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Grade 8 Earth/Space Posttest
Grade 8 Earth/Space Posttest

... ____ 23. The heliocentric model over time replaced the geocentric model as the explanation that astronomers accepted for their observed movements of planet, stars, and other objects in the sky. Which statement best explains the basic principles of the heliocentric model? A. The heliocentric model sh ...
Asteroids, Comets & Meteors Teacher's Guide
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... as they fall through Earth’s upper atmosphere. 99.9% of all meteors seen are very small rocks no larger than single grains of sand or even specks of dust. The small particles are often the remains of dust and pebbles released from comets. The 0.1% remaining meteors are often larger and burn much bri ...
Comet Lulin - indstate.edu
Comet Lulin - indstate.edu

... Since Comet Lulin will be moving opposite the motion of the Earth, it will appear to approach us and move away especially fast. Beginning in February 2009, Comet Lulin will rise at about midnight local time, and will be about 6th or 7th magnitude. This won't be bright enough to go out and look at ...
A Survey for “Normal” Irregular Satellites Around Neptune: Limits to
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... the infrared.[3] This system falsifies the idea that disks create Earth sized objects because the proto-planetary disk model absolutely requires that the disk be present for millions of years.[4] The infrared glowing is simply the result of a series of giant collision events that create trillions of ...
The Star Finder Book - Starpath School of Navigation
The Star Finder Book - Starpath School of Navigation

... special training. The problem with cloudy skies we cover here is that of identifying unknown stars in isolated patches of clear sky. Such stars may be in view for a few minutes only, just long enough to get a sextant sight of them. New navigators soon learn that these unknown stars may offer the onl ...
New Light on the Solar System
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... On the scale of the Milky Way, 100,000 light-years across, our solar system can seem like a puny rut in which to be stuck. Having glimpsed countless exotic stars and galaxies, surely the human imagination will rapidly weary of just one yellow sun, eight or nine planets (depending on your feelings ab ...
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... contained in Ceres, the largest object and the only dwarf planet in the asteroid belt. Add in Vesta, Pallas, and Hygiea, the next three largest asteroids, and half the belt’s mass is accounted for. The main belt starts at 2.06 AU, where objects make four orbits around the Sun in the time it takes Ju ...
Comets, the Kuiper Belt and the Oort Cloud
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... of the planet Neptune wherein there have now been observed on the order of 2000 bodies orbiting the sun. In reality these should be simply referred to as trans-Neptunian objects (TNOs) because there is no good reason to suppose that our solar system abruptly stops at the orbit of Pluto. The first KB ...
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... It was named after the Greek god Neptune. During the Greek mythology times, astronomers named the 4 inner planets after the most important gods. Astronomers eventually found the outer planets and keep the tradition of naming them after the gods. Once they got to Neptune, they decided to name it afte ...
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... you do not know a single star in the sky, the NexStar will have you aligned in minutes by asking for basic information like the date, time and location. Then you simply need to aim the telescope to any three bright celestial objects in the sky. Since SkyAlign requires no knowledge of the night sky i ...
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... white dwarfs is orbiting each other at only 50,000 miles (1/5th the distance to the moon) every 5 minutes at an orbital speed of one million miles per hour. The orbit period is decreasing by 1.2 milliseconds/year which means they are moving closer to each other by 2 feet every day. This system shoul ...
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... ____ 29. Parallax is the apparent change in location of an object due to the motion of the observer. ____ 30. Both Stonehenge and the Big Horn Medicine Wheel contain alignments that indicate the summer solstice sunrise. ____ 31. Many classical astronomers believed Earth could not move because they d ...
1 We finished our last lecture by examining the “Jovian planets” of
1 We finished our last lecture by examining the “Jovian planets” of

... Many other very large Kuiper Belt objects were soon discovered, but because these bodies are so similar to the comets of the Kuiper Belt – and so different from the terrestrial and Jovian planets – only a few astronomers (mostly those associated with their discovery!) really suggested thinking of th ...
A magnetic communication scenario for hot Jupiters
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... assuming the stellar magnetic dipole to be tilted, but fails to do so also for υ And. As pointed out by McIvor et al. (2006), the scenario is complicated when Alfvén waves are taken into account, as during their travel time to the star, the planet moves a non-negligible distance along its orbit. In ...
A new method to determine the mean density of massive Solar
A new method to determine the mean density of massive Solar

... Over several decades, many researchers have been studying mean densities of celestial bodies. The enormous work has resulted in the gravitational and non-gravitational methods to estimate the mean densities, as well as in numerous estimates and analyses of the mean densities of a variety of objects: ...
Volume 19 Issue 1 – January/February 2017 Edition
Volume 19 Issue 1 – January/February 2017 Edition

... Kepler proposed light spreads out from a point, and that its  intensity decreases the farther it travels from its source [4].  An illustra on of this is that Jupiter being about five  mes  more distant from the Sun than the Earth is, each square  meter on Jupiter gets only one twenty-fi h of the Sun ...
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Definition of planet



The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies. Greek astronomers employed the term asteres planetai (ἀστέρες πλανῆται), ""wandering stars"", for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different objects, from the Sun and the Moon to satellites and asteroids.By the end of the 19th century the word planet, though it had yet to be defined, had become a working term applied only to a small set of objects in the Solar System. After 1992, however, astronomers began to discover many additional objects beyond the orbit of Neptune, as well as hundreds of objects orbiting other stars. These discoveries not only increased the number of potential planets, but also expanded their variety and peculiarity. Some were nearly large enough to be stars, while others were smaller than Earth's moon. These discoveries challenged long-perceived notions of what a planet could be.The issue of a clear definition for planet came to a head in 2005 with the discovery of the trans-Neptunian object Eris, a body more massive than the smallest then-accepted planet, Pluto. In its 2006 response, the International Astronomical Union (IAU), recognised by astronomers as the world body responsible for resolving issues of nomenclature, released its decision on the matter. This definition, which applies only to the Solar System, states that a planet is a body that orbits the Sun, is massive enough for its own gravity to make it round, and has ""cleared its neighbourhood"" of smaller objects around its orbit. Under this new definition, Pluto and the other trans-Neptunian objects do not qualify as planets. The IAU's decision has not resolved all controversies, and while many scientists have accepted the definition, some in the astronomical community have rejected it outright.
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