Photo © Anglo-Australian Observatory/Royal Observatory, Edinburgh, David Malin (html)
- RA 16:30, Dec -25 (Scorpio/Ophiuchus)
- Type: emission / reflection nebulae
- Distance: Antares – 520 ly; M 4 – 7500 ly
- The star in the yellow region is Antares (Alpha Scorpii); the star in the blue region at the right is Rho Ophiuchi surrounded by the emission nebula IC 4604; the star in the red region at the bottom is Sigma Scorpii; just below Antares is the globular cluster M 4.
- The bright region just to the left of Rho Ophiuchi shows evidence of new star formation.
- Antares (aka “Le Coeur de Scorpion” — the Heart of the Scorpion) is a red supergiant star some 700 times larger in diameter than the Sun, though it is “only” 9000 times more luminous and “only” 10 or 15 times more massive.
- Note that M 4 is much more distant than the Antares/Rho Ophiuchi nebulosity; we see it thru the intervening gasses.
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(David Malin)
Bill Arnett |