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Qué (quién) es Saturn"s rings - definición
BOOK BY W.G. SEBALD
The rings of saturn; The Rings of Saturn (novel)
Rings of Saturn
![Propeller moonlet Santos-Dumont from lit (top) and unlit sides of rings](https://commons.wikimedia.org/wiki/Special:FilePath/A Ring propeller "Santos-Dumont" (PIA 21433).jpg?width=200 "Propeller moonlet Santos-Dumont from lit (top) and unlit sides of rings")
![Detail of Galileo's drawing of [[Saturn]] in a letter to Belisario Vinta (1610)](https://commons.wikimedia.org/wiki/Special:FilePath/Anillos de Satruno - Galileo Galilei.png?width=200 "Detail of Galileo's drawing of [[Saturn]] in a letter to Belisario Vinta (1610)")
![Mimas]].](https://commons.wikimedia.org/wiki/Special:FilePath/Cassini Division.jpg?width=200 "Mimas]].")
![Spitzer]] image of part of the ring](https://commons.wikimedia.org/wiki/Special:FilePath/Infrared Ring Around Saturn.jpg?width=200 "Spitzer]] image of part of the ring")
![Pan]]'s orbit, implying its particles oscillate in [[horseshoe orbit]]s.](https://commons.wikimedia.org/wiki/Special:FilePath/PIA06534 Encke Division.jpg?width=200 "Pan]]'s orbit, implying its particles oscillate in [[horseshoe orbit]]s.")
![gallery]]).](https://commons.wikimedia.org/wiki/Special:FilePath/PIA08319 Daphnis in Keeler Gap.jpg?width=200 "gallery]]).")
![Anthe]]](https://commons.wikimedia.org/wiki/Special:FilePath/PIA11101 Anthe ring arc.jpg?width=200 "Anthe]]")
![E]] rings.](https://commons.wikimedia.org/wiki/Special:FilePath/PIA17172 Saturn eclipse mosaic bright crop.jpg?width=200 "E]] rings.")
![F Ring]].](https://commons.wikimedia.org/wiki/Special:FilePath/Saturn, its rings, and a few of its moons.jpg?width=200 "F Ring]].")
![C Ring]] is just inside the B Ring.](https://commons.wikimedia.org/wiki/Special:FilePath/Saturn HST 2004-03-22.jpg?width=200 "C Ring]] is just inside the B Ring.")
![The outer rings seen back-illuminated by the [[Sun]]](https://commons.wikimedia.org/wiki/Special:FilePath/Saturn outer rings labeled.svg?width=200 "The outer rings seen back-illuminated by the [[Sun]]")
![radio-occultation]]-derived particle size data. The [[attenuation]] of 0.94-, 3.6-, and 13-cm signals sent by ''Cassini'' through the rings to Earth shows abundance of particles of sizes similar to or larger than those wavelengths. Purple (B, inner A Ring) means few particles are < 5 cm (all signals similarly attenuated). Green and blue (C, outer A Ring) mean particles < 5 cm and < 1 cm, respectively, are common. White areas (B Ring) are too dense to transmit adequate signal. Other evidence shows rings A to C have a broad range of particle sizes, up to m across.](https://commons.wikimedia.org/wiki/Special:FilePath/Unraveling Saturn's Rings.jpg?width=200 "radio-occultation]]-derived particle size data. The [[attenuation]] of 0.94-, 3.6-, and 13-cm signals sent by ''Cassini'' through the rings to Earth shows abundance of particles of sizes similar to or larger than those wavelengths. Purple (B, inner A Ring) means few particles are < 5 cm (all signals similarly attenuated). Green and blue (C, outer A Ring) mean particles < 5 cm and < 1 cm, respectively, are common. White areas (B Ring) are too dense to transmit adequate signal. Other evidence shows rings A to C have a broad range of particle sizes, up to m across.")
