Scientists’ research answers big question about our system’s largest planet

UAF scientist's research answers big question about our system's largest planet
The aurora was photographed in 2014 throughout a sequence of Hubble Area Telescope Imaging Spectrograph far-ultraviolet-light observations happening as NASA’s Juno spacecraft approached and entered into orbit round Jupiter. Credit score: NASA, ESA and J. Nichols, College of Leicester

New discoveries about Jupiter may result in a greater understanding of Earth’s personal area surroundings and affect a long-running scientific debate in regards to the photo voltaic system’s largest planet.

“By exploring a bigger area reminiscent of Jupiter, we will higher perceive the basic physics governing Earth’s magnetosphere and thereby enhance our area climate forecasting,” stated Peter Delamere, a professor on the UAF Geophysical Institute and the UAF School of Pure Science and Arithmetic.

“We’re one massive area climate occasion from dropping communication satellites, our energy grid belongings, or each,” he stated.

Area climate refers to disturbances within the Earth’s magnetosphere brought on by interactions between the photo voltaic wind and the Earth’s magnetic area. These are usually related to photo voltaic storms and the solar’s coronal mass ejections, which might result in magnetic fluctuations and disruptions in energy grids, pipelines and communication methods.

Delamere and a staff of co-authors detailed their findings about Jupiter’s magnetosphere in a paper in AGU Advances. Geophysical Institute analysis affiliate professor Peter Damiano, UAF graduate scholar researchers Austin Smith and Chynna Spitler, and former scholar Blake Mino are among the many co-authors.

Delamere’s analysis exhibits that our photo voltaic system’s largest planet has a magnetosphere consisting of largely closed magnetic area strains at its polar areas however together with a crescent-shaped space of open area strains. The magnetosphere is the defend that some planets have that deflects a lot of the photo voltaic wind.

The talk over open versus closed on the poles has raged for greater than 40 years.

An open magnetosphere refers to a planet having some open-ended magnetic area strains close to its poles. These are beforehand closed strains which have been damaged aside by the photo voltaic wind and left to increase into area with out re-entering the planet.

This creates areas on Jupiter the place the photo voltaic wind, which carries a few of the solar’s magnetic area strains, instantly interacts with the planet’s ionosphere and environment.

Photo voltaic particles transferring towards a planet on open area strains don’t trigger the aurora, which largely happens on closed area strains. Nevertheless, the vitality and momentum of photo voltaic wind particles on open area strains does switch to the closed system.

Earth has a largely open magnetosphere at its poles, with aurora occurring on closed area strains.. It’s the transferred vitality on these open strains that may disrupt energy grids and communications.

As a way to examine Jupiter’s magnetosphere, Delamere ran quite a lot of fashions utilizing information acquired by the NASA Juno spacecraft, which entered Jupiter’s orbit in 2016 and has an elliptical polar orbit.

“We by no means had information from the polar areas, so Juno has been transformative when it comes to the planet’s auroral physics and serving to additional the dialogue about its magnetic area strains,” Delamere stated.

Scientist's research answers big question about our system's largest planet
A detailed-up of Jupiter’s aurora exhibits auroral footprints of three moons: Io (alongside the left-hand limb), Ganymede (close to the middle) and Europa (slightly below and to the correct of Ganymede’s footprint). These emissions circulation on Jupiter’s magnetic area. Credit score: NASA picture, John Clarke, College of Michigan

The talk started with the 1979 flybys of Jupiter by NASA’s Voyager 1 and Voyager 2. That information led many to imagine that the planet had a usually open magnetosphere at its poles.

Different scientists argued that Jupiter’s auroral exercise, which is way totally different from Earth’s, indicated the planet had a principally closed magnetosphere on the poles. Delamere, a longtime researcher of Jupiter’s magnetic area, revealed a paper supporting that view in 2010.

In 2021, he was a co-author on a paper by Binzheng Zhang of the College of Hong Kong that steered via modeling that Jupiter’s magnetosphere had two areas of open magnetic area strains at its poles.

The mannequin exhibits one set of open-ended area strains rising from the poles and trailing outward behind the planet within the magnetotail, the slim teardrop-shaped portion of the magnetosphere pointing away from the solar. The opposite set emerges from Jupiter’s poles and goes off to the perimeters into area, carried by the photo voltaic wind.

“The Zhang end result offered a believable rationalization for the open area line areas,” Delamere stated. “And this yr we offered the compelling proof within the Juno information to help the mannequin end result.

“It’s a main validation of the Zhang paper,” he stated.

Delamere stated it is necessary to review Jupiter to higher perceive Earth.

“Within the massive image, Jupiter and Earth signify reverse ends of the spectrum—open versus closed area strains,” he stated. “To totally perceive magnetospheric physics, we have to perceive each limits.”

Delamere’s proof got here through an instrument on the Juno spacecraft that exposed a polar space the place ions flowed in a path reverse Jupiter’s rotation.

Subsequent modeling confirmed an identical ion circulation in the identical space—and close to the open area strains proposed within the 2021 paper by Zhang and Delamere.

“The ionized fuel on [closed] magnetic area strains linked to Jupiter’s northern and southern hemispheres rotates with the planet,” Delamere’s new paper concludes, “whereas ionized fuel on [open] area strains that connect with the photo voltaic wind transfer with the photo voltaic wind.”

Delamere writes that the polar location of open magnetic area strains “could signify a attribute function of rotating big magnetospheres for future exploration.”

Different contributors are from the College of Colorado Boulder, Johns Hopkins College, Andrews College, Embry-Riddle Aeronautical College, College of Hong Kong, College of Texas San Antonio, Southwest Analysis Institute and O.J. Brambles Consulting in the UK.

Delamere will current the analysis in July on the Convention on Magnetospheres of the Outer Planets on the College of Minnesota.

Extra data:
P. A. Delamere et al, Signatures of Open Magnetic Flux in Jupiter’s Dawnside Magnetotail, AGU Advances (2024). DOI: 10.1029/2023AV001111

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Scientists’ analysis solutions massive query about our system’s largest planet (2024, Might 6)
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