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Topic: NASA’s Cassini Mission

NASA’s Cassini mission and Hubble Space Telescope provides new details about moons Enceladus and Europa

 

Written by Felicia Chou
NASA Headquarters

NASA - National Aeronautics and Space AdministrationWashington, D.C. – Two veteran NASA missions are providing new details about icy, ocean-bearing moons of Jupiter and Saturn, further heightening the scientific interest of these and other “ocean worlds” in our solar system and beyond. The findings are presented in papers published Thursday by researchers with NASA’s Cassini mission to Saturn and Hubble Space Telescope.

In the papers, Cassini scientists announce that a form of chemical energy that life can feed on appears to exist on Saturn’s moon Enceladus, and Hubble researchers report additional evidence of plumes erupting from Jupiter’s moon Europa.

This artist's rendering shows Cassini diving through the Enceladus plume in 2015. New ocean world discoveries from Cassini and Hubble will help inform future exploration and the broader search for life beyond Earth. (NASA/JPL-Caltech)

This artist’s rendering shows Cassini diving through the Enceladus plume in 2015. New ocean world discoveries from Cassini and Hubble will help inform future exploration and the broader search for life beyond Earth. (NASA/JPL-Caltech)

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NASA’s Cassini mission to Saturn inspires people of Earth

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Although the motivation behind NASA’s Cassini mission to Saturn was scientific, part of the planet’s allure has long been in its undeniable physical beauty.

Since Cassini arrived at Saturn in 2004, dramatic views from the spacecraft’s imaging cameras — and other sensors that observe in infrared, ultraviolet and radio frequencies — have revealed the ringed planet and its moons in unprecedented detail for scientists to study.

Saturn Mosaic by Ian Regan. (NASA/JPL-Caltech/SSI/Ian Regan)

Saturn Mosaic by Ian Regan. (NASA/JPL-Caltech/SSI/Ian Regan)

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NASA’s Cassini mission works to determine the length of a Saturn Day

 

Written by Jay Thompson
Cassini Public Engagement, NASA-JPL

NASA - National Aeronautics and Space AdministrationPasadena, CA – Humans sometimes struggle to adjust to Daylight Saving Time, but just measuring the exact length of a Saturn day is one of the big challenges for scientists on NASA’s Cassini mission. Over more than a decade in Saturn orbit, Cassini’s instruments have wrestled with confusing measurements to determine the planet’s precise rotation rate.

The mission’s final year and unprecedented trajectory will carry Cassini to unexplored regions so near to Saturn that scientists might finally answer the question:

Just how long is a day on Saturn?

Saturn as seen by NASA's Cassini spacecraft in 2008. Long-term tracking of the spacecraft's position has revealed no unexplained perturbations in Cassini's orbit. (NASA/JPL/Space Science Institute)

Saturn as seen by NASA’s Cassini spacecraft in 2008. Long-term tracking of the spacecraft’s position has revealed no unexplained perturbations in Cassini’s orbit. (NASA/JPL/Space Science Institute)

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NASA’s Cassini Spacecraft data used to weigh Saturn’s biggest ring

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – It seems intuitive that an opaque material should contain more stuff than a more translucent substance. For example, muddier water has more suspended particles of dirt in it than clearer water. Likewise, you might think that, in the rings of Saturn, more opaque areas contain a greater concentration of material than places where the rings seem more transparent.

But this intuition does not always apply, according to a recent study of the rings using data from NASA’s Cassini mission. In their analysis, scientists found surprisingly little correlation between how dense a ring might appear to be — in terms of its opacity and reflectiveness — and the amount of material it contains.

The B ring is the brightest of Saturn's rings when viewed in reflected sunlight. (NASA/JPL-Caltech/Space Science Institute)

The B ring is the brightest of Saturn’s rings when viewed in reflected sunlight. (NASA/JPL-Caltech/Space Science Institute)

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NASA’s Cassini data shows eruptions on Saturn’s Moon Enceladus’ could be curtain like eruptions instead of discrete jets

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – New research using data from NASA’s Cassini mission suggests most of the eruptions from Saturn’s moon Enceladus might be diffuse curtains rather than discrete jets.

Many features that appear to be individual jets of material erupting along the length of prominent fractures in the moon’s south polar region might be phantoms created by an optical illusion, according to the new study.

The research is being published on Thursday, May 7th, in the journal Nature.

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NASA’s Cassini spacecraft data helps Scientists solve mystery behind Saturn’s Storms

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – The long-standing mystery of why Saturn seethes with enormous storms every 30 years may have been solved by scientists working with data from NASA’s Cassini mission. The tempests, which can grow into bright bands that encircle the entire planet, are on a natural timer that is reset by each subsequent storm, the researchers report.

