Topic: NASA’s Cassini Spacecraft

NASA’s Cassini Spacecraft discovers possible Activity on Saturn’s Moon Dione

May 30, 2013 |

Written by Jia-Rui Cook
NASA’s Jet Propulsion Laboratory

Pasadena, CA – From a distance, most of the Saturnian moon Dione resembles a bland cueball.

Thanks to close-up images of a 500-mile-long (800-kilometer-long) mountain on the moon from NASA’s Cassini spacecraft, scientists have found more evidence for the idea that Dione was likely active in the past. It could still be active now.

The Cassini spacecraft looks down, almost directly at the north pole of Dione. The feature just left of the terminator at bottom is Janiculum Dorsa, a long, roughly north-south trending ridge. (Image credit: NASA/JPL/Space Science Institute)

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NASA’s Cassini Spacecraft data suggests Wild Weather for Saturn’s Moon Titan this Summer

May 23, 2013 |

Written by Jia-Rui C. Cook
NASA’s Jet Propulsion Laboratory

Pasadena, CA – Saturn’s moon Titan might be in for some wild weather as it heads into its spring and summer, if two new models are correct. Scientists think that as the seasons change in Titan’s northern hemisphere, waves could ripple across the moon’s hydrocarbon seas, and hurricanes could begin to swirl over these areas, too.

The model predicting waves tries to explain data from the moon obtained so far by NASA’s Cassini spacecraft. Both models help mission team members plan when and where to look for unusual atmospheric disturbances as Titan summer approaches.

Ligeia Mare, shown in here in data obtained by NASA’s Cassini spacecraft, is the second largest known body of liquid on Saturn’s moon Titan. It is filled with liquid hydrocarbons, such as ethane and methane, and is one of the many seas and lakes that bejewel Titan’s north polar region. Cassini has yet to observe waves on Ligeia Mare and will look again during its next encounter on May 23rd, 2013. (Image credit: NASA/JPL-Caltech/ASI/Cornell)

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NASA’s Cassini Spacecraft discovers Plasma changes at Saturn

May 3, 2013 |

Written by Jia-Rui Cook
NASA’s Jet Propulsion Laboratory

Pasadena, CA – Researchers working with data from NASA’s Cassini spacecraft have discovered one way the bubble of charged particles around Saturn — known as the magnetosphere — changes with the planet’s seasons.

The finding provides an important clue for solving a riddle about the planet’s naturally occurring radio signal. The results might also help scientists better understand variations in Earth’s magnetosphere and Van Allen radiation belts, which affect a variety of activities at Earth, ranging from space flight safety to satellite and cell phone communications.

This is an artist’s concept of the Saturnian plasma sheet based on data from Cassini magnetospheric imaging instrument. It shows Saturn’s embedded “ring current,” an invisible ring of energetic ions trapped in the planet’s magnetic field. (Image credit: NASA/JPL/JHUAPL)

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NASA’s Cassini spacecraft spots huge Hurricane at Saturn’s North Pole

April 30, 2013 |

Written by Dr. Tony Phillips
Science at NASA

Washington, D.C. – NASA’s Cassini spacecraft has provided scientists the first close-up, visible-light views of a behemoth hurricane swirling around Saturn’s north pole.

In high-resolution pictures and video, scientists see the hurricane’s eye is about 1,250 miles (2,000 kilometers) wide, 20 times larger than the average hurricane eye on Earth. Thin, bright clouds at the outer edge of the hurricane are traveling 330 mph(150 meters per second). The hurricane swirls inside a large, mysterious, six-sided weather pattern known as the hexagon.

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NASA’s Cassini spacecraft sees Meteors crash into Saturn’s Rings

April 27, 2013 |

Written by Jia-Rui C. Cook
NASA’s Jet Propulsion Laboratory

Pasadena, CA – NASA’s Cassini spacecraft has provided the first direct evidence of small meteoroids breaking into streams of rubble and crashing into Saturn’s rings.

These observations make Saturn’s rings the only location besides Earth, the moon and Jupiter where scientists and amateur astronomers have been able to observe impacts as they occur. Studying the impact rate of meteoroids from outside the Saturnian system helps scientists understand how different planet systems in our solar system formed.

