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Star · M3

Gl 695B

Gl 695B is a main-sequence star of spectral type M3 in the constellation Hercules, 27.2 light-years from the Sun.

ConstellationHercules
Distance27.2 light-years (8.34 pc)
Apparent magnitudemagnitude 10.35
Absolute magnitudemagnitude 10.74
Spectral typeM3
Surface temperature3,810 K
Luminosity0.0155 L☉
Radius0.286 R☉
Mass0.31 M☉ (estimated)
Right ascension (J2000)17h 46m 25.5s
Declination (J2000)+27° 42′ 58″
Space velocity (relative to the Sun)38.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 10.35. Visible from the whole Northern Hemisphere and south to latitude 62° S. North of latitude 62° 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 1999. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 483 thousand years.

The Sun seen from there

From a planet around Gl 695B, the Sun would look like a star of magnitude 4.44, in the direction where our sky has the constellation Columba. It would be visible 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.