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 9,434 of 10,823    |
|    Alan Ianson to All    |
|    Daily APOD Report    |
|    04 Feb 24 01:31:52    |
      MSGID: 1:153/757.0 34b89c9c       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 February 4        A starfield is shown that has only a few bright stars. Vertically        through the center is a large reddish brown nebula that has a few stars        embedded. Please see the explanation for more detailed information.               The Cone Nebula from Hubble        Image Credit: Hubble Legacy Archive, NASA, ESA - Processing & Licence:        Judy Schmidt               Explanation: Stars are forming in the gigantic dust pillar called the        Cone Nebula. Cones, pillars, and majestic flowing shapes abound in        stellar nurseries where natal clouds of gas and dust are buffeted by        energetic winds from newborn stars. The Cone Nebula, a well-known        example, lies within the bright galactic star-forming region NGC 2264.        The Cone was captured in unprecedented detail in this close-up        composite of several observations from the Earth-orbiting Hubble Space        Telescope. While the Cone Nebula, about 2,500 light-years away in        Monoceros, is around 7 light-years long, the region pictured here        surrounding the cone's blunted head is a mere 2.5 light-years across.        In our neck of the galaxy that distance is just over half way from our        Sun to its nearest stellar neighbors in the Alpha Centauri star system.        The massive star NGC 2264 IRS, seen by Hubble's infrared camera in        1997, is the likely source of the wind sculpting the Cone Nebula and        lies off the top of the image. The Cone Nebula's reddish veil is        produced by dust and glowing hydrogen gas.               Tomorrow's picture: carina's crazy core        __________________________________________________________________               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: 15/0 90/1 105/81 106/201 128/260 129/305 134/100 135/225       SEEN-BY: 153/135 143 757 802 6809 7083 7715 218/700 840 221/1 6 226/30       SEEN-BY: 227/114 229/110 112 113 206 307 317 400 426 428 470 664 700       SEEN-BY: 240/1120 266/512 282/1038 291/111 301/1 113 812 320/219 322/757       SEEN-BY: 335/364 341/66 342/200 396/45 460/58 256 1124 633/280 712/848       SEEN-BY: 5020/400 1042 5054/30 5075/35       PATH: 153/757 221/6 301/1 460/58 229/426           |
[   << oldest   |   < older   |   list   |   newer >   |   newest >>   ]
(c) 1994, bbs@darkrealms.ca