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Star · ?

Gl 774B

Gl 774B is a main-sequence star of spectral type ? in the constellation Pavo, 41.9 light-years from the Sun.

ConstellationPavo
Distance41.9 light-years (12.8 pc)
Apparent magnitudemagnitude 12.82
Absolute magnitudemagnitude 12.28
Spectral type?
Surface temperature3,710 K
Luminosity0.00437 L☉
Radius0.16 R☉
Mass0.178 M☉ (estimated)
Right ascension (J2000)20h 04m 02.5s
Declination (J2000)−65° 36′ 06″
Space velocity (relative to the Sun)62.1 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 12.82. Visible from the whole Southern Hemisphere and north to latitude 24° N. South of latitude 24° S it never sets. 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 1984. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 743 thousand years.

The Sun seen from there

From a planet around Gl 774B, the Sun would look like a star of magnitude 5.37, in the direction where our sky has the constellation Camelopardalis. 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.