Vortices Bump into a Hot Spot in Jupiter's Atmosphere

In this series of images from NASA's Cassini spacecraft, a dark, rectangular hot spot (top) interacts with a line of vortices that approaches from on the upper-right side (second panel). The interaction distorts the shape of the hot spot (third panel), leaving it diminished (bottom). The black scale bar is about 6,200 miles (10,000 kilometers) wide, or about twice as wide as the United States.

From top to bottom, these images were taken on November 21, November 24, November 27 and December 3, 2000 by Cassini's imaging science subsystem.

Image credit: NASA/JPL-Caltech/SSI/GSFC

Note: For more information, see 'Hot Spots' Ride a Merry-Go-Round on Jupiter.

Dark Hot Spot in Jupiter's Atmosphere

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. The bluish clouds to the right are in the upper troposphere, or perhaps higher still, in the stratosphere. The reddish gyre under the hot spot to the right and the large reddish plume at its lower left are in the lower troposphere. In addition, a high, gauzy haze covers part of the frame. An annotated version of this image highlights the hot spot in the middle with an arrow and boxes around the plume and the gyre.

This image was taken on December 13, 2000, by Cassini's imaging science subsystem.

Image credit: NASA/JPL-Caltech/SSI/GSFC

Note: For more information, see 'Hot Spots' Ride a Merry-Go-Round on Jupiter.

Europa Ocean and Geyser Hypothesis

Based on new evidence from Jupiter's moon Europa, astronomers hypothesize that chloride salts bubble up from the icy moon's global liquid ocean and reach the frozen surface where they are bombarded with sulfur from volcanoes on Jupiter's innermost large moon, Io. The new findings propose answers to questions that have been debated since the days of NASA's Voyager and Galileo missions. This illustration of Europa (foreground), Jupiter (right) and Io (middle) is an artist's concept.

Illustration credit: NASA/JPL-Caltech

Europa

This view of Jupiter's moon Europa features several regional-resolution mosaics overlaid on a lower resolution global view for context. The regional views were obtained during several different flybys of the moon by NASA's Galileo mission, and they stretch from high northern to high southern latitudes. Prominent here are the long, arcuate (or arc-shaped) and linear markings called lineae (Latin for strings or threads), which are a signature feature of Europa's surface. Color saturation has been enhanced to bring out the subtle red coloration present along many of the lineae. The color data extends into the infrared, showing bluish ice (indicating larger ice grains) in the polar regions.

The terrain in this view stretches from the side of Europa that always trails in its orbit at left (west), to the side that faces away from Jupiter at right (east). In addition to the lineae, the regional-scale images contain many interesting features, including lenticulae (small spots), chaos terrain, maculae (large spots), and the unusual bright band known as Agenor Linea in the south.

The regional-resolution mosaics enhance the amount of detail visible in a previously released view of the same region on Europa, [see PIA02590]. While the earlier image uses much of the same low-resolution data, its images are projected from a different angle and are processed with greater color saturation.

This view is an orthographic projection centered on 5.53 degrees south latitude, 214.5 degrees west longitude and has a resolution of 1600 feet (500 meters) per pixel. An orthographic view is like the view seen by a distant observer looking through a telescope.

The mosaic was constructed from individual images obtained by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft during six flybys of Europa between 1996 and 1999 (flybys designated G1, E11, E14, E15, E17, and E19).

Image credit: NASA/JPL-Caltech/University of Arizona

Note: For more new information on Europa, see A Window into Europa's Ocean Right at the Surface, PIA16826: Taste of the Ocean on Europa's Surface (Artist's Concept) and Long-stressed Europa Likely Off-kilter at One Time.

Juno's Two Deep Space Maneuvers are 'Back-To-Back Home Runs'

NASA's Juno spacecraft successfully executed a second Deep Space Maneuver, called DSM-2 last Friday, September 14. The 30 minute firing of its main engine refined the Jupiter-bound spacecraft's trajectory, setting the stage for a gravity assist from a flyby of Earth on October 9, 2013. Juno will arrive at Jupiter on July 4, 2016.

