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Jupiter’s interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft

机译:木星的内部和深层大气:朱诺号航天器最初的两极间通过

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摘要

On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing less than 5000 kilometers above the equatorial cloud tops. Images of Jupiter’s poles show a chaotic scene, unlike Saturn’s poles. Microwave sounding reveals weather features at pressures deeper than 100 bars, dominated by an ammonia-rich, narrow low-latitude plume resembling a deeper, wider version of Earth’s Hadley cell. Near-infrared mapping reveals the relative humidity within prominent downwelling regions. Juno’s measured gravity field differs substantially from the last available estimate and is one order of magnitude more precise. This has implications for the distribution of heavy elements in the interior, including the existence and mass of Jupiter’s core. The observed magnetic field exhibits smaller spatial variations than expected, indicative of a rich harmonic content.
机译:2016年8月27日,朱诺号航天器获得了木星的科学观测结果,并在赤道云顶上方不到5000公里处通过。与土星的极点不同,木星的极点图像显示出混乱的景象。微波探测显示出压力大于100巴的天气特征,其特征是富含氨的狭窄低纬度羽流,类似于地球的哈德利电池的更深,更宽的版本。近红外图显示出显着的下行区域内的相对湿度。朱诺的测得重力场与最新的估算值大不相同,并且精确度高出一个数量级。这对内部重元素的分布具有影响,包括木星核心的存在和质量。观察到的磁场表现出比预期小的空间变化,这表明谐波含量丰富。

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