New findings from NASAs Juno probe orbiting Jupiter provide a fuller picture of how the planets distinctive and colorful atmospheric features offer clues about the unseen processes below its clouds. The results highlight the inner workings of the belts and zones of clouds encircling Jupiter, as well as its polar cyclones and even the Great Red Spot.
Researchers published several papers on Junos atmospheric discoveries today in the journal Science and the Journal of Geophysical Research: Planets. Additional papers appeared in two recent issues of Geophysical Research Letters.
These new observations from Juno open up a treasure chest of new information about Jupiters enigmatic observable features, said Lori Glaze, director of NASAs Planetary Science Division at the agencys headquarters in Washington. Each paper sheds light on different aspects of the planets atmospheric processes a wonderful example of how our internationally-diverse science teams strengthen understanding of our solar system.
Juno entered Jupiters orbit in 2016. During each of the spacecrafts 37 passes of the planet to date, a specialized suite of instruments has peered below its turbulent cloud deck.
Previously, Juno surprised us with hints that phenomena in Jupiters atmosphere went deeper than expected, said Scott Bolton, principal investigator of Juno from the Southwest Research Institute in San Antonio and lead author of the Journal Science paper on the depth of Jupiters vortices. Now, were starting to put all these individual pieces together and getting our first real understanding of how Jupiters beautiful and violent atmosphere works in 3D.
Junos microwave radiometer (MWR) allows mission scientists to peer beneath Jupiters cloud tops and probe the structure of its numerous vortex storms. The most famous of these storms is the iconic anticyclone known as the Great Red Spot. Wider than Earth, this crimson vortex has intrigued scientists since its discovery almost two centuries ago.
The new results show that the cyclones are warmer on top, with lower atmospheric densities, while they are colder at the bottom, with higher densities. Anticyclones, which rotate in the opposite direction, are colder at the top but warmer at the bottom.
The findings also indicate these storms are far taller than expected, with some extending 60 miles (100 kilometers) below the cloud tops and others, including the Great Red Spot, extending over 200 miles (350 kilometers). This surprise discovery demonstrates that the vortices cover regions beyond those where water condenses and clouds form, below the depth where sunlight warms the atmosphere.
The height and size of the Great Red Spot means the concentration of atmospheric mass within the storm potentially could be detectable by instruments studying Jupiters gravity field. Two close Juno flybys over Jupiters most famous spot provided the opportunity to search for the storms gravity signature and complement the MWR results on its depth.
With Juno traveling low over Jupiters cloud deck at about 130,000 mph (209,000 kph) Juno scientists were able to measure velocity changes as small 0.01 millimeter per second using a NASAs Deep Space Network tracking antenna, from a distance of more than 400 million miles (650 million kilometers). This enabled the team to constrain the depth of the Great Red Spot to about 300 miles (500 kilometers) below the cloud tops.
The precision required to get the Great Red Spots gravity during the July 2019 flyby is staggering, said Marzia Parisi, a Juno scientist from NASAs Jet Propulsion Laboratory in Southern California and lead author of a paper in the Journal Science on gravity overflights of the Great Red Spot. Being able to complement MWRs finding on the depth gives us great confidence that future gravity experiments at Jupiter will yield equally intriguing results.
Belts and Zones
In addition to cyclones and anticyclones, Jupiter is known for its distinctive belts and zones white and reddish bands of clouds that wrap around the planet. Strong east-west winds moving in opposite directions separate the bands. Juno previously discovered that these winds, or jet streams, reach depths of about 2,000 miles (roughly 3,200 kilometers). Researchers are still trying to solve the mystery of how the jet streams form. Data collected by Junos MWR during multiple passes reveal one possible clue: that the atmospheres ammonia gas travels up and down in remarkable alignment with the observed jet streams.
By following the ammonia, we found circulation cells in both the north and south hemispheres that are similar in nature to Ferrel cells, which control much of our climate here on Earth, said Keren Duer, a graduate student from the Weizmann Institute of Science in Israel and lead author of the Journal Science paper on Ferrel-like cells on Jupiter. While Earth has one Ferrel cell per hemisphere, Jupiter has eight each at least 30 times larger.
Junos MWR data also shows that the belts and zones undergo a transition around 40 miles (65 kilometers) beneath Jupiters water clouds. At shallow depths, Jupiters belts are brighter in microwave light than the neighboring zones. But at deeper levels, below the water clouds, the opposite is true which reveals a similarity to our oceans.
We are calling this level the Jovicline in analogy to a transitional layer seen in Earths oceans, known as the thermocline where seawater transitions sharply from being relative warm to relative cold, said Leigh Fletcher, a Juno participating scientist from the University of Leicester in the United Kingdom and lead author of the paper in the Journal of Geophysical Research: Planets highlighting Junos microwave observations of Jupiter’s temperate belts and zones.
Juno previously discovered polygonal arrangements of giant cyclonic storms at both of Jupiters poles eight arranged in an octagonal pattern in the north and five arranged in a pentagonal pattern in the south. Now, five years later, mission scientists using observations by the spacecrafts Jovian Infrared Auroral Mapper (JIRAM) have determined these atmospheric phenomena are extremely resilient, remaining in the same location.
Jupiters cyclones affect each others motion, causing them to oscillate about an equilibrium position, said Alessandro Mura, a Juno co-investigator at the National Institute for Astrophysics in Rome and lead author of a recent paper in Geophysical Research Letters on oscillations and stability in Jupiters polar cyclones. The behavior of these slow oscillations suggests that they have deep roots.
JIRAM data also indicates that, like hurricanes on Earth, these cyclones want to move poleward, but cyclones located at the center of each pole push them back. This balance explains where the cyclones reside and the different numbers at each pole.
More About the Mission
JPL, a division of Caltech in Pasadena, California, manages the Juno mission. Juno is part of NASAs New Frontiers Program, which is managed at NASAs Marshall Space Flight Center in Huntsville, Alabama, for the agencys Science Mission Directorate in Washington. Lockheed Martin Space in Denver built and operates the spacecraft.