ι Trianguli Australis (iota Trianguli Australis)

ι Trianguli Australis is a double sub-giant star of spectral class F4 in the constellation of Triangulum Australe.

ι Trianguli Australis visual magnitude is 5.27. Because of its faintness, ι Trianguli Australis is visible to the naked eye only from locations with very dark skies, while it is not visible at all from skies affected by light pollution.

Celestial Coordinates

Apparent

J2000

Galactic Coordinates

Finder Chart

Magnitude, Color, Spectral Class

The red dot in the diagram below shows where ι Trianguli Australis is situated in the Hertzsprung–Russell diagram.

Star System Properties

ι Trianguli Australis is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the ι Trianguli Australis double sysyem:

Distance, Radial Speed, Proper Motion

ι Trianguli Australis is distant 131.72 light years from the Sun and it is moving towards the Sun at the speed of 5 kilometers per second.

Alternative Designations

Visibility from Your Location

ι Trianguli Australis (iota Trianguli Australis) is circumpolar and transits at 12:51 UTC (altitude: 63.8°)