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Unexpected details of Jupiter revealed by the Webb Space Telescope

23 août 2022

Under the sharp gaze of the Webb Space Telescope, Jupiter is revealed in a new light. Captured in July-August 2022 as part of an "Early Science" demonstration program co-led by an astrophysicist from Paris Observatory - PSL, the images are breathtaking.

Image de Jupiter prise par le télescope spatial Webb
Les nouvelles images de Jupiter prises par le télescope spatial Webb affichent une richesse de détails étonnante. Un filtre sensible à l’émission aurorale de l’hydrogène ionisé (cartographié dans le canal rouge) révèle des ovales auroraux sur le disque de la planète qui s’étendent jusqu’à de hautes altitudes au-dessus des pôles nord et sud. Un autre filtre sensible aux brumes de haute altitude (cartographié dans le canal vert) met en évidence les brumes polaires qui tournent autour des pôles nord et sud, tandis qu’un troisième filtre met en évidence la lumière réfléchie par le nuage principal plus profond (cartographié dans le canal bleu). La grande tache rouge, la région équatoriale et les régions nuageuses compactes (y compris les plus petites) apparaissent en blanc (ou blanc rougeâtre) sur cette image en fausses couleurs. Les régions avec une faible couverture nuageuse apparaissent comme des rubans sombres au nord de la région équatoriale mais également à côté de la grande tache rouge et dans les structures cycloniques de l’hémisphère sud, tout comme observé habituellement en lumière visible.
NASA, ESA, Jupiter ERS Team ; image processing by Judy Schmidt)

Captured on July 27, the infrared images — artificially colored to make specific features stand out — show fine filigree along the edges of the colored bands and around the Great Red Spot and also provide an unprecedented view of the auroras over the north and south poles.

One wide-field image presents a unique lineup of the planet, its faint rings and two of Jupiter’s smaller satellites — Amalthea and Adrastea — against a background of galaxies.

“We’ve never seen Jupiter like this. It’s all quite incredible,” said planetary astronomer Imke de Pater, professor emerita of the University of California, Berkeley, who led the scientific observations of the planet with Thierry Fouchet, a professor at the Paris Observatory. “We hadn’t really expected it to be this good, to be honest. It’s really remarkable that we can see details on Jupiter together with its rings, tiny satellites and even galaxies in one image.”

Image composite en fausses couleurs de Jupiter a été obtenue avec l’instrument NIRCam
Cette image composite en fausses couleurs de Jupiter a été obtenue avec l’instrument NIRCam à bord du JWST le 27 juillet 2022. Les couleurs sont différentes de la figure car ce mode d’imagerie a utilisé des temps d’exposition différents et seulement 2 filtres, cartographiés en couleurs orange et cyan. L’image montre les anneaux de Jupiter et certains de ses petits satellites ainsi que des galaxies en arrière-plan. Amalthea ( 250x150 km de diamètre) et le petit Adrastea ( 20 km de diamètre) sont visibles sur cette image. Le motif de diffraction créé par les structures brillantes comme les zones aurorales ainsi que la lune Io (juste à gauche, non visible sur l’image) forment un arrière-plan complexe de lumière diffusée autour de Jupiter.
NASA, ESA, Jupiter ERS Team ; traitement d’image par Ricardo Hueso [UPV/EHU] et Judy Schmidt

De Pater, Fouchet and their team released the images today (Aug. 22) as part of the telescope’s Early Release Science program.

In addition to the enormous storm referred to as the Great Red Spot, numerous storm systems — seen as small pallid ovals —are also visible, as are tiny bright plumes of cloud particles. The transition between organized zonal flows and the chaotic vortex patterns at higher latitudes is also clearly visible.

“Although we have seen many of these features on Jupiter before, JWST’s infrared wavelengths give us a new perspective,” said de Pater. “JWST’s combination of images and spectra at near- and mid-infrared wavelengths will allow us to study the interplay of dynamics, chemistry and temperature structure in and above the Great Red Spot and the auroral regions.”
Amalthea and Adrastea

JWST’s Near Infrared Camera (NIRCam) also captured a wide-field view of Jupiter revealing its rings and two of its moons.

“This image illustrates the sensitivity and dynamic range of JWST’s NIRCam instrument,” Fouchet said. “It reveals the bright waves, swirls and vortices in Jupiter’s atmosphere and simultaneously captures the dark ring system, 1 million times fainter than the planet, as well as the moons Amalthea and Adrastea, which are roughly 200 and 20 kilometers across, respectively. This one image sums up the science of our Jupiter system program, which studies the dynamics and chemistry of Jupiter itself, its rings and its satellite system.”

The JWST images were processed with the help of citizen scientist Judy Schmidt of Modesto, California, who has worked with Hubble Space Telescope and other telescope images for the past 10 years, and Ricardo Hueso, who studies planetary atmospheres at the University of the Basque Country in Spain. Hueso is one of several coinvestigators on the Early Release Science (ERS) program, and is leading the NIRCam observations of Jupiter’s atmosphere.

Schmidt’s love of astronomy images has led her to process images of nebulae, globular clusters, stellar nurseries and more spectacular cosmic objects.

“Something about it just stuck with me, and I can’t stop. I could spend hours and hours every day,” she said. Her goal, she added, is to “… try to get it to look natural, even if it’s not anything close to what your eye can see.”

Spectroscopic observations of Jupiter’s auroras are scheduled for later this year, while detailed spectroscopic observations of Jupiter’s Great Red Spot were taken on July 27 in the near-infrared and August 14-15 at mid-infrared wavelengths. The Great Red Spot observations are a joint project between the Early Release Science (ERS) team — with de Pater and Fouchet as co-principal investigators — and a program of Solar System observations developed by Heidi Hammel of the Association of Universities for Research in Astronomy (AURA), with the Jupiter observations led by Leigh Fletcher, a professor at the University of Leicester in England.