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Star · M

Gl 895.1

Gl 895.1 is a main-sequence star of spectral type M in the constellation Grus, 104.1 light-years from the Sun.

Other namesHIP 115648
ConstellationGrus
Distance104.1 light-years (31.9 pc)
Apparent magnitudemagnitude 11.27
Absolute magnitudemagnitude 8.75
Spectral typeM
Surface temperature3,900 K
Luminosity0.0868 L☉
Radius0.645 R☉
Mass0.543 M☉ (estimated)
Right ascension (J2000)23h 25m 42.1s
Declination (J2000)−45° 36′ 35″
Space velocity (relative to the Sun)71.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.27. Visible from the whole Southern Hemisphere and north to latitude 44° N. South of latitude 44° S it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1922. 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 Gl 895.1, the Sun would look like a star of magnitude 7.35, in the direction where our sky has the constellation Ursa Major. 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.