Dance Of Light

Cosmic Spider © Spitzer

Hubble Views Lopsided Galaxy NGC 2276 by NASA Goddard Photo and Video

NGC 7822: The Question Mark © Gabe Shaughnessy

M31, Andromeda

NGC 1512 (Hubble + Webb) by NASA's James Webb Space Telescope

A busy patch of the Great Attractor by Hubble ESA

Seahorse in Cepheus, B150 © Aleix Roig

Amazing

Though a doomed star exploded some 20,000 years ago, its tattered remnants continue racing into space at breakneck speeds—and the Hubble Space Telescope has caught the action.

The nebula, called the Cygnus Loop, forms a bubble-like shape that is about 120 light-years in diameter. The distance to its center is approximately 2,600 light-years. The entire nebula has a width of six full Moons as seen on the sky.

"Hubble is the only way that we can actually watch what's happening at the edge of the bubble with such clarity," said Ravi Sankrit, an astronomer at the Space Telescope Science Institute in Baltimore, Maryland.

"The Hubble images are spectacular when you look at them in detail. They're telling us about the density differences encountered by the supernova shocks as they propagate through space, and the turbulence in the regions behind these shocks."

The Cygnus Loop was discovered in 1784 by William Herschel, using a simple 18-inch reflecting telescope. He could have never imagined that a little over two centuries later we'd have a telescope powerful enough to zoom in on a very tiny slice of the nebula for this spectacular view.

Credit: Video - NASA, ESA, STScI; Acknowledgment - NSF's NOIRLab, Akira Fujii, Jeff Hester, Davide De Martin, Travis A. Rector, Ravi Sankrit (STScI), DSS.

IC 443 Jellyfish Closeup © Scott Johnstone

NGC 6357, Stellar Wonderland