High-Level Project Summary
This project is about the Jupiter.
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Detailed Project Description
This image, taken at Jupiter's north pole, contains swirls of varying colours and sizes. This indicates that there are storms of gas on the surface of Jupiter.
The region shown in this photo is in Jupiter's NNNNTB region, above 44 degrees north latitude. The shooting time is November 3, 2019.We think this large and unique spiral cyclone forms for similar reasons to solar activity such as flares. This is because Jupiter's composition is similar to that of stars.
An anticyclonic storm is created due to persistent high pressure regions in Jupiter's atmosphere. Because of the high air pressure required, we feel that large storms are uncommon on Jupiter, are dominated by small or irregular phenomena, and may all appear on a large scale.
Jupiter on November 29, 2021, will have two large rotating storms at 50°5'N latitude. The apparent "pop" is partly due to the shadows cast by the clouds above. From the color, we can guess that the two storms are not composed of the same gas, and we don't think the two storms will mix together in the end.
This is Jupiter's "Clyde point", which goes from a simple structure to a complex one. We speculate that this happens because of drastic changes in Jupiter's interior, such as gas eruptions, airflow at the bottom, and so on. This vision has the potential to exist for a long time.
This is the region known as JetN7, where Jupiter's strong winds create many visible swirling storms near the top of its atmosphere. External factors make our understanding of Jupiter more difficult.
This white storm was located around 40 degrees north latitude and was photographed on October 29, 2018. Based on the images we've collected, we think there will be more storms in Jupiter's north than in other parts, with smaller storms often surrounding large storms.
We believe that the thin strip running through the center of the image from top to bottom is the result of Jupiter's rapid rotation. In addition to this, we also suspect that it was formed by strong storms or other phenomena on the surface of Jupiter.
This image was taken on December 16, 2017, of Jupiter's equatorial region. Since there are fewer storms here, we think this can be used as an entrance if we want to explore Jupiter in the future.
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