James Webb Found A Space Penguin!!!

First Light 200mm Takumar M42 - Imaging

Hubble on Its Way by NASA Hubble

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.

Hubble Captures Majestic Barred Spiral by NASA’s Marshall Space Flight Center

Approximately 1 billion light years across, the largest known structure in the universe consists of 830 galaxies nestled within 4 connecting galaxy clusters.

As above, so below.

Credits to the lovely people over at NASA and ESA. Image by Science Photo Library.

Instagram: @ spacestrikes

ESO 350-40, Cartwheel Galaxy

Butterfly nebula

The star or stars at its center are responsible for the nebula's appearance. In their death throes, they have cast off layers of gas periodically over the past couple thousand years. The "wings" of NGC 6302 are regions of gas heated to more than 36,000 degrees Fahrenheit that are tearing across space at more than 600,000 miles an hour.

NGC 6302 lies between 2,500 and 3,800 light-years away in the constellation Scorpius.

Credit: NASA, ESA, Joel Kastner (RIT)

M24, Sagittarius Star Cloud

NGC 6164: Dragon's Egg Nebula and Halo

Strike a pose, vogue! 📸

The galaxy on the left looks like it went with extreme eye makeup, while the one on the right went with a more natural look. Together, they’re known as Arp 107, a pair of colliding galaxies.

The glamorous galaxy on the left is an extremely energetic galaxy with a very active core. Its small companion is connected to it by a faint “bridge” of gas and dust. This view was captured by the Hubble Space Telescope.

Credit: ESA/Hubble & NASA, J. Dalcanton.

ALT TEXT: A pair of merging galaxies. The galaxy on the left has a single, large spiral arm curving out from the core toward 3 o’clock and wrapping counterclockwise, ending in a straighter line pointing toward the bottom of the frame. This arm is bright blue with shades of brown mixed in. The right-hand galaxy has a bright core that is approximately the same size as the galaxy at left, but only a tiny bit of very faint material surrounds it. A broad curtain of gas connects the two galaxies’ cores and hangs beneath them. Small stars and galaxies are scattered throughout the black background of space.