Join Dr Becky as she discusses her favorite planet, Saturn, with Professor Geraint Jones and Professor John Zarnecki. They delve into topics such as Saturn's captivating rings, mysterious dark markings, NASA's Dragonfly mission on Titan, Saturn's atmosphere, and the possibility of Earth getting a ring. Dr Robert Massey also shares stargazing tips and takes listener questions.
Saturn's rings are not evenly spread out due to the presence of moons and resonances, creating gaps and structures within the rings.
Saturn's atmosphere does not significantly affect its moons, but connections exist such as material falling from the rings impacting the temperature of Saturn's atmosphere and Saturn's magnetic field protecting moons from solar wind.
Deep dives
Saturn's Rings: Gaps and Structure
Saturn's rings are not evenly spread out due to the presence of moons and resonances. Moons like Pan and Daphnis create gaps in the rings as they clear out debris. Resonances caused by strong gravity interactions between moons and particles lead to the formation of structure and gaps. The F ring was likely formed from debris caused by the collision of moons, while the E ring consists of material ejected from the plumes of Enceladus. The rings are dynamic and relatively young, and the current moons do not pose a significant risk of becoming future rings.
Saturn's Atmosphere and Moons
Saturn's atmosphere does not significantly extend out to its moons. The moons are not affected by the atmosphere in terms of drag or significant interaction. However, some connections exist between the atmosphere and moons. For example, material falling in from the rings can affect the temperature of Saturn's atmosphere. Additionally, the presence of Saturn's large and powerful magnetic field, like the one enveloping Titan, can help protect the moon's atmosphere and prevent the solar wind from stripping it away.
Enceladus's Jet and South Pole Activity
Enceladus's jet activity is primarily located at its South Pole. The crust in the South Pole is younger and more tectonically active, leading to the presence of fractures and ridges. This activity provides an outlet for plumes of material to escape from beneath the moon's ocean, potentially due to impacts or tectonic interactions. The specific location of this activity is determined by the moon's surface features and geological processes.
It's FINALLY happening. Izzie is letting Dr Becky have an entire episode about her favourite planet, Saturn.
Professor Geraint Jones from UCL's Mullard Space Science Laboratory tells the Supermassive Team about the Saturnian system. Plus, Professor John Zarnecki shares his experiences of being involved with the Cassini-Huygens mission. And, as always, Dr Robert Massey is on hand to take on listener questions and share his stargazing tips for the month.
The Supermassive Podcast is a Boffin Media production for The Royal Astronomical Society by Izzie Clarke and Richard Hollingham.
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