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|  Message 10341  |
|  Alan Ianson to All  |
|  Daily APOD Report  |
|  02 May 25 00:04:06  |
 
MSGID: 1:153/757.0 f8a96025
TZUTC: -0700
CHRS: LATIN-1 2
Astronomy Picture of the Day
Discover the cosmos! Each day a different image or photograph of our
fascinating universe is featured, along with a brief explanation
written by a professional astronomer.
2025 May 2
See Explanation. Clicking on the picture will download the highest
resolution version available.
Young Star Cluster NGC 346
Science - NASA, ESA, CSA, Olivia C. Jones (UK ATC), Guido De Marchi
(ESTEC), Margaret Meixner (USRA)
Processing - Alyssa Pagan (STScI), Nolan Habel (USRA), Laura Lenki-ç
(USRA), Laurie E. U. Chu (NASA Ames)
Explanation: The most massive young star cluster in the Small
Magellanic Cloud is NGC 346, embedded in our small satellite galaxy's
largest star forming region some 210,000 light-years distant. Of course
the massive stars of NGC 346 are short lived, but very energetic. Their
winds and radiation sculpt the edges of the region's dusty molecular
cloud triggering star-formation within. The star forming region also
appears to contain a large population of infant stars. A mere 3 to 5
million years old and not yet burning hydrogen in their cores, the
infant stars are strewn about the embedded star cluster. This
spectacular infrared view of NGC 346 is from the James Webb Space
Telescope's NIRcam. Emission from atomic hydrogen ionized by the
massive stars' energetic radiation as well as molecular hydrogen and
dust in the star-forming molecular cloud is detailed in pink and orange
hues. Webb's sharp image of the young star-forming region spans 240
light-years at the distance of the Small Magellanic Cloud.
Tomorrow's picture: Titan's Shangra-La
__________________________________________________________________
Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
NASA Official: Amber Straughn Specific rights apply.
NASA Web Privacy Policy and Important Notices
A service of: ASD at NASA / GSFC,
NASA Science Activation
& Michigan Tech. U.
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