Ring Nebula Deep Field (2009 November 6 APOD)
Posted: Fri Nov 06, 2009 4:01 pm
http://apod.nasa.gov/apod/ap091106.html
http://en.wikipedia.org/wiki/Ring_Nebula wrote:
<<Within the last two thousand years, the central star of the Ring Nebula has left the asymptotic giant branch after exhausting its supply of hydrogen fuel. Thus it no longer produces its energy through nuclear fusion and, in evolutionary terms, it is now becomimg a compact white dwarf star. This planetary nebula nucleus (PNN) now consists primarily of carbon and oxygen with a thin outer envelope composed of lighter elements. Its mass is about 0.61–0.62 solar mass, with a surface temperature of 125,000K. Currently it is 200 times more luminous than the Sun, but its apparent magnitude is only +15.75.>>
http://en.wikipedia.org/wiki/Friedrich_von_Hahn wrote:
<<Friedrich II Graf von Hahn (July 27, 1742 – October 9, 1805) was a German nobleman, a philosopher and astronomer. Von Hahn was born in Neuhaus, Holstein. In 1793 he started the construction of a private observatory, the first in Mecklenburg, which was well equipped. He owned some of the largest mirrors made by William Herschel and precision instruments for determining the position of stars. In 1800, he discovered the central star in M57, the Ring Nebula in the constellation Lyra. After his death, his son, the "theatrical count", squandered his fortune and all books and instruments were sold. The best instruments were bought by Friedrich Wilhelm Bessel for the new observatory in Königsberg.>>