Moon - Blog Posts
What’s Enceladus?
Before we tell you about Enceladus, let’s first talk about our Cassini spacecraft…
Our Cassini mission to Saturn is one of the most ambitious efforts in planetary space exploration ever mounted. Cassini is a sophisticated robotic spacecraft orbiting the ringed planet and studying the Saturnian system in detail.
Cassini completed its initial four-year mission to explore the Saturn System in June 2008. It has also completed its first mission extension in September 2010. Now, the health spacecraft is making exciting new discoveries in a second extension mission!
Enceladus
Enceladus is one of Saturn’s many moons, and is one of the brightest objects in our solar system. This moon is about as wide as Arizona, and displays at least five different types of terrain. The surface is believed to be geologically “young”, possibly less than 100 million years old.
Cassini first discovered continually-erupting fountains of icy material on Enceladus in 2005. Since then, the Saturn moon has become one of the most promising places in the solar system to search for present-day habitable environments.
Scientists found that hydrothermal activity may be occurring on the seafloor of the moon’s underground ocean. In September, it was announced that its ocean –previously thought to only be a regional sea – was global!
Since Cassini is nearing the end of its mission, we are able to make a series of three close encounters with Enceladus, one of Saturn’s moons.
Close Encounters
On Oct. 14, Cassini performed a mid-range flyby of Enceladus, but the main event will take place on Oct. 28, when Cassini will come dizzyingly close to the icy moon. During this flyby, the spacecraft will pass a mere 30 miles above the moon’s south polar region!
This will be the deepest-ever dive through the moon’s plume of icy spray, where Cassini can collect images and valuable data about what’s going on beneath the frozen surface.
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Super Blood Moon Photo Contest
This Sunday, Sept. 27 a Super Blood Moon will be visible in the U.S. and much of the world. This is the first time in more than 30 years that you’ll be able to witness a supermoon in combination with a lunar eclipse!
What is a supermoon? It’s a new or full moon that occurs when it is at, or near its closest approach to Earth. This event, combined with Earth’s shadow slowly swallowing the moon during the lunar eclipse, will provide for a spectacular night.
To make this lunar event even more exciting (not that it really needed it), we will be hosting a photo contest! During the event, we invite you to send us your best image of the Super Blood Moon on our Facebook page. Enter HERE.
After the entry window is closed, six finalists will be selected. These finalists will have their image voted on by the public. The winning image will be featured on our official social media platforms and on NASA.gov.
Are you interested? Here are the details:
Contest Entry Opens: Sept. 27 at 10:00 p.m. EDT
Contest Entry Closes: Sept. 28 at 10:00 a.m. EDT
Voting on Finalists Opens: Sept. 28 3:00 p.m. EDT
Voting on Finalists Closes: Sept. 29 11:59 p.m. EDT
For more information and specifics about the lunar event, visit our page on NASA.gov, and make sure that this Sunday, Sept. 27, you get outside, look up and take some awesome pictures!
ENTER HERE: http://go.nasa.gov/superbloodmoon-contest
Full Terms and Conditions can be found HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com
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/