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Glossary term: 大红斑

Description: 大红斑是木星大气层中的一个巨大的反气旋风暴,位于其赤道以南22度处。大红斑约15,000公里长,接近12,000公里宽,目前的尺寸比地球稍大,而在过去它曾达到更大的规模。大红斑内部的风速可超过400公里每小时(250英里每小时)。大红斑呈红色的原因尚不清楚,目前存在多种相互竞争的假说。天文学家乔瓦尼·卡西尼(Giovanni Cassini)在1665年发现了木星上的一个大红斑,并对其进行了长达半个世纪的观测。然而,由于之后的一百年内缺乏观测记录,尚不确定该红斑是否与过去两百年间观测到的大红斑为同一风暴。

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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

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The planet Jupiter with horizontal cloud ribbons and the great red spot

Jupiter

Caption: This full disk view of Jupiter was obtained on 21 April 2014 with Hubble's Wide Field Camera 3 (WFC3). It shows the prominent great red spot, a gigantic cyclone. Cloud ribbons cover the surface, whose colours stem from gases like ammonia and other chemical compounds.
Credit: NASA, ESA, and A. Simon (Goddard Space Flight Center) credit link

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