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hpiers.obspm.fr/eop-pc/models/constants.html
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Geodetic constants. Earth's equatorial radius, a, 6 378 136.6(1), m, 0.015, IERS Numerical Standards (IAG 1999). Equatorial moment of inertia, A, 8.0101(2) ...
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www.earth.sinica.edu.tw/~bfchao/publication/eng/1991-Li...
www.earth.sinica.edu.tw/~bfchao/publication/eng/1991-Liu&Chao-The%20Earth's%20equatorial%20principal%20axes%20and%20moments%20of%20inertia.pdf
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Let the Earth's equatorial principal moments of inertia be A and B, where A < B, and the corresponding principal axes be a and b. Explicit formulae are here ...
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www.gps.caltech.edu/classes/ge131/notes/Ch11.pdf
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We saw that J2 can be related to the difference in the moments of inertia about equatorial and polar axes. An independent piece of information is often available ...
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MMR06 - Wikipedia, the free encyclopedia
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en.wikipedia.org/wiki/MMR06
center of wind pressure, 1 m. Axial moment of inertia at launch, 0.87 kg/m². Axial moment of inertia at burn-out, 0.25 kg/m². Equatorial moment of inertia at launch ...
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www.uwgb.edu/dutchs/PSEUDOSC/IceCaps.HTM
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Mar 12, 2007 ... We can calculate them, but the figures are already tabulated. Equatorial moment of inertia: 8.0095 E+37 kg m2; Rotational velocity 7.27220 E-5 ...
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en.allexperts.com/q/Astronomy-1360/Earth-Orbitory-Movem...
en.allexperts.com/q/Astronomy-1360/Earth-Orbitory-Movement.htm
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Jun 29, 2005 ... To be specific, the equatorial moment of inertia is roughly 1/300 of the axial moment. This may seem like an insignificant difference - but when ...
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www.mendeley.com/research/monitoring-and-evaluation-of-...
www.mendeley.com/research/monitoring-and-evaluation-of-the-convention-appliance-public-involvement-and-participation/
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(1991) Liu, Chao. Geophysical Journal International. Read by researchers in: 100% Earth Sciences. The earth's equatorial principal moments of inertia are given ...
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onlinelibrary.wiley.com/doi/10.1111/j.1365-246X.1991.tb...
onlinelibrary.wiley.com/doi/10.1111/j.1365-246X.1991.tb06341.x/pdf
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Let the Earth's equatorial principal moments of inertia be A and B, where A < B, and the corresponding principal axes be a and b. Explicit formulae are here ...
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www.lpi.usra.edu/meetings/lpsc2012/pdf/2230.pdf
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core polar minus equatorial moment of inertia differ- ence due to CMB flattening is weakly significant. This strengthens the case for a fluid lunar core. Future ap- ...
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