Tag Archives: Ganymede

Clearest images yet of Europa and Ganymede from Earth

Astronomers have revealed the most stunning and detailed images of two of Jupiter’s largest moons ever obtained from the surface of Earth.

The images show the icy surfaces and details of the processes that shape the chemical composition of Europa and Ganymede, two of Jupiter‘s four Galilean moons, which are named after the astronomer who first observed them. And scientists hope that the new images, captured by the Very Large Telescope (VLT) in Chile, will lay the groundwork for future space missions focused on these worlds.

The highly detailed observations reveal geological features on the two frozen Jovian moons including a long, rift-like marking that cuts across the surface of Europa, a type of deformation referred to by planetary scientists as a “linae.”

Related: Juno photos reveal more stunning glimpses of Jupiter’s ice-covered moon Europa

Both the observations of Europa, which is around the size of Earth’s moon, and of Ganymede, the solar system’s largest moon and larger than Mercury, record the amount of sunlight reflected from the moons’ icy surfaces. This observation produces what astronomers call a reflectance spectrum, which they can then analyze via a process called spectroscopy to reveal the chemical “fingerprints” of specific elements. These reflectance spectra allowed the scientists to determine the chemical composition of both Jovian moons.

The analysis of Europa showed that its crust is primarily composed of frozen water ice with non-ice materials, including a variety of different salts that reflectance spectroscopy couldn’t identify, across its surface.

“We mapped the distributions of the different materials on the surface, including sulfuric acid frost, which is mainly found on the side of Europa that is most heavily bombarded by the gasses surrounding Jupiter,” team leader and University of Leicester School of Physics and Astronomy Ph.D. student Oliver King, said in a statement. “The modeling found that there could be a variety of different salts present on the surface but suggested that infrared spectroscopy alone is generally unable to identify which specific types of salt are present.”

The team’s observations of Ganymede, meanwhile, revealed two types of terrain across the moon’s surface. Younger areas were marked by large amounts of water ice than much older regions, which are made up of a dark gray material that the team has not yet been able to identify.

The moons of Jupiter Europa and Ganymede as they orbit Jupiter.  (Image credit: ESO/King & Fletcher. Jupiter background image: NASA, ESA, A. Simon (Goddard Space Flight Center), and M. H. Wong (University of California, Berkeley) and the OPAL team)

Seen as blue-colored areas in the VLT image, the icy regions of Ganymede include its polar ice caps and craters where asteroid impacts have freshly exposed the ice that makes up the Galilean moon’s crust. King and his colleagues also used the images to map the size of ice grains across Ganymede’s surface and determine how different salts may be distributed over it. 

“[The VLT] has allowed us to carry out detailed mapping of Europa and Ganymede, observing features on their surfaces smaller than 150 kilometers [90 miles] across — all at distances over 600 million kilometers [370 million miles] from the Earth,” King said. “Mapping at this fine scale was previously only possible by sending spacecraft all the way to Jupiter to observe the moons up close.”

This research doesn’t mean that future missions to these moons are off the table, however. On the contrary, this mapping of Europa and Ganymede makes the prospect of these spacecraft missions even more enticing. 

Setting the scene for future exploration 

Leigh Fletcher supervised the VLT investigation of Europa and Ganymede and is also a member of the science teams for ESA’s Jupiter Icy Moons Explorer (JUICE) and NASA’s Europa Clipper mission, each set to explore these Jovian moons in the early 2030s. 

The missions will begin when JUICE launches in 2023 to study Europa and Ganymede, as well as a third Jovian moon, Callisto, plus the gas giant’s atmosphere and magnetic field.  

“These ground-based observations whet the appetite for our future exploration of Jupiter’s moons,” Fletcher said. “Planetary missions operate under tough operating constraints and we simply can’t cover all the terrain that we’d like to, so difficult decisions must be taken about which areas of the moons’ surfaces deserve the closest scrutiny.” Now, those decisions can incorporate additional context. 

NASA’s Europa Clipper mission will follow JUICE to the launch pad in 2024 and will focus on determining whether the ocean hiding below the moon’s icy surface has conditions favorable to life. Unlike JUICE, Europa Clipper will keep its focus firmly on Europa, analyzing both the internal ocean and the dynamics of the ice shell.

