Chandra Release - February 1, 2012

Visual Description: G350.1-0.3

The X-ray and infrared image of the supernova remnant G350.1-0.3 depicts a celestial object that has undergone a catastrophic explosion, leaving behind a cosmic debris field. The image is characterized by various textures, colors, and forms. In the center of the image, there is a large, irregularly-shaped cloud of gas and dust, resembling a puffy, cotton-candy-like texture. This cloud is primarily composed of hydrogen and helium atoms, which have been ionized – that is, stripped of their electrons – by the intense heat and radiation released during the supernova explosion. The color of this cloud is predominantly pinkish-white, with some purple and blue hues, reflecting the temperature and composition of the gas and dust particles. Surrounding the central nebula, there are numerous small, bright dots scattered throughout the image. These dots represent individual stars that have formed as a result of the supernova explosion. Some of these stars are still in the process of forming, while others have already reached maturity and are shining brightly in the infrared part of the electromagnetic spectrum. The overall structure of the image is three-dimensional, with the nebula and stars appearing to be suspended in space.