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Cosmic Dawn pp 153-172 | Cite as

The Weight, Shape, and Fate of the Universe

  • George Rhee
Chapter
Part of the Astronomers' Universe book series (ASTRONOM)

Abstract

In order to estimate the size, luminosity and mass of galaxies we need to know the Hubble constant and the density of the universe. In recent years, these numbers have been measured to better than 1% accuracy. This is a remarkable improvement on the situation 20 years ago when the Hubble constant was not known to better than a factor of 2.

Three observations taken together have made this improvement possible. The first is the observation of the variations in brightness of the cosmic background radiation. The second is the observation of distant supernova explosions. The third is the observation of the clustering of galaxies. The attempt to better constrain the density of the universe using supernovas led to the remarkable discovery that instead of slowing down as we might, expect the expansion of the universe is in fact accelerating. This discovery implies the existence of a new force in the universe that astronomers call dark energy.

Keywords

Dark Matter Dark Energy Background Radiation Supernova Explosion Hubble Constant 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© Springer Science+Business Media, LLC 2013

Authors and Affiliations

  • George Rhee
    • 1
  1. 1.Department of Physics & AstronomyUniversity of NevadaLas VegasUSA

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