Anisotropy of Space and the Orientation of Planetary Orbits in the Milky Way Galaxy
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Gravitational forces are calculated for a jclauaet moving witla the sun in the MilkyWay galaxy, using the linearized Eiuasteixt tlaeory. Two terms are foutad to beanisotropic: one nnay be called a "gravitouatagn?etic force", and tlae otlaer is expressedas an anisotropic effective mass of a planet experiencing tlae Nexvtonian grax'itationalforce exerted by tlae sun. In tlae direction of constellation Cygnus the effectix'e mass ofa planet of intrinsic mass /77 is 777(If(1/2)7'), and it is 777(l -(l/2)P) in tlte otlaerdirections. Tlae polarization P is the antisotropy of space and laas magxaitude of1.0X10-" (M. Mizuslaima: J. Plays. Soc. Jpn. 61 (1992) 1125). Because of tlais"anisotropic-uaaass effect" tlae equilibrium orientation of planetary orbits is in tlaeplane perpendicular to the direction of Cyguaus. Tlae gravitomaguaetic force shifts theequilibrium orientation of tlae planetary orbital plane to the direction perpendicularto constellation Lyra. Thus, tlte presenat orieu?tation of the plauaetary orbital plane isunderstood as the equilibrium orientation due to these two anisotropxc effects.gravity, general relativity, solar system, au?isotropy of space, Milky Way
- 社団法人日本物理学会の論文
- 1992-08-15
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