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Star · K5

GJ 9757

GJ 9757 is a main-sequence star of spectral type K5 in the constellation Capricornus, 100.0 light-years from the Sun.

Other namesHIP 107758
ConstellationCapricornus
Distance100.0 light-years (30.7 pc)
Apparent magnitudemagnitude 10.85
Absolute magnitudemagnitude 8.42
Spectral typeK5
Surface temperature4,010 K
Luminosity0.105 L☉
Radius0.672 R☉
Mass0.569 M☉ (estimated)
Right ascension (J2000)21h 49m 45.9s
Declination (J2000)−11° 40′ 57″
Space velocity (relative to the Sun)66.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 10.85. Visible from the whole Southern Hemisphere and north to latitude 78° N. South of latitude 78° S it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1926. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.8 million years.

The Sun seen from there

From a planet around GJ 9757, the Sun would look like a star of magnitude 7.26, in the direction where our sky has the constellation Leo. It would be invisible 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.