Changes

Perhaps observing a widening divergence between observation and theory, the authors declared that "it seems unlikely that this test of relativistic gravity will be improved significantly."<ref>J. M. Weisberg and J. H. Taylor, ''[http://arxiv.org/PS_cache/astro-ph/pdf/0407/0407149v1.pdf Relativistic Binary Pulsar B1913+16: Thirty Years of Observations and Analysis]'' (July 7, 2004).</ref>

Perhaps observing a widening divergence between observation and theory, the authors declared that "it seems unlikely that this test of relativistic gravity will be improved significantly."<ref>J. M. Weisberg and J. H. Taylor, ''[http://arxiv.org/PS_cache/astro-ph/pdf/0407/0407149v1.pdf Relativistic Binary Pulsar B1913+16: Thirty Years of Observations and Analysis]'' (July 7, 2004).</ref>

No data observed after 2003 have been published about this binary pulsar, which suggests that the data have diverged even further from the predictions of the [[General Theory of Relativity]].  It would be easy to post the data on the internet for the public to view and draw their own conclusions.

Observations made since this time and published in a 2010 issue of The Astrophysical Journal<ref>http://iopscience.iop.org/0004-637X/722/2/1030/</ref> have shown that the energy loss within the system through [[Gravitational waves]] matches predictions made by the Theory of General Relativity.

==References==

==References==