Pic of the Week: Grand Design Spiral Galaxy NGC 5643

Posted on by onespaceman2000
Image (Credit): Spiral galaxy NGC 5643, which is located roughly 40 million light-years away in the constellation Lupus. (ESA/Hubble & NASA, A. Riess, D. Thilker, D. De Martin (ESA/Hubble), M. Zamani (ESA/Hubble))

This week’s image comes from the NASA/European Space Agency’s (ESA) Hubble Space Telescope. It shows colorful spiral galaxy NGC 5643, which is located roughly 40 million light-years away in the constellation Lupus.

Here is more on the spiral galaxy from the ESA Hubble site:

NGC 5643 is what’s known as a grand design spiral, referring to how the galaxy’s two large, winding spiral arms are clear to see. The spiral arms are defined by bright blue stars, lacy reddish-brown dust clouds and pink star-forming regions. As fascinating as the galaxy appears at visible wavelengths, some of NGC 5643’s most interesting features are invisible to the human eye. Ultraviolet and X-ray images and spectra of NGC 5643 show that the galaxy hosts an active galactic nucleus: an especially bright galactic core powered by a feasting supermassive black hole. When a supermassive black hole ensnares gas from its surroundings, the gas collects in a disc that heats up to hundreds of thousands of degrees. The superheated gas shines brightly across the electromagnetic spectrum, but especially at X-ray wavelengths.

NGC 5643’s active galactic nucleus isn’t the brightest source of X-rays in the galaxy, though. Researchers using ESA’s XMM-Newton discovered an even brighter X-ray-emitting object, called NGC 5643 X-1, on the galaxy’s outskirts. What could be a more powerful source of X-rays than a supermassive black hole? Surprisingly, the answer appears to be a much smaller black hole!

While the exact identity of NGC 5643 X-1 is not yet known, evidence points to a black hole that is about 30 times more massive than the Sun. Locked in an orbital dance with a companion star, the black hole ensnares gas from its stellar companion, creating a superheated disc that outshines the galactic centre.

Pic of the Week: The Best of 2024

Posted on by onespaceman2000
Image (Credit): Odysseus Leaves Earth. (Intuitive Machines)

This week’s image is the best space exploration image winner in The Planetary Society’s Best of 2024 contest. It shows the Odysseus lunar lander, launched on February 15, leaving the Earth behind as it travels to the Moon. You can read more about the lunar mission to the lunar South Pole by visiting this NASA mission page.

Visit The Planetary Society for more on the Best of 2024 winners, including the most exciting upcoming planetary science mission. I won’t spoil the news. You can read about it yourself.

Pic of the Week: Thanksgiving on the ISS

Posted on by onespaceman2000
Image (Credit): Expedition 72 astronauts on the ISS celebrating Thanksgiving. (NASA)

This week’s image shows the four US astronauts aboard the International Space Station (ISS) showing their Thanksgiving meal to all of us (contained in the white plastic bags). The astronauts pictured (clockwise from bottom left) are Nick Hague, Suni Williams, Butch Wilmore, and Don Pettit. You also watch a video where they share their holiday messages.

Pic of the Week: Collision in the Coma Galaxy Cluster

Posted on by onespaceman2000
Image (Credit): Interacting spiral galaxies called MCG+05-31-045 as captured by the Hubble Space Telescope. (ESA/Hubble & NASA, R. J. Foley (UC Santa Cruz))

This week’ image was captured by the Hubble Space Telescope. It captures the interplay between two galaxies in what is called MCG+05-31-045 that is part of the Coma galaxy cluster. These two galaxies are about 390 million light-years away.

Here is more on the image from NASA:

The Coma Cluster is a particularly rich cluster that contains over a thousand known galaxies. Amateur astronomers can easily spot several of these in a backyard telescope (See Caldwell 35). Most of them are elliptical galaxies, and that’s typical of a dense galaxy cluster like the Coma Cluster: many elliptical galaxies form through close encounters between galaxies that stir them up, or even collisions that rip them apart. While the stars in interacting galaxies can stay together, their gas is twisted and compressed by gravitational forces and rapidly used up to form new stars. When the hot, massive, blue stars die, there is little gas left to form new generations of young stars to replace them. As spiral galaxies interact, gravity disrupts the regular orbits that produce their striking spiral arms. Whether through mergers or simple near misses, the result is a galaxy almost devoid of gas, with aging stars orbiting in uncoordinated circles: an elliptical galaxy.

It’s very likely that a similar fate will befall MCG+05-31-045. As the smaller spiral galaxy is torn up and integrated into the larger galaxy, many new stars will form, and the hot, blue ones will quickly burn out, leaving cooler, redder stars behind in an elliptical galaxy, much like others in the Coma Cluster. But this process won’t be complete for many millions of years.

Pic of the Week: The Red Monsters

Posted on by onespaceman2000
Image (Credit): The “Red Monsters” as captured by the JWST. (NASA/CSA/ESA, M. Xiao & P. A. Oesch (University of Geneva), G. Brammer (Niels Bohr Institute), Dawn JWST Archive)

This week’s image from the James Webb Space Telescope (JWST) was highlighted by researchers at the University of Bath. It represents three ultra-massive galaxies about the size of our Milky Way from the first billion years of the universe following the Big Bang.

The researchers discuss this in their paper in Nature, Accelerated Formation of Ultra-massive Galaxies in the First Billion Years. The abstract is a bit too technical, but suffice it to say that this is a significant discovery.

As noted in Tech Exporist, Dr. Mengyuan Xiao, lead author of the new study and postdoctoral researcher in the Department of Astronomy at UNIGE Faculty of Science, stated:

These results indicate that galaxies in the early Universe could form stars with unexpected efficiency. As we study these galaxies in more depth, they will offer new insights into the conditions that shaped the Universe’s earliest epochs. The ‘Red Monsters’ are just the beginning of a new era in our exploration of the early Universe.