Five images of Saturn’s rings, taken by NASA’s Cassini spacecraft between 2009 and 2012, show clouds of material ejected from impacts of small objects into the rings. (Image Credit: NASA/JPL-Caltech/Space Science Institute/Cornell)

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NASA says Saturn to make it’s closest approach to Earth April 28th

April 26, 2013 |

Written by Dr. Tony Phillips
Science at NASA

Washington, D.C. – The Solar System is a beautiful place filled with wonders that NASA space probes are only beginning to discover. There’s a tendency, though, for people to become indifferent; every year Hubble, Cassini, MESSENGER and other spacecraft beam back gigabytes of jaw-dropping images. After a while, you don’t have any more “gasps” left in you.

Well, maybe just one more. Inhale deeply, because at the end of April, Saturn will put on a breathtaking display.

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NASA funded study shows rain from Saturn’s Rings falls across the Planet

April 14, 2013 |

Written by Jia-Rui Cook
NASA’s Jet Propulsion Laboratory

Pasadena, CA – A new study tracks the “rain” of charged water particles into the atmosphere of Saturn and finds there is more of it and it falls across larger areas of the planet than previously thought.

The study, whose observations were funded by NASA and whose analysis was led by the University of Leicester, England, reveals that the rain influences the composition and temperature structure of parts of Saturn’s upper atmosphere. The paper appears in this week’s issue of the journal Nature.

This artist’s concept illustrates how charged water particles flow into the Saturnian atmosphere from the planet’s rings, causing a reduction in atmospheric brightness. (Image credit: NASA/JPL-Caltech/Space Science Institute/University of Leicester)

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NASA’s Cassini spacecraft sees Ice Clouds forming in atmosphere of Saturn’s moon Titan

April 12, 2013 |

Written by Jia-Rui C. Cook
NASA’s Jet Propulsion Laboratory

Pasadena, CA – An ice cloud taking shape over Titan’s south pole is the latest sign that the change of seasons is setting off a cascade of radical changes in the atmosphere of Saturn’s largest moon.

Made from an unknown ice, this type of cloud has long hung over Titan’s north pole, where it is now fading, according to observations made by the composite infrared spectrometer (CIRS) on NASA’s Cassini spacecraft.

The recently formed south polar vortex stands out in the color-swaddled atmosphere of Saturn’s largest moon, Titan, in this natural color view from NASA’s Cassini spacecraft. (Image credit: NASA/JPL-Caltech/Space Science Institute)

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NASA’s Cassini spacecraft data reveals Saturn’s moons may have formed during our solar systems creation

March 29, 2013 |

Written by Jia-Rui Cook
NASA’s Jet Propulsion Laboratory

Pasadena, CA – A new analysis of data from NASA’s Cassini spacecraft suggests that Saturn’s moons and rings are gently worn vintage goods from around the time of our solar system’s birth.

Though they are tinted on the surface from recent “pollution,” these bodies date back more than 4 billion years. They are from around the time that the planetary bodies in our neighborhood began to form out of the protoplanetary nebula, the cloud of material still orbiting the sun after its ignition as a star.

The Cassini spacecraft observes three of Saturn’s moons set against the darkened night side of the planet. (Image Credit: NASA/JPL/Space Science Institute)

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NASA’s Cassini spacecraft photos reveals the movement of Jupiter’s Hot Spots through it’s atmosphere

March 15, 2013 |

Written by Jia-Rui C. Cook
NASA’s Jet Propulsion Laboratory

Pasadena, CA – In the swirling canopy of Jupiter’s atmosphere, cloudless patches are so exceptional that the big ones get the special name “hot spots.” Exactly how these clearings form and why they’re only found near the planet’s equator have long been mysteries.

Now, using images from NASA’s Cassini spacecraft, scientists have found new evidence that hot spots in Jupiter’s atmosphere are created by a Rossby wave, a pattern also seen in Earth’s atmosphere and oceans. The team found the wave responsible for the hot spots glides up and down through layers of the atmosphere like a carousel horse on a merry-go-round.

The dark hot spot in this false-color image from NASA’s Cassini spacecraft is a window deep into Jupiter’s atmosphere. All around it are layers of higher clouds, with colors indicating which layer of the atmosphere the clouds are in. (Image credit: NASA/JPL-Caltech/SSI/GSFC)

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