this post was submitted on 08 Dec 2023
4 points (83.3% liked)

Autour du monde

53 readers
1 users here now

Communauté dédiée à l'exploration des mondes. 🔭

« L'Espérance voit ce qui n'est pas encore et qui sera. Elle aime ce qui n'est pas encore et qui sera. Dans le futur du temps et de l'éternité. »

Invite-nous dans un pays imaginaire ou non par ses livres, son cinéma, son histoire et sa culture.

Règles de jlai.lu

Règles de Autour du monde


Culture


Jardin


founded 1 year ago
MODERATORS
 

https://www.nasa.gov/missions/webb/nasas-webb-reveals-new-features-in-heart-of-milky-way/ Image: Sagittarius C (NIRCam)

The latest image from NASA’s James Webb Space Telescope shows a portion of the dense center of our galaxy in unprecedented detail, including never-before-seen features astronomers have yet to explain. The star-forming region, named Sagittarius C (Sgr C), is about 300 light-years from the Milky Way’s central supermassive black hole, Sagittarius A*.

A crowded region of space, full of stars and colorful clouds, more than twice as wide as it is tall. A funnel-shaped region of space appears darker than its surroundings with fewer stars. It is wider at the top edge of the image, narrowing towards the bottom. Toward the narrow end of this dark region a small clump of red and white appears to shoot out streamers upward and left. A large, bright cyan-colored area surrounds the lower portion of the funnel-shaped dark area, forming a rough U shape. The cyan-colored area has needle-like, linear structures and becomes more diffuse in the center of the image. The right side of the image is dominated by clouds of orange and red, with a purple haze.

The NIRCam (Near-Infrared Camera) instrument on NASA’s James Webb Space Telescope’s reveals a portion of the Milky Way’s dense core in a new light. An estimated 500,000 stars shine in this image of the Sagittarius C (Sgr C) region, along with some as-yet unidentified features. A large region of ionized hydrogen, shown in cyan, contains intriguing needle-like structures that lack any uniform orientation. NASA, ESA, CSA, STScI, and S. Crowe (University of Virginia).

“There’s never been any infrared data on this region with the level of resolution and sensitivity we get with Webb, so we are seeing lots of features here for the first time,” said the observation team’s principal investigator Samuel Crowe, an undergraduate student at the University of Virginia in Charlottesville. “Webb reveals an incredible amount of detail, allowing us to study star formation in this sort of environment in a way that wasn’t possible previously.”

no comments (yet)
sorted by: hot top controversial new old
there doesn't seem to be anything here