ZME Science
No Result
View All Result
ZME Science
No Result
View All Result
ZME Science

Home → Space → Astrophysics

Saturn creates largest, hottest gas storm ever recorded in the Solar System

Mihai AndreibyMihai Andrei
October 26, 2012
in Astrophysics, Space
A A
Share on FacebookShare on TwitterSubmit to Reddit

The Cassini spacecraft recorded the aftermath of the largest, hottest gas vortex ever recorded in our solar system, making astrophysicists think there’s much more to Saturn’s atmosphere than meets the eye.

The Cassini-Huygens spacecraft (often just called Cassini) is a robotic ship sent out to monitor the Saturn system. It sent out surprising, valuable data not only from Saturn itself, but also from its many satellites (most notably Titan). This time, something truly remarkable caught its mechanical eye.

Not only was the storm of Gargantuan size (it could cover North America from top to bottom and go round the Earth many times), but what it was made of also baffled astronomers. The event was created when two warm spots on Saturn merged, and even though the result was invisible to the human eye, it was easily observed in infrared wavelength.

“This temperature spike is so extreme it’s almost unbelievable,” said Brigette Hesman, the study’s lead author who works at Goddard. “To get a temperature change of the same scale on Earth, you’d be going from the depths of winter in Fairbanks, Alaska, to the height of summer in the Mojave Desert,” Hesman said in a statement released by NASA.

All this action was caused by the “Great Springtime Storm” that raged on Saturn in 2010 and 2011. The storm was so huge that it actually reached its own tail at the other end of the planet, and created huge temperatures. Researchers believed the hype was over, but continued to study the aftermath.

What they found was that the two remaining warm spots refused to cool down and continued to roam the planet, getting closer and closer to each other – finally merging in a catastrophic event. Temperatures in the storm skyrocketed to 150 degrees Fahrenheit, and a huge amount of ethylene suddenly appeared. Ethylene is an odorless hydrocarbon not usually found on Saturn; the amount of released ethylene is 100 times more than scientists believed possible – and no one knows where the hydrocarbon comes from.

RelatedPosts

How climate change leads to more frequent thunderstorms
NASA plans to send an autonomous submarine into space — for a very good reason
Why does Jupiter lack a true ring structure?
Destruction of Saturn’s moon could have led to its famous rings

The storm is expected to cool down by 2013, but astronomers are reluctant to make any more predictions, as they expect Saturn to hold even more surprises. Goddard scientists describe the unprecedented belch of energy in a paper which will be published in the Nov. 20 issue of the Astrophysical Journal.

Source: NASA

Tags: ethylenesaturnstorm

ShareTweetShare
Mihai Andrei

Mihai Andrei

Dr. Andrei Mihai is a geophysicist and founder of ZME Science. He has a Ph.D. in geophysics and archaeology and has completed courses from prestigious universities (with programs ranging from climate and astronomy to chemistry and geology). He is passionate about making research more accessible to everyone and communicating news and features to a broad audience.

Related Posts

Climate

The Longest Lightning Flash Ever Recorded Stretched 829 Kilometers From Texas to Missouri

byTudor Tarita
2 weeks ago
News

NASA Astronaut Snaps Rare Sprite Flash From Space and It’s Blowing Minds

byTibi Puiu
1 month ago
News

Astronomers Discover 128 New Moons Around Saturn Securing Its Title as the Moon King and Leaving Jupiter in the Dust

byTibi Puiu
5 months ago
Astronomy

Titan’s seas look more and more like Earth’s — except they’re made of methane

byMihai Andrei
1 year ago

Recent news

The UK Government Says You Should Delete Emails to Save Water. That’s Dumb — and Hypocritical

August 16, 2025

In Denmark, a Vaccine Is Eliminating a Type of Cervical Cancer

August 16, 2025
This Picture of the Week shows a stunning spiral galaxy known as NGC 4945. This little corner of space, near the constellation of Centaurus and over 12 million light-years away, may seem peaceful at first — but NGC 4945 is locked in a violent struggle. At the very centre of nearly every galaxy is a supermassive black hole. Some, like the one at the centre of our own Milky Way, aren’t particularly hungry. But NGC 4945’s supermassive black hole is ravenous, consuming huge amounts of matter — and the MUSE instrument at ESO’s Very Large Telescope (VLT) has caught it playing with its food. This messy eater, contrary to a black hole’s typical all-consuming reputation, is blowing out powerful winds of material. This cone-shaped wind is shown in red in the inset, overlaid on a wider image captured with the MPG/ESO telescope at La Silla. In fact, this wind is moving so fast that it will end up escaping the galaxy altogether, lost to the void of intergalactic space. This is part of a new study that measured how winds move in several nearby galaxies. The MUSE observations show that these incredibly fast winds demonstrate a strange behaviour: they actually speed up far away from the central black hole, accelerating even more on their journey to the galactic outskirts. This process ejects potential star-forming material from a galaxy, suggesting that black holes control the fates of their host galaxies by dampening the stellar birth rate. It also shows that the more powerful black holes impede their own growth by removing the gas and dust they feed on, driving the whole system closer towards a sort of galactic equilibrium. Now, with these new results, we are one step closer to understanding the acceleration mechanism of the winds responsible for shaping the evolution of galaxies, and the history of the universe. Links  Research paper in Nature Astronomy by Marconcini et al. Close-up view of NGC 4945’s nucleus

Astronomers Find ‘Punctum,’ a Bizarre Space Object That Might be Unlike Anything in the Universe

August 15, 2025
  • About
  • Advertise
  • Editorial Policy
  • Privacy Policy and Terms of Use
  • How we review products
  • Contact

© 2007-2025 ZME Science - Not exactly rocket science. All Rights Reserved.

No Result
View All Result
  • Science News
  • Environment
  • Health
  • Space
  • Future
  • Features
    • Natural Sciences
    • Physics
      • Matter and Energy
      • Quantum Mechanics
      • Thermodynamics
    • Chemistry
      • Periodic Table
      • Applied Chemistry
      • Materials
      • Physical Chemistry
    • Biology
      • Anatomy
      • Biochemistry
      • Ecology
      • Genetics
      • Microbiology
      • Plants and Fungi
    • Geology and Paleontology
      • Planet Earth
      • Earth Dynamics
      • Rocks and Minerals
      • Volcanoes
      • Dinosaurs
      • Fossils
    • Animals
      • Mammals
      • Birds
      • Fish
      • Amphibians
      • Reptiles
      • Invertebrates
      • Pets
      • Conservation
      • Animal facts
    • Climate and Weather
      • Climate change
      • Weather and atmosphere
    • Health
      • Drugs
      • Diseases and Conditions
      • Human Body
      • Mind and Brain
      • Food and Nutrition
      • Wellness
    • History and Humanities
      • Anthropology
      • Archaeology
      • History
      • Economics
      • People
      • Sociology
    • Space & Astronomy
      • The Solar System
      • Sun
      • The Moon
      • Planets
      • Asteroids, meteors & comets
      • Astronomy
      • Astrophysics
      • Cosmology
      • Exoplanets & Alien Life
      • Spaceflight and Exploration
    • Technology
      • Computer Science & IT
      • Engineering
      • Inventions
      • Sustainability
      • Renewable Energy
      • Green Living
    • Culture
    • Resources
  • Videos
  • Reviews
  • About Us
    • About
    • The Team
    • Advertise
    • Contribute
    • Editorial policy
    • Privacy Policy
    • Contact

© 2007-2025 ZME Science - Not exactly rocket science. All Rights Reserved.