Huygens' Landing Site 10.27.04 Shown here are two images of the expected landing site of Cassini's Huygens' probe (latitude 10.6 S, longitude 191 W). The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov. Both images were taken by Cassini's imaging science subsystem through near-infrared filters. This site is maintained by the Planetary Science Communications team at, Titan Radar Swath (T-56 Flyby - June 6, 2009), Dawn Spacecraft Gathering Spectral Data from Vesta (Artist's Concept), Artist Concept of Particle Population in Saturn's Magnetosphere -- Labeled, October 2020 - Part II: The Next Full Moon is a Halloween Hunter's Moon and "Micro" Moon, Greenland's Retreating Glaciers Could Impact Local Ecology, NASA's Perseverance Rover Is Midway to Mars, Juno Data Indicates 'Sprites' or 'Elves' Frolic in Jupiter's Atmosphere, NASA Scientists Discover ‘Weird' Molecule in Titan's Atmosphere, NASA's OSIRIS-REx Spacecraft Goes for Early Stow of Asteroid Sample. At right is a wide-angle image showing most of Titan's disc, with a scale of 10 kilometers (6.2 miles) per pixel. To get the best experience possible, please download a compatible browser. Dr. Lori Glaze The landing site is located on the boundary between the bright region called Adiri and the dark one called Shangri-la. At left is a narrow-angle image of the landing site at a scale of 0.83 kilometers (.5 miles) per pixel (location shown by black box at right). This image was obtained by Cassini's radar instrument during a flyby on June 6, 2009. Social Media Lead: This infrared global map of Saturns icy moon Enceladus was created using images acquired by NASAs Cassini spacecraft. The small moon Mimas passes in front of the larger moon Rhea, which is partly obscured by Saturn's rings, in this movie from NASA's Cassini spacecraft. The mosaic is overlaid on a Cassini orbiter radar image. The hypothesis presented favors lo... Janus floats above the meandering clouds of Saturn. It shows Cassini imaging science sub-system images, radar images and visual and infrared mapping spectrometer images of the Huygens probe landing area. Phillips Davis This composite image shows a mosaic of the European Space Agency's Huygens probe landing site, as seen by the descent imager/spectral radiometer on the Huygens probe. The camera filter used for this image captures light at wavelengths where atmospheric gases like methane are fairly transparent, allow... Saturn's north polar hexagon appears to be a long-lived feature of the atmosphere, having been spotted in images of Saturn in the early 1980s, again in the 1990s, and then by the Cassini spacecraft... A propeller-shaped structure created by an unseen moon appears dark in this image obtained by NASA’s Cassini spacecraft of the unilluminated side of Saturn's rings. The radar image was taken on an Oct. 28, 2005, flyby. These images from NASA's Dawn spacecraft, located in asteroid Vesta's Marcia quadrangle, in Vesta's northern hemisphere, demonstrate a special analytical technique, which results in shadowed areas ... + View Full Res If you know your browser is up to date, you should check to ensure that The rest of the movie consists of mosaics from the descent … The lower-resolution imaging sequences are outlined in blue. This was the first - and, so far, the only - landing in the outer solar system. This is an artist's concept of the Saturnian plasma sheet based on data from Cassini magnetospheric imaging instrument. NASA - National Aeronautics and Space Administration, Follow this link to skip to the main content. The lander returned the first in situ measurements of Titan’s atmosphere, determining its pressure, density and temperature from an altitude of 1400km down to the surface. Bill Dunford. The Cassini spacecraft finds oddly-shaped Atlas gliding along the edge of the A ring. North is tilted about 45 degrees from the top of both images. New results from NASA's Juno mission suggest that either "sprites" or "elves" could be dancing in the upper atmosphere of Jupiter. Spacecraft: Cassini Orbiter, Huygens Probe, Instrument: Descent Imager/Spectral Radiometer, Radar Mapper, Image credit: ESA/NASA/JPL-Caltech/University of Arizona/USGS. NASA Official: The mosaic is overlaid on a Cassini orbiter radar image. Enceladus Global View with Plume (Artist's Rendering), Site Editors: Tony Greicius, Randal Jackson, Naomi Hartono. Kristen Erickson This image provides a comparison between the Huygens landing site on Titan as viewed by the Cassini Imaging Science Subsystem (ISS) and the NACO/SDI instrument mounted on the 8-meter Yepun telescope of the VLT (Very Large Telescope) station, in Chile. The mosaic shows two large impact craters. The surface has bright and dark markings with a streamlined pattern consistent with motion from a fluid, such as the atmosphere, moving from west to east (upper left to lower right). NASA’s OSIRIS-REx mission is ready to perform an early stow on Tuesday, Oct. 27, of the large sample it collected from the surface of asteroid Bennu. NASA's Cassini spacecraft from a distance of ... Craters of Tethys This graphic, constructed from data obtained by NASA's Cassini spacecraft, shows the percentage of cloud coverage across the surface of Saturn's moon Titan. This infrared view of Saturn's southern hemisphere shows the bright, high altitude equatorial band at the top, and the now familiar dark bull's-eye that marks the planet's south pole. The imaging team is based at the Space Science Institute, Boulder, Colo. For the latest news about the Cassini-Huygens mission, visit http://www.nasa.gov/cassini. This image from NASA's Dawn mission reveals the creeping dawn over the north pole of the giant asteroid Vesta now that sunlight is shining over that area. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. Bright, high altitude clouds, like those imaged here, often appear more filamentary or streak-like than clouds imaged at slightly deeper levels in Saturn's atmosphere. The red color on the NACO/SDI image corresponds to an atmospheric filter at 1.625 micron, while the blue color corresponds to a filter for the surface at 1.600 and 1.575 micron. October 23, 2000 Identifying the landing site will improve the understanding of Titan to be gained by comparing localized data that the probe returned with larger-scale observations by the orbiter. The radar image was taken on an Oct. 28, 2005, flyby.   Huygens Landing Site This composite image shows a mosaic of the European Space Agency's Huygens probe landing site, as seen by the descent imager/spectral radiometer on the Huygens probe. Both of Saturn's F-ring shepherd moons are seen in this Cassini spacecraft view, which also features narrow ringlets in the Encke gap at left. It shows Saturn's embedded "ring current," an invi... Saturn's northern storm marches through the planet's atmosphere in the top right of this false-color mosaic from NASA's Cassini spacecraft. The Huygens probe successfully landed on Saturn's largest moon Titan at about 11:30 UTC on January 14, 2005. Full-Res: PIA06518

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