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Summative Assessment 1
Summative Assessment 1

... 5. Which two planets are very much alike? (They are close to the same size. Their temperature is very close. Their rotation period is very similar.) 6. Which planet takes longest to rotate around the sun? 7. Name one of the two planets that have a stronger known gravitational pull than the Earth? 8. ...
Key 3 - UNLV Physics
Key 3 - UNLV Physics

... 35. Which of the following describes the Doppler Method of detecting planets? (a) looking for reduced light as a planet passes between us and the star. (b) looking for the change in position of a star on the sky (c) looking at the change in velocity of a star from its spectra (d) looking at locatio ...
Terms - HULK SCIENCE
Terms - HULK SCIENCE

The Structure of Comets - Oregon State University
The Structure of Comets - Oregon State University

... comfortably within the United States. • Charon orbits Pluto at a steep angle to the ecliptic, and Pluto’s axis is heavily tipped as well. • Two new moons were discovered in 2005, and were named Nix and Hydra in 2006. • Pluto is a mix of water ice, rock, methane and frozen nitrogen. • When Pluto is w ...
Things to do today Terminal, “Astronomy is Fun”
Things to do today Terminal, “Astronomy is Fun”

... • The distance between the two cities is 7/360 times the Earth’s circumference. • His result of 42,000 km is very close to the right number: 40,000 km. ...
Kuiper belt objects - Rosemary`s ePortfolio
Kuiper belt objects - Rosemary`s ePortfolio

The Solar System - Teachers TryScience
The Solar System - Teachers TryScience

... • A solar system consists of a star and objects that revolve around it. • Our Solar System consists of the Sun and nine known planets and the moons that orbit those planets. • The force of gravity keeps planets in orbit around the sun. ...
AP Physics - Universal Gravitation
AP Physics - Universal Gravitation

... the projectile is to rise to a height of 2R above the surface of the planet? Disregard any dissipative effects of the atmosphere. A) B) C) D) E) 6. What is the kinetic energy of a 200-kg satellite as it follows a circular orbit of radius 8.0 × 106 m around the Earth? (Mass of Earth = 6.0 × 1024 kg.) ...
25drake6s
25drake6s

... Simulations of inner planet formation produce a planet in the habitable zone much of the time ...
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star (yes, the sun is really a star)

... each planet to keep all of the planets in orbit around it. – The planets all exert gravitational force (pull) on their moons and any spacecraft that come near them. – A bigger planet exerts a greater gravitational force than a smaller planet. ...
Student Activity DOC - TI Education
Student Activity DOC - TI Education

... asteroids. Scientists use a variety of characteristics to analyze and classify a celestial body. One characteristic of a celestial body is its orbital radius. This is the distance an object is from its orbiting body. Planets in our solar system orbit around the Sun, so the orbital radius for each pl ...
Student Activity PDF - TI Education
Student Activity PDF - TI Education

... asteroids. Scientists use a variety of characteristics to analyze and classify a celestial body. One characteristic of a celestial body is its orbital radius. This is the distance an object is from its orbiting body. Planets in our solar system orbit around the Sun, so the orbital radius for each pl ...
mars
mars

... a speed of around 42 kilometres per second (26 miles per second). •The first man made object sent into space was in 1957 when the Russian satellite named Sputnik was launched. •Jupiter's 4 biggest moons are named Europa, Ganymede, Calisto. It is because of the Sun & Moons gravity that we have high & ...
The Solar System
The Solar System

... therefore is known as one of the Gas Giants. • Jupiter is the largest planet in out SS. • In a way Jupiter behaves like its own SS, with 63 known moons orbiting it and one of them (Ganymede) is larger than Mercury. • Jupiter exerts pull on the other planets in the SS. ...
Chapter 29, Section 2
Chapter 29, Section 2

... The existence of Neptune was predicted before it was discovered.  After the discovery of Uranus, astronomers noted variations in Uranus’ expected orbit.  The only thing that could cause such variations would be a large gravity source.  Scientists in the 1800s accurately predicted where Neptune sh ...
Rocket Science
Rocket Science

... surface of a planet is vo… …then the velocity needed to launch a rocket into orbit of radius r; altitude of r-rp is v2 = vo2 + vL2 vL2 = v2 - vo2 ...
Moon PowerPoint Template
Moon PowerPoint Template

... Earth Earth is the third planet from the Sun. Earth is the largest of the terrestrial planets in the Solar System in diameter, mass and density. It is also referred to as the World and Terra. Home to millions of species, including humans, Earth is the only place in the universe where life is known ...
Exploring Space What’s Out There?
Exploring Space What’s Out There?

Orbits, Asteroids, and Comets
Orbits, Asteroids, and Comets

... • Used a lifetime of data kept by another astronomer (Brahe) to explain the motion of the planets • Two main ideas: – Objects orbiting the Sun move faster when they are near ...
The Outer Solar System
The Outer Solar System

... Pluto is much smaller than the inner or outer planets. Its diameter is about half that of Mercury. The density of Pluto is similar to that of Triton, suggesting a mixture of ice and rock. ...
Kepler`s Laws and Planetary Motion
Kepler`s Laws and Planetary Motion

... The questions below are challenging, yet strike at the heart of the meaning of Kepler's third law. For any two planets orbiting the same central body (e.g., the Sun), the square of the ratio of their periods is equal to the cube of the ratio of their radii of orbit. a. If planet A is twice as far fr ...
Solar System Do you think our planet is the only place in the
Solar System Do you think our planet is the only place in the

... Eight of the nine planets in our solar system fall into two groups called the inner planets and the outer planets. The four planets closest to the Sun are called the inner planets. They are Mercury, Venus, Earth, and Mars. The inner planets are also called the rocky planets, because they are made ma ...
KS2 Primary Teacher Document The Solar System Experience 18
KS2 Primary Teacher Document The Solar System Experience 18

... KS2 Primary Teacher Document The Solar System Experience 18-20 October 2016 STRICTLY KS2- spaces are restricted. The aim of this experience is to increase student’s understanding of the solar system, our planet and the International Space Station in a fun and engaging way. By using the planetarium a ...
CHAPTER 6: The Solar System
CHAPTER 6: The Solar System

... Do not hit the Earth… they burn up Haven’t been able to study them until recently Tails vaporize as they get close to the Sun and we use Spectroscopic study to study tails. ...
Geocentric Model of the Solar System
Geocentric Model of the Solar System

... • Pluto is the only planet not visited by spacecraft. We are not sure of its composition. Based on current data, scientists believe it is a small, rocky planet. • Pluto seems to lie on its side: its equator points straight up, and one of its poles points directly at the sun. • Pluto has only one moo ...
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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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