Saturday, March 16, 2013

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.

Friday, March 15, 2013

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.

Thursday, March 7, 2013

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

Wednesday, March 6, 2013

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.