https://www.youtube.com/watch?v=4a3eY5siRRk
Must watch. The video was made by ESA.
[1] milligrams isn't a unit of force, but hopefully you know what I mean; milli-ounces sounds too weird.
The comet[1] that Rosetta is orbiting has a mass of 10^13 kg and an orbit semi-major axis of 518,060,000 km. This gives the comet a Sphere of Influence[2] of roughly 62 km.
What this means is that within 62 km or so, the comet is the dominant gravitational body, so orbits of 16, 20, and 30 km (in the video) are perfectly reasonable.
The orbital period[3] of the larger 30 km orbit is around 40 ksec or 11.1 hours.
[1]: http://en.wikipedia.org/wiki/67P/Churyumov%E2%80%93Gerasimen...
[2]: http://en.wikipedia.org/wiki/Sphere_of_influence_(astrodynam...
Maybe another look at the units:
G - 6.67384e-11 [N (m/kg)^2] = [m^3 / (kg s^2)]
M - 1.0e13 [kg]
a - 30000 [m]
sqrt([m^3] / ([m^3 / (kg s^2)] * [kg]))
= sqrt([s^2]) = [s]
2*pi*sqrt(30000^3 / (6.67384e-11 * 1.0e13))
= 1,263,787 s
= 14.6 days
Well, how about that :-)The reason for the maneuvers is to maintain line of sight with the Philae lander so that communications between Earth and Philae can be relayed, hence "relay phase". Then the probe inserts itself back into an orbit.
Thinking about navigating in zero gravity became a lot easier for me when I realised that you can arbitrarily redefine “down” as whatever direction is convenient. Gravity assists and orbits, for example, are simply falling around a bend.