The maneuver began at 3:30 p.m. PDT (6:30 p.m. EDT), when the Leros-1b main engine began to fire. The burn ended at 4 p.m. PDT (7 p.m. EDT). Based on telemetry, the Juno project team believes the burn was accurate, changing the spacecraft's velocity by about 867 mph (388 meters a second) while consuming about 829 pounds (376 kilograms) of fuel.

The burn occurred when Juno was more than 298 million miles (480 million kilometers) from Earth.

Juno executed its first deep space maneuver (DSM-1), one of comparable duration and velocity change, on August 30. Together, both maneuvers placed Juno on course for its Earth flyby, which will occur as the spacecraft is completing one elliptical orbit around the sun. The Earth flyby will boost Juno's velocity by 16,330 mph (about 7.3 kilometers per second), placing the spacecraft on its final flight path for Jupiter. The closest approach to Earth, on October 9, 2013, will occur when Juno is at an altitude of about 348 miles (560 kilometers).

"It feels like we hit back-to-back home runs here with the near-flawless propulsion system performance seen during both DSM-1 and DSM-2." said Juno Project Manager Rick Nybakken of NASA's Jet Propulsion Laboratory in Pasadena, California. "These successes move us closer to being ready for our most critical mission event, the Jupiter Orbit Insertion main engine burn in July 2016. We're not in the playoffs yet, as that will come in 2016 when we arrive at Jupiter, but it does feel fantastic to have hit both of these DSMs out of the park."

Juno was launched on August 5, 2011. Once in orbit, the spacecraft will circle Jupiter 33 times, from pole to pole, and use its collection of eight science instruments to probe beneath the gas giant's obscuring cloud cover. Juno's science team will learn about Jupiter's origins, structure, atmosphere and magnetosphere, and look for a potential solid planetary core.

Juno's name comes from Greek and Roman mythology. The god Jupiter drew a veil of clouds around himself to hide his mischief, and his wife, the goddess Juno, was able to peer through the clouds and reveal Jupiter's true nature.

Illustration credit: NASA/JPL-Caltech

The Big Dipper by Juno

The Big Dipper as imaged on March 21, 2012, by the JunoCam instrument aboard NASA's Jupiter-bound Juno spacecraft.

Photo credit: NASA/JPL-Caltech/SWRI/MSSS Note: For more information, see NASA's Juno Spacecraft Images Big Dipper.

Jupiter Jet Stream

Following the path of one of Jupiter's jet streams, a line of v-shaped chevrons travels west to east just above Jupiter's Great Red Spot. Most of the planet is unfolded here in a single flat map made on December 11 and 12, 2000, when NASA's Cassini spacecraft flew past Jupiter. At the left, the chevrons run into another storm called the South Equatorial Disturbance (SED).

Photo credit: NASA/JPL-Caltech/Space Science Institute

Note: For more information, see Cassini Spies Wave Rattling Jet Stream on Jupiter.

Io

This is the highest resolution color picture taken so far [as of that date] of Jupiter's volcanic moon Io by NASA's Galileo spacecraft. At 3 kilometers (about 2 miles) per picture element, the fiery satellite is seen against a backdrop of Jupiter's cloud tops, which appear blue in this false-color composite. Among the surprises seen on the moon's surface are several small, distinctly greenish patches and subtle violet hues at the cores and margins of bright sulfur dioxide-rich regions (like the one in the lower right). Dark spots, many flagged by bright red pyroclastic deposits, (deposits from explosive ejecta), mark the sites of current volcanic activity. Most of Io's riotous color is due to the presence of sulfur compounds, but the dark materials that make up the flows and calderas are probably silicate rock.

North is to the top of the picture. The images used to construct this composite were taken in the 1-micron, green and violet filters of the solid state imaging camera system on NASA's Galileo spacecraft. The images were taken on March 29, 1998 at a range of 294,000 kilometers (about 183,000 miles).

