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TTh HW03 key
TTh HW03 key

Objective – I can describe and explain the forces that keep objects in
Objective – I can describe and explain the forces that keep objects in

lec03_30sep2011
lec03_30sep2011

... -~7% of solar-type stars have >Mj planets in the “terrestrial planet” region. Extrapolation of current incompeteness suggests >12% w/planets @ <20 AU. - multiple planetary systems are ~common - planetary resonances are ~common ...
UT 3.4 - Homeschool Academy
UT 3.4 - Homeschool Academy

... surfaces. Because these four planets are all so large, they are often called the gas giants. The fifth outer planet, Pluto, is small and rocky, like the terrestrial planets. Like the sun, the gas giants are composed mainly of hydrogen and helium. Because they are so massive, they exert a much strong ...
(1) Why is the Pleiades star cluster visible all night around
(1) Why is the Pleiades star cluster visible all night around

... in middle of night, and at dawn. These two charts of the orbits of the planets, one showing Mercury through Mars, and the other Mercury through Saturn, depict the view as seen from the north side, or “above” the solar system. In these views, the direction of revolution of the planets about the Sun i ...
d. Demonstrate the relative size and order from the sun of the
d. Demonstrate the relative size and order from the sun of the

... a. Venus, Earth, Mars, Mercury b. Mercury, Earth, Venus, Mars c. Mercury, Venus, Earth, Mars d. Earth, Mercury, Mars, Venus Answer: c What is the order of the planets, starting with the planet closest to the Sun? a. Mercury, Venus, Earth, Jupiter, Mars, Saturn, Neptune, Uranus b. Mercury, Venus, Ear ...
Homework 2
Homework 2

... Earth is closer to the Sun in January than in July. Therefore, in accord with Kepler’s second law: (a) Earth travels faster in its orbit around the Sun in July than in January. (b) Earth travels faster in its orbit around the Sun in January than in July. (c) It is summer in January and winter in Jul ...
Question 1:
Question 1:

Unit 3 *The Solar System* 6th Grade Space Science
Unit 3 *The Solar System* 6th Grade Space Science

... System by characteristics, such as: shape, and appearance, what they orbit, how large they are, and how far away their orbits are from the Sun. ...
ASTR100 Class 01 - University of Maryland Astronomy
ASTR100 Class 01 - University of Maryland Astronomy

1 Chapter 2 - University of Minnesota
1 Chapter 2 - University of Minnesota

... 1) Except for a truly negligible precession, the direction of the earth’s rotation axis remains fixed in space, providing us with an invaluably constant frame of reference. 2) The earth’s rotation axis is used to define the north and south celestial poles, and also the celestial equator. 3) The nort ...
The night sky - Mr. Champion
The night sky - Mr. Champion

Solar system rotation curves: student activity
Solar system rotation curves: student activity

... Activity: Rotation curves for the solar system. ...
Solar System Test Review - Clearview Local Schools
Solar System Test Review - Clearview Local Schools

... it is in, Mars A. has rings around it. B. is small and made mostly of rock. C. is large and made mostly of ...
Planet formation
Planet formation

No Slide Title
No Slide Title

... 7-15. Solar System Fundamentals ...
The definition of a planet - the Solar System Support Pages
The definition of a planet - the Solar System Support Pages

NASA - Go to the Head of the Solar System
NASA - Go to the Head of the Solar System

... Check your answers with the correct answers below. 1. I travel around the sun faster than any other planet. (b.) Mercury It only takes 88 days for Mercury to orbit around the sun. No other planet travels around the sun faster. 2. My name says I am the prettiest planet. I am Earth's twin sister -- th ...
formation of the solar system
formation of the solar system

... tilt. Some have elliptical orbits (compared with near circular orbits of planets) More than 10,00 have been identified and catalogued. Probably a huge number of yet unknown small asteroids. Very large asteroids (few hundred kilometers in radius – much less than ½ Moon’s radius. Comets are small icy ...
Intro ES Sense of Time and Space Test Key
Intro ES Sense of Time and Space Test Key

... Part 3: Answer the following questions briefly and clearly! 38. (3 points) Does the spectrum of a star or galaxy which is moving away from the earth moves towards the red or blue end of the visible color spectrum?_______*red_______ This is called the _______*Doppler ____ effect. Is this evidence tha ...
Planet Profile for Uranus
Planet Profile for Uranus

... 2. Mercury's surface resembles our moon as that both are covered with craters. 3. Mercury's temperature varies from 800 degrees F. in the sun to -280 degrees F in the darkness. 4. We have only been able to view 40% of Mercury's surface, while there is still 60% that has not been seen. 5. Mercury has ...
Explore the Galaxy
Explore the Galaxy

... 2. Carefully cut out each circle. Line up the planets in order of distance from the Sun. Mercury should be the first one on the left and Pluto should be the last one on the right. 3. Cut a different length of string for each planet. 4. Use a hole punch to make nine holes around the edge of the Sun. ...
1448
1448

... a planet, we count at least 110 known planets in our Solar System (Figure 1). This number continues to grow as astronomers discover more planets in the Kuiper Belt [e.g., 7]. Certainly 110 planets is more than students should be expected to memorize, and indeed they ought not. Instead, students shou ...
Solar System Power Point
Solar System Power Point

... the solar system compare with each other.  To show those things, you would need a piece of paper hundreds of meter long.  The Solar System Song ...
Unformatted file
Unformatted file

... If one asks why our wonderful instruments cannot settle these points, one must be reminded that Mars is never nearer than 34,000,000 miles from the earth, and _only approaches to this distance once in fifteen or seventeen years. The image of Mars on the photographic negative taken in a big telescope ...
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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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