Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:

 

Extreme Volcanism: Image Captures one of the Brightest Volcanoes Ever Seen in the Solar System

05.08.2014

During the middle of 2013, Jupiter’s moon Io came alive with volcanism. Now, an image from the Gemini Observatory captures what is one of the brightest volcanoes ever seen in our solar system.

The image, obtained on August 29, reveals the magnitude of the eruption that was the “grand finale” in a series of eruptions on the distant moon. Io’s volcanism is caused by the tidal push-and-pull of massive Jupiter, which heats the satellite’s interior – making it our Solar System’s most volcanically active known body.


Figure 1. Image of Io taken in the near-infrared with adaptive optics at the Gemini North telescope on August 29. In addition to the extremely bright eruption on the upper right limb of the satellite, the lava lake Loki is visible in the middle of Io’s disk, as well as the fading eruption that was detected earlier in the month by de Pater on the southern (bottom) limb. Io is about one arcsecond across. Image credit: Katherine de Kleer/UC Berkeley/Gemini Observatory/AURA


Figure 2. Images of Io taken in the near-infrared with adaptive optics at the Gemini North telescope tracking the evolution of the eruption as it decreased in intensity over 12 days. Due to Io’s rapid rotation, a different area of the surface is viewed on each night; the outburst is visible with diminishing brightness on August 29 & 30 and September 1, 3, & 10. Image credit: Katherine de Kleer/UC Berkeley/Gemini Observatory/AURA

According to University of California Berkeley (UCB) astronomer Katherine de Kleer, the Gemini observations, “… represent the best day-by-day coverage of such an eruption – thanks to Gemini’s rapid and flexible scheduling capabilities.” De Kleer, who led one of a pair of two papers published today in the journal Icarus, adds that the Gemini data allowed the team to monitor the evolution of the extreme volcanic activity over nearly the first two weeks of the eruption – which provided a critical new perspective on the outburst events.

De Kleer’s paper examines the powerful late-August eruption in detail, concluding that the energy emitted was about 20 Terawatts and expelled many cubic kilometers of lava. “At the time we observed the event, an area of newly-exposed lava on the order of tens of square kilometers was visible” says de Kleer. “We believe that it erupted in fountains from long fissures on Io’s surface, which were over ten-thousand-times more powerful than the lava fountains during the 2010 eruption of Eyjafjallajokull, Iceland, for example.”

The original detection of the volcano was made simultaneously at Gemini and NASA’s Infrared Telescope Facility (IRTF), and was the first of a series of observations monitoring Io at both facilities over the following year. These particular observations were timed to follow up on a different outburst eruption that was detected earlier in the month by Imke de Pater, also of UCB.

This record of the spate of activity began when de Pater first spotted a hotspot using the W.M. Keck Observatory in mid-August (see UCB press release, also released today at: http://newscenter.berkeley.edu/2014/08/04/a-hellacious-two-weeks-on-jupiters-moon-io/), which the team followed with further observations from Mauna Kea. The late August Gemini observations of the most extreme outburst (see Figure 1) used adaptive optics on the Gemini North telescope to produce this super-sharp near-infrared image. Gemini also recorded a series of images chronicling the massive eruption’s evolution as it faded over the next 12 days (see Figure 2).

In addition to de Kleer and de Pater, the lead authors on the two publications discussing these events, the research team included Máté Ádámkovics of UCB, Ashley Davies from the Jet Propulsion Laboratory and David Ciardi of Caltech's NASA Exoplanet Science Institute. The work is funded by the National Science Foundation and NASA’s Outer Planets Research and Planetary Geology and Geophysics Program.

The papers are available in the journal Icarus (subscription required).

