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|    ESSNASA    |    Earth & Space Sci-Tech + NASA    |    10,823 messages    |
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|    Message 8,540 of 10,823    |
|    Alan Ianson to All    |
|    Daily APOD Report    |
|    09 Nov 22 01:02:42    |
      MSGID: 1:153/757.0 d0dc758c       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.               2022 November 9        The featured image shows a complex nebula that is more dense and more        blue on one side than the other. Please see the explanation for more        detailed information.               The Asymmetric Nebula Surrounding Wolf-Rayet Star 18        Image Credit & Copyright: Alex Woronow               Explanation: Why does the nebula around the star WR-18 shine brighter        on one side? Also known as NGC 3199, this active star and its        surrounding nebula lie about 12,000 light-years away toward the        nautical southern constellation of Carina. The featured deep image has        been highly processed to bring out filamentary details of the glowing        gas in the bubble-shaped nebula. The nebula is about 75 light-years        across. Near the nebula's center is a Wolf-Rayet star, WR-18, which is        a massive, hot, short-lived star that generates an intense and complex        stellar wind. In fact, Wolf-Rayet stars are known to create nebulas        with interesting shapes as their powerful winds sweep up surrounding        interstellar material. In this case, the bright right edge was        initially thought to indicate that a bow shock was being produced as        the star plowed through a uniform medium, like a boat through water.        Recent measurements and analyses, however, have shown the star is not        moving quickly toward the bright edge. A more likely explanation has        emerged that the material surrounding the star is not uniform, but        clumped and denser near the bright edge.               Tomorrow's picture: open space        __________________________________________________________________               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: 1/19 123 15/0 16/0 19/10 37 90/1 105/81 106/201 120/340 123/130       SEEN-BY: 123/131 129/305 134/100 142/104 153/135 757 6809 7715 203/0       SEEN-BY: 218/700 840 221/1 6 242 360 226/30 227/114 229/110 111 112       SEEN-BY: 229/113 114 206 317 400 424 426 428 470 664 700 240/5832       SEEN-BY: 266/512 280/5003 5006 282/1038 301/1 317/3 320/119 219 319       SEEN-BY: 322/0 757 335/364 341/66 342/200 396/45 423/81 460/58 633/280       SEEN-BY: 712/848 4500/1       PATH: 153/757 221/6 1 320/219 229/426           |
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