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We then continue this orbit segment until (29) is satisfied.
We then continue this orbit segment by imposing the boundary conditions textstylebegin{cases} u(0) in L^{a}_{1} = { z=-30 } cap S^{a}, u(1) in varSigma _{1} = { z=30 }, end{cases} (31) and letting (u(0)) vary along (L^{a}_{1}).
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This allows us to continue the orbit segments in a chosen parameter and analyse the precise nature of their continuous deformation even over exponentially small parameter variations.
Any planets that survive this process will continue to orbit this body, but will receive little thermal radiation and become frigid bodies.
This will continue to orbit and observe 67P for at least a further year.
Continuing this process, we get an orbit of at satisfying the following: (2.10).
Continuing this process, we get an orbit of at such that (2.56).
Continuing this process, we get an orbit of in such that (2.8).
Continuing this process, we get an orbit { u n } of T in X such that u n + 1 ∈ J b u n ⊆ T ( u n ), (23).
Continuing this way, we construct an orbit { y 0 = y 1 = y 2 = ⋯ = 0 } for ( f, T ) at u 0 = 1.
The Rosetta orbiter will continue to orbit 67P for the next 13 months, monitoring the comet as it draws closer to the sun and ever more of its subsurface ice sublimes, or outgasses, driving jets of gas and dust.
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