![Mimas]]. The shadow is attenuated by the denser B ring. The [[Maxwell Gap]] is below center.](https://commons.wikimedia.org/wiki/Special:FilePath/PIA11660- Mimas' shadow cut off by B ring (trimmed).jpg?width=200 "Mimas]]. The shadow is attenuated by the denser B ring. The [[Maxwell Gap]] is below center.")
![Epimetheus]]. These encounters lead to periodic minor disruptions in the wave pattern.}}](https://commons.wikimedia.org/wiki/Special:FilePath/PIA21627 - Janus 2-to-1 spiral density wave in Saturn's inner B Ring.jpg?width=200 "Epimetheus]]. These encounters lead to periodic minor disruptions in the wave pattern.}}")
![Huygens Gap]]) and the bright (from this viewing geometry) ringlets to their left comprise the [[Cassini Division]].](https://commons.wikimedia.org/wiki/Special:FilePath/Spokes in Saturn's B Ring.jpg?width=200 "Huygens Gap]]) and the bright (from this viewing geometry) ringlets to their left comprise the [[Cassini Division]].")
![B Ring]] spokes.](https://commons.wikimedia.org/wiki/Special:FilePath/Srings.jpg?width=200 "B Ring]] spokes.")
![spiral density waves]].](https://commons.wikimedia.org/wiki/Special:FilePath/PIA06099 Enke Gap.jpg?width=200 "spiral density waves]].")
![Daphnis]].](https://commons.wikimedia.org/wiki/Special:FilePath/Daphnis makes waves - 4x vertical stretch.jpg?width=200 "Daphnis]].")
![Pandora]] orbit just inside and outside the [[F Ring]], but only Prometheus acts as a ring shepherd.](https://commons.wikimedia.org/wiki/Special:FilePath/Prometheus und Pandora.jpg?width=200 "Pandora]] orbit just inside and outside the [[F Ring]], but only Prometheus acts as a ring shepherd.")
![F ring]] dynamism, probably due to perturbing effects of small moonlets orbiting close to or through the ring's core.](https://commons.wikimedia.org/wiki/Special:FilePath/F Ring Dynamism PIA08290.jpg?width=200 "F ring]] dynamism, probably due to perturbing effects of small moonlets orbiting close to or through the ring's core.")
PLANAR ASSEMBLAGE OF ICY PARTICLES ORBITING SATURN
Cassini Division; Encke Division; Encke gap; Encke division; R/2004 S 1; A Ring; B Ring; Crepe Ring; C Ring; D Ring; F Ring; F ring; S/2004 1R; R/2004 S 2; Saturn's rings; Keeler Gap; Keeler gap; Cassini division; Rings of saturn; Maxwell Gap; Saturns rings; Encke Gap; Maxwell Division; Keeler Division; Rings Of Saturn; Crepe ring; Phoebe ring; C-Ring; Propeller moonlet; Bleriot (moonlet); Bleriot (moon); Saturn ring; C Ring of Saturn; E Ring of Saturn; F Ring of Saturn; Methone Ring Arc; Huygens Gap; Huygens Ringlet; Saturn's Rings; Saturnian rings; Saturn rings; Saturn Ring System; Ring system of Saturn; Saturnian Ring System; Ring System of Saturn; Saturn's ring system; Saturn's Ring System; Saturnian ring system; Saturn ring system; Saturn Rings; Saturnian Rings; Phoebe Ring; Saturn’s rings; Roche Division; Janus/Epimetheus Ring; Janus Ring; Epimetheus Ring; A Ring (ring of Saturn); C Ring (ring of Saturn); B Ring (ring of Saturn); D Ring (ring of Saturn); E Ring (ring of Saturn); Colombo Ringlet; G Ring (ring of Saturn); F Ring (ring of Saturn); Colombo Gap; Methone ring arc; Anthe ring arc; Titan Ringlet; Pallene ring; Maxwell Ringlet; Earhart (moon); Earhart (moonlet); Santos-Dumont (moon); Santos-Dumont (moonlet); Saturn's Ring
The rings of Saturn are the most extensive ring system of any planet in the Solar System. They consist of countless small particles, ranging in size from micrometers to meters, that orbit around Saturn.
