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Topic: Saturn

NASA’s Cassini spacecraft takes first look at Saturn’s Atmosphere

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA’s Cassini spacecraft has sent to Earth its first views of Saturn’s atmosphere since beginning the latest phase of its mission. The new images show scenes from high above Saturn’s northern hemisphere, including the planet’s intriguing hexagon-shaped jet stream.

Cassini began its new mission phase, called its Ring-Grazing Orbits, on November 30th. Each of these weeklong orbits — 20 in all — carries the spacecraft high above Saturn’s northern hemisphere before sending it skimming past the outer edges of the planet’s main rings.

This view from NASA's Cassini spacecraft was obtained about half a day before its first close pass by the outer edges of Saturn's main rings during its penultimate mission phase. (NASA/JPL-Caltech/Space Science Institute)

This view from NASA’s Cassini spacecraft was obtained about half a day before its first close pass by the outer edges of Saturn’s main rings during its penultimate mission phase. (NASA/JPL-Caltech/Space Science Institute)

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NASA’s Cassini spacecraft completes first dive into outer edges of Saturn’s Rings

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA’s Saturn-orbiting Cassini spacecraft has made its first close dive past the outer edges of Saturn’s rings since beginning its penultimate mission phase on November 30th.

Cassini crossed through the plane of Saturn’s rings on December 4th at 5:09am PST (8:09am EST) at a distance of approximately 57,000 miles (91,000 kilometers) above Saturn’s cloud tops. This is the approximate location of a faint, dusty ring produced by the planet’s small moons Janus and Epimetheus, and just 6,800 miles (11,000 kilometers) from the center of Saturn’s F ring.

This graphic shows the closest approaches of Cassini's final two orbital phases. Ring-grazing orbits are shown in gray (at left); Grand Finale orbits are shown in blue. The orange line shows the spacecraft's Sept. 2017 final plunge into Saturn. (NASA/JPL-Caltech)

This graphic shows the closest approaches of Cassini’s final two orbital phases. Ring-grazing orbits are shown in gray (at left); Grand Finale orbits are shown in blue. The orange line shows the spacecraft’s Sept. 2017 final plunge into Saturn. (NASA/JPL-Caltech)

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NASA’s Cassini Spacecraft to begin first phase of it’s end mission

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – A thrilling ride is about to begin for NASA’s Cassini spacecraft. Engineers have been pumping up the spacecraft’s orbit around Saturn this year to increase its tilt with respect to the planet’s equator and rings. And on November 30th, following a gravitational nudge from Saturn’s moon Titan, Cassini will enter the first phase of the mission’s dramatic endgame.

Launched in 1997, Cassini has been touring the Saturn system since arriving there in 2004 for an up-close study of the planet, its rings and moons. During its journey, Cassini has made numerous dramatic discoveries, including a global ocean within Enceladus and liquid methane seas on Titan.

This is an artists concept of the Cassini Spacecraft orbiting Saturn Orbit. (NASA/JPL)

This is an artists concept of the Cassini Spacecraft orbiting Saturn Orbit. (NASA/JPL)

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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 observes Methane Clouds moving across Saturn’s moon Titan

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA’s Cassini spacecraft watched clouds of methane moving across the far northern regions of Saturn’s largest moon, Titan, on October 29­­­­th and 30th, 2016.

Several sets of clouds develop, move over the surface and fade during the course of this movie sequence, which spans 11 hours, with one frame taken every 20 minutes. Most prominent are long cloud streaks that lie between 49 and 55 degrees north latitude.

New video shows bright clouds of methane drifting across Saturn's largest moon, Titan. (NASA/JPL-Caltech/Space Science Institute)

New video shows bright clouds of methane drifting across Saturn’s largest moon, Titan. (NASA/JPL-Caltech/Space Science Institute)

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NASA’s Voyager 2 Spacecraft data suggests Uranus may have Two Additional Moons

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA’s Voyager 2 spacecraft flew by Uranus 30 years ago, but researchers are still making discoveries from the data it gathered then. A new study led by University of Idaho researchers suggests there could be two tiny, previously undiscovered moonlets orbiting near two of the planet’s rings.

Rob Chancia, a University of Idaho doctoral student, spotted key patterns in the rings while examining decades-old images of Uranus’ icy rings taken by Voyager 2 in 1986. He noticed the amount of ring material on the edge of the alpha ring — one of the brightest of Uranus’ multiple rings — varied periodically. A similar, even more promising pattern occurred in the same part of the neighboring beta ring.

