The data for the shrinking of the Hulse Taylor binary pulsar is on wikipedia and so can be compared with the results from the new ECE2 shrinkage equation. A two variable least mean squares fit could be used to find the angular velocity and angular acceleration needed to describe the Hulse Taylor binary pulsar. Presumably there are many other binary pulsars now known to the astronomers, and many other S2 star type systems. ECE2 can explain essentially everything with a bit of thought, being the first successful unified field theory.

### Like this:

Like Loading...

*Related*

This entry was posted on September 3, 2018 at 5:34 am and is filed under asott2. You can follow any responses to this entry through the RSS 2.0 feed.
Both comments and pings are currently closed.