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 either that the data have diverged even further from the predictions of the [[General Theory of Relativity]] or that the pulsar has not been observed since 2003.  It would be easy to post the data on the internet for the public to view and draw their own conclusions.

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.

==References==

==References==