Murison was unable to travel to Kitt Peak for the third run of the dFTS on the Steward Observatory 90-inch. Andrew Cenko graciously filled in. Murison also put to paper some of his "M-lens" design notes, as well as formal calculations of guider box AO mirror calibration errors.

Murison worked out a new design for an eight-beam differential image motion monitor which will enable characterization of atmospheric turbulence (which, furthermore, affects the behavior of atmospheric refraction).

Murison continued work on his Kepler equation paper.

Murison continued work on his new restricted three-body code for research (in collaboration with Efroimsky) on satellite capture.