The team’s work is published in two separate papers; the Europa research is detailed in The Planetary Science Journal and the team’s Ganymede findings are discussed in a paper accepted for publication in the journal JGR: Planets and currently available on preprint server ArXiv

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Sharpest Earth-Based Images of Jupiter’s Moons Europa and Ganymede Reveal Their Icy Landscape

Jupiter’s moon Europa captured by ESO’s Very Large Telescope (VLT). Credit: ESO/King & Fletcher

The most detailed images ever taken of two of

Europa is named for a woman who, in Greek mythology, was abducted by the god Zeus – Jupiter in Roman mythology. It may be the most promising place in our solar system to find present-day environments suitable for some form of life beyond Earth. With an equatorial diameter of 1,940 miles, Europa is about 90 percent the size of Earth’s Moon. It orbits Jupiter every 3.5 days.

As some of the sharpest images of Jupiter’s moons ever acquired from a ground-based observatory, they reveal new insights into the processes shaping the chemical composition of these massive moons – including geological features such as the long rift-like linae cutting across Europa’s surface.

Ganymede and Europa are two of the four largest moons orbiting Jupiter, a quartet known as the Galilean satellites. While Europa is quite similar in size to our own Moon, Ganymede is the largest moon in the entire Solar System.

The Leicester team, led by PhD student Oliver King, used the European Southern Observatory’s

The new observations recorded the amount of sunlight reflected from Europa and Ganymede’s surfaces at different infrared wavelengths, producing a reflectance spectrum. These reflectance spectra are analyzed by developing a computer model that compares each observed spectrum to spectra of different substances that have been measured in laboratories.

The images and spectra of Europa, published in the Planetary Science Journal, reveal that Europa’s crust is mainly composed of frozen water ice with non-ice materials contaminating the surface.

Jupiter’s moon Ganymede captured by ESO’s Very Large Telescope (VLT). Credit: ESO/King & Fletcher

Oliver King from the University of Leicester School of Physics and Astronomy said: “We mapped the distributions of the different materials on the surface, including sulphuric

“The modeling found that there could be a variety of different salts present on the surface, but suggested that infrared spectroscopy alone is generally unable to identify which specific types of salt are present.”

Ganymede is not only Jupiter’s largest moon, but the largest moon in our solar system. In fact, it is bigger than the planet Mercury and the dwarf planet

Oliver King adds: “This has allowed us to carry out detailed mapping of Europa and Ganymede, observing features on their surfaces smaller than 150 km across – all at distances over 600 million kilometers from the Earth. Mapping at this fine scale was previously only possible by sending spacecraft all the way to Jupiter to observe the moons up-close.”

Professor Leigh Fletcher, who supervised the VLT study, is a member of the science teams for ESA’s Jupiter Icy Moons Explorer (JUICE) and NASA’s Europa Clipper mission, which will explore Ganymede and Europa up close in the early 2030s. JUICE is scheduled to launch in 2023, and University of Leicester scientists play key roles in its proposed study of Jupiter’s atmosphere, magnetosphere, and moons.

Professor Fletcher said: “These ground-based observations whet the appetite for our future exploration of Jupiter’s moons.”

“Planetary missions operate under tough operating constraints and we simply can’t cover all the terrain that we’d like to, so difficult decisions must be taken about which areas of the moons’ surfaces deserve the closest scrutiny. Observations at 150-km scale such as those provided by the VLT, and ultimately its enormous successor the ELT (Extremely Large Telescope), help to provide a global context for the spacecraft observations.”

References:

“Global Modelling of Ganymede’s Surface Composition: Near-IR Mapping from VLT/SPHERE” by Oliver King and Leigh N. Fletcher, Accepted, JGR: Planets.
arXiv:2209.01976

“Compositional mapping of Europa using MCMC modelling of Near-IR VLT/SPHERE and Galileo/NIMS observations” by Oliver King, Leigh N. Fletcher and Nicolas Ligier (2022), 31 March 2022, Planetary Science Journal.
DOI: 10.3847/PSJ/ac596d

This work was funded by a Royal Society Enhancement Award number 180071 to Professor Leigh Fletcher in the School of Physics and Astronomy, entitled “The diversity of Jupiter’s Galilean moons: Earth-based pathfinder observations in preparation for JUICE.”



