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Our Solar System
Our Solar System

... Very similar to Jupiter as far as atmospheric conditions. Most prominent ring system (about 1000 rings) a) the total ring thickness is 40,000 km b) each ring is about 100 m thick c) particles in the ring are mostly icy particles, the size of buses. 3. Rings were discovered by Galileo in 1610. 4. The ...
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Toilet Paper Solar System

... Interplanetary travel is extremely difficult due to the almost unimaginable distances between the planets in our solar system. Voyager II, traveling at nearly 50,000 mph took 12 years to reach the planet Neptune! This gives you an idea of just how far our planets are from each other. However, we can ...
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Solar System Drawing Example-Word

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... Jupiter. A “failed planet” kept from forming by Jupiter’s gravitational tugs. Cratered, and rocky. Not large enough for gravity to pull them into round shapes. ...
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Solar System Notes

... Uranus and Neptune  Uranus revolves around the Sun once about every 84 years.  Both Uranus and Neptune have a core of rocky material surrounded by water and ice.  Uranus and Neptune have an atmosphere of hydrogen and helium  Average temperature on Uranus is-210 OC (-350 OF)  Average temperatur ...
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The Solar System - MHS-Integrated
The Solar System - MHS-Integrated

... Nebula are cosmic clouds of gas and dust floating in space. Nebulae are the basic building blocks of the universe. They contain the elements from which stars and solar systems are ...
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... Mars tilts the same as Earth and allows it to have seasons also. They have volcanoes; however they have not been activated because Mars does not have moving tectonic plates as Earth does. It is believe that water once exited on Mars in a liquid state due to erosion. ...
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... planets in their places. 13. The time it takes for the earth to go round the sun. 15. A group of stars. 17. This is caused by a shadow and causes either the sun or the moon not to be seen. 19. The planet nearest the sun. 20. The 8th planet from the sun. It spins in a different direction from the oth ...
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... In 1992, Pluto’s orbit was recognized to be part of the Kuiper belt. With more than 200 million Kuiper belt objects, Pluto has failed the test of clearing other bodies out its orbit. From what you’ve read above, do you think Pluto should be called a planet? Why are people hesitant to take away Pluto ...
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... Earth is a little larger than Venus, but the scale size is still pretty close to the size of a quarter. Earth, our home planet, is the only planet in our solar system known to harbor life. All of the things we need to survive are provided under a thin layer of atmosphere that separates us from the u ...
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AIM: What is Astronomy? Do Now:

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... 1. What is the order of the planets in our solar system? Ask students to arrange in order. Correct order is: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto. 2. Name key characteristics of each planet and how the sizes the planets compare to each other.  Earth- only planet to s ...
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... Revolving and Rotating Our Solar System is made up of one star, planets, moons, asteroids and comets. We used to have nine planets but now we only have eight. Most diagrams still show Pluto. Pluto doesn't fit with the definition of a planet – it is too small. One part of the definition of a planet i ...
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... Revolving and Rotating Our Solar System is made up of one star, planets, moons, asteroids and comets. We used to have nine planets but now we only have eight. Most diagrams still show Pluto. Pluto doesn't fit with the definition of a planet – it is too small. One part of the definition of a planet i ...
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AST111, Lecture 1b

... Center and JPL’s Solar System Dynamics Group. • MPL is a good site to get locations of comets and asteroids. • If you find a new object you report your observations to this site and they help you calculate the orbital elements. This allows others to find the object again later. Minor Planet Electron ...
The Solar System
The Solar System

... • A solar system consists of a star and objects that revolve around it. • Our Solar System consists of the Sun and nine known planets and the moons that orbit those planets. • The force of gravity keeps planets in orbit around the sun. ...
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... o Used perfect circles to represent the orbits of the planets.  There was a problem though! The planets seemed to stray from their predicted positions….wonder why? SEE KEPLER! Brahe - 1546-1601 (Denmark)  Brahe’s observations, especially of Mars, were far more precise than any made previously.  T ...
Chapter 29 Our Solar System
Chapter 29 Our Solar System

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The Planets

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Section 2: Inner Planets

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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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