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Astronomy Club of Asheville May 2016 Sky Events
Astronomy Club of Asheville May 2016 Sky Events

... month. Saturn reaches opposition – closest position to Earth for the year on June 3rd.  Venus, Uranus and Neptune are all too close to the Sun in the sky to observe easily this month.  You will have only one chance to see Mercury this month, and that is during the daytime hours of May 9th when the ...
Distances intheSolar System
Distances intheSolar System

... This figure is the radius of their circle. So this is the distance they need to measure from the central spot. Help each group to draw a circle at the correct distance from the Sun using the measuring tape. The children should mark the distance at least at every quarter of the circle. The greater t ...
The Discovery of Planets beyond the Solar System
The Discovery of Planets beyond the Solar System

... The planet closest to its star moves at only 0.04 of the Earth-Sun distance. The planet moving the farthest away is at 2.8 times the EarthSun distance from its star. In the Solar System, all planets move in near-circular orbits (except Pluto); among the discovered extrasolar planets, almost a third ...
PowerPoint Presentation - Small Bodies in the Solar System
PowerPoint Presentation - Small Bodies in the Solar System

... more than 900 km in diameter - too small to be a planet. • Most asteroids are located in the asteroid belt, between Mars & Jupiter. • Some asteroids that orbit planets are considered moons. • Some astronomers consider them to be minor planets (like the moons of Mars and Saturn). ...
THE SOLAR SYSTEM
THE SOLAR SYSTEM

... Jovian). Pluto is considered by many astronomers to no longer be a planet, since there are now several known objects in orbits similar to Pluto's and of similar size - these are believed to be members of the Kuiper-belt. In addition to the major planets, there are a large number of moons, asteroids, ...
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ph709-09

... COROT-7b (previously named COROT-Exo-7b)[4][5] is a reported exoplanet orbiting around the star COROT-7. It was detected by the French-led COROT mission in 2009. It is the smallest exoplanet to have its diameter measured, at 1.7 times that of the Earth (which would give it a volume 4.9 times Earth's ...
Lecture 4 (pdf from the powerpoint)
Lecture 4 (pdf from the powerpoint)

... If the Sun were suddenly replaced by a solarmass black hole, the Earth would a) move off the current orbit in a straight line b) remain in the same orbit c) move into a smaller orbit d) be pulled into the black hole ...
The Planets - Andrew's Blog
The Planets - Andrew's Blog

... The rest of the missions we’re called the Ulysses, the Cassini, and the New Horizons! How wonderful it is to know most of these mission’s accomplishments and goals so you could get a better recap of them. The planet Jupiter's four largest moons are called the Galilean satellites, after Italian astro ...
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ppt file

... good to <1’ – Duel: who is a better mathematician???? ...
Homes for life
Homes for life

Kepler`s Laws, Newton`s Laws, and the Search for New Planets
Kepler`s Laws, Newton`s Laws, and the Search for New Planets

... now know that everything is moving: the entire solar system is circling the galaxy, the whole galaxy is moving with respect to other galaxies, and roughly speaking, “all motion is relative”—and also for the mathematical reason that we can choose coordinates in which anything we like is fixed. Howeve ...
Universe - Sci-Port
Universe - Sci-Port

... Asteroid: Also called minor planet. Any of the thousands of small bodies from 480 miles (775 km) to less than one mile (1.6 km) in diameter that revolve about the sun in orbits lying mostly between those of Mars and Jupiter. Asteroid Belt: The region of space between the orbits of mars and Jupiter i ...
Anomalous diffusion in generalised Ornstein
Anomalous diffusion in generalised Ornstein

Our Unique Planet - Ball State University
Our Unique Planet - Ball State University

... combination for complex life to exist. There are two planetary attributes that this activity looks at which are necessary for life support: planetary distance from the sun and the size of the planet. One of the most basic needs for the support of life on a planet is liquid water on its surface. Wate ...
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If Earth had no tilt, what else would happen?

... • He observed a supernova in 1572 and with this showed that the heavens were both changing and had a dimension of distance; this troubled scholars who previously thought the heavens were unchanging. • He showed that comets were objects that occurred in the region of the planets, not in Earth’s atmos ...
Orbits and Applications
Orbits and Applications

... A: It generates a gravitational force equal and opposite the earth's pull. B: The net force on it is zero. C: It is beyond the main pull of Earth’s gravity. D: It is being pulled by the Sun and planets as well as by Earth. E: none of the above The moon falls to earth all the time! There is a large f ...
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... because of their composition (what they are made of). They have different colors and different features because of their rocks, their atmosphere (air) and their temperatures. For this lesson, you will find out about the different characteristics of the nine planets in our solar system. ...
Name - Physics
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... The motion of objects orbiting a planet (orbital mechanics) can be described and predicted by combining the relationships between uniform circular velocity, gravitational attraction and centripetal acceleration. a. Use these three relationships to derive two formulas, one for orbital velocity in ter ...
The development of science during the renaissance The
The development of science during the renaissance The

... Ptolomeus said, but in ellipses. Due this he also found out that the planets closer to the sun move faster than planets far away. The last thing he discovered was that the time it took for a planet to go around the sun in one year; so that length of a year could differ between two planets. To prove ...
holiday ho holiday homework
holiday ho holiday homework

... planet at more than two hundred twenty mph. Violent winds shoot sand made of silicate around Venus’s very dry, arid surface. The temperature averages nine hundred degrees, and the pressure’s ninety times that on Earth. It takes two hundred and twenty four days to orbit the sun. Like Mercury, Venus w ...
Chapter 8 Moons, Rings, and Plutoids
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... The first Kuiper belt objects were observed in the 1990s, and more than 700 are now known. Some of them are comparable in size to Pluto. These images show Eris and its moon ...
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... 9. Why did the model of the universe proposed by Copernicus gain support soon after its publication? a. It more accurately predicted the position of planets. b. It gave a better explanation for the phases of the Moon. c. It was a more elegant explanation of retrograde motion. d. The old system of Pt ...
Planetary Orbit Simulator – Student Guide
Planetary Orbit Simulator – Student Guide

... limited the semi-major axis to 50 AU since that covers most of the objects in which we are interested in our solar system and have limited eccentricity to 0.7 since the ellipses would be hard to fit on the screen for larger values. Note that the semi-major axis is aligned horizontally for all ellipt ...
Exploring the Solar System - Rourke Publishing eBook Delivery
Exploring the Solar System - Rourke Publishing eBook Delivery

... to learn about the nature of the universe. Because the universe is so large, astronomers have to use what they know about math and physics to create theories about what is difficult to observe. For instance, physicists know that light travels at 186,282 miles (299,792 kilometers) per second. They ca ...
Voyage: A Journey Through Our Solar System Grades K
Voyage: A Journey Through Our Solar System Grades K

... The Sun is a star. Why does it look so big and bright compared to the other stars? Because it is much closer than the other stars, not because it is bigger—it is only an average sized star. Did the position of Mercury surprise you? Mercury orbits the Sun faster than any other planet (once every 88 d ...
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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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