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Rukbat

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Alp Sgr · Corona Australis

Its story

Rukbat is a small, G-type star situated within the constellation CrA. Its magnitude – a simple number – is 3.95. Approximately 180 light years away, Rukbat possesses a known parallax of 18.11 mas, meaning its distance from Earth is discernible by astronomers. The star’s known distance is a fundamental fact – it exists at 180 light years from us.

Rukbat is recognizable within the night sky as a relatively bright, reddish-orange star, primarily observed in the constellation CrA. These stars offer a captivating visual element amongst the more diffuse groupings of stars present. Its position—specifically its radial velocity—is somewhat anomalous within the observed patterns of the constellation, a noticeable point of observation for those tracking its movement across the cosmos. It's a steady, consistent luminosity suggesting a relatively stable environment for stellar evolution in its current orbit.

While a star's significance often extends beyond simply its physical properties, Rukbat’s presence within the CrA constellation warrants thoughtful consideration regarding its symbolic potential for individuals. It’s easy to see a celestial body – such as a small point of light – as holding a particular meaning in the context of celestial placement.

The categorization of Rukbat as a comparatively modest star in a fairly dispersed region of the cosmos implies a degree of quiet beauty and constancy -- a timeless companion for the observation of the cosmos.

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Compose this star
FactsHIP 95347
Right ascension
19h 23m 53s
Declination
−40° 36′ 59″
Magnitude
3.95
Distance
≈ 180 ly
Data: gaia-dr3