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                           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.   
      
                                  2026 January 22   
      
                          LDN 1622: Dark Nebula in Orion   
                      Image Credit & Copyright: Chris Fellows   
      
      Explanation: The silhouette of an intriguing dark nebula inhabits this   
      cosmic scene. Lynds' Dark Nebula (LDN) 1622 appears against a faint   
      background of glowing hydrogen gas only visible in long telescopic   
      exposures of the region. In contrast, a brighter reflection nebula, vdB   
      62, is more easily seen just above the dusty dark nebula. LDN 1622 lies   
      near the plane of our Milky Way Galaxy, close on the sky to Barnard's   
      Loop, a large cloud surrounding the rich complex of emission nebulae   
      found in the Belt and Sword of Orion. With swept-back outlines, the   
      obscuring dust of LDN 1622 is thought to lie at a similar distance,   
      perhaps 1,500 light-years away. At that distance, this 3 degree wide   
      field of view would span about 100 light-years. Young stars do lie   
      hidden within the dark expanse and have been revealed in Spitzer Space   
      telescope infrared images. Still, the foreboding visual appearance of   
      LDN 1622 inspires its popular name, the Boogeyman Nebula.   
      
                  Tomorrow's picture: the faint and mostly round   
        __________________________________________________________________   
      
          Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)   
               NASA Official: Amber Straughn Specific rights apply.   
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                         A service of: ASD at NASA / GSFC,   
                              NASA Science Activation   
                                & Michigan Tech. U.   
      
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