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Diameter of iapetus

WebPhoebe (/ ˈ f iː b i / FEE-bee) is the most massive irregular satellite of Saturn with a mean diameter of 213 km (132 mi). It was discovered by William Henry Pickering on March 18, 1899 from photographic plates that had been taken starting on 16 August 1898 at the Boyden Station of the Carmen Alto Observatory near Arequipa, Peru, by DeLisle … WebFeb 22, 2012 · Here's the fairy tale: As Iapetus was forming, very far from Saturn, it either captured a 100-kilometer-diameter satellite or suffered a giant impact whose debris …

Phoebe (moon) - Wikipedia

WebIapetus has a diameter of 1471 kilometers (914 miles). The right-hand panel, released previously as PIA08384 , shows a mosaic of 60 different images, obtained on September … WebDec 19, 2024 · Tethys is Saturn's fifth largest moon. Its irregular shape is 331 miles (533 kilometers) in mean radius, with dimensions 669 x 657 x 654 miles (1076.8 x 1057.4 x … pools by lowell inc https://northernrag.com

Iapetus (moon) - Wikipedia

WebOct 5, 2024 · Its equator has a diameter of 1,492 kilometers compared to its pole-to-pole diameter of just 1,424 kilometers, which would represent hydrostatic equilibrium if … http://www.seasky.org/solar-system/saturn-moons.html WebA proto-Hyperion could have been 350–1,000 km (220–620 mi) in diameter (which ranges from a little below the size of Mimas to a little below the size ... that got past Iapetus. Hyperion is redder than Phoebe and closely matches the color of the dark material on Iapetus. Hyperion has a porosity of about 0.46. Although Hyperion is the eighth ... pools by lagasse

NASA - Iapetus in 3D

Category:Iapetus Article about Iapetus by The Free Dictionary

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Diameter of iapetus

NASA - Saturn

Iapetus is a moon of Saturn. It is the 24th of Saturn’s 83 known moons. With an estimated diameter of 1,469 km, it is the third-largest moon of Saturn and the eleventh-largest in the Solar System. Named after the Titan Iapetus, the moon was discovered in 1671 by Giovanni Domenico Cassini. A relatively low-density body made up mostly of ice, Iapetus is home to severa… WebIapetus (/ a ɪ ˈ æ p ɪ t ə s /) is ... The largest, Turgis, has a diameter of 580 km (360 mi); its rim is extremely steep and includes a scarp about 15 km (9.3 mi) high. Iapetus is known to support long-runout landslides or sturzstroms, possibly supported by ice sliding. Enhanced-color map (27.6 MB). The leading hemisphere is at the right.

Diameter of iapetus

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WebJan 10, 2005 · With a diameter of about 1,400 kilometers (890 miles), Iapetus is Saturn’s third largest moon. It was discovered by Jean-Dominique Cassini in 1672. It was Cassini, for whom the Cassini-Huygens ... WebThe Solar System is the gravitationally bound system of the Sun and the objects that orbit it. It formed 4.6 billion years ago from the gravitational collapse of a giant interstellar molecular cloud.The vast majority (99.86%) of the system's mass is in the Sun, with most of the remaining mass contained in the planet Jupiter.The planetary system around the Sun …

WebIapetus is an elder Titan born from the primordial gods Uranus and Gaia. His parents were some of the first two beings to exist. According to “The Illiad” by Homer, he almost didn’t … WebIapetus has a diameter of 1471 kilometers (914 miles). The right-hand panel, released previously as PIA08384 , shows a mosaic of 60 different images, obtained on September 10, 2007. The left-hand panel is a color composite of three images obtained through infrared, green and ultraviolet spectral filters (centered at 752, 568 and 338 nanometers ...

WebOct 19, 2024 · Mean diameter: 914 miles (1,470 km) Iapetus features a high-contrast surface of light and dark. As such, it has been dubbed the yin and yang of the Saturn moons. Iapetus, like Rhea, is thought to ... WebStudy with Quizlet and memorize flashcards containing terms like What causes the leading side of Saturn's small moon Iapetus to differ from its trailing side?, In which way does Saturn differ from Jupiter?, How did Uranus and Neptune come to have less hydrogen and helium than Jupiter and Saturn? and more.

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WebUsing Zircon Isotope Compositions to Constrain Crustal Structure and Pluton Evolution: the Iapetus Suture Zone Granites in Northern Britain shared datingWebCassini's flyby of Iapetus in 2007 also postulated a third theory, which is thermal segregation. Iapetus only rotates once every 79 days or so, stretching out the daily temperature cycle. shared ddcWebSep 15, 2024 · Saturn and its rings and all of its moons interior to Iapetus orbit in the same plane: tilted 26.7 degrees relative to the Sun. Iapetus, ever the outlier with its equatorial ridge highlighted here ... shared data warehouse dodWebDec 10, 2009 · Published: December 10, 2009. Three different false-color views of Saturn's moon Iapetus show the boundary of the global "color dichotomy" on the hemisphere of this moon facing away from Saturn. The "color dichotomy," which has been detected in images from the Cassini imaging team, is a second global pattern found on Iapetus besides the … pools by ron schulzWebDec 10, 2009 · Iapetus has a diameter of 1471 kilometers (914 miles). The right-hand panel, released previously as PIA08384 , shows a mosaic of 60 different images, obtained on September 10, 2007. The left-hand panel … shared days wiltshireWebAtlas [AT-lus] is the second of Saturn's known moons. It was named after the Titan condemned by Zeus to carry the heavens on his shoulders. He was the son of Iapetus and the nymph Clymene and brother of Prometheus and Epimetheus. Atlas was discovered by R. Terrile in 1980 using images received from the Voyager spacecraft. poolsbyround.comWebDec 17, 2004 · Iapetus' Dark Side November 16, 2004 Full-Res: PIA06521 This image shows the dark, leading hemisphere of the mysterious moon Iapetus. The dark area is the Cassini region, named for Giovanni Cassini, who discovered the moon in 1672. The diameter of Iapetus is 1,436 kilometers (892 miles). Cassini noted that he was able to … shared db documents - all documents