Saturn"s rings - определение. Что такое Saturn"s rings
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Что (кто) такое Saturn"s rings - определение

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
  • Detail of Galileo's drawing of [[Saturn]] in a letter to Belisario Vinta (1610)
  • ''Cassini'' space probe view of the unilluminated side of Saturn's rings (May 9, 2007).
  • Mimas]].
  • Near Saturn's equinox, Daphnis and its waves cast shadows on the A Ring.
  • Location of the first four moonlets detected in the A ring.
  • Huygens' ring theory in ''Systema Saturnium'' (1659)
  • Spitzer]] image of part of the ring
  • Pan]]'s orbit, implying its particles oscillate in [[horseshoe orbit]]s.
  • View of the outer C Ring; the Maxwell Gap with the Maxwell Ringlet on its right side are above and right of center. The Bond Gap is above a broad light band towards the upper right; the Dawes Gap is within a dark band just below the upper right corner.
  • The small moons Pandora (left) and Prometheus (right) orbit on either side of the F ring. Prometheus acts as a ring shepherd and is followed by dark channels that it has [http://ciclops.org/view.php?id=3806 carved] into the inner strands of the ring.
  • gallery]]).
  • Anthe]]
  • E]] rings.
  • A ''Cassini'' image of the faint D Ring, with the inner C Ring below
  • The Roche Division (passing through image center) between the A Ring and the narrow F Ring. Atlas can be seen within it. The Encke and Keeler gaps are also visible.
  • The illuminated side of Saturn's rings with the major subdivisions labeled
  • F Ring]].
  • C Ring]] is just inside the B Ring.
  • A 2007 artist impression of the aggregates of icy particles that form the 'solid' portions of Saturn's rings. These elongated clumps are continually forming and dispersing. The largest particles are a few meters across.
  • The outer rings seen back-illuminated by the [[Sun]]
  • Lo-res version of this video]]
  • Simulated appearance of Saturn as seen from Earth over the course of one Saturn year
  • 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 <&nbsp;5 cm (all signals similarly attenuated). Green and blue (C, outer A Ring) mean particles <&nbsp;5 cm and <&nbsp;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.
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         
  • left
  • [[Galileo Galilei]] observed the rings of Saturn in 1610, but was unable to determine what they were
  • Auroral lights at Saturn's north pole
  • ''Pioneer 11'' image of Saturn
  • Artist conception of Saturn, its rings and major icy moons—from Mimas to Rhea
  • Amateur telescopic view of Saturn
  • left
  • left
  • Diagram of Saturn, to scale
  • 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" />
  • 41px
  • Simulated appearance of Saturn as seen from Earth (at opposition) during an orbit of Saturn, 2001–2029
  • 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         
  • left
  • [[Galileo Galilei]] observed the rings of Saturn in 1610, but was unable to determine what they were
  • Auroral lights at Saturn's north pole
  • ''Pioneer 11'' image of Saturn
  • Artist conception of Saturn, its rings and major icy moons—from Mimas to Rhea
  • Amateur telescopic view of Saturn
  • left
  • left
  • Diagram of Saturn, to scale
  • 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" />
  • 41px
  • Simulated appearance of Saturn as seen from Earth (at opposition) during an orbit of Saturn, 2001–2029
  • 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 a planet of the solar system, sixth in order from the sun and circled by broad flat rings.
Derivatives
Saturnian adjective

Википедия

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.