The rings of Saturn have puzzled astronomers since Galileo Galilei discovered them with his telescope in 1610. Detailed study by the Voyager 1 and Voyager 2 spacecraft in the 1980s only increased the mystery.
There are thousands of rings made of up billions of particles of ice and rock. The particles range in size from a grain of sugar to the size of a house. The rings are believe [sic] to be pieces of comets, asteroids or shattered moons that broke up before they reached the planet. Each ring orbits at a different speed around the planet. Information from NASA's Cassini mission will help reveal how they formed, how they maintain their orbit and, above all, why they are there in the first place.
While the other three gas planets in the solar system - Jupiter, Uranus and Neptune - have rings orbiting around them, Saturn's are by far the largest and most spectacular. With a thickness of about 1 kilometer (3,200 feet) or less, they span up to 282,000 km (175,000 miles), about three quarters of the distance between the Earth and its moon.
Named alphabetically in the order they were discovered, the rings are relatively close to each other, with the exception of the Cassini Division, a gap measuring 4,700 kilometers (2,920 miles). The main rings are, working outward from the planet, known as C, B, and A. The Cassini Division is the largest gap in the rings and separates Rings B and A. In addition a number of fainter rings have been discovered more recently. The D Ring is exceedingly faint and closest to the planet. The F Ring is a narrow feature just outside the A Ring. Beyond that are two far fainter rings named G and E. The rings show a tremendous amount of structure on all scales; some of this structure is related to gravitational perturbations by Saturn's many moons, but much of it remains unexplained.
To enter Saturn's orbit, Cassini flew through the gap between the F and the G rings, farther from the planet than the Cassini Division. As a safe measure, during the crossing of the ring plane, instruments and cameras onboard the spacecraft were shut off temporarily. However, the spectacular crossing into Saturn's orbit brought incredible information, images and footage, while the instruments onboard are still collecting unique data that may answer many questions about the rings' composition.
Reference: USGS Astrogeology: Gazetteer of Planetary Nomenclature - Ring Nomenclature
Source: The NASA website. All emphases are mine.
So what’s with all this astro mumbo-jumbo?
This serves as an invitation to a group reading of the novel The Rings of Saturn by the sublime German writer W. G. Sebald. The discussion is happening in Shelfari and it starts on April 4. You need to be a member of Shelfari and of the Sebald group in order to join. Registration is free. Here's the chapter-by-chapter schedule:
I – II: Week 1: April 4-10: pages 1-48
III – IV: Week 2: April 11-17: pages 49-99
V – VI: Week 3: April 18-24: pages 101-166
VII – VIII: Week 4: April 25 - May 1: pages 167-237
IX – X: Week 5: May 2-8: pages 239-296
That's two chapters a week for five weeks. The book is 296 pages long so we’re reading around 60 pages per week. The week refers to the start of discussion by chapter. That means the actual reading is done before the indicated week. You can of course read ahead of schedule. The pages are based on the English translation by Michael Hulse. Readers of the book in the original German language and in other translations can join us in the discussion but we'll be discussing in English.
We hope you can join us.
Post a Comment