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Star · M1.0 V

GJ 740

GJ 740 is a main-sequence star of spectral type M1.0 V in the constellation Serpens, 36.2 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGl 740 · HIP 93101
ConstellationSerpens
Distance36.2 light-years (11.1 pc)
Apparent magnitudemagnitude 9.22
Absolute magnitudemagnitude 8.99
Spectral typeM1.0 V
Surface temperature3,910 K
Luminosity0.0622 L☉
Radius0.56 R☉
Mass0.58 M☉
Metallicity [Fe/H]0.08
Right ascension (J2000)18h 58m 00.2s
Declination (J2000)+5° 54′ 29″
Space velocity (relative to the Sun)65.9 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.22. Visible from the whole Northern Hemisphere and south to latitude 84° S. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1990. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 643 thousand years.

The Sun seen from there

From a planet around GJ 740, the Sun would look like a star of magnitude 5.06, in the direction where our sky has the constellation Monoceros. It would be visible 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.