Saturn
![[[Galileo Galilei]] observed the rings of Saturn in 1610, but was unable to determine what they were](https://commons.wikimedia.org/wiki/Special:FilePath/Galileo.arp.300pix.jpg?width=200 "[[Galileo Galilei]] observed the rings of Saturn in 1610, but was unable to determine what they were")
![Cassini]]''. The rings are visible, including the F Ring.](https://commons.wikimedia.org/wiki/Special:FilePath/Saturn eclipse.jpg?width=200 "Cassini]]''. The rings are visible, including the F Ring.")
![Cassini]]'' in 2007) are the most massive and conspicuous in the Solar System.<ref name="NMM Saturn" />](https://commons.wikimedia.org/wiki/Special:FilePath/Saturn from Cassini Orbiter (2007-01-19).jpg?width=200 "Cassini]]'' in 2007) are the most massive and conspicuous in the Solar System.<ref name=\"NMM Saturn\" />")
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![outer planets]] orbiting around the Sun](https://commons.wikimedia.org/wiki/Special:FilePath/Solar system orrery outer planets.gif?width=200 "outer planets]] orbiting around the Sun")
SIXTH PLANET FROM THE SUN AND THE SECOND-LARGEST PLANET IN THE SOLAR SYSTEM, AFTER JUPITER
Planet Saturn; Saturnus (planet); Saturn's; Saturn (astronomy); Sixth planet; 6th planet; Sol VI; Saturn (Planet); Saturn (planet); Atmosphere of Saturn; Sol-6; Sol 6; Saturno (planet); Weather of Saturn; Structure of Saturn; History of Saturn; Orbit of Saturn; Rotation of Saturn; The planet Saturn; Phainon; Climate of Saturn; Saturnian atmosphere; Saturn’s atmosphere; Cronocentric orbit
·noun The metal lead.
II. Saturn ·noun One of the elder and principal deities, the son of Coelus and Terra (Heaven and Earth), and the father of Jupiter. The corresponding Greek divinity was Kro`nos, later CHro`nos, Time.
III. Saturn ·noun One of the planets of the solar system, next in magnitude to Jupiter, but more remote from the sun. Its diameter is seventy thousand miles, its mean distance from the sun nearly eight hundred and eighty millions of miles, and its year, or periodical revolution round the sun, nearly twenty-nine years and a half. It is surrounded by a remarkable system of rings, and has eight satellites.
Saturn
SIXTH PLANET FROM THE SUN AND THE SECOND-LARGEST PLANET IN THE SOLAR SYSTEM, AFTER JUPITER
Planet Saturn; Saturnus (planet); Saturn's; Saturn (astronomy); Sixth planet; 6th planet; Sol VI; Saturn (Planet); Saturn (planet); Atmosphere of Saturn; Sol-6; Sol 6; Saturno (planet); Weather of Saturn; Structure of Saturn; History of Saturn; Orbit of Saturn; Rotation of Saturn; The planet Saturn; Phainon; Climate of Saturn; Saturnian atmosphere; Saturn’s atmosphere; Cronocentric orbit
¦ noun a planet of the solar system, sixth in order from the sun and circled by broad flat rings.
Derivatives
Saturnian adjective
Wikipedia
The Rings of Saturn
The Rings of Saturn (German: Die Ringe des Saturn: Eine englische Wallfahrt - An English Pilgrimage) is a 1995 novel by the German writer W. G. Sebald. Its first-person narrative arc is the account by a nameless narrator (who resembles the author in typical Sebaldian fashion) on a walking tour of Suffolk. In addition to describing the places he sees and people he encounters, including translator Michael Hamburger, Sebald discusses various episodes of history and literature, including the introduction of silkworm cultivation to Europe and the writings of Thomas Browne, which attach in some way to the larger text. The book was published in English in 1998.
