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Star · F3IV

ε CrA

ε CrA is a subgiant star of spectral type F3IV in the constellation Corona Australis, 102.5 light-years from the Sun.

Other namesHIP 93174
ConstellationCorona Australis
Distance102.5 light-years (31.4 pc)
Apparent magnitudemagnitude 4.83
Absolute magnitudemagnitude 2.34
Spectral typeF3IV
Surface temperature6,900 K
Luminosity9.81 L☉
Radius2.19 R☉
Mass1.77 M☉ (estimated)
Right ascension (J2000)18h 58m 43.4s
Declination (J2000)−37° 06′ 26″
Space velocity (relative to the Sun)59.2 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.83). Visible from the whole Southern Hemisphere and north to latitude 53° N. South of latitude 53° 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 1923. 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 ε CrA, the Sun would look like a star of magnitude 7.32, in the direction where our sky has the constellation Auriga. 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.