home bbs files messages ]

Just a sample of the Echomail archive

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

 Message 10345 
 Alan Ianson to All 
 Daily APOD Report 
 04 May 25 04:04:44 
 
MSGID: 1:153/757.0 3b6d36ab
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.

                                 2025 May 4
    An artistic illustration of a black hole is shown. The black spot in
        the center is the black hole, while the accretion disk of gas
    surrounding it is shown in orange. Stars and the darkness of space is
    shown near the top in the background. Please see the explanation for
                         more detailed information.

                    Spin up of a Supermassive Black Hole
             Illustration Credit: Robert Hurt, NASA/JPL-Caltech

   Explanation: How fast can a black hole spin? If any object made of
   regular matter spins too fast -- it breaks apart. But a black hole
   might not be able to break apart -- and its maximum spin rate is really
   unknown. Theorists usually model rapidly rotating black holes with the
   Kerr solution to Einstein's General Theory of Relativity, which
   predicts several amazing and unusual things. Perhaps its most easily
   testable prediction, though, is that matter entering a maximally
   rotating black hole should be last seen orbiting at near the speed of
   light, as seen from far away. This prediction was tested by NASA's
   NuSTAR and ESA's XMM satellites by observing the supermassive black
   hole at the center of spiral galaxy NGC 1365. The near light-speed
   limit was confirmed by measuring the heating and spectral line
   broadening of nuclear emissions at the inner edge of the surrounding
   accretion disk. Pictured here is an artist's illustration depicting an
   accretion disk of normal matter swirling around a black hole, with a
   jet emanating from the top. Since matter randomly falling into the
   black hole should not spin up a black hole this much, the NuSTAR and
   XMM measurements also validate the existence of the surrounding
   accretion disk.

               Hole New Worlds: It's Black Hole Week at NASA!
                      Tomorrow's picture: planet lines
     __________________________________________________________________

       Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
            NASA Official: Amber Straughn Specific rights apply.
                  NASA Web Privacy, Accessibility, Notices;
                      A service of: ASD at NASA / GSFC,
                           NASA Science Activation
                             & Michigan Tech. U.

--- BBBS/Li6 v4.10 Toy-7
 * Origin: The Rusty MailBox - Penticton, BC Canada (1:153/757)
SEEN-BY: 19/10 105/81 106/201 128/187 129/305 134/100 153/135 143
SEEN-BY: 153/148 151 153 757 6809 7083 7715 154/110 218/700 840 221/1
SEEN-BY: 221/6 360 226/30 227/114 229/110 114 206 307 317 400 426
SEEN-BY: 229/428 470 664 700 705 240/1120 266/512 291/111 301/1 113
SEEN-BY: 301/812 320/219 322/757 335/364 341/66 342/200 396/45 460/58
SEEN-BY: 460/256 1124 633/280 712/848 902/26 5020/400 1042 8912 5054/30
SEEN-BY: 5075/35
PATH: 153/757 221/6 301/1 460/58 229/426


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

(c) 1994,  bbs@darkrealms.ca