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Orbital and Physical Characteristics of Extrasolar Planets Systems
Orbital and Physical Characteristics of Extrasolar Planets Systems

... has been made also by the authors of [6–10]; • The previous analyses established that the number of planets increases with the distance from star [1, 9, 11, 12]. The present analysis shows that the distribution of semimajor axis increases considerably to planets, which orbits with à<1AU. Among them ...
Research Paper Trojans in Habitable Zones
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Standard Four: Earth in Space
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... Enduring Understanding: There are observable, predictable patterns of movement in the Earth, Moon, and Sun system that account for day and night. Enduring Understanding: Technology expands our knowledge of the Earth, Moon, and Sun System. All students in Kindergarten will be able Building upon the K ...
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Seventh planet - Copeland Science Online
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Revision sheet - Nour Al Maaref International School
Revision sheet - Nour Al Maaref International School

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OBSERVATIONS (1)
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... On the other hand, the Moon rotates on its axis at exactly the same rate that it revolves around us. That is why we always see the same face. This is not magic, there is a simple physical basis for it called “tidal locking”. Eventually that same basis will apply to Earth as well and we will rotate a ...
CHAPTER 3, Diurnal Motion - The College of New Jersey
CHAPTER 3, Diurnal Motion - The College of New Jersey

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... refract light from the occulted star away from the direction to the observer. In either case, the key uncertainty is the distance between the 1250 km reference radius probed by occultations and the surface, and this distance remains unknown. If we assume that the radius derived from mutual events is ...
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Solar System



The Solar System comprises the Sun and the planetary system that orbits it, either directly or indirectly. Of those objects that orbit the Sun directly, the largest eight are the planets, with the remainder being significantly smaller objects, such as dwarf planets and small Solar System bodies such as comets and asteroids. Of those that orbit the Sun indirectly, two are larger than the smallest planet.The Solar System formed 4.6 billion years ago from the gravitational collapse of a giant interstellar molecular cloud. The vast majority of the system's mass is in the Sun, with most of the remaining mass contained in Jupiter. The four smaller inner planets, Mercury, Venus, Earth and Mars, are terrestrial planets, being primarily composed of rock and metal. The four outer planets are giant planets, being substantially more massive than the terrestrials. The two largest, Jupiter and Saturn, are gas giants, being composed mainly of hydrogen and helium; the two outermost planets, Uranus and Neptune, are ice giants, being composed largely of substances with relatively high melting points compared with hydrogen and helium, called ices, such as water, ammonia and methane. All planets have almost circular orbits that lie within a nearly flat disc called the ecliptic.The Solar System also contains smaller objects. The asteroid belt, which lies between Mars and Jupiter, mostly contains objects composed, like the terrestrial planets, of rock and metal. Beyond Neptune's orbit lie the Kuiper belt and scattered disc, populations of trans-Neptunian objects composed mostly of ices, and beyond them a newly discovered population of sednoids. Within these populations are several dozen to possibly tens of thousands of objects large enough to have been rounded by their own gravity. Such objects are categorized as dwarf planets. Identified dwarf planets include the asteroid Ceres and the trans-Neptunian objects Pluto and Eris. In addition to these two regions, various other small-body populations, including comets, centaurs and interplanetary dust, freely travel between regions. Six of the planets, at least three of the dwarf planets, and many of the smaller bodies are orbited by natural satellites, usually termed ""moons"" after the Moon. Each of the outer planets is encircled by planetary rings of dust and other small objects.The solar wind, a stream of charged particles flowing outwards from the Sun, creates a bubble-like region in the interstellar medium known as the heliosphere. The heliopause is the point at which pressure from the solar wind is equal to the opposing pressure of interstellar wind; it extends out to the edge of the scattered disc. The Oort cloud, which is believed to be the source for long-period comets, may also exist at a distance roughly a thousand times further than the heliosphere. The Solar System is located in the Orion Arm, 26,000 light-years from the center of the Milky Way.
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