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.
Details of the Heart Nebula
space.by.jase
IC 405 Flaming Star © cosmic_background
Cosmic Jellyfish: Interacting Galaxies UGC 9326/7 ©
NASA’s new images of Uranus captured by James Webb Space Telescope (2024)
This winter snow angel is out of this world! The Hubble Space Telescope captured this festive image of the bipolar star-forming region Sharpless 2-106. A massive, young star, IRS 4 is responsible for the furious star birth we see in this nebula. Twin lobes of super-hot gas, glowing blue in this image, stretch outward from the central star. This hot gas creates the “wings” of the celestial angel.
A ring of dust and gas orbiting the star acts like a belt, cinching the expanding nebula into an hourglass shape. Hubble's sharp resolution reveals ripples and ridges in the gas as it interacts with the cooler interstellar medium.
Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA).
ALT TEXT: Looking somewhat like an angel with outstretched wings, this blue-and-orange star-forming region is set against a black background punctuated by bright stars of various sizes. Some of the stars are white, while others are orange, and one in the bottom-right corner is bright red. Many of these stars have starburst-like diffraction spikes. The “angel’s” long wings are cavities outlined in a feathery pattern of blue and white. Its flowing, “dress” is a triangular, orange area of denser, dustier gas that trails off into the blackness of space. At its waist is a bright white-and-orange, centrally located star.
Arp 240, Bridge Between Galaxies
Stardust From Comet Halley Falls To Earth
ESO 593-8, Stardust Angel
NGC 6357, Celestial Cathedral