Jupiter’s moon Io is the most volcanically active world in our solar system. The energy that drives its geological activity comes from tidal forces the moon experiences from Jupiter and from other Jovian moons. These forces flex the moon and heat its interior via friction. Previous models of Io’s tidal heating assumed a solid body, but their results predicted volcanoes in locations that did not match observations of the moon. A new study suggests that the missing piece of the puzzle is a subsurface ocean of magma. Highly viscous liquids like magma also generate heat when deformed by tidal forces, and applying this model to Io allowed scientists to better match the volcano distribution actually seen on the world. For more, check out NASA’s article. (Image credit: NASA; via Gizmodo; submitted by jshoer)
Tag: Jupiter
Jovian Dynamics
Our solar system’s largest planet is a mysterious and majestic font of fluid dynamics. Unlike rocky Earth, Jupiter is made entirely of fluids. Beneath its massive gaseous atmosphere lies an ocean of liquid hydrogen. The lack of solid ground to weaken storms may explain some of the longevity of Jupiter’s Great Red Spot, a hurricane that’s been raging on the planet for more than a hundred and fifty years. Part of the challenge of understanding Jupiter’s dynamics is that most of our data consists of observations of the uppermost layer of the atmosphere. It’s kind of like trying to describe an entire ocean based on the surface alone; what we see is part of the story, but it’s only a small portion of a much greater whole. (Image credit: NASA; submitted by jshoer)
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Jupiter Timelapse
This timelapse video shows Jupiter as seen by Voyager 1. In it, each second corresponds to approximately 1 Jupiter day, or 10 Earth hours. Be sure to fullscreen it so that you can appreciate the details. The timelapse highlights the differences in velocity (and even flow direction!) between Jupiter’s cloud bands. It is these velocity differences that create the shear forces which cause Kelvin-Helmholtz instabilities–the series of overturning eddies–seen between the bands. Earth also has bands of winds moving in opposite directions, but there are fewer of them and the composition of our atmosphere is such that they do not make for such a dramatic naked eye view of large-scale fluid dynamics. (Video credit: NASA/JPL/B. Jónsson/I. Regan)
Shrinking Red Spot
Observations show Jupiter’s iconic Great Red Spot is shrinking, most recently at a rate of more than 900 km a year. As it gets smaller, the storm is also changing shape and becoming more circular. Scientists don’t yet have an explanation for the shrinkage or its recent acceleration, but this is unsurprising given the rich complexity of the storm. For example, the source of the Red Spot’s longevity–it may be more than 300 years old–is still an open topic of research. Some of the most recent observations show smaller eddies feeding into the storm; the current hypothesis is that these eddies may be increasing the Red Spot’s dissipation and accelerating its breakup. (Photo credit: NASA/ESA; h/t to io9)
Fluids Round-up – 7 December 2013
Fluids round-up time! I missed out last weekend because of the holidays, so this is a long list of links. There’s a lot of really great stuff here, including some neat fluidsy geophysics and astronomy.
- xkcd’s Randall Munroe explains why you can’t boil your tea by stirring it.
- LATimes describes a flying jellyfish robot.
- Wired takes a detailed look at archerfish physics, including some of the fluid dynamics we’ve discussed previously. (via iamaponyrocket)
- Several readers have also pointed out this ASCII CFD simulator, seen in action in this video.
- New models suggest that Europa’s chaotic terrain features may be due to turbulence in its lower latitudes.
- In a similar vein, nearby Jupiter’s Great Red Spot may owe its longevity to existing in three-dimensions.
- NASA revealed new movies and images of Saturn’s polar hexagon this week. For more, see some of the earlier photos and laboratory recreations of the hexagon and this summary from io9. (submitted by @AndrisPiebalgs)
- Continuing with the astronomical bent, check out Anders Sandberg’s musings on what a habitable planet twice the size of Earth would be like.
- Back here on Earth, NASA released some impressive images of global weather patterns as computed by their high-resolution models.
- PhysicsBuzz takes a look at the fluid dynamics of flying fish.
- I’ve seen plenty of videos of people doing crazy things with non-Newtonian fluids, but Hard Science adds an interesting new one: attempting to ride a bike across a pool of oobleck.
- PopSci reported from CES 2013 about a non-Newtonian fluid for protecting tech gadgets from impacts.
- Drummer Ali Siadat shows how to blow the perfect smoke rings using a bass drum. (via Jennifer Ouellette)
- Finally, this week’s lead image comes from the Grand Canyon where a strong temperature inversion created spectacular fog-filled vistas.
(Photo credit: E. Whittaker)
The Beauty of the Great Red Spot
Jupiter is home to one of the most famous storms in the solar system, the Great Red Spot, which Earth observations place at a minimum of 180 (Earth) years in duration. Some evidence suggests that it may have been observed by humans as early as 1665. The magnitude of such a storm is almost unimaginable. At its narrowest point, the storm is still as wide as our entire planet and observations from the Voyager crafts indicate that the storm has 250 mph winds. The scale of mixing and turbulence around the storm, seen in photographs, is stunning and beautiful. (Photo credits: NASA/Voyager 1 and Michael Benson; submitted by oneheadtoanother)
The Cloud Bands of Jupiter
The cloud bands of Jupiter stripe the planet with turbulence. Throughout its upper atmosphere, Jupiter shows signs of gravity waves and complicated wave patterns. Near the equator, the cloud bands are driven by planetary winds that reach speeds of 500 kph, whereas near the poles, the clouds show greater evidence of mottling and convection. At present, the reasons for this patterning are undetermined. (Image Credit: NASA; via APOD)
Portrait of Gas Giants
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Here raw footage from NASA’s Cassini and Voyager missions has been combined in a stunning portrait of Saturn and Jupiter. Watch as tiny moons create gravity waves in the rings of Saturn and observe the complicated relative motion between the cloud bands on Jupiter and the swirls and vortices that result. Fluid dynamics are truly everywhere. (Video credit: Sander van den Berg; submitted by Daniel B)
Where Jupiter Got Its Swirls
When layers of a fluid are moving at different relative velocities, they shear against one another. This shear can trigger the Kelvin-Helmholtz instability, which develops as a waves along the interface. Here Hubble captures Kelvin-Helmholtz waves along the cloud bands of Jupiter, but such clouds are also not uncommon here on Earth. (Photo credit: J. Spencer and NASA)
Jovian Storms
Home to storms capable of lasting for a hundred years or more, Jupiter’s atmosphere is a highly turbulent place. Currently, no comprehensive theory exists to explain the symmetry of Jupiter’s bands of clouds and the persistence of vortices such as the Great Red Spot, however, the mixing and stratification visible on the planet remains a beautiful reminder of the power of fluid dynamics. (Photo credits:Cassini – 1, 2, Voyager 1, New Horizons – 1, 2)
