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Our Juno mission completed a close flyby of Jupiter on Thursday, February 2, its latest science orbit of the mission. All of Juno's science instruments and the spacecraft's JunoCam were operating during the flyby to collect data that is now being returned to Earth.
Want to know more? Using NASA's Eyes on the Solar System and simulated data from the Juno flight team you can ride onboard the Juno spacecraft in real-time at any moment during the entire mission.
Cassini Project Scientist Linda Spilker and mission planner Molly Bittner take questions about the mission's "Ring-Grazing" orbits during Facebook Live. Watch it now: www.facebook.com/NASA/videos/10154861046561772/
The deadline is Friday, February 24 for U.S. student in grades 5 to 12. For international students, visit the page for more info!
More: solarsystem.nasa.gov/educ/Scientist-For-a-Day/2016-17/videos/intro
Dione's lit hemisphere faces away from Cassini's camera, yet the moon's darkened surface are dimly illuminated in this image, due to the phenomenon of Saturnshine. Although direct sunlight provides the best illumination for imaging, light reflected off of Saturn can do the job as well. In this image, Dione (698 miles or 1,123 kilometers across) is above Saturn's day side, and the moon's night side is faintly illuminated by sunlight reflected off the planet's disk.
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This Monday, Aug. 17, marks the final targeted flyby of Dione, one of Saturn’s many moons, in Cassini’s long mission. During this flyby, the science team will conduct a gravity experiment that will contribute to our knowledge of the internal structure of Dione. We will also learn more about its outer ice shell, and will be able to compare this with Saturn’s other icy moons.
Beyond the icy moons, Saturn is adorned with thousands of beautiful ringlets, While all four gas giant planets in our solar system have rings -- made of chunks of ice and rock -- none are as spectacular or as complicated as Saturn's. Like the other gas giants, Saturn is mostly a massive ball of hydrogen and helium.
This image of Saturn was taken using an infrared filter. Using this type of filter can help scientists determine the location of clouds in the planet’s atmosphere. The darker areas reveal clouds that are lower in the atmosphere, while the bright areas are higher altitude clouds.
Since Cassini reached Saturn in 2004, it has captured important data and images. This spacecraft has the ability to “see” in wavelengths that the human eye cannot, and it can “feel” things about magnetic fields and tiny dust particles that no human hand could detect. These heightened “senses” have allowed us to have a better understanding of Saturn, its moons and the solar system.
Learn more about Cassini & Saturn: http://saturn.jpl.nasa.gov/