Abstract ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …

Jupiter's atmosphere has a system of zones and belts punctuated by small and large
vortices, the largest being the Great Red Spot. How these features change with depth is …

The Juno spacecraft has been collecting data to shed light on the planet's origin and
characterize its interior structure. The onboard gravity science experiment based on X-band …

We present a reanalysis (using the Minnaert limb‐darkening approximation) of visible/near‐
infrared (0.3–2.5 μm) observations of Uranus and Neptune made by several instruments. We …

Giant planets acquire gas, ices and rocks during the early formation stages of planetary
systems and thus inform us on the formation process itself. Proceeding from inside out …

Context. The precise mechanism that forms jets and large-scale vortices on the giant planets
is unknown. An inverse cascade has been suggested by several studies. Alternatively …

摘要2021 年全球空间科学探索与发现热点竞相涌现. 聚焦非载人航天, 按空间天文, 日球层物理,
行星科学, 空间地球科学等学科领域, 梳理了各国空间科学任务的年度重要代表性成果 …

The polar cyclone at Jupiter's south pole and the five cyclones surrounding it oscillate in
position and interact. These cyclones, observed since 2016 by NASA's Juno mission …

Saturn's C ring contains multiple structures that appear to be density waves driven by time-
variable anomalies in the planet's gravitational field. Semiempirical extensions of density …

Jupiter's equatorial eastward zonal flows reach wind velocities of∼ 100 ms− 1, while on
Saturn they are three times as strong and extend about twice as wide in latitude, despite the …