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  • [[Category:Galaxies]] ...
    329 bytes (49 words) - 00:05, 11 March 2013
  • === Spiral galaxies === === Elliptical galaxies === ...
    6 KB (950 words) - 11:37, 2 November 2016
  • ...ay [[universe]], including the existence of large-scale structures such as galaxies. The theory was proposed by [[Alan Guth]] in the 1970s. ...oblem solved by inflation is the origin of large-scale structures, such as galaxies. Inflation theory says that in a slow expansion of the universe, [[quantum ...
    3 KB (494 words) - 23:28, 18 October 2015
  • [[Star]]<nowiki/>s, [[Galaxy|galaxies]] and other objects emit energy in the form of [[radiation]]. It is [[Measu ...
    1 KB (225 words) - 11:44, 21 June 2017
  • |[[Image:Messier51.jpg|thumb|200px|The arms of [[Spiral galaxy|spiral galaxies]] often have the shape of a logarithmic spiral, here the [[Whirlpool Galaxy ...pitch angle for a galaxy such as the Milky Way. In general, arms in spiral galaxies have pitch angles ranging from about 10 to 40 degrees. ...
    7 KB (1,062 words) - 18:16, 9 March 2015
  • ...e, measurement of eclipsing binaries offers a way to gauge the distance to galaxies. Accuracy at the 5% level up to a distance of around 3 million parsecs.<ref ...sions to be used as standard candles to measure the distance to their host galaxies, because the visual magnitude of the supernovae depends primarily on the di ...
    10 KB (1,469 words) - 22:59, 15 September 2015
  • ...e universe, hidden far beyond our vision. They could have formed their own galaxies and solar systems too. ...
    5 KB (898 words) - 00:12, 25 April 2016
  • ...The first stage is the formation of condensations ultimately to become the galaxies; this, as we have seen, started off an expansion, which then '''automatical ...and million years, he sees us shrinking; atoms, animals, planets, even the galaxies, all shrink alike; only the intergalactic spaces remain the same. The earth ...
    23 KB (3,626 words) - 09:52, 1 September 2017