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Star · G2V

Gl 677B

Gl 677B is a main-sequence star of spectral type G2V in the constellation Hercules, 76.9 light-years from the Sun.

ConstellationHercules
Distance76.9 light-years (23.6 pc)
Apparent magnitudemagnitude 9.93
Absolute magnitudemagnitude 8.07
Spectral typeG2V
Surface temperature5,780 K
Luminosity0.0551 L☉
Radius0.234 R☉
Mass0.484 M☉ (estimated)
Right ascension (J2000)17h 29m 19.6s
Declination (J2000)+29° 23′ 24″
Space velocity (relative to the Sun)38.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.93. Visible from the whole Northern Hemisphere and south to latitude 61° S. North of latitude 61° N it never sets. It stands highest at midnight in June, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1949. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.4 million years.

The Sun seen from there

From a planet around Gl 677B, the Sun would look like a star of magnitude 6.69, in the direction where our sky has the constellation Columba. 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.