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Identification of new orbits to enable future mission opportunities for the human exploration of the martian moon Phobos

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Academic year: 2019

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Figure 1:the equatorial and orbital planes of theMartian moons.Figure 3:analysis. Vertical dotted lines indicateDifferential perturbations2Figure 2: Misalignment angle betweenx(dashed line) and ellipsoid (plain line)
Figure 4: Sun-Mars eclipse at Phobos.Eclipse times are defined for a singleeclipse during one Phobos’ rotation.Figure 5: Sun-Phobos eclipse.Lightfunction of the dual-cone model
Figure 8: Lighting conditions around Phobos. On the left,light field around Phobos in the radial-vertical plane of theCR3BP frame, averaged over a year, a spring equinox month, asummer solstice month
Figure 9: Sky occultation around Phobos. Occultation fieldaround Phobos in the radial-vertical plane of the CR3BP frame.
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