Uranus is seen in this false-color view from NASA's Hubble Space Telescope from August 2003. The brightness of the planet's faint rings and dark moons has been enhanced for visibility. (NASA/Erich Karkoschka (Univ. Arizona))

Uranus is seen in this false-color view from NASA’s Hubble Space Telescope from August 2003. The brightness of the planet’s faint rings and dark moons has been enhanced for visibility. (NASA/Erich Karkoschka (Univ. Arizona))

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NASA’s Cassini Spacecraft observes Changes of Seasons on Saturn’s moon Titan

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – As southern winter solstice approaches in the Saturn system, NASA’s Cassini spacecraft has been revealing dramatic seasonal changes in the atmospheric temperature and composition of Saturn’s largest moon, Titan.

Winter is taking a grip on Titan’s southern hemisphere, and a strong, whirling atmospheric circulation pattern — a vortex — has developed in the upper atmosphere over the south pole. Cassini has observed that this vortex is enriched in trace gases — gases that are otherwise quite rare in Titan’s atmosphere. Cassini’s observations show a reversal in the atmosphere above Titan’s poles since the spacecraft arrived at Saturn in 2004, when similar features were seen in the northern hemisphere.

Slipping into shadow, the south polar vortex at Saturn's moon Titan still stands out against the orange and blue haze layers that are characteristic of Titan's atmosphere. (NASA/JPL-Caltech/Space Science Institute)

Slipping into shadow, the south polar vortex at Saturn’s moon Titan still stands out against the orange and blue haze layers that are characteristic of Titan’s atmosphere. (NASA/JPL-Caltech/Space Science Institute)

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NASA’s New Horizons Spacecraft sees what could be Clouds on Pluto

 

Written by Guy Webster
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – The next target for NASA’s New Horizons mission — which made a historic flight past Pluto in July 2015 — apparently bears a colorful resemblance to its famous, main destination.

NASA’s Hubble Space Telescope data suggests that 2014 MU69, a small Kuiper Belt object (KBO) about a billion miles (1.6 billion kilometers) beyond Pluto, is as red, if not redder, than Pluto. This is the first hint at the surface properties of the far-flung object that New Horizons will survey on January 1st, 2019.

Pluto's present, hazy atmosphere is almost entirely free of clouds. However, scientists from NASA's New Horizons mission have identified some cloud candidates -- suggestive of possible, rare condensation clouds -- in images taken during the spacecraft's July 2015 flight through the Pluto system. (NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Center)

Pluto’s present, hazy atmosphere is almost entirely free of clouds. However, scientists from NASA’s New Horizons mission have identified some cloud candidates — suggestive of possible, rare condensation clouds — in images taken during the spacecraft’s July 2015 flight through the Pluto system. (NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Center)

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NASA’s Hubble Space Telescope spots what may be water vapor plumes on Jupiter’s moon Europa

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Astronomers using NASA’s Hubble Space Telescope have imaged what may be water vapor plumes erupting off the surface of Jupiter’s moon Europa. This finding bolsters other Hubble observations suggesting the icy moon erupts with high altitude water vapor plumes.

The observation increases the possibility that missions to Europa may be able to sample Europa’s ocean without having to drill through miles of ice.

“Europa’s ocean is considered to be one of the most promising places that could potentially harbor life in the solar system,” said Geoff Yoder, acting associate administrator for NASA’s Science Mission Directorate in Washington. “These plumes, if they do indeed exist, may provide another way to sample Europa’s subsurface.”

This composite image shows suspected plumes of water vapor erupting at the 7 o'clock position off the limb of Jupiter's moon Europa. The plumes, photographed by NASA's Hubble's Space Telescope Imaging Spectrograph, were seen in silhouette as the moon passed in front of Jupiter. (NASA/ESA/W. Sparks (STScI)/USGS Astrogeology Science Center)

This composite image shows suspected plumes of water vapor erupting at the 7 o’clock position off the limb of Jupiter’s moon Europa. The plumes, photographed by NASA’s Hubble’s Space Telescope Imaging Spectrograph, were seen in silhouette as the moon passed in front of Jupiter. (NASA/ESA/W. Sparks (STScI)/USGS Astrogeology Science Center)

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NASA’s Cassini Spacecraft observes Mystery Cloud on Saturn’s moon Titan

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – The puzzling appearance of an ice cloud seemingly out of thin air has prompted NASA scientists to suggest that a different process than previously thought — possibly similar to one seen over Earth’s poles — could be forming clouds on Saturn’s moon Titan.

Located in Titan’s stratosphere, the cloud is made of a compound of carbon and nitrogen known as dicyanoacetylene (C4N2), an ingredient in the chemical cocktail that colors the giant moon’s hazy, brownish-orange atmosphere.

The hazy globe of Titan hangs in front of Saturn and its rings in this natural color view from NASA's Cassini spacecraft. (NASA/JPL-Caltech/Space Science Institute)

The hazy globe of Titan hangs in front of Saturn and its rings in this natural color view from NASA’s Cassini spacecraft. (NASA/JPL-Caltech/Space Science Institute)

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