The Gemini Observatory is an international collaboration with two identical 8-meter telescopes. The Frederick C. Gillett Gemini Telescope is located on Mauna Kea, Hawai'i (Gemini North) and the other telescope on Cerro Pachón in central Chile (Gemini South); together the twin telescopes provide full coverage over both hemispheres of the sky. The telescopes incorporate technologies that allow large, relatively thin mirrors, under active control, to collect and focus both visible and infrared radiation from space.The Gemini Observatory provides the astronomical communities in six partner countries with state-of-the-art astronomical facilities that allocate observing time in proportion to each country's contribution. In addition to financial support, each country also contributes significant scientific and technical resources. The national research agencies that form the Gemini partnership include: the US National Science Foundation (NSF), the Canadian National Research Council (NRC), the Chilean Comisión Nacional de Investigación Cientifica y Tecnológica (CONICYT), the Australian Research Council (ARC), the Argentinean Ministerio de Ciencia, Tecnología e Innovación Productiva, and the Brazilian Ministério da Ciência, Tecnologia e Inovação. The observatory is managed by the Association of Universities for Research in Astronomy, Inc. (AURA) under a cooperative agreement with the NSF. The NSF also serves as the executive agency for the international partnership.

Media Contacts:

Peter Michaud
Public Information and Outreach Manager
Gemini Observatory, Hilo, HI
Email: pmichaud"at"gemini.edu
Cell: (808) 936-6643
Desk: (808) 974-2510

Science Contacts:

Katherine de Kleer
University of California Berkeley
Email: kdekleer"at"berkeley.edu

Imke de Pater
University of California Berkeley
Email: imke"at"berkeley.edu

Peter Michaud | Eurek Alert!
Further information:
http://www.gemini.edu/node/12233

Further reports about: Gemini Icarus NSF Observatory Telescope UCB Volcanoes activity telescopes

More articles from Physics and Astronomy:

nachricht A New Litmus Test for Chaos?
29.07.2015 | American Institute of Physics (AIP)

nachricht First detection of lithium from an exploding star
29.07.2015 | ESO

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: On the crest of the wave: Electronics on a time scale shorter than a cycle of light

Physicists from Regensburg and Marburg, Germany have succeeded in taking a slow-motion movie of speeding electrons in a solid driven by a strong light wave. In the process, they have unraveled a novel quantum phenomenon, which will be reported in the forthcoming edition of Nature.

The advent of ever faster electronics featuring clock rates up to the multiple-gigahertz range has revolutionized our day-to-day life. Researchers and...

Im Focus: Superfast fluorescence sets new speed record

Plasmonic device has speed and efficiency to serve optical computers

Researchers have developed an ultrafast light-emitting device that can flip on and off 90 billion times a second and could form the basis of optical computing.

Im Focus: Unlocking the rice immune system

Joint BioEnergy Institute study identifies bacterial protein that is key to protecting rice against bacterial blight

A bacterial signal that when recognized by rice plants enables the plants to resist a devastating blight disease has been identified by a multi-national team...

Im Focus: Smarter window materials can control light and energy

Researchers in the Cockrell School of Engineering at The University of Texas at Austin are one step closer to delivering smart windows with a new level of energy efficiency, engineering materials that allow windows to reveal light without transferring heat and, conversely, to block light while allowing heat transmission, as described in two new research papers.

By allowing indoor occupants to more precisely control the energy and sunlight passing through a window, the new materials could significantly reduce costs for...

Im Focus: Simulations lead to design of near-frictionless material

Argonne scientists used Mira to identify and improve a new mechanism for eliminating friction, which fed into the development of a hybrid material that exhibited superlubricity at the macroscale for the first time. Argonne Leadership Computing Facility (ALCF) researchers helped enable the groundbreaking simulations by overcoming a performance bottleneck that doubled the speed of the team's code.

While reviewing the simulation results of a promising new lubricant material, Argonne researcher Sanket Deshmukh stumbled upon a phenomenon that had never been...

All Focus news of the innovation-report >>>

Anzeige

Anzeige

Event News

3rd Euro Bio-inspired - International Conference and Exhibition on Bio-inspired Materials

23.07.2015 | Event News

Clash of Realities – International Conference on the Art, Technology and Theory of Digital Games

10.07.2015 | Event News

World Conference on Regenerative Medicine in Leipzig: Last chance to submit abstracts until 2 July

25.06.2015 | Event News

 
Latest News

Surprising similarity in fly and mouse motion vision

30.07.2015 | Life Sciences

Efficient Infrared Heat Saves Time and Energy in the Manufacture of Motor Vehicle Carpets

30.07.2015 | Trade Fair News

Roentgen prize goes to Dr Eleftherios Goulielmakis

30.07.2015 | Awards Funding

VideoLinks
B2B-VideoLinks
More VideoLinks >>>