home bbs files messages ]

Just a sample of the Echomail archive

Cooperative anarchy at its finest, still active today. Darkrealms is the Zone 1 Hub.

   ESSNASA      Earth & Space Sci-Tech + NASA      10,823 messages   

[   << oldest   |   < older   |   list   |   newer >   |   newest >>   ]

   Message 8,669 of 10,823   
   Alan Ianson to All   
   Daily APOD Report   
   13 Jan 23 00:11:52   
   
   MSGID: 1:153/757.0 9195b6a5   
   TZUTC: -0800   
   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.   
      
                                  2023 January 13   
      
                            Young Star Cluster NGC 346   
      Image Credit: Science - NASA, ESA, CSA, Olivia C. Jones (UK ATC), Guido   
                    De Marchi (ESTEC), Margaret Meixner (USRA)   
        Processing - Alyssa Pagan (STScI), Nolan Habel (USRA), Laura Lenkic   
                       (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 and 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: light-weekend   
        __________________________________________________________________   
      
          Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)   
               NASA Official: Phillip Newman Specific rights apply.   
                   NASA Web Privacy Policy and Important Notices   
                         A service of: ASD at NASA / GSFC,   
                              NASA Science Activation   
                                & Michigan Tech. U.   
      
   --- BBBS/Li6 v4.10 Toy-6   
    * Origin: The Rusty MailBox - Penticton, BC Canada (1:153/757)   
   SEEN-BY: 1/123 15/0 90/1 92/1 103/705 105/81 106/201 120/340 123/131   
   SEEN-BY: 129/305 134/100 153/135 757 6809 7715 218/700 840 221/1 6   
   SEEN-BY: 221/100 226/30 227/114 229/110 111 112 113 114 206 307 317   
   SEEN-BY: 229/400 424 426 428 470 664 700 240/1120 266/512 282/1038   
   SEEN-BY: 301/1 113 812 317/3 320/219 322/757 335/364 341/66 342/200   
   SEEN-BY: 396/45 460/58 633/280 712/620 848 770/1 4500/1 5020/1042   
   PATH: 153/757 221/6 301/1 712/848 229/426   
      

[   << oldest   |   < older   |   list   |   newer >   |   newest >>   ]


(c) 1994,  bbs@darkrealms.ca