Why does Jupiter boil so much? The answer hidden in the moon blazing with colorful lights and volcanoes

Why does Jupiter boil so much? The answer hidden in the moon blazing with colorful lights and volcanoes

Temperature maps are detailed in detail with the help of the Keck telescope. From this it was found that the temperature inside the aurora was very high and for the first time it was found that because of these the planet was hot.

According to Jupiter's distance from the Sun, its temperature should have been 72 ° C, but actually it is 425 ° C. Why is that? This question kept scientists confused for a long time, but now its answer seems to be found in its beautiful Aurora. Scientists from the University of Lesta, in collaboration with the US Space Agency, prepared Jupiter's temperature maps and found that due to the aurora, temperatures on this large planet were very high, while still distributing just over 10% of space.


The charged particles from the volcanic moon of Jupiter (Io) form ultraviolet auroras. Previous forms of Jupiter's winds suggest that winds from the aurora to the equator turn west while Jupiter rotates 43 miles per hour a day. The heat of this aurora cannot get out of the poles. However, a new study has found that something different is actually happening in Jupiter.



According to Japan's JAXA Space Agency researcher and author of the study, Dr. James Donog states that Jupiter's first global warming map was developed. Temperature maps are detailed in detail with the help of the Keck telescope. From this it was found that the temperature inside the aurora was very high and for the first time it was found that because of these the planet was hot.



Investigators prepared five maps. Two high-resolution maps found that the aurora's winds were a bit weak. From the map, the temperature in the upper part of the atmosphere is slightly lower than the equator. According to research co-author Tom Stallard, A region seen away from the aurora that has never been seen before. It is believed to be an air column traveling from the aurora to the equator.