass0.075 M☉ (estimated)
Right ascension (J2000)3h 55m 31.5s
Declination (J2000)+47° 43′ 59″
Space velocity (relative to the Sun)38.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 23.70. Visible from the whole Northern Hemisphere and south to latitude 42° S. North of latitude 42° 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 1976. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 879 thousand years.

The Sun seen from there

From a planet around UGPS J03553200+4743588, the Sun would look like a star of magnitude 5.74, in the direction where our sky has the constellation Norma. 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.