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Sharpest Earth-based images of Europa and Ganymede reveal their icy landscapes

Europa. Credit:ESO/King & Fletcher

The cocktail of chemicals that make up the frozen surfaces on two of Jupiter’s largest moons are revealed in the most detailed images ever taken of them by a telescope on Earth.

Planetary scientists from the University of Leicester’s School of Physics and Astronomy have unveiled new images of Europa and Ganymede, two future destinations for exciting new missions to the Jovian system.

Some of the sharpest images of Jupiter’s moons ever acquired from a ground-based observatory, they reveal new insights into the processes shaping the chemical composition of these massive moons—including geological features such as the long rift-like linae cutting across Europa’s surface.

Ganymede and Europa are two of the four largest moons orbiting Jupiter, known as the Galilean moons. Whilst Europa is quite similar in size to our own Moon, Ganymede is the largest moon in the whole Solar System.

The Leicester team, led by Ph.D. student Oliver King, used the European Southern Observatory’s Very Large Telescope (VLT) in Chile to observe and map the surfaces of these two worlds.

The new observations recorded the amount sunlight reflected from Europa and Ganymede’s surfaces at different infrared wavelengths, producing a reflectance spectrum. These reflectance spectra are analyzed by developing a computer model that compares each observed spectrum to spectra of different substances that have been measured in laboratories.

The images and spectra of Europa, published in the Planetary Science Journal, reveal that Europa’s crust is mainly composed of frozen water ice with non-ice materials contaminating the surface.

Oliver King from the University of Leicester School of Physics and Astronomy says that they “mapped the distributions of the different materials on the surface, including sulfuric acid frost which is mainly found on the side of Europa that is most heavily bombarded by the gases surrounding Jupiter.”

Ganymede. Credit: ESO/King & Fletcher

“The modeling found that there could be a variety of different salts present on the surface, but suggested that infrared spectroscopy alone is generally unable to identify which specific types of salt are present.”

The observations of Ganymede, published in the journal JGR: Planets, show how the surface is made up to two main types of terrain: young areas with large amounts of water ice, and ancient areas mainly consisting of a dark gray material, the composition of which is unknown.

The icy areas (blue in the images) include Ganymede’s polar caps and craters—where an impact event has exposed the fresh clean ice of Ganymede’s crust. The team mapped how the size of the grains of ice on Ganymede varies across the surface and the possible distributions of a variety of different salts, some of which may originate from within Ganymede itself.

Located at high altitude in northern Chile, and with mirrors over 8 meters across, the Very Large Telescope is one of the most powerful telescope facilities in the world.

Oliver King adds that “this has allowed us to carry out detailed mapping of Europa and Ganymede, observing features on their surfaces smaller than 150 km across—all at distances over 600 million kilometers from the Earth. Mapping at this fine scale was previously only possible by sending spacecraft all the way to Jupiter to observe the moons up-close.”

Professor Leigh Fletcher, who supervised the VLT study, is a member of the science teams for ESA’s Jupiter Icy Moons Explorer (JUICE) and NASA’s Europa Clipper mission, which will explore Ganymede and Europa up close in the early 2030s. JUICE is scheduled to launch in 2023, and University of Leicester scientists play key roles in its proposed study of Jupiter’s atmosphere, magnetosphere, and moons.

Professor Fletcher says that “these ground-based observations whet the appetite for our future exploration of Jupiter’s moons.”

“Planetary missions operate under tough operating constraints and we simply can’t cover all the terrain that we’d like to, so difficult decisions must be taken about which areas of the moons’ surfaces deserve the closest scrutiny. Observations at 150-km scale such as those provided by the VLT, and ultimately its enormous successor the ELT (Extremely Large Telescope), help to provide a global context for the spacecraft observations.”