In 140 years of telescope observations, great storms have erupted on Saturn six times. Cassini and observers on Earth tracked the most recent of these storms from December 2010 to August 2011. During that time, the storm exploded through the clouds, eventually winding its way around Saturn.

This series of images from NASA's Cassini spacecraft shows the development of a huge storm of the type that erupts about every 30 years on Saturn. (NASA/JPL-Caltech/SSI)

This series of images from NASA’s Cassini spacecraft shows the development of a huge storm of the type that erupts about every 30 years on Saturn. (NASA/JPL-Caltech/SSI)

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NASA missions have discovered an abundance of Water in our Solar System

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – As NASA missions explore our solar system and search for new worlds, they are finding water in surprising places. Water is but one piece of our search for habitable planets and life beyond Earth, yet it links many seemingly unrelated worlds in surprising ways.

“NASA science activities have provided a wave of amazing findings related to water in recent years that inspire us to continue investigating our origins and the fascinating possibilities for other worlds, and life, in the universe,” said Ellen Stofan, chief scientist for the agency. “In our lifetime, we may very well finally answer whether we are alone in the solar system and beyond.”

NASA is exploring our solar system and beyond to understand the workings of the universe, searching for water and life among the stars. (NASA)

NASA is exploring our solar system and beyond to understand the workings of the universe, searching for water and life among the stars. (NASA)

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NASA’s Cassini Mission data reveals Jupiter’s Red Spot probably created by Chemical reaction to Sunlight

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – The ruddy color of Jupiter’s Great Red Spot is likely a product of simple chemicals being broken apart by sunlight in the planet’s upper atmosphere, according to a new analysis of data from NASA’s Cassini mission. The results contradict the other leading theory for the origin of the spot’s striking color — that the reddish chemicals come from beneath Jupiter’s clouds.

The results are being presented this week by Kevin Baines, a Cassini team scientist based at NASA’s Jet Propulsion Laboratory, Pasadena, California, at the American Astronomical Society’s Division for Planetary Science Meeting in Tucson, Arizona.

Research suggests effects of sunlight produce the color of Jupiter's Great Red Spot. The feature's clouds are much higher than those elsewhere on the planet, and its vortex nature confines the reddish particles once they form. (NASA/JPL-Caltech/ Space Science Institute)

Research suggests effects of sunlight produce the color of Jupiter’s Great Red Spot. The feature’s clouds are much higher than those elsewhere on the planet, and its vortex nature confines the reddish particles once they form. (NASA/JPL-Caltech/ Space Science Institute)

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NASA’s Cassini spacecraft finds two new features about Saturn’s moon Titan’s Hydrocarbon Seas

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA’s Cassini mission continues its adventures in extraterrestrial oceanography with new findings about the hydrocarbon seas on Saturn’s moon Titan.

During a flyby in August, the spacecraft sounded the depths near the mouth of a flooded river valley and observed new, bright features in the seas that might be related to the mysterious feature that researchers dubbed the “magic island.”

The findings are being presented this week at the Division for Planetary Sciences Meeting of the American Astronomical Society held in Tucson, Arizona.

Cassini radar data reveal the depth of a liquid methane/ethane sea on Saturn's moon Titan near the mouth of a large, flooded river valley. (NASA/JPL-Caltech/ASI/Cornell)

Cassini radar data reveal the depth of a liquid methane/ethane sea on Saturn’s moon Titan near the mouth of a large, flooded river valley. (NASA/JPL-Caltech/ASI/Cornell)

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NASA’s Cassini mission images suggests Saturn’s moon Mimas has a frozen core or a liquid ocean

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – A new study focused on the interior of Saturn’s icy moon Mimas suggests its cratered surface hides one of two intriguing possibilities: Either the moon’s frozen core is shaped something like a football, or the satellite contains a liquid water ocean.

Researchers used numerous images of Mimas taken by NASA’s Cassini mission to determine how much the moon wobbles as it orbits Saturn. They then evaluated several possible models for how its interior might be arranged, finding two possibilities that fit their data.The study is published in the October 17th issue of the journal Science.

This mosaic of Saturn's moon Mimas was created from images taken by NASA's Cassini spacecraft during its closest flyby of the moon on Feb. 13, 2010. (NASA/JPL-Caltech/Space Science Institute)

This mosaic of Saturn’s moon Mimas was created from images taken by NASA’s Cassini spacecraft during its closest flyby of the moon on Feb. 13, 2010. (NASA/JPL-Caltech/Space Science Institute)

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