NANCY BY ERNIE BUSHMILLER LET’S GO IN HERE FOR OUR POPCORN NO---LET'S GO TO THAT OTHER PLACE WHY DO YOU WANT TO GO IN HERE ? BECAUSE THIS CLERK HATES HIS BOSS

Nancy By Ernie Bushmiller
January 30,1952

Praying that everyone finds the clit in 2025🙏🏽

I’ve decided I’m going to be a clown.

Anya Taylor-Joy

Glad to have Bluesky now specifically because I hate Elon Musk🫶🏽

chappell roan and sabrina carpenter

chappell roan and sabrina carpenter

chappell roan and sabrina carpenter

MY BELOVEDS

Comet, Aldebaran and Mars over stonehenge Uk.

A spiral galaxy with a wide, oval-shaped disc. It has a shining spot at the centre from which two curving, pale red spiral arms emerge, wrapping once each around the galaxy. They’re surrounded by a whirl of bright threads and patches of dust, with spots of star formation scattered throughout. The glow of the disc fades smoothly into the background where some patches of dust can be seen, as well as foreground stars.

Image of a galaxy on the black background of space. The galaxy is a very oblong, blue disk that extends from left to right at an angle (from about 10 o’clock to 5 o’clock). The galaxy has a small bright core at the center. There is an inner disk that is clearer, with speckles of stars scattered throughout. The outer disk of the galaxy is whiteish-blue, and clumpy, like clouds in the sky. There are different colored dots, distant galaxies, speckled among the black background of space surrounding the galaxy.

Two spiral galaxies take the shape of a colorful beaded mask that sits above the nose. The galaxy at left, IC 2163, is smaller, taking up a little over a quarter of the view. The galaxy at right, NGC 2207, takes up half the view, with its spiral arms reaching the edges. IC 2163 has a bright orange core, with two prominent spiral arms that rotate counter clockwise and become straighter towards the ends, the left side extending almost to the edge. Its arms are a mix of pink, white, and blue, with an area that takes the shape of an eyelid appearing whitest. NGC 2207 has a very bright core. Overall, it appears to have larger, thicker spiral arms that spin counter clockwise. This galaxy also contains more and larger blue areas of star formation that poke out like holes from the pink spiral arms. In the middle, the galaxies’ arms appear to overlap. The edges show the black of space, including extremely distant galaxies that look like orange and red smudges, and a few foreground stars.

A large spiral galaxy takes up the entirety of the image. The core is mostly bright white, but there are also swirling, detailed structures that resemble water circling a drain. There is small white and pale blue light that emanates from stars and dust at the core’s center, but it is tightly limited to the core. The rings feature colors of deep red and orange and highlight filaments of dust around cavernous black bubbles.

jwst’s recent images 🌌

Stars form in large clouds of gas and dust called nebulae that scatter the visible wavelengths of light our eyes can see. The longer wavelengths of infrared light can pass through the cloud relatively undisturbed. Hubble’s near-infrared capabilities and high resolving power make it an important tool in the study of how stars form. Dubbed “Mystic Mountain,” this is a region of the much more extensive Carina Nebula. In it, towers of cool hydrogen gas laced with dust are seen to rise along the nebula’s wall. At the top, a three-light-year-tall pillar of gas and dust is being eaten away by the brilliant light and winds from nearby stars. The pillar is also being pushed apart from within, as infant stars buried inside it fire off jets of gas that can be seen streaming left and right from the tips of the peaks. NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)

“Mystic Mountain,” this is a region of the much more extensive Carina Nebula.
Credit: NASA, ESA,Hubble