mirror of
https://github.com/cosinekitty/astronomy.git
synced 2026-03-29 20:03:36 -04:00
The smaller the slope magnitude |df/dt| is, the larger the uncertainty in dt. That means we are better off using an estimated value for the slope each time than underestimating the time error like we were doing. This also simplifies the code, and does not make it very much slower.