2014
DOI: 10.1134/s003809461406001x
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Effects of a physical librations of the moon caused by a liquid core, and determination of the fourth mode of a free libration

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Cited by 12 publications
(3 citation statements)
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“…Also, as we have already noted, having N fcn 1, considerably reduces the amplitude of the resonance. Indirect observation of the FCN based on its resonance with weaker modes of physical libration have been proposed (Barkin et al 2014;Petrova et al 2018). Our results show that such measurements would not give T fcn directly, but rather a value 10% smaller.…”
Section: Implications For Mars and The Moonmentioning
confidence: 54%
“…Also, as we have already noted, having N fcn 1, considerably reduces the amplitude of the resonance. Indirect observation of the FCN based on its resonance with weaker modes of physical libration have been proposed (Barkin et al 2014;Petrova et al 2018). Our results show that such measurements would not give T fcn directly, but rather a value 10% smaller.…”
Section: Implications For Mars and The Moonmentioning
confidence: 54%
“…In addition, as we have already noted, having N 1 fcn  considerably reduces the amplitude of the resonance. Indirect observation of the FCN based on its resonance with weaker modes of physical libration has been proposed (Barkin et al 2014;Petrova et al 2018). Our results show that such measurements would not give T fcn ☾ directly, but rather a value 10% smaller.…”
Section: Implications For Mars and The Moonmentioning
confidence: 54%
“…Improved seismic equipment on the Moon may eventually give the densities of the lunar inner and outer cores and hence constrain its concentration of S. Currently, lunar libration data do not provide useful constrains on lunar core density [ Barkin et al ., ; Williams and Boggs , ]. The presence or absence of any molten silicates in the deep Moon is another constraint.…”
Section: Minor and Trace Elementsmentioning
confidence: 99%