Add support for a third mode of nav.colocate that finds the planet's center based on cross-correlation between models and observations of planetary rings. This is useful because rings are often less time-variable than stormy planets, and they are also larger on the sky; together, this promises higher-accuracy centroiding.
Add support for a third mode of nav.colocate that finds the planet's center based on cross-correlation between models and observations of planetary rings. This is useful because rings are often less time-variable than stormy planets, and they are also larger on the sky; together, this promises higher-accuracy centroiding.