Photo credit: NASA/JPL/University of Arizona

Jupiter's Great Red Spot

This Voyager 2 image shows the region of Jupiter extending from the equator to the southern polar latitudes in the neighborhood of the Great Red Spot. A white oval, different from the one observed in a similar position at the time of the Voyager 1 encounter, is situated south of the Great Red Spot. The region of white clouds now extends from east of the red spot and around its northern boundary, preventing small cloud vortices from circling the feature. The disturbed region west of the red spot has also changed since the equivalent Voyager 1 image. It shows more small scale structure and cloud vortices being formed out of the wave structures. The picture was taken on July 3, 1979 from 6 million kilometers (3.72 million miles).

Photo credit: NASA/JPL

Rotation of Jupiter

Jupiter observed with the 1 meter telescope at the Pic du Midi observatory and a Basler Scout Camera; images taken between October 10 and October 15, 2011.

Video credit: S2P/IMCCE/OPM/JL Dauvergne/Elie Rousset/Eric Meza/Philippe Tosi/François Colas/Jean Pajus/Xavi Nogués/Emil Kraaikamp

Jupiter and Io

Jupiter's four largest satellites, including Io, the golden ornament in front of Jupiter in this image from NASA's Cassini spacecraft, have fascinated Earthlings ever since Galileo Galilei discovered them in 1610 in one of his first astronomical uses of the telescope. This true-color composite frame, made from narrow angle images taken on December 12, 2000, captures Io and its shadow in transit against the disk of Jupiter. The distance of the spacecraft from Jupiter was 19.5 million kilometers. The image scale of the high resolution image is 117 kilometers per pixel. The entire body of Io, about the size of Earth's Moon, is periodically flexed as it speeds around Jupiter and feels, as a result of its non-circular orbit, the periodically changing gravitational pull of the planet. The heat arising in Io's interior from this continual flexure makes it the most volcanically active body in the solar system, with more than 100 active volcanoes. The white and reddish colors on its surface are due to the presence of different sulfurous materials. The black areas are silicate rocks.

Photo credit: NASA/JPL/University of Arizona

Earth and Moon, by Juno

On its way to the biggest planet in the solar system -- Jupiter, NASA's Juno spacecraft took time to capture its home planet and its natural satellite -- the Moon.

"This is a remarkable sight people get to see all too rarely," said Scott Bolton, Juno principal investigator from the Southwest Research Institute in San Antonio. "This view of our planet shows how Earth looks from the outside, illustrating a special perspective of our role and place in the universe. We see a humbling yet beautiful view of ourselves."

The image was taken by the spacecraft’s camera, JunoCam, on August 26 when the spacecraft was about 6 million miles (9.66 million kilometers) away. The image was taken as part of the mission team’s checkout of the Juno spacecraft. The team is conducting its initial detailed checks on the spacecraft’s instruments and subsystems after its launch on August 5.

Juno covered the distance from Earth to the Moon (about 250,000 miles or 402,000 kilometers) in less than one day's time. It will take the spacecraft another five years and 1,740 million miles (2,800 million kilometers) to complete the journey to Jupiter. The spacecraft will orbit the planet's poles 33 times and use its eight science instruments to probe beneath the gas giant's obscuring cloud cover to learn more about its origins, structure, atmosphere and magnetosphere, and look for a potential solid planetary core.

The solar-powered Juno spacecraft lifted off from Cape Canaveral Air Force Station in Florida at 9:25 a.m. PDT (12:25 p.m. EDT) on August 5 to begin its five-year journey to Jupiter.

Photo credit: NASA/JPL-Caltech

Jupiter from the Ground

Ground-based astronomers will be playing a vital role in NASA's Juno mission. Because Jupiter has such a dynamic atmosphere, images from the amateur astronomy community are needed to help the JunoCam instrument team predict what features will be visible when the camera's images are taken.

