We detect
orbital motion over more than one year and characterise the possible Keplerian orbits.
Not exact matches
The researchers» interpretation is that the jet is «serpentine and inhomogeneous» because it emits radiation
over a range of frequencies and from different zones, which change their orientation due to the instabilities in the jet, or to
orbital motions.
The tides produced by these two bodies are roughly comparable in magnitude, but the
orbital motion of the Moon results in tidal patterns that vary
over the course of a month.