This brand-new collection of images from NASA’s Chandra area telescope– which introduced in 1999– reveals what various things in area appear like with an included layer of X-ray vision.

While the Hubble Space Telescope images the universes in mainly noticeable light and the James Webb Space Telescope (JWST) counts on infrared light that’s beyond the limitations of human vision, Chandra focuses just on high-energy X-ray light.

Each of these area telescopes for that reason sees deep space through a various part of the electro-magnetic spectrum, and integrating these makes it possible for scientists to study the universes in higher information.

Chandra’s capability to see in X-ray light suggests it can find hot, energetic areas like great voids, supernova residues and pockets of super-hot gas. In the recently launched imagesthese energetic X-rays are displayed in pink and purple shades.

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The leading row reveals N79 (left), an area of star development in the Large Magellanic Cloud, which is a little satellite next-door neighbor galaxy to the Milky Way. In Chandra’s image, N79 blazes with hot gas formed by energetic stars. NGC 2146 (middle) is a spiral nebula rupturing with X-ray-emitting phenomena like supernova residues and winds from huge stars. And IC 348 (right) is another star-forming area that sparkles with reflective interstellar wisps and spread young stars.

The middle row reveals 2 spiral nebula: the Milky Way-like M83 (left) and NGC 1068 (right). The latter galaxy’s core is brightened by high-energy X-rays created by winds from its great void, which blow at 1 million miles per hour (1.6 million km/h). M82 (center) is a starburst galaxy, including plumes of superheated gas produced as stars form at an amazing rate.