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... • This explains the large sizes and low densities of the Jovian planets. • Nebular capture also explains the formation of the diverse satellite systems of the jovian planets. ...
CH .20 The Solar System I. Observing the solar system – sun
CH .20 The Solar System I. Observing the solar system – sun

... 1. Many rings – largest and most visible of all planetary rings a. all gas giants have some rings b. made of ice and small rock 2. moons a. Titan – largest moon in solar system D. Uranus – twice as far from Sun as Saturn 1. not Discovered until 1781 by Herschel 2. rotates sideways 3. many moons E. N ...
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Is Pluto a Planet

... physically meaningful definition under which we'd have nine planets", because at least a half-dozen main-belt asteroids (along with several recently discovered trans-neptunian objects*) are large, spherical objects that would also satisfy definitions of "major planethood" if sphericity is the crite ...
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... The 13 rings and satellites are also in this plane.. There must have been a catastrophic collision with another body to create this situation. However its magnetic axis is tipped over 60 degrees from the axis of rotation. ...
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... The sun’s a star in the Milky Way spinnin’ with the galaxy And the planets orbit ‘round the sun with great velocity. Mercury, Venus, Earth and Mars, the inner planets go Jupiter, Saturn, U-ran-us, Neptune, NOT Pluto! The Solar System, eight planets ‘round the sun Ro-tating and revolving too In orbit ...
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... 4. When a meteoroid enters Earth’s atmosphere, friction causes it to burn up and produce a streak of light called a(n) _______________ . 5. A chunk of ice and dust whose orbit is usually a long narrow ellipse is a(n) _______________. 6. If a meteoroid hits Earth’s surface, it is called a(n) ________ ...
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... countless numbers of small rocks and even large asteroids hurdling aimlessly through space, there are many asteroids and comets. There also seem to be a few larger rocks which aren’t quite planets which seem to be caught revolving around the enormous sun, dwarf planets. NASA states in one of its art ...
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Colburn Earth Science Museum - Asheville Museum of Science

... planets in our solar system, Pluto does not orbit along the same orbital plane. Tilted at 17 degrees, Pluto orbits on a more elliptical path than the 8 planets. Additionally, it crosses another planet’s orbit (Neptune), something no other planet does. For these afore mentioned reasons, Pluto present ...
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... • All other bodies in the Solar system are called SSSB’s – Small Solar System Bodies • These include: – Minor Planets or Asteroids – Kuiper Belt Objects (KBO’s) also known as Trans Neptunian Objects (TNO’s) – Comets ...
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... Terrestrial, Dwarf planets (Planetodal), and Asteroidal. These classifications are listed in order from largest to smallest. Jovian bodies are gas giants. Terrestrial bodies are rocky worlds larger than 1000 km in diameter. Planetodal bodies are rocky with a size between 250 and 1000 km in diameter. ...
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... Uranus is usually one smooth color, but light and dark areas often appear on Neptune. Clouds of methane ice crystals can form high enough in the atmosphere of Neptune to look white. Storm systems can appear in darker shades of blue than the rest of the planet. One storm, seen during the flyby of the ...
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... 11. What do we call the motion of a body as it orbits another body in space? 12. What do we call the time it takes for an object to revolve around the sun once? 13. What are the differences between prograde rotation and retrograde rotation? Which applies to the Earth? 14. Which planet is considered ...
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... 1. How far is Venus from the Sun? Venus is 0.4 astronomical units far from the Sun. 2. How long does the Earth need to make one complete orbit around the Sun? The Earth needs one year to make one complete orbit around the Sun. 3. How long does Uranus need to orbit the Sun? Uranus needs 83.7 years t ...
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... • Pluto’s size was overestimated after its discovery in 1930, and nothing of similar size was discovered for several decades. • Now other large objects have been discovered in Kuiper belt, including Eris. • The International Astronomical Union (IAU) now classifies Pluto and Eris as dwarf planets. • ...
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Solar System Survey

...  Pluto and similar objects don’t fit either planet family  Astronomers have discovered more than 200 objects like Pluto orbiting the Sun  In 2006, a new family was introduced – the dwarf planets  Massive enough to pull themselves spherical  Orbits have not been swept clear of debris ...
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... the Rocky Mountains on Earth. Pluto's surface is also covered in an abundance of methane ice (New Horizons scientists observed significant differences in the way the ice reflects light across the dwarf planet's surface.) a large heart-shaped region known unofficially as ...
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... Sedna for an Inuit goddess who lives at the bottom of the frigid Arctic ocean, approaches the sun only briefly during its 10,500-year solar orbit. It never enters the Kuiper Belt, whose outer boundary region lies at about 55 AU -- instead, ...
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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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