Webb and Hubble telescopes watched Jupiter’s auroras at the same time. For some reason, they did not see the same

The Great red spot, Polar cyclones, Cloud bands. Jupiter is known for its colossal dimensions and eternal storms. But their auroras are not far behind, and only now We are seeing them in detail Thanks to the power of the James Webb space telescope. A Christmas gift. Newly published with a study of Nature Communicationsthe images were captured on December 25, 2023 with the Nircam Chamber of the Webb Telescope. The most immediate conclusion is that the jovian auroras are of another level. Hundreds of times brighter and more energy than those of the Earth, not only feed, as on our planet, of the particles loaded with the solar wind, but also of the volcanic material expelled by the active moon ío. Hyperactive. The team that led the observations took a surprise when analyzing the data. They hoped to see slow and gradual changes in the auroras, but instead they found “the entire bullendo region and exploding of light”, a hyperactive show that “varied in a matter of seconds.” “What a Christmas gift was that, he left me hallucinated!” Confesses the researcher Jonathan Nichols of the University of Leicester, the United Kingdom. A mystery. To round the study, the team coordinated Webb’s observations in infrared with Simultaneous observations of the Hubble Space Telescope in the ultraviolet spectrum. And here was the puzzle: the brightest lights observed by the Webb in Jupiter’s atmosphere did not have a counterpart in the Hubble images. The webb focused on trihydrogen cation emissions (H3+), a molecule that shines intensely in infrared when high -energy electrons impact molecular hydrogen. But to produce the combination of brightness observed by both telescopes, a huge amount of very low energy particles would be needed by hitting Jupiter’s atmosphere, something that until now was considered practically impossible. What follows. The team plans to study this difference between webb and Hubble data, and explore its implications for Jupiter’s environment. Webb’s next observations will be compared with NASA Juno probe data to try to unravel the origin of the broadcast. The findings will be used to guide the Juice Mission of ESA, who travels now to Jupiter. Seven of their instruments, including their two cameras, will dedicate themselves to study the Jovian auroras when the probe reaches their destination. Its nearby measurements will help astronomers better understand the interaction between the magnetic field and the planet’s atmosphere, in addition to the moon ío. Images | NASA, ESA, CSA In Xataka | These real images were unthinkable before the Webb Telescope: they are planets orbiting other stars to 130 light years

NASA is about to launch two rockets toward the auroras. The objective: understand their hypnotic movements

The auroras have fascinated those who have observed them for millennia, but they continue to hold all kinds of mysteries. despite current sensors. In order to better understand your blinks and pulses, NASA will fly directly to them from the region of the United States where they appear most frequently. Meanwhile, in Alaska. Although almost all of America’s space activity occurs in warm Florida, NASA’s Goddard Space Flight Center has everything ready to launch a sounding rocket from Alaska. Delayed on numerous occasions due to bad weather (today they expect snowfall and tomorrow, minimum temperatures of -28 ºC), the launch is scheduled for this week from Poker Flat Research Camp from Fairbanks. A flight to the auroras. The mission is called Ground Imaging to Rocket investigation of Auroral Fast Features (whose acronym is “GIRAFF”but I don’t know who they’re trying to fool, we all know they put the acronym first). The objective is to fly, with separate sounding rockets, to two subtypes of northern lights: Fast-pulsing aurorae, which flicker in a rhythmic pattern of pulsations every second, are related to a type of electromagnetic waves in the magnetosphere called Alfvén waves. Flickering auroras, whose variability is slower and more irregular, and are characterized by flickers in the sky that appear to move or shift according to the flow of charged particles in the magnetosphere Aboard a modified missile. For this mission, NASA will use Black Brant XI sounding rocketswhose first stage is derived from the US Talos naval missile. With three stages of solid fuel, the small rocket is capable of launching a payload of up to 600 kg to a height of 250 kilometers. The GIRAFF mission rockets are equipped with instruments to measure the processes responsible for creating the optical variations in auroras, hypnotic movements observable from Earth that occur at relatively high frequencies of up to 15 Hz or more. The GIRAFF mission. NASA researchers want to understand why some auroras flicker, others pulse, and others appear to have holes. This research focuses on two specific energy coupling mechanisms with such saccharine names as low-altitude electromagnetic ion cyclotron wave-particle interactions and chorus wave modulation in the equatorial magnetosphere. To better understand the mechanisms of these interactions, what better than to fly directly into a flickering aurora and a fast pulsating aurora with two identical rockets? A second mission will launch two more rockets into the dark spots or “holes” of the auroras to better study this other phenomenon. Images | NASA/Lee Wingfield/Sebastian Saarloos In Xataka | This is what the Northern Lights look like from space

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