Jupiter is the largest planet in our solar system and a celestial body full of mysteries. For many years, humans have been studying Jupiter and trying to solve its many mysteries. This article will explore the unsolved mysteries of Jupiter and try to provide some possible answers.

Jupiter's surface is composed of a gaseous atmosphere and has no actual "surface." However, scientists have observed some interesting features on Jupiter through space probes and telescopes.

The most famous of these are the Europa Lineaments on Io. These lineaments may be caused by the movement and fracture of panels under liquid water. Europa also has the potential to have an ocean of liquid water, making it one of the most promising targets for the search for extraterrestrial life.

Jupiter's magnetic field is one of the most powerful in the solar system, being about 20 times the size of Earth's magnetic field. It is generated by currents inside Jupiter, generated by liquid metallic hydrogen spinning inside the planet. There is a transition region between this liquid metallic hydrogen layer and the solid rock core called the "core-mantle boundary," which may have a significant impact on Jupiter's magnetic field.

Unlike other planets such as Earth, Jupiter has a very irregular magnetic field pattern. It does not have distinct north and south poles but is composed of several regions. Some of these regions are very strong, while others are relatively weak. In addition, under certain circumstances, Jupiter's magnetic field can show anomalies, such as auroral outbursts.

Compared to other planets, Jupiter's magnetic field is very tilted. This means that the angle between its magnetic axis and its rotation axis is very large, about 11 degrees. This unusual tilt may be due to the presence of the core-mantle boundary.

The strength of Jupiter's magnetic field varies over time. This variation may be caused by the flow of liquid metallic hydrogen in Jupiter's interior. In addition, variations in the strength of Jupiter's magnetic field may also be related to the solar wind and other particles and radiation in the space environment near the planet.

Jupiter's Great Red Spot has existed on the surface of Jupiter for at least 400 years, but scientists still have unanswered questions about its origin and evolution. The Great Red Spot is a large and persistent storm located in the northern hemisphere of Jupiter's surface.

It looks like a spinning vortex with a diameter of about 1.3 times the diameter of Earth. This storm spins several times a day at speeds exceeding 400 km/h. Due to its intense wind speed and persistent nature, scientists often describe it as an "eternal" storm.

There are several different theories about the origin of the Great Red Spot. One theory suggests that it may be driven by energy generated by an explosion on the surface of Jupiter. This explosion may be related to some form of energy release occurring deep inside Jupiter.

The other theory suggests that the origin of the Great Red Spot may be related to Jupiter's magnetic field. Jupiter has an extremely strong magnetic field, which may lead to the formation of ionospheres and plasma in its atmosphere. These materials may form a stable circulation that leads to the formation of the Great Red Spot.

Recent observations show that the Great Red Spot is gradually getting smaller. In the early 20th century, it was about 4 times the diameter of Earth; now, it has shrunk to about 1.3 times the diameter of Earth. This change may be related to the movement of certain materials in Jupiter's atmosphere.

In addition, outburst events occur frequently in the Great Red Spot. These outbursts can cause storms to become shorter in duration and cause disturbances in the surrounding region.

Why is the Great Red Spot so stable? Although it has existed for hundreds of years, it still maintains a relatively stable shape and position. Why is the Great Red Spot gradually shrinking? Scientists are still unsure of the cause of this change.

Another mystery surrounding the Great Red Spot is the structure of the material inside it. Scientists have been striving to understand the composition and movement of the material within the storm to gain insight into its evolutionary process.

Similar to Saturn, Jupiter also possesses a ring system. However, Jupiter's rings are very faint and challenging to observe. Scientists are uncertain about the composition of these rings and why they appear so faint.

Jupiter remains an enigmatic object, and scientists are diligently studying all aspects of it. Although our understanding of Jupiter is not yet complete, advancements in technology and research methods continue to offer hope for unraveling more of its unanswered questions.