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Worcester Public Schools
Worcester Public Schools

... Essential Questions: 1.What planets make up the solar system? 2. What are the different sizes, densities, temperatures, and compositions of each planet in the solar system and how do they compare to Earth? 3. What are the different orbits, rotations, and distances from the sun of each planet in the ...
Goal: To understand life in our universe.
Goal: To understand life in our universe.

Mountain Skies - Pisgah Astronomical Research Institute
Mountain Skies - Pisgah Astronomical Research Institute

... moves away from it but still outshines any of the stars in the sky. The observer with a good telescope can still make out some of the markings on the surface. (With the exception of Mercury, Mars is the only planet whose surface marking can be observed from the earth and even they are sometimes obsc ...
How Planets Form (990L)
How Planets Form (990L)

... In addition, all the planets proceed along their orbits in the same direction. It's not that some go clockwise and others go counterclockwise. They're like horses on a carousel, all aimed the same way. These facts convince astronomers that the solar system began when a large, cold lump of interstell ...
Lecture 1: Properties of the Solar System Properties of the Solar
Lecture 1: Properties of the Solar System Properties of the Solar

... Large size, low density and in outer solar system: Jupiter, Saturn, Uranus, Neptune. ...
Chap. 4: Gravitation and the Waltz of the Planets
Chap. 4: Gravitation and the Waltz of the Planets

... Why did Copernicus (1473-1543) think that the Earth and the other planets go around the Sun? How did Tycho Brahe (1546-1601) attempt to test the ideas of Copernicus? What paths do the planets follow as they move around the Sun? Johannes Kepler (1571-1630) What did Galileo (1564-1642) see in his tele ...
History of astronomy - Part I.
History of astronomy - Part I.

... or a trillionth of a second after the Big Bang by carrying ...
Newton*s Theory of Gravity and Planetary Motion
Newton*s Theory of Gravity and Planetary Motion

Science 9 Unit 5: Space Name
Science 9 Unit 5: Space Name

... remote-controlled ‘landers’ that put equipment on or close to planets where no human has gone before. Probes have done remote sensing on Mercury and Jupiter, taken soil samples on Mars, landed on Venus, and studied Saturn’s rings up close. The most recent probes to explore Mars are still there. The ...
Making the Cards - Teaching Made Practical
Making the Cards - Teaching Made Practical

... Use the information from the trading cards to answer the questions below. Create a chart, putting the planets in order from least number of moons to greatest number of ...
The Earth in the Universe
The Earth in the Universe

... • When a moon orbits a planet, or a planet orbits a star, both bodies are orbiting around a point that lies outside the larger body. • The moon does not orbit the exact center of the Earth, but a point about 1710 km below the Earth’s surface. • The sun is not stationary in the solar system. It moves ...
localhost
localhost

... density of Mercury (Mercury seems to have been larger at one point, but might have underwent a collision sometime after the planet differentiated. This would account for the size of Mercury’s iron core and high density.) - the peculiar rotation of Uranus (its rotation axis is tilted such that its eq ...
our solar system - brinson1to1presentation
our solar system - brinson1to1presentation

... People didn’t know how the Earth orbited the Sun. They thought the Sun orbited the Earth. But it really was the other way around. Neptune is more than two billion miles from the Earth. It has a Great Dark Spot similar to Jupiter’s Red Spot. Not all astronomers use telescopes. Some use mathematics. T ...
The Motions of Celestial Bodies, and Newton`s Laws of Motion
The Motions of Celestial Bodies, and Newton`s Laws of Motion

... The orbits of the planets are ellipses, with the Sun at one focus of the ellipse. Planets move proportionally faster in their orbits when they are nearer the Sun (cover equal areas in equal time. More distant planets take proportionally longer to orbit the Sun ...
Presentazione di PowerPoint - Istituto Nazionale di Fisica
Presentazione di PowerPoint - Istituto Nazionale di Fisica

Understanding the Solar System
Understanding the Solar System

... Day 1: Introduce the eight planets to the class. Ask what the students already know about planets. Have a brief class discussion about the planets. Hand out the “Introduction to the Solar System” sheet for students to follow along with; then explain to the students about the solar system (found on h ...
Is Pluto a planet or a Kuiper Belt comet?
Is Pluto a planet or a Kuiper Belt comet?

... • Kuiper Belt objects have been found that approach Pluto’s size. • Kuiper Belt comets have similar orbital resonances with Neptune. • Kuiper Belt comets can have moons. • Triton (a captured moon) is even larger than Pluto. ...
tremaine_stanford
tremaine_stanford

... Kozai oscillations • now subject the orbit to a weak, time-independent external force • because the orbit orientation is fixed even weak external forces can act for a long time in a fixed direction relative to the orbit and therefore change the angular momentum or eccentricity • if Fexternal / ² th ...
Neptune
Neptune

... discovered Nereid Was discovered by Gerard P. Kuiper in 1949. The third moon named Larissa was first observed by Harold J. Reitsema, William B. Hubbard, Larrt A. Lebofsky and David J. Tholen on May 24, 1981. The Voyager 2 discovered 5 inner moons Naiad, Thalassa, Despina Glatea and Proteus. In 2002 ...
Find the Sun9/16/2010 - Home
Find the Sun9/16/2010 - Home

The Ceres Connection - MIT Lincoln Laboratory
The Ceres Connection - MIT Lincoln Laboratory

... Classes of Minor Planets Minor planets represent material left over from the formation of the solar system, most likely material that never coalesced into a planet because of Jupiter’s gravitational influence. The estimated total mass of all the minor planets is much less than that of Earth’s Moon. ...
Transits
Transits

... http://www.nasa.gov/mission_pages/spitzer/news/070221/index.html ...
planet research paper
planet research paper

... Something Special: Is there anything special about your planet? This can often be the best part of the report, taking you off on interesting topics. For example, are there 100-year-long storms on your planet? Are there giant volcanos? Does your planet have a very tilted axis (giving it extreme seaso ...
Question 1
Question 1

... • Planets whose orbits are between the Sun and the asteroid belt as inner planets and those beyond the asteroid belt as outer planets. ...
chapter 8 Notes
chapter 8 Notes

... •  Planets whose orbits are between the Sun and the asteroid belt as inner planets and those beyond the asteroid belt as outer planets. •  The other system classifies planets whose orbits are between Earth’s orbit and the Sun as inferior planets, and those whose orbits are beyond Earth’s orbit as su ...
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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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