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Wonderous strange! This unusual arrangement in the sky was one of only 100 known polar-ring galaxies when it was captured by the Hubble Space Telescope in 1999. Officially known to astronomers as NGC 4650A, the polar-rings may be the result of two galaxies colliding. Gas from the smaller galaxy would have been stripped off and captured by the larger galaxy, forming a new ring of dust, gas, and stars, which orbit the inner galaxy almost at right angles to the old disk. In addition to learning about galaxy interaction, astronomers use polar-ring galaxies like this to study dark matter, which does not emit light or interact with normal matter (except through gravity), making it difficult to understand. Both the old, rotating disk and the dark matter surrounding this galaxy pull on its polar ring. The alignment of the ring along the pole of the inner disk's rotation allows scientists to probe this combination of tugs and thus the distribution of dark matter. Credit: NASA, ESA, STScI. ALT TEXT: Two galaxies appear to intersect at right angles. Vertically there is a bright column of dust and stars, and horizontally there is a smaller hazy yellow band, brighter at its center, with no discernable stars. In the space around and behind the intersecting forms are smaller stars and distant galaxies colored yellow and red.

What is casting dark shadows across 36,000 light-years of space in this Hubble Space Telescope image?

The mysterious dark rays appearing to emanate from galaxy IC 5063 have intrigued astronomers, and there are a few different ideas about what is causing them. They could be like the shadows of clouds when light from the setting Sun pierces through them.

Astronomers have traced the rays back to the galaxy’s core, the location of an active supermassive black hole. One idea suggests that the shadows are being cast into space by an inner tube-shaped ring, or torus, of dusty material surrounding the black hole.

Credit: NASA, ESA, and W.P. Maksym (CfA).

ALT TEXT: Rust-colored view of space, with a bright, narrow purple region at the center, a galaxy. Background stars and galaxies are scattered sparsely—this is a dusty rather than starry scene. To the upper left of the bright central region are dark dust lanes. Opposite these to the lower right, one dark area extends from the central bright region and splits into two dark rays. Similar dark rays can be seen to the top left, behind the dust lanes. The edges of the entire image are dark, fading from the colored center.

2023 December 29

Shakespeare in Space Image Credit: NASA, ESA, CSA, STScI

Explanation: In 1986, Voyager 2 became the only spacecraft to explore ice giant planet Uranus close up. Still, this newly released image from the NIRCam (Near-Infrared Camera) on the James Webb Space Telescope offers a detailed look at the distant world. The tilted outer planet rotates on its axis once in about 17 hours. Its north pole is presently pointed near our line of sight, offering direct views of its northern hemisphere and a faint but extensive system of rings. Of the giant planet’s 27 known moons, 14 are annotated in the image. The brighter ones show hints of Webb’s characteristic diffraction spikes. And though these worlds of the outer Solar System were unknown in Shakespearean times, all but two of the 27 Uranian moons are named for characters in the English Bard’s plays.

∞ Source: apod.nasa.gov/apod/ap231229.html

Messier-20 is called the “Trifid Nebula” because of the three bright lobes in the lower purple-coloured area. This purple region is emitting light, while the upper blue area is just reflecting it.

It is a local star-forming region in our Milky Way galaxy (4,000 light years away). (at Bordeaux, France) https://www.instagram.com/p/B1bxBljC5H9/?igshid=1g0i6zddk37k

The NGC 70 Group // Michael Legary

Picture of the Day!

NASA's James Webb Space Telescope has captured a stunning image of the iconic Pillars of Creation, a region where new stars are being born within thick clouds of gas and dust. The three-dimensional pillars resemble towering rock formations, yet they are much more porous. Composed of cool interstellar gas and dust, they sometimes appear semi-transparent in near-infrared light.

Cosmic fireworks ahead! This dramatically colorful image shows MACS J0717, one of the most complex and distorted galaxy clusters known. It was formed by the collision of four smaller galaxy clusters. A visible-light image from the Hubble Space Telescope shows hundreds of galaxies, both within the cluster and throughout the background, and myriad foreground stars. A pink overlay represents radio data from the Karl G. Jansky Very Large Array, which traces enormous shock waves and turbulence. The diffuse emission in blue, from the Chandra X-ray Observatory, highlights gas with temperatures of millions of degrees. Credit: NASA, ESA, CXC, NRAO/AUI/NSF, STScI, and R. van Weeren (Harvard-Smithsonian Center for Astrophysics); NASA, ESA, J. Lotz (STScI), and the Hubble Frontier Fields team. ALT TEXT: Hundreds of small galaxies of various shapes on the black background of space. They are concentrated near the center of the image. Dramatic pink ribbons form a curving L shape near the center. Below them, a linear pink feature with a blue blob in the middle extends from upper left to lower right. Diffuse blue light fills much of the field of view and is brightest just to the right of the pink ribbons.

Wed. 7/31: We'll be closed tonight due to clouds. Stay tuned for updates about August!

The Horsehead Nebula (Barnard 33, below center) and the Flame Nebula (NGC 2024, below left of center) // AstroFortWayne