Hubble finds evidence of persistent water vapor in one hemisphere of Europa


More information:
Oliver King et al, Compositional Mapping of Europa Using MCMC Modeling of Near-IR VLT/SPHERE and Galileo/NIMS Observations, The Planetary Science Journal (2022). DOI: 10.3847/PSJ/ac596d

Oliver King et al, Global Modeling of Ganymede’s Surface Composition: Near-IR Mapping from VLT/SPHERE, JGR: Planets (2022). doi.org/10.1029/2022JE007323

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University of Leicester

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Ganymede Casts a Massive Shadow Across Jupiter in Spectacular New Image From NASA’s Juno Spacecraft

Figure 1. Citizen scientist Thomas Thomopoulos created this enhanced-color image using raw data from the JunoCam instrument. At the time the raw image was taken, the Juno spacecraft was about 44,000 miles (71,000 kilometers) above Jupiter’s cloud tops, at a latitude of about 55 degrees south, and 15 times closer than Ganymede, which orbits about 666,000 miles (1.1 million kilometers) away from Jupiter. Credit: NASA/JPL-Caltech/SwRI/MSSS, Image processing by Thomas Thomopoulos © CC BY

An observer at Jupiter’s cloud tops within the oval shadow would experience a total eclipse of the Sun. Total eclipses are more common on Jupiter than Earth for several reasons. Jupiter has four major moons (Galilean satellites) that often pass between Jupiter and the Sun: in seven days, Ganymede transits once; Europa, twice; and Io, four times. And since Jupiter’s moons orbit in a plane close to Jupiter’s orbital plane, the moon shadows are often cast upon the planet.

Figure 2. Illustration of the approximate geometry of the Ganymede’s shadow projected onto a globe of Jupiter.
Credit: NASA/JPL-Caltech/SwRI/MSSS, Image processing by Brian Swift © CC BY

JunoCam captured this image from very close to Jupiter, making Ganymede’s shadow appear especially large. Figure 2, created by citizen scientist Brian Swift using JunoCam data, illustrates the approximate geometry of the visible area, projected onto a globe of Jupiter.

JunoCam’s raw images are available for the public to peruse and process into image products at https://missionjuno.swri.edu/junocam/processing.

Jupiter is the largest planet in the Solar System and the fifth planet from the Sun. It is a gas giant with a mass that is more than two and a half times that of all the other planets in the Solar System combined, but is only about one-thousandth the mass of the Sun. Jupiter, behind the Moon and



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NASA probe snaps stunning photos of crescent Jupiter and its moon Ganymede

Data captured by NASA’s Juno spacecraft is revealing incredible new images of Jupiter and its moon Ganymede.

In a blog post on Monday (Feb. 14), Juno mission team members shared images of a huge crater on Ganymede as well as a backlit picture of Jupiter that the spacecraft captured during its dips in and out of Jupiter’s radiation-filled environment. 

“If you could ride along with NASA’s Juno spacecraft as it approaches Jupiter during one of its regular close passes by the giant planet, you would be treated to a striking vista similar to this one,” the website stated about the Jupiter images.

In photos: NASA’s Juno Mission to Jupiter

Dark rays of ejecta surround crater Kittu on Ganymede, in this Juno image. (Image credit: ASA/JPL-Caltech/SwRI/MSSS. Image processing by Thomas Thomopoulos © CC BY)

The image of Ganymede (above) was captured during a June 2021 pass when Juno flew only 650 miles (1,046 kilometers) above Ganymede’s surface. Citizen scientist Thomas Thomopoulos created this enhanced-color image using data from the JunoCam camera.

The image shows the large crater Kittu, which is roughly 9 miles (15 kilometers) across and has darker material surrounding it that ejected when a small asteroid crashed into the surface. 

“Most of Ganymede’s craters have bright rays extending from the impact scar, but about one percent of the craters have dark rays,” the blog post stated. 

“Scientists believe that contamination from the impactor produced the dark rays,” the post added. “As time passes, the rays stay dark because they are a bit warmer than the surroundings, so ice is driven off to condense on nearby colder, brighter terrain.”

A backlit image of Jupiter captured by Juno. (Image credit: NASA/JPL-Caltech/SwRI/MSSS Image processing by Kevin M. Gill © CC BY­­)

Gill created the backlit image of Jupiter (above) using raw data from the JunoCam instrument, including seven images taken by Juno’s 39th close pass of Jupiter on Jan. 12. 

NASA noted that this view of Jupiter is impossible from Earth, even in a telescope, because Jupiter’s orbit is always outside Earth’s and thus is only visible (from our planet) in full illumination from the sun.

