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A Very Fast Symplectic Integrator for Planetary Systems: WHFast512 in x86 Assembly

  • Authors: Rishit Dagli, Hanno Rein

Rishit Dagli and Hanno Rein 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 2.

The absolute relative semimajor axis error, the sign of the semimajor axis error, and the number of iterations in the Kepler solver. Here, a test particle is integrated for one time step of 5 days. The current locations of the solar system planets are shown in each plot. See the text for a description of the lines.

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