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Solar System Summary Sheet File
Solar System Summary Sheet File

... so much mass that it exerts a very large gravitational pull on the other objects. The shape of the orbit is known as an ellipse. All the objects which orbit the Sun orbit in the same direction of rotation. Asteroids are made of rocky material. Asteroids can be thought of as broken bits of planet i.e ...
Words
Words

... What was the main point of the Planet Nine story? How many planets are there in our solar system? What is the purpose of the Backyard Worlds project? Backyard Worlds is a ________________ science project. What do the eight planets orbit? Which planet is closest to the sun? When was it decided that P ...
Planet Nine
Planet Nine

... What was the main point of the Planet Nine story? How many planets are there in our solar system? What is the purpose of the Backyard Worlds project? Backyard Worlds is a ________________ science project. What do the eight planets orbit? Which planet is closest to the sun? When was it decided that P ...
Newton derives Kepler`s laws
Newton derives Kepler`s laws

... b) What is the kinetic energy of Jupiter in motion around the Sun? ...
14. 1 A Travel Guide to the Outer Planets 14.2 Jupiter 14.3 Saturn
14. 1 A Travel Guide to the Outer Planets 14.2 Jupiter 14.3 Saturn

... Saturn's rings are composed of icy particles ranging in size from boulders to dust. In some regions the ice is purer than in other regions. Grooves and other features in the rings can be produced by resonances w ith moons or by w aves that propagate through the rings. Narrow rings and sharp ring edg ...
Astronomy Assignment #1
Astronomy Assignment #1

... Why would the other methods not be able to find small exoplanets like the Earth? The Transit method has sufficient sensitivity to detect very small planets from the very small dimming of star light as the planets transits across the stars surface. It appears that the Radial Velocity Method may never ...
School Powerpoint Presentation on Planet X 2011
School Powerpoint Presentation on Planet X 2011

... Oort Cloud Anomaly • The Oort cloud is thought to occupy a vast space from ~2,000AU (~0.03 ly) to ~ 50,000 AU (0.79 ly) from the Sun. Some estimates place the outer edge at between 100,000 and 200,000 AU (1.58 and 3.16 ly) • Long-period comets come from the Oort Cloud ...
Pocket Solar System - Faculty Web Sites at the University of Virginia
Pocket Solar System - Faculty Web Sites at the University of Virginia

... closest planet. This only holds true if we treat the asteroid belt like a planet. Why didn’t a planet form at the distance of the asteroid belt? There are two reasons why no planet formed at the distance of the asteroid belt. First, even though there are many asteroids, most are ver ...
Name the eight planets in order by increasing distance from the sun:
Name the eight planets in order by increasing distance from the sun:

... 1. Name the eight planets in order by increasing distance from the sun: A: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune 2. What are two pieces of technology that have helped scientists explore the solar system? A: space shuttles, probes, telescopes 3. What two things combine/balance ...
Lesson Review
Lesson Review

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Chapter 9 Solar System Test Multiple Choice Identify the choice that
Chapter 9 Solar System Test Multiple Choice Identify the choice that

Astrobiology News for July 2013: What Makes a Planet Habitable
Astrobiology News for July 2013: What Makes a Planet Habitable

... the  stars  themselves  experience  strong  flares  and  HZ  planets  would  have  to  orbit   close  enough  to  their  stars  to  be  “tidally  locked”  (meaning  the  same  face  of  the   planet  would  continuously  face  the  st ...
Applications of Light to Astronomy
Applications of Light to Astronomy

... o Observing which wavelengths are missing after reflection tells you about the composition of the reflecting surface! o Observing which wavelengths are missing after passing through material (e.g. atmosphere of a planet or star) tells you about that material ƒ Most of the stuff in the universe is hy ...
WORD - UWL faculty websites
WORD - UWL faculty websites

... o Observing which wavelengths are missing after reflection tells you about the composition of the reflecting surface! o Observing which wavelengths are missing after passing through material (e.g. atmosphere of a planet or star) tells you about that material  Most of the stuff in the universe is hy ...
Spring `03 final exam study guide
Spring `03 final exam study guide

... absolute magnitude white dwarf+ electron degeneracy+ Hertzsprung-Russell diagram planetary nebula+ Chandrasekhar limit+ Supernova+ The following questions might also be asked: 1. What makes the constellations of the zodiac special? 2. Name the planets that are never seen very far from the Sun in the ...
The Other Distant Giants Are Kindred Planets with Individual Quirks
The Other Distant Giants Are Kindred Planets with Individual Quirks

The Solar System
The Solar System

... Astronomers have classified Pluto as a dwarf planet. Dwarf means “small.” Pluto is made of ice. It has a moon almost as large as it is. It takes Pluto 249 years to orbit the sun. ...
Our Amazing Solar System
Our Amazing Solar System

...  Saturn is a very large gas planet which spins very rapidly on its axis. It spins so fast that it flattens out the top and the bottom of the planet. The fast spin also causes Saturn to bulge at its equator. Saturn's atmosphere has winds which can blow at over 1800 kilometers per hour! The white spo ...
Our Amazing Solar System
Our Amazing Solar System

...  Saturn is a very large gas planet which spins very rapidly on its axis. It spins so fast that it flattens out the top and the bottom of the planet. The fast spin also causes Saturn to bulge at its equator. Saturn's atmosphere has winds which can blow at over 1800 kilometers per hour! The white spo ...
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Our Solar system

... the area around its orbit • Gravity is too weak to attract nearby debris • Orbits in a zone with other small bodies • Made of a combination of ice & rock ...
Ch 27-Planets of Solar System
Ch 27-Planets of Solar System

... – 248 yr orbital period, but closer to sun than Neptune about 20 of those yrs – Smaller than Earth’s moon – Frozen methane, rock, and ice – Very thin nitrogen atmosphere ...
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... neighbourhood around their orbit” of similarly sized objects (8 planets) • Dwarf planets are big enough to be spherical due to self-gravity, but have not cleared their orbits of similarly sized objects [think belts], and are not moons of larger objects (Ceres, Pluto, Eris) • All other objects direct ...
Astronomy Unit Notes - sciencepowerpoint.com
Astronomy Unit Notes - sciencepowerpoint.com

... up 90% of the universe; it is invisible (does not absorb or emit light) Dark Energy – A hypothetical form of energy that permeates space and exerts a negative pressure, which would have gravitational effects to account for the differences between the theoretical and observational results of gravitat ...
Are Cool Stars Popular? Better Ask Sol
Are Cool Stars Popular? Better Ask Sol

... surface features such as sunspots, which are cool dark spots on the surface that are footprints of magnetic activity, and the solar wind, which is the flow of particles that get ejected from the sun's outer layers. More ...
Test and answer key  - Solar Physics and Space Weather
Test and answer key - Solar Physics and Space Weather

... A at conjunction—when it appears closest to the Sun. B at maximum eastern or western elongation and is farthest away from the Sun in our sky at sunrise or sunset. C high above our southern horizon at sunrise or sunset. D *at opposition—hence closest to Earth. 17. The zones and belts of Jupiter A *ar ...
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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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