Follow Elizabeth Howell on Twitter @howellspace. Follow us on Twitter @Spacedotcom and on Facebook



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NASA Releases Ghostly Sounds Recorded at Ganymede by The Juno Probe

In another context, Jupiter’s moon Ganymede might have been a planet.

As the largest moon in our Solar System, it’s one of the most intriguing locations in the neighborhood. Which is great, because it just so happens that Jupiter probe Juno is in the vicinity. Now, it’s sent back some curious noises. 

 

On 7 June 2021, Juno conducted a close flyby of Ganymede, and recorded the moon’s electromagnetic waves – electric and magnetic waves produced in the magnetosphere – with its Waves instrument.

When the frequency of these emissions is shifted into the audio range, the result is a wonderfully eerie set of alien shrieks and howls. This audio was unveiled at the American Geophysical Union Fall Meeting 2021.

“This soundtrack is just wild enough to make you feel as if you were riding along as Juno sails past Ganymede for the first time in more than two decades,” says physicist Scott Bolton of the Southwest Research Institute, Juno’s principal investigator.

“If you listen closely, you can hear the abrupt change to higher frequencies around the midpoint of the recording, which represents entry into a different region in Ganymede’s magnetosphere.”

Transposing the data into audio frequencies isn’t just for fun; it’s a different way of accessing and experiencing the data, which can in turn help to pick up on fine details that otherwise might have been overlooked. We’ve been recording the “sounds” of the Solar System with a range of probes, including the Voyager spacecraft, as well as planetary missions.

Ganymede – which is even bigger than Mercury – has a fully differentiated core, and might have a liquid ocean deep beneath its icy crust that could support life. On top of all that, it has its own magnetic field, the only one of the Solar System’s moons to have one.

 

The Galileo spacecraft, which studied Jupiter in the 1990s and early 2000s, also sampled the space around Ganymede, leading to the revelation that plasma waves are a million times stronger around the moon than the median activity at corresponding distances around Jupiter. It’s unclear whether that has anything to do with the moon’s magnetic field, but it seems likely.

Juno flew down as low as 1,038 kilometers (645 miles) from the moon’s surface, at a relative velocity of 67,000 kilometers per hour (41,600 mph). What the new data will reveal is a work in progress, but scientists already have a few ideas.

“It is possible the change in the frequency shortly after closest approach is due to passing from the nightside to the dayside of Ganymede,” says physicist and astronomer William Kurth of the University of Iowa.

Of course, the new discoveries were not confined to Ganymede. Juno has also been busily taking observations of Jupiter, obtaining the most detailed map yet of the gas giant’s magnetic field. This map has taken 32 orbits to compile, and has provided new insights into the equatorial magnetic anomaly known as the Great Blue Spot.

 

The data suggest Jupiter’s magnetic field has undergone a change in the last five years, and that the Great Blue Spot, being pulled apart by the powerful Jovian winds, is moving eastward at four centimeters per second relative to the rest of the planet’s interior. This suggests it completes a lap every 350 years.

Because a planetary magnetosphere is produced by a dynamo in the planet’s interior – a rotating, convecting, and electrically conducting fluid that converts kinetic energy into magnetic energy – studying a magnetic field allows scientists to understand that dynamo. The team’s new map suggests Jupiter’s dynamo is generated by a deep layer of metallic hydrogen surrounding its core.

Scientists also studied the Juno data to understand turbulence in the Jovian atmosphere. The similarity of this turbulence to the turbulence of phytoplankton in Earth’s oceans led oceanographer Lia Siegelman of Scripps Institution of Oceanography to try and connect the dots. She learnt that, on Jupiter, patterns of vortices form spontaneously and will hang around long-term.

(NASA OBPG OB.DAAC/GSFC/Aqua/MODIS/NASA/JPL/SwRI/MSSS/Gerald Eichstädt)

Above: Plankton bloom on Earth compared to the clouds of Jupiter.

Finally, the researchers unveiled a new photo of something rarely seen: Jupiter’s tenuous main dust ring, associated with dust released by its moons Metis and Adrastea. Juno imaged the structure from inside the ring, looking out into the stars, capturing the arm of the constellation Perseus.

Jupiter’s ring. (NASA/JPL-Caltech)

“It is breathtaking that we can gaze at these familiar constellations from a spacecraft a half-billion miles away,” says astronomer Heidi Becker of NASA’s Jet Propulsion Laboratory.

