Liis Lepik
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Iowa Highway 186 (1930-1980)
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Natalya Zhedik
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Asmaaffan
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Lepricavark
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List of indoor arenas in the Philippines
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List of Love You Two episodes
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Iowa Highway 152 (1926-1980)
contributor: AnomieBOT
language: en
type: Document
primary topic: Iowa Highway 152 (1926-1980)

LoC.gov
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Mark Steketee
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Vivek Oberoi
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Ranu Mondal
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birth year: 1960
birth date: 1960-11-05
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Sawol
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Arslan-San
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Iowa Highway 152 (1926-1980)
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Cochrane (surname)
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Ninjago: Masters of Spinjitzu (TV series)
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Bogger
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LoC.gov
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contributor: Bogger

CD Lugo
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Iowa Highway 186 (1930-1980)
contributor: AnomieBOT
type: Document
language: en
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AnomieBOT
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Uttaran
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Oort cloud
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comment: The Oort cloud (), named after the Dutch astronomer Jan Oort, sometimes called the Öpik–Oort cloud, is a theoretical cloud of predominantly icy planetesimals proposed to surround the Sun at distances ranging from 2,000 to 200,000 au (0.03 to 3.2 light-years). It is divided into two regions: a disc-shaped inner Oort cloud (or Hills cloud) and a spherical outer Oort cloud. Both regions lie beyond the heliosphere and in interstellar space. The Kuiper belt and the scattered disc, the other two reservoirs of trans-Neptunian objects, are less than one thousandth as far from the Sun as the Oort cloud.
abstract: The Oort cloud (), named after the Dutch astronomer Jan Oort, sometimes called the Öpik–Oort cloud, is a theoretical cloud of predominantly icy planetesimals proposed to surround the Sun at distances ranging from 2,000 to 200,000 au (0.03 to 3.2 light-years). It is divided into two regions: a disc-shaped inner Oort cloud (or Hills cloud) and a spherical outer Oort cloud. Both regions lie beyond the heliosphere and in interstellar space. The Kuiper belt and the scattered disc, the other two reservoirs of trans-Neptunian objects, are less than one thousandth as far from the Sun as the Oort cloud. The outer limit of the Oort cloud defines the cosmographical boundary of the Solar System and the extent of the Sun's Hill sphere. The outer Oort cloud is only loosely bound to the Solar System, and thus is easily affected by the gravitational pull both of passing stars and of the Milky Way itself. These forces occasionally dislodge comets from their orbits within the cloud and send them toward the inner Solar System. Based on their orbits, most of the short-period comets may come from the scattered disc, but some may still have originated from the Oort cloud. Astronomers conjecture that the matter composing the Oort cloud formed closer to the Sun and was scattered far into space by the gravitational effects of the giant planets early in the Solar System's evolution. Although no confirmed direct observations of the Oort cloud have been made, it may be the source of all long-period and Halley-type comets entering the inner Solar System, and many of the centaurs and Jupiter-family comets as well. The existence of the Oort cloud was first postulated by Estonian astronomer Ernst Öpik in 1932. Oort independently proposed it in 1950.
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List of awards and nominations received by J Balvin
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Lugnuts
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