Encyclopedia of the Solar System 2nd ed

780 Encyclopedia of the Solar System FIGURE 10 Orthographic projections of the lunar near and far sides: (a) Elevation; (b–d) ab ...

Remote Chemical Sensing Using Nuclear Spectroscopy 781 FIGURE 10 (Continued) A large portion of the western near side is enriche ...

782 Encyclopedia of the Solar System that comprise the mare. The highest concentrations of TiO 2 are found in Tranquillitatis as ...

Remote Chemical Sensing Using Nuclear Spectroscopy 783 TABLE 2 Sensitivity of neutron energy ranges to Mars surface and atmosphe ...

784 Encyclopedia of the Solar System FIGURE 12 Global map of the abundance (weight fraction) of WEH. The map gives a lower bound ...

Remote Chemical Sensing Using Nuclear Spectroscopy 785 FIGURE 13 (a) Orthographic projections of epithermal counting rates in no ...

786 Encyclopedia of the Solar System During their respective winters, the counting rate at high latitudes increases towards the ...

100-C 25-C 50-C 75-C C+M 50-C+M C+Y 50-C+Y M+Y 50-M+Y 100-M 25-M 50-M 75-M 100-Y 25-Y 50-Y 75-Y 100-K 25-K 25-19-19 50-K50-40-40 ...

788 Encyclopedia of the Solar System In this article the basic orbital properties of solar sys- tem objects (planets, moons, min ...

Solar System Dynamics: Regular and Chaotic Motion 789 Z R X N O P f i M  Ω FIGURE 2 Geometry of an orbit in three dimensions. T ...

790 Encyclopedia of the Solar System of massM, the circular velocity is vc= √ GM r . (9) Thus the orbital period (the time to mo ...

Solar System Dynamics: Regular and Chaotic Motion 791 bodies, including the mean longitudes (i.e., the location of the bodies in ...

792 Encyclopedia of the Solar System (L 4 andL 5 ) form equilateral triangles with the two massive bodies. Particles displaced s ...

Solar System Dynamics: Regular and Chaotic Motion 793 − 400 − 200 0 200 400 600 − 400 − 300 − 200 − 100 0 100 200 300 − 400 − 20 ...

794 Encyclopedia of the Solar System plane: μ^2 = 2 n^2 −κ^2. (29) For a perfectly spherically symmetric planet,μ=κ=n. Since Sat ...

Solar System Dynamics: Regular and Chaotic Motion 795 a test massless particle moves under the gravitational effect of both mass ...

796 Encyclopedia of the Solar System the particle’s motion is always restricted to thex−yplane. The existence of the Jacobi cons ...

Solar System Dynamics: Regular and Chaotic Motion 797 50 100 150 200 250 300 0.675 0.68 0.685 0.69 0.695 Semimajor axis Time (Ju ...

798 Encyclopedia of the Solar System 50 100 150 200 250 300 0.2 0.24 0.28 0.32 Eccentricity Time (Jupiter periods) FIGURE 9 The ...

Solar System Dynamics: Regular and Chaotic Motion 799 0.5 0.6 0.7 0.8 0.9 -0.4 -0.2 0 0.2 0.4 x x . FIGURE 11 A surface of secti ...