“But everything looks pretty much the same as when we appreciate them from our backyards here on Earth. It’s an awe-inspiring reminder of how small we are and how much there is left to explore.”

Juno’s extended mission will run until June 2025, and is expected to continue to provide amazing insights into our Solar System’s complex, weird and wonderful colossus, Jupiter.

The results were presented at the AGU Fall Meeting 2021.

 

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NASA Debuts Audio of What Jupiter’s Ganymede Moon Sounds Like

Imagining Ganymede, Jupiter’s icy moon and the largest moon in our Solar System, can be quite the challenge. (I’m still at, “Whoa, that’s a big moon.”) Understanding it is a whole other story, and scientists are still working on that. Whether you’re seeking to learn more about the gigantic moon or unravel its scientific mysteries, you now “listen” to what Ganymede sounds like in space.

NASA’s Jet Propulsion Laboratory on Friday published the 50-second audio track, which you can listen to below, created with data captured by the Juno spacecraft during its close flyby of Ganymede on June 7. Data for the recording was gathered with Juno’s Waves instrument, which measures electric and magnetic waves produced in Jupiter’s magnetosphere. NASA then proceeded to shift the frequency of the collected emissions into the audio range to make the audio track.

Scott Bolton, a principal investigator on the Juno mission from the Southwest Research Institute in San Antonio, presented the recording at the fall meeting of the American Geophysical Union. Launched in 2011, the Juno mission aims to advance our understanding of how giant planets form and the role they played in the creation of the Solar System.

“This soundtrack is just wild enough to make you feel as if you were riding along as Juno sails past Ganymede for the first time in more than two decades,” Bolton said in a NASA news article. “If you listen closely, you can hear the abrupt change to higher frequencies around the midpoint of the recording, which represents entry into a different region in Ganymede’s magnetosphere.”

Juno’s flyby of Ganymede occurred on its 34th trip around Jupiter and was the closest a spacecraft has ever gotten to the Solar System’s largest moon, which is bigger than the planet Mercury, since the Galileo spacecraft’s approach in 2000.

The spacecraft managed to get within 645 miles (1,038 kilometers) of Ganymede’s surface while traveling at a velocity of 41,600 mph (67,000 kph).

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Listen to the ‘sound’ of Jupiter’s moon Ganymede thanks to the Juno probe

You’d think moons would be quiet compared to their host planets, but that’s not entirely true — if you know how to listen. The principal investigator for NASA’s Juno mission, Scott Bolton, has produced an audio recording of magnetic field activity around Jupiter’s moon Ganymede as the Juno spacecraft flew past on June 7th, 2021. The 50-second clip reveals a sharp change in activity as the probe entered a different part of Ganymede’s magnetosphere, possibly as it left the night side to enter the daylight.

The audio came from shifting electric and magnetic frequencies into the audible range. Jupiter’s magnetosphere dominates that of its moons and is present in the recording, but Ganymede is the only moon in the Solar System to have a magnetic field (likely due to its liquid iron core). This isn’t a feat you could replicate elsewhere in the near future.

The soundtrack was part of a larger Juno briefing where the mission team revealed the most detailed map yet of Jupiter’s magnetic field. The data showed how long it would take the Great Red Spot and the equatorial Great Blue Spot to move around the planet (roughly 4.5 years and 350 years respectively). The findings also showed that east-west jetstreams are ripping the Great Blue Spot apart, and that polar cyclones behave much like ocean vortices on Earth.

You wouldn’t hear these sounds if you could visit Ganymede yourself. However, they’re a reminder that even seemingly dead worlds are frequently brimming with activity you can detect using the right instruments. It’s just a question of how easy it is to notice that activity.