This image was acquired by Damian Peach on September 12, 2010, when Jupiter was close to opposition. South is up and the "Great Red Spot" is visible. Two of Jupiter's moons, Io and Ganymede, can also be seen in this image.

Photo credit: NASA/Damian Peach, Amateur Astronomer

What Juno Will See at Jupiter's South Pole

This simulated view of the south pole of Jupiter illustrates the unique perspective of NASA's Juno mission. The spacecraft's polar orbit will allow Juno's camera, called JunoCam, to image Jupiter's clouds from a vantage point never accessed by other spacecraft.

JunoCam was designed to return the best-ever images of Jupiter's pole. It has a 58-degree-wide field of view encompassing the entire polar region. The view illustrated here simulates an image taken 40 minutes before Juno's closest approach to Jupiter. At closest approach, JunoCam's images of Jupiter's cloudtops will have a resolution better than 3.1 miles (5 kilometers).

Illustration credit: NASA/JPL-Caltech/Malin Space Science Systems

Covering Jupiter from Earth and Space

Ground-based astronomers will be playing a vital role in NASA's Juno mission. Because Jupiter has such a dynamic atmosphere, images from the amateur astronomy community are needed to help the JunoCam instrument team predict what features will be visible when the camera's images are taken.

This image was acquired by Freddy Willems on July 26, 2011. The level of detail captured here illustrates how well ground-based astronomers are able to image the planet. The views acquired by Juno's camera, called JunoCam, as the spacecraft travels through its polar orbit provide a unique vantage point not available to Earth-based observers. JunoCam images therefore complement equatorial views like this one, allowing scientists to study the global dynamics of this giant planet's atmosphere. South is up in this image.

Photo credit: NASA/Freddy Willems, Amateur Astronomer

The Launch of Juno

The first video is an "official" video, compiled from several different camera angles and including, toward the end, some animation sequences showing events in the launch sequence that could not be captured with cameras. The second video is a compilation of a number of launch videos from various cameras both on the ground and on board the rocket.

NASA's Juno spacecraft is on its way to Jupiter after being launched aboard an Atlas V rocket from the Cape Canaveral Air Force Station, Florida on August 5 at 11:25 a.m. Eastern. The solar-powered spacecraft will arrive at Jupiter in July 2016 and orbit its poles 33 times to find out more about the gas giant's interior, atmosphere and aurora. Scientists believe Jupiter holds the key to better understanding the origins of our solar system.

Video credit: NASA

Juno on the Launch Pad

NASA's Juno spacecraft awaits launch from inside the payload fairing atop a United Launch Alliance Atlas V-551 launch vehicle. Juno and its rocket are at Space Launch Complex 41 on Cape Canaveral Air Force Station in Florida.

Photo credit: NASA/Kennedy Space Center

Amateurs to Take a Crack at Juno Images

Data from the camera onboard NASA's Juno mission, called JunoCam, will be made available to the public for processing into their own images. An example of this type of collaboration is illustrated here with an image of Jupiter taken by NASA's Voyager mission, and processed by Björn Jónsson. The image highlights Jupiter's "Great Red Spot."

Photo credit: NASA/JPL-Caltech

Juno Being Lowered into Position

At Space Launch Complex 41, the Juno spacecraft, enclosed in an Atlas payload fairing, was transferred into the Vertical Integration Facility where it was positioned on top of the Atlas rocket stacked inside.

Photo credit: NASA/Kennedy Space Center

Juno's Solar Array

In this image technicians stow for launch solar array #2 for NASA's Juno spacecraft. The photo was taken on May 20, 2011 at the Astrotech payload processing facility in Titusville, Florida. NASA's Juno spacecraft is scheduled to launch aboard an Atlas V rocket from Cape Canaveral, Florida. August 5. The solar-powered spacecraft will orbit Jupiter's poles 33 times to find out more about the gas giant's origins, structure, atmosphere and magnetosphere and investigate the existence of a solid planetary core.

Photo credit: NASA/JPL-Caltech/KSC