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Birthday · January 8, 2015

Stars and Dust in Corona Australis

January 8, 2015

The constellations may be old, but the person celebrating beneath them is gloriously new by cosmic standards.

Stars and Dust in Corona Australis

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APOD published January 8, 2015. Credit: CHART32 Team. A publication-date match, not a photo taken on your date. Independent of NASA.

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Stars and Dust in Corona Australis

Original APOD · January 8, 2015

Cosmic dust clouds and young, energetic stars inhabit this telescopic vista, less than 500 light-years away toward the northern boundary of Corona Australis, the Southern Crown. The dust clouds effectively block light from more distant background stars in the Milky Way. But the striking complex of reflection nebulae cataloged as NGC 6726, 6727, and IC 4812 produce a characteristic blue color as light from the region's young hot stars is reflected by the cosmic dust. The dust also obscures from view stars still in the process of formation. At the left, smaller yellowish nebula NGC 6729 bends around young variable star R Coronae Australis. Just below it, glowing arcs and loops shocked by outflows from embedded newborn stars are identified as Herbig-Haro objects. On the sky this field of view spans about 1 degree. That corresponds to almost 9 light-years at the estimated distance of the nearby star forming region. APOD Talk: Friday, January 9 in New York City

Image credit: CHART32 Team

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