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NASA’s Juno Spacecraft “Hears” Jupiter’s Moon Ganymede – Listen to the Dramatic Flyby of the Icy Orb

This JunoCam image shows two of Jupiter’s large rotating storms, captured on Juno’s 38th perijove pass, on November 29, 2021. Credit: NASA/JPL-Caltech/SwRI/MSSS Image processing: Kevin M. Gill CC BY

An audio track collected during
Radio emissions collected during Juno’s June 7, 2021, flyby of Jupiter’s moon Ganymede are presented here, both visually and in sound. Credit: NASA/

This image of the Jovian moon Ganymede was obtained by the JunoCam imager aboard NASA’s Juno spacecraft during its June 7, 2021, flyby of the icy moon. Credit: NASA/JPL-Caltech/SwRI/MSSS

In contrast, the Great Red Spot – the long-lived atmospheric anticyclone just south of Jupiter’s equator – is drifting westward at a relatively rapid clip, circling the planet in about four-and-a-half years.

In addition, the new map shows that Jupiter’s zonal winds (jet streams that run east to west and west to east, giving Jupiter’s its distinctive banded appearance) are pulling the Great Blue Spot apart. This means that the zonal winds measured on the surface of the planet reach deep into the planet’s interior.

The new magnetic field map also allows Juno scientists to make comparisons with Earth’s magnetic field. The data suggests to the team that dynamo action – the mechanism by which a celestial body generates a magnetic field – in Jupiter’s interior occurs in metallic hydrogen, beneath a layer expressing “helium rain.”

Data Juno collects during its extended mission may further unravel the mysteries of the dynamo effect not only at Jupiter but those of other planets, including Earth.

Earth’s Oceans, Jupiter’s Atmosphere

Lia Siegelman, a physical oceanographer and postdoctoral fellow at Scripps Institution of Oceanography at the University of California, San Diego, decided to study the dynamics of Jupiter’s atmosphere after noticing that the cyclones at Jupiter’s pole appear to share similarities with ocean vortices she studied during her time as a doctoral student.

“When I saw the richness of the turbulence around the Jovian cyclones, with all the filaments and smaller eddies, it reminded me of the turbulence you see in the ocean around eddies,” said Siegelman. “These are especially evident in high-resolution satellite images of vortices in Earth’s oceans that are revealed by plankton blooms that act as tracers of the flow.”

The simplified model of Jupiter’s pole shows that geometric patterns of vortices, like those observed on Jupiter, spontaneously emerge, and survive forever. This means that the basic geometrical configuration of the planet allows these intriguing structures to form.

Although Jupiter’s energy system is on a scale much larger than Earth’s, understanding the dynamics of the Jovian atmosphere could help us understand the physical mechanisms at play on our own planet.

Arming Perseus

The Juno team has also released its latest image of Jupiter’s faint dust ring, taken from inside the ring looking out by the spacecraft’s Stellar Reference Unit navigation camera. The brightest of the thin bands and neighboring dark regions scene in the image are linked to dust generated by two of Jupiter’s small moons, Metis and Adrastea. The image also captures the arm of the constellation Perseus.

“It is breathtaking that we can gaze at these familiar constellations from a spacecraft a half-billion miles away,” said Heidi Becker, lead co-investigator of Juno’s Stellar Reference Unit instrument at NASA’s Jet Propulsion Laboratory in Pasadena. “But everything looks pretty much the same as when we appreciate them from our backyards here on Earth. It’s an awe-inspiring reminder of how small we are and how much there is left to explore.”

This artist’s rendering shows Juno above Jupiter’s north pole, with the auroras glowing brightly. Jupiter’s magnetic field surrounds the planet. A radio wave from the auroras is shown traveling past the spacecraft, where it is intercepted by the Waves investigation, whose sensors are highlighted in bright green. Credit: NASA

Juno Waves

The Waves instrument measures radio and (function(d, s, id){ var js, fjs = d.getElementsByTagName(s)[0]; if (d.getElementById(id)) return; js = d.createElement(s); js.id = id; js.src = "https://connect.facebook.net/en_US/sdk.js#xfbml=1&version=v2.6"; fjs.parentNode.insertBefore(js, fjs); }(document, 'script', 'facebook-jssdk'));

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Juno flyby reveals stunning new images of Jupiter, sounds of its moon Ganymede

The NASA Juno mission, which began orbiting Jupiter in July 2016, just recently made its 38th close flyby of the gas giant. The mission was extended earlier this year, adding on a flyby of Jupiter’s moon Ganymede in June.

The data and images from these flybys is rewriting everything we know about Jupiter, said Scott Bolton, Juno principal investigator at the Southwest Research Institute in San Antonio, during a briefing at the American Geophysical Union Fall Meeting in New Orleans on Friday.

