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Star · M3.5 V

LHS 475

LHS 475 is a main-sequence star of spectral type M3.5 V in the constellation Octans, 40.7 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGJ 4102
ConstellationOctans
Distance40.7 light-years (12.5 pc)
Apparent magnitudemagnitude 12.70
Absolute magnitudemagnitude 12.22
Spectral typeM3.5 V
Surface temperature3,300 K
Luminosity0.00862 L☉
Radius0.279 R☉
Mass0.262 M☉
Right ascension (J2000)19h 20m 00.7s
Declination (J2000)−82° 33′ 50″
Space velocity (relative to the Sun)75.5 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 12.70. Visible from the whole Southern Hemisphere and north to latitude 7° N. South of latitude 7° S it never sets.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1985. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 722 thousand years.

The Sun seen from there

From a planet around LHS 475, the Sun would look like a star of magnitude 5.31, in the direction where our sky has the constellation Camelopardalis. It would be visible to the naked eye.

Planets

Neighbours

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

Open in the simulation

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