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    Spin state and moment of inertia of Venus

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    Fundamental properties of the planet Venus, such as its internal mass distribution and variations in length of day, have remained unknown. We used Earth-based observations of radar speckles tied to the rotation of Venus obtained in 2006-2020 to measure its spin axis orientation, spin precession rate, moment of inertia, and length-of-day variations. Venus is tilted by 2.6392 ±\pm 0.0008 degrees (1σ1\sigma) with respect to its orbital plane. The spin axis precesses at a rate of 44.58 ±\pm 3.3 arcseconds per year (1σ1\sigma), which gives a normalized moment of inertia of 0.337 ±\pm 0.024 and yields a rough estimate of the size of the core. The average sidereal day on Venus in the 2006-2020 interval is 243.0226 ±\pm 0.0013 Earth days (1σ1\sigma). The spin period of the solid planet exhibits variations of 61 ppm (∼\sim20 minutes) with a possible diurnal or semidiurnal forcing. The length-of-day variations imply that changes in atmospheric angular momentum of at least ∼\sim4% are transferred to the solid planet.Comment: 20 pages, 7 figures, supplementary information. Submitted to Nature Astronomy on October 14, 202
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