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5) Earth in space and time. The student understands the solar
5) Earth in space and time. The student understands the solar

... A star with a planet will move in its own small orbit in response to the planet's gravity. This leads to variations in the speed with which the star moves toward or away from Earth. I.e. the variations are in the radial velocity of the star with respect to Earth This has been by far the most produc ...
Exploring Our Solar System - Northern Stars Planetarium
Exploring Our Solar System - Northern Stars Planetarium

... that it reflects 100% of the light that hits it; 0.0 means it absorbs 100% of the light or reflects 0% of the light. Our moon’s albedo is a low 0.07, while Venus has a high albedo of 0.7. Asteroid Also called Minor Planets, they are small rocky objects that orbit the Sun. Most (95%) are found in the ...
Solar System Bead Distance Activity
Solar System Bead Distance Activity

... planets as revolving around the Sun, but rarely consider how far each planet is from the Sun. Furthermore, we fail to appreciate the even greater distances to the other stars. Astronomers use the distance from the Sun to the Earth as one “astronomical unit”. This unit provides an easy way to calcula ...
Key Stage 2: Teacher`s Pack
Key Stage 2: Teacher`s Pack

... many years and there are no waste products, until the end of the mission. 8. Which two planets have not been seen on the Planet Path yet? Uranus and Neptune 9. How far away from the Sun is the most distant planet in the Solar System? 4,500 million km (4.5 billion km) 10. There used to be a ninth pla ...
The Family of Stars
The Family of Stars

... without knowing the tilt of its orbit, because Doppler shift tells us only the velocity toward or away from us. • Doppler data give us lower limits on masses. ...
- MrKowalik.com
- MrKowalik.com

... 21. Eccentricity of an ellipse is compared to what special type of ellipse? ____________ ...
The Solar System
The Solar System

... "viper"),[1] is a region of the Solar System beyond the planets extending from the orbit of Neptune (at 30 AU) to approximately 55 AU from the Sun.[2] It is similar to the asteroid belt, although it is far larger—20 times as wide and 20 to 200 times as massive.[3][4] Like the asteroid belt, it consi ...
A lesson on Gravity and the Solar System - ICE-CSIC
A lesson on Gravity and the Solar System - ICE-CSIC

...  P.4 Why the Moon does not fall towards the Earth? ---As sling.  Gravity Earth-Moon: like invisible rope (thread)  How many of did go to Italy?  Where is the center of the Universe?  How many different forces are there in Nature? ---Magnets ...
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Science 8
Science 8

... 13. Ice crystals made of frozen ammonia form the high white clouds. TRUE or FALSE 14. A giant storm called _____________________________________ has lasted for over 100 years. 15. Why does Jupiter have very strong winds? ___________________________________________________ ...
1 Overview of the Solar System - University of Iowa Astrophysics
1 Overview of the Solar System - University of Iowa Astrophysics

... The semimajor axes of the orbits of the Jovian planets are 5.20, 9.54, 19.18, and 30.06 AU, respectively. See Appendix A3 of your book. Jupiter and Saturn are easily visible to the naked eye, and both are in the night sky now. Uranus and Nepture are so far away that they are invisible without binocu ...
File - Miss S. Harvey
File - Miss S. Harvey

... the name given to the four planets beyond Mars: Jupiter, Saturn, Gas giants Uranus, and Neptune; also known as the outer planets; their atmospheres consist mainly of hydrogen and helium gases the name given to the four planets closest to the Sun: Mercury, Venus, Earth, and Mars; also known as the te ...
Orientation and Conferencing Plan Stage 1
Orientation and Conferencing Plan Stage 1

... numbers. If you spin one of those numbers, go back to 19. ...
Planet Finding
Planet Finding

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Chapter 22

... SUN – FUSION – atoms FUSE together **It is estimated that the sun has enough mass for nuclear fusion to continue for 5 billion more years! ...
Part 2: Solar System Formation
Part 2: Solar System Formation

... (planetesimals) may stick together. • In the outer parts of the Solar Nebula the planets become large enough to have a significant gravitational pull and collect gas around them. – Ice is ten times more abundant than silicates and iron compounds, therefore there is more planet building material in t ...
Our solar system - astronomyuniverse
Our solar system - astronomyuniverse

... By studying meteorites, which are thought to be left over from this early phase of the solar system, scientists have found that the solar system is about 4.6 billion years old! ...
Ethan - St. Brigid
Ethan - St. Brigid

... ©At least 16 moons. ©It has two rings. ©12 earth years is one year. ©One day is 9.8 hours. ...
The Outer Planets
The Outer Planets

... • a great storm in the southern hemisphere called the “Great Dark Spot" is about half the size of Jupiter's Great Red Spot • Spot is about the same diameter as the Earth • at least one other smaller storm spot has been detected. • Neptune has the fastest planetary winds in the Solar System, reaching ...
Periodic mass extinctions and the Planet X model reconsidered
Periodic mass extinctions and the Planet X model reconsidered

... albedos. Pluto’s average albedo is 0.58. If Planet X has a low albedo of say 0.05 then the relative reflected flux would be further reduced to 0.024, making it about 4 magnitudes dimmer than Pluto, or magnitude 18.5. A planet of visual magnitude 16 - 18.5 currently located well out of the ecliptic c ...
Today`s Powerpoint
Today`s Powerpoint

... The sun will cross in front of the center of the Milky Way But this has happened many times before No significant increase in gravitational interaction ...
Our Solar System
Our Solar System

...  12 known moons  Triton largest moon  Great Dark Spot thought to be a hole, similar to the hole in the ozone layer on Earth ...
Make a Solar System necklace!
Make a Solar System necklace!

... large storms in its atmosphere - one of them is the “Great Red Spot” observed by large telescopes and shown in most photos and illustrations of Jupiter. Jupiter is often the third brightest object in the night sky and has 4 large moons that can be easily seen with small telescopes like you might hav ...
Rings, Moons, etc
Rings, Moons, etc

... If a large moon, held together by gravity, gets too close to Saturn, tidal force breaks it into pieces, at a radius called the Roche Limit. Rings inside Roche Limit => pieces can’t reassemble into moon. Not clear whether rings are as old as Saturn or much younger (about 100 million years). Collision ...
PATTERNS OF MASS AND DENSITY IN THE SOLAR SYSTEM
PATTERNS OF MASS AND DENSITY IN THE SOLAR SYSTEM

... Why are the inner and outer planets densities so different? Consider both what you found out on your graph and also what you know about composition to support your statements ...
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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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