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AAO image reference AAT 30. « Previous || Next » ![]() Top left is NE. Image width is about 6 arc min Image and text © 1986-2010, Australian Astronomical Observatory, photograph by David Malin. Vast clouds of hydrogen mixed with tiny dust grains are distributed throughout the Milky Way. The hydrogen only becomes visible when it is illuminated by ultraviolet light very hot stars, which causes the gas to glow (fluoresce) with its characteristic red colour. In most cases, such as here, the hot stars formed recently from the hydrogen cloud. The stars found at the heart of the Trifid Nebula are here seen associated with dust lanes which are silhouetted against the glowing background. This nebula is in the constellation of Sagittarius at a distance of about 3000 light years. Related Images AAT 12. The Trifid nebula, Messier 20 (wide field) AAT 12a. The Trifid nebula, Messier 20 (wide field) AAT 69. Reflection nebula around M20 AAT 69a. Reflection nebula around M20 (wide field) UKS 7. Reflection nebula around M20 UKS 26. The field of M8 and M20 in Sagittarius Constellation of Sagittarius (external site) For details of photographic exposure, search technical table by AAT reference number |