“Webb’s powerful infrared
instruments provide detail we’ve never been able to see before, which will help
us to understand some of the still-elusive mysteries of massive star formation
and why Sagittarius B2 is so much more active than the rest of the galactic
center,” said astronomer Adam Ginsburg of the University of Florida, principal
investigator of the program.
Image A: Sagittarius B2 (NIRCam
Image)
Stars, gas and cosmic dust in the Sagittarius B2 molecular cloud glow in near-infrared light, captured by Webb’s NIRCam instrument. Full image and caption below.
Credits: Image: NASA, ESA, CSA, STScI, Adam Ginsburg (University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo (University of Florida); Image Processing: Alyssa Pagan (STScI)
Sagittarius B2 is located only a few hundred light-years from the supermassive black hole at the heart of the galaxy called Sagittarius A*, a region densely packed with stars, star-forming clouds, and complex magnetic fields. The infrared light that Webb detects is able to pass through some of the area’s thick clouds to reveal young stars and the warm dust surrounding them.
However, one of the most notable
aspects of Webb’s images of Sagittarius B2 are the portions that remain dark.
These ironically empty-looking areas of space are actually so dense with gas
and dust that even Webb cannot see through them. These thick clouds are the raw
material of future stars and a cocoon for those still too young to shine.
The high resolution and
mid-infrared sensitivity of Webb’s MIRI (Mid-Infrared Instrument) revealed this
region in unprecedented detail, including glowing cosmic dust heated by very
young massive stars. The reddest area on the right half of MIRI’s image, known
as Sagittarius B2 North, is one of the most molecularly rich regions known, but
astronomers have never seen it with such clarity. (Note: North is to the right
in these Webb images.)
Image B: Sagittarius B2 (MIRI
Image)
Webb’s MIRI instrument shows the Sagittarius B2 region
in mid-infrared light, with warm dust glowing brightly. Only the brightest
stars emit strongly enough to appear through the dense clouds as blue
pinpoints.
Image: NASA, ESA, CSA, STScI, Adam Ginsburg
(University of Florida), Nazar Budaiev (University of Florida), Taehwa Yoo
(University of Florida); Image Processing: Alyssa Pagan (STScI)
The difference longer wavelengths of
light make, even within the infrared spectrum, are stark when comparing the images
from Webb’s MIRI and NIRCam (Near-Infrared Camera) instruments. Glowing gas and
dust appear dramatically in mid-infrared light, while all but the brightest
stars disappear from view.
In contrast to MIRI, colorful stars
steal the show in Webb’s NIRCam image, punctuated occasionally by bright clouds
of gas and dust. Further research into these stars will reveal details of their
masses and ages, which will help astronomers better understand the process of
star formation in this dense, active galactic center region. Has it been going
on for millions of years? Or has some unknown process triggered it only
recently?
Image C: Compare NIRCam and MIRI
Images of Sagittarius B2
Follow link: NASA's
Webb Explores Largest Star-Forming Cloud in Milky Way - NASA Science
Astronomers hope Webb will shed light on
why star formation in the galactic
center is so disproportionately low. Though the region is stocked with plenty
of gaseous raw material, on the whole it is not nearly as productive as
Sagittarius B2. While Sagittarius B2 has only 10 percent of the galactic
center’s gas, it produces 50 percent of its stars.
“Humans have been studying the stars for
thousands of years, and there is still a lot to understand,” said Nazar
Budaiev, a graduate student at the University of Florida and the co-principal
investigator of the study. “For everything new Webb is showing us, there are
also new mysteries to explore, and it’s exciting to be a part of that ongoing
discovery.”
The James Webb Space Telescope is the
world’s premier space science observatory. Webb is solving mysteries in our
solar system, looking beyond to distant worlds around other stars, and probing
the mysterious structures and origins of our universe and our place in it. Webb
is an international program led by NASA with its partners, ESA (European Space
Agency) and CSA (Canadian Space Agency).
To learn more about Webb, visit: https://science.nasa.gov/webb
Source: NASA's
Webb Explores Largest Star-Forming Cloud in Milky Way - NASA Science
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