There, Bolton revealed 50 seconds of sound created when Juno flew by Ganymede over the summer. The clip of the moon’s audio was created by electric and magnetic radio waves produced by the planet’s magnetic field and picked up by the spacecraft’s Waves instrument, designed to detect these waves. The sounds are like a trippy space age soundtrack.

“This soundtrack is just wild enough to make you feel as if you were riding along as Juno sails past Ganymede for the first time in more than two decades,” Bolton said. “If you listen closely, you can hear the abrupt change to higher frequencies around the midpoint of the recording, which represents entry into a different region in Ganymede’s magnetosphere.”

The Juno team continues to analyze the data from the Ganymede flyby. At the time, Juno was about 645 miles (1,038 kilometers) from the moon’s surface and zipping by at 41,600 mph (67,000 kilometers per hour).

“It is possible the change in the frequency shortly after closest approach is due to passing from the nightside to the dayside of Ganymede,” said William Kurth, lead co-investigator of the Waves instrument, who is based at the University of Iowa in Iowa City, in a statement.

The team also shared stunning new images that resemble artistic views of Jupiter’s swirling atmosphere.

“You can see how incredibly beautiful Jupiter is,” Bolton said. “It’s really an artist’s palette. This is almost like a Van Gogh painting. You see these incredible vortices and swirling clouds of different colors.”

These visually stunning images serve to help scientists better understand Jupiter and its many mysteries. Images of cyclones at Jupiter’s poles intrigued Lia Siegelman, a scientist working with the Juno team who typically studies Earth’s oceans. She saw similarities between Jupiter’s atmospheric dynamics and vortices in Earth’s oceans.

“When I saw the richness of the turbulence around the Jovian cyclones, with all the filaments and smaller eddies, it reminded me of the turbulence you see in the ocean around eddies,” said Siegelman, a physical oceanographer and postdoctoral fellow at Scripps Institution of Oceanography at the University of California, San Diego, in a statement.

“These are especially evident in high-resolution satellite images of vortices in Earth’s oceans that are revealed by plankton blooms that act as tracers of the flow.”

Mapping Jupiter’s magnetic field

Data from Juno is also helping scientists to map Jupiter’s magnetic field, including the Great Blue Spot. This region is a magnetic anomaly located at Jupiter’s equator — not to be confused with the Great Red Spot, a centuries-long atmospheric storm south of the equator.

Since Juno’s arrival at Jupiter, the team has witnessed a change in Jupiter’s magnetic field. The Great Blue Spot is moving eastward about 2 inches (5.1 centimeters) per second and will complete a lap around the planet in 350 years.

Meanwhile, the Great Red Spot is moving westward and will cross that finish line much quicker, in about 4.5 years.

But the Great Blue Spot is being pulled apart by Jupiter’s jet streams, which give it a striped appearance. This visual pattern tells scientists that these winds extend down much deeper into the planet’s gaseous interior.

The map of Jupiter’s magnetic field, generated by Juno data, also revealed that the planet’s dynamo action, which creates the magnetic field from Jupiter’s interior, originates from metallic hydrogen beneath a layer of “helium rain.”

Juno was also able to take a look at the very faint ring of dust around Jupiter from inside the ring. This dust is actually created by two of the planet’s small moons, named Metis and Adrastea. The observations allowed the researchers to see part of the Perseus constellation from a different planetary perspective.

“It is breathtaking that we can gaze at these familiar constellations from a spacecraft a half-billion miles away,” said Heidi Becker, lead co-investigator of Juno’s Stellar Reference Unit instrument at NASA’s Jet Propulsion Laboratory in Pasadena, California, in a statement.

“But everything looks pretty much the same as when we appreciate them from our backyards here on Earth. It’s an awe-inspiring reminder of how small we are and how much there is left to explore.”

In the fall of 2022, Jupiter will fly by Jupiter’s moon Europa, which will be visited by its own mission, the Europa Clipper, set to launch in 2024. Europa intrigues scientists because a global ocean is located beneath its ice shell. Occasionally, plumes eject from holes in the ice out into space. Europa Clipper could investigate this ocean by “tasting” and flying through the plumes — and learn if life is possible on this ocean world.

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