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Star · M4.5 V

LP 261-75 A

LP 261-75 A is a main-sequence star of spectral type M4.5 V in the constellation Leo Minor, 110.9 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationLeo Minor
Distance110.9 light-years (34.0 pc)
Apparent magnitudemagnitude 15.42
Absolute magnitudemagnitude 12.76
Spectral typeM4.5 V
Surface temperature3,140 K
Luminosity0.0082 L☉
Radius0.308 R☉
Mass0.22 M☉
Age0.2 billion years
Right ascension (J2000)9h 51m 04.4s
Declination (J2000)+35° 58′ 07″
Space velocity (relative to the Sun)32.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 15.42. Visible from the whole Northern Hemisphere and south to latitude 54° S. North of latitude 54° N it never sets. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1915. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.0 million years.

The Sun seen from there

From a planet around LP 261-75 A, the Sun would look like a star of magnitude 7.49, in the direction where our sky has the constellation Piscis Austrinus. It would be invisible to the naked eye.

Planets

Neighbours

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

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Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.