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|    Message 9,494 of 10,823    |
|    Alan Ianson to All    |
|    Daily APOD Report    |
|    06 Mar 24 01:08:36    |
      MSGID: 1:153/757.0 99d372c0       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.               2024 March 6        A starfield is shown with an unusual horizontal line segment running        throug the middle. The segment is an edge-on galaxy and many brown dust        filaments are visible. Please see the explanation for more detailed        information.               M102: Edge-on Disk Galaxy        Image Credit: NASA, ESA, Hubble; Processing: Ehsan Ebahimian               Explanation: What kind of celestial object is this? A relatively normal        galaxy -- but seen from its edge. Many disk galaxies are actually just        as thin as NGC 5866, the Spindle galaxy, pictured here, but are not        seen edge-on from our vantage point. A perhaps more familiar galaxy        seen edge-on is our own Milky Way galaxy. Also cataloged as M102, the        Spindle galaxy has numerous and complex dust lanes appearing dark and        red, while many of the bright stars in the disk give it a more blue        underlying hue. The blue disk of young stars can be seen in this Hubble        image extending past the dust in the extremely thin galactic plane.        There is evidence that the Spindle galaxy has cannibalized smaller        galaxies over the past billion years or so, including multiple streams        of faint stars, dark dust that extends away from the main galactic        plane, and a surrounding group of galaxies (not shown). In general,        many disk galaxies become thin because the gas that forms them collides        with itself as it rotates about the gravitational center. The Spindle        galaxy lies about 50 million light years distant toward the        constellation of the Dragon (Draco).               Tomorrow's picture: not a distant galactic nebula        __________________________________________________________________               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.              --- BBBS/Li6 v4.10 Toy-6        * Origin: The Rusty MailBox - Penticton, BC Canada (1:153/757)       SEEN-BY: 1/19 15/0 16/0 19/37 90/1 105/81 106/201 123/130 128/260       SEEN-BY: 129/305 134/100 135/225 142/104 153/135 143 148 757 802 6809       SEEN-BY: 153/7083 7715 203/0 218/700 840 221/1 6 242 360 226/30 227/114       SEEN-BY: 229/110 112 113 206 307 317 400 426 428 470 664 700 240/5832       SEEN-BY: 266/512 280/5003 5006 282/1038 291/111 301/1 320/119 219       SEEN-BY: 320/319 2119 322/757 335/364 341/66 342/200 396/45 423/81       SEEN-BY: 460/58 633/280 712/848 5020/400 5075/35       PATH: 153/757 221/6 1 320/219 229/426           |
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