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The probe circled around the nearest point of Saturn's five moons and found that these small circular moons were covered with debris, including earth, ice, and particles of the larger Enceladus. Small in size, they look like pasta with raffioli.
"While touring these extraterrestrial micro-satellites, we discovered their interaction with the rings of Saturn," said Bonnie Burani of NASA's Jet Propulsion Laboratory. "We are seeing more evidence of interaction and dynamism between the rings of Saturn and the lunar system." The researchers say that Kazini's data is likely to help us understand the other planets in our solar system.
Scientists used the data collected during Kazini's return to Saturn in 2017 and were able to capture the planet's best imagery and many objects in its orbit and region.In addition to confirming the capture of satellites for materials, the team discovered that these satellites, including Atlas, Pan, Davens and Pandora Epimethios, porous porous.
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"We found that these satellites contain dirt and snow from the rings, which have the shape of small skirts around the orbit, and that the body closest to the bullet is due to the gravity that leads inside. "
The two moons being the closest to Saturn, the other three satellites were covered with ice particles from Inclados.
Cassini, who spent 13 years near the planet, entered Saturn between two rings and continued to transmit data to the Earth until she left service on September 13, 2017, 20 years after its launch.
The moons that are closer to Saturn seem much redder, like the main rings, while other satellites are more blue and there seems to be much more to know about these satellites and their information. Researchers will also use kazini data to design new sensors that can help Ensemble, and the acceleration that causes the appearance of satellites to the west can also give us a look of confidence on the rings of Saturn.
"This process can be done in loops because the larger ring particles also accelerate around the satellites," said Linda Spielker, co-author of the project. This detailed information gives us more information on the behavior of the annular particles themselves. "
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