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MS The Solar System Worksheets
MS The Solar System Worksheets

... Read this passage based on the text and answer the questions that follow. Jupiter Jupiter is the largest planet in our solar system. Its mass is 318 times the mass of Earth, and its volume is more than 1300 times the volume of Earth. Because Jupiter is so large, it reflects a lot of sunlight. When i ...
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ANSWER

... sizes of the terrestrial and gas giant planets? ANSWER: Terrestrial planets are smaller than gas giant planets. 7. What is the difference between the distance between the terrestrial and gas giant planets? ANSWER: The distances between the gas giant planets are much larger than the distances between ...
Getting to Know: Rotation, Orbits, and the Seasons
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... rotates in the opposite direction of Earth, and Uranus is turned on its side so its rotation is at approximately a 90º angle to that of Earth. A few moons and other small bodies in our solar system also turn clockwise. ...
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MIT

... • Since the nearest star is 4.22 light-years away, the Solar System size could extend almost half-way to the nearest star. • Astronomers think that the Sun's gravitational field dominates the gravitational forces of the other stars in the Solar System out to this distance. ...
Untitled
Untitled

... circle; they orbit it in an …………………………………………….. shape. The sun provides light and thermal ……………………………………. The Earth is at the perfect distance from the Sun to allow us to have life on it. It takes ………………… days for the Earth to rotate around the Sun. Eight planets, their satellites and other objects ...
The Dwarf Planets
The Dwarf Planets

... The Dwarf Planets While we can't see most of the objects in the Kuiper belt well enough to determine whether they are round or not, we can estimate how big an object has to be before it becomes round and therefore how many objects in the Kuiper belt are likely round. In the asteroid belt Ceres, wit ...
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leo 1. episode 1

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dwarf planets - Daytona State College
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... well inclined to the plane of the Solar System and so eccentric that it brings Pluto closer to the Sun than Neptune for a few years. Much later, it was found that Pluto is an icy body that reflects light very efficiently. This brought its calculated diameter to just over that of the Moon. Then many ...
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... Why does the Earth go round the Sun? How do we figure out what a planet is made up off? Why do we weigh less on the moon? Why does the Earth have an atmosphere while the moon does not? ...
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... adds the word "classical" to the collective name of Following active discussion among IAU scientists the eight planets Mercury through Neptune. at the IAU 2006 General Assembly in Prague, draft Resolution 6b (issued 16 August 2006) has been Resolution 6A creates for IAU usage a new class of updated ...
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... tiny dot centered in one of those rays of light. X-Ray Sun This is an x-ray movie of the Sun taken from a geosynchronous weather satellite. In addition to monitoring weather on Earth these satellites are also equipped with instruments to monitor the space environment. This movie spans a period of 17 ...
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... Changes in the length and direction of an object’s shadow show the changing position of the Sun during the day although the patterns of the stars in the sky, to include the Sun, stay the same. Orbit- The path an object takes as it moves around another object in space Planet- A large body of rock or ...
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Return Visit Optimization for Planet Finding
Return Visit Optimization for Planet Finding

... Conclusions and Future Work We can draw several important conclusions from the last simulation: • There is no single optimal return strategy: a combination of these (and other) strategies must be employed, along with all available information about the candidate stars, to produce an optimal revisit ...
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... Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto. Scientists commonly divide these into two groups. The terrestrial planets (also called inner planets), Mercury, Venus, Earth and Mars and the gas planets of Jupiter, Saturn, Uranus, and Neptune. Pluto is considered a terrestrial planet ...
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1.10.1.2.SS - WordPress.com

... Its moons are, however, solid planetary bodies that contain geologic wonders. ...
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Planets beyond Neptune



Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and culminated at the start of the 20th with Percival Lowell's quest for Planet X. Lowell proposed the Planet X hypothesis to explain apparent discrepancies in the orbits of the giant planets, particularly Uranus and Neptune, speculating that the gravity of a large unseen ninth planet could have perturbed Uranus enough to account for the irregularities.Clyde Tombaugh's discovery of Pluto in 1930 appeared to validate Lowell's hypothesis, and Pluto was officially named the ninth planet. In 1978, Pluto was conclusively determined to be too small for its gravity to affect the giant planets, resulting in a brief search for a tenth planet. The search was largely abandoned in the early 1990s, when a study of measurements made by the Voyager 2 spacecraft found that the irregularities observed in Uranus's orbit were due to a slight overestimation of Neptune's mass. After 1992, the discovery of numerous small icy objects with similar or even wider orbits than Pluto led to a debate over whether Pluto should remain a planet, or whether it and its neighbours should, like the asteroids, be given their own separate classification. Although a number of the larger members of this group were initially described as planets, in 2006 the International Astronomical Union reclassified Pluto and its largest neighbours as dwarf planets, leaving Neptune the farthest known planet in the Solar System.Today, the astronomical community widely agrees that Planet X, as originally envisioned, does not exist, but the concept of Planet X has been revived by a number of astronomers to explain other anomalies observed in the outer Solar System. In popular culture, and even among some astronomers, Planet X has become a stand-in term for any undiscovered planet in the outer Solar System, regardless of its relationship to Lowell's hypothesis. Other trans-Neptunian planets have also been suggested, based on different evidence. As of March 2014, observations with the WISE telescope have ruled out the possibility of a Saturn-sized object out to 10,000 AU, and a Jupiter-sized or larger object out to 26,000 AU.
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