Astronomy 1010
... Primitive meteorites may be either rocky or carbon-rich These 2 types are formed at different distances from the Sun Processed meteorites can be removed from the surface of a planet by an impact. There are meteorites from Moon and Mars found on Earth. ...
... Primitive meteorites may be either rocky or carbon-rich These 2 types are formed at different distances from the Sun Processed meteorites can be removed from the surface of a planet by an impact. There are meteorites from Moon and Mars found on Earth. ...
A. Comet: dust and rock particles combined with frozen water
... breaks up, pieces spread out. The dust and rock fragments are called Meteoroids. ...
... breaks up, pieces spread out. The dust and rock fragments are called Meteoroids. ...
DIRECTIONS - Cloverleaf Local
... • C)A small body that orbits the sun, made from solar radiation • D) a bright flying object in space consisting of a tail and a head ...
... • C)A small body that orbits the sun, made from solar radiation • D) a bright flying object in space consisting of a tail and a head ...
Planet Powerpoint
... smaller named moons and twenty-three more recently discovered but not named moons. We’ll take a look at the four large Galilean moons which were first observed by Galileo in 1610. ...
... smaller named moons and twenty-three more recently discovered but not named moons. We’ll take a look at the four large Galilean moons which were first observed by Galileo in 1610. ...
The Solar System
... Fact: Possible collision with an earth sized object may have knocked Uranus on it’s side as a result, it roll around in an orbit. ...
... Fact: Possible collision with an earth sized object may have knocked Uranus on it’s side as a result, it roll around in an orbit. ...
Solar System Notes - Miller`s Science Classroom
... Solar System Notes The Solar System Our solar system is made up of the sun and everything that travels around it. This includes 8 planets and their natural satellites such as Earth’s moon; dwarf planets such as Pluto and Ceres; asteroids, comets and meteoroids. Formed 4.6 billion years ago. Located ...
... Solar System Notes The Solar System Our solar system is made up of the sun and everything that travels around it. This includes 8 planets and their natural satellites such as Earth’s moon; dwarf planets such as Pluto and Ceres; asteroids, comets and meteoroids. Formed 4.6 billion years ago. Located ...
Small Solar System Bodies
... Dwarf Planets and Small Solar System Bodies typically have orbits that are highly tilted with respect to the classical planets (technically referred to as a large orbital inclination). They also typically have orbits that are far from being perfectly circular (technically referred to as having a lar ...
... Dwarf Planets and Small Solar System Bodies typically have orbits that are highly tilted with respect to the classical planets (technically referred to as a large orbital inclination). They also typically have orbits that are far from being perfectly circular (technically referred to as having a lar ...
The Planets in our Solar System
... The atmosphere blends seamlessly with the outer core. Composition: Liquid molecular hydrogen and helium outer mantle, liquid metallic hydrogen inner mantle, and ice and rock core Core pressure is about 100 million atmospheres ...
... The atmosphere blends seamlessly with the outer core. Composition: Liquid molecular hydrogen and helium outer mantle, liquid metallic hydrogen inner mantle, and ice and rock core Core pressure is about 100 million atmospheres ...
Dwarf Planets
... Planet Searching • After Uranus and Neptune, some began searching for yet another planet, among them was Percival Lowell from 1905-1916 • Search resumed in 1929 by Clyde Tombaugh, who identified a candidate on 2/18/1930 ...
... Planet Searching • After Uranus and Neptune, some began searching for yet another planet, among them was Percival Lowell from 1905-1916 • Search resumed in 1929 by Clyde Tombaugh, who identified a candidate on 2/18/1930 ...
Astro 1050 HW #2
... 19. Compare the rings of Jupiter, Saturn, Uranus, and Neptune. 20. The low average densities of Jupiter and Saturn compared with Earth suggest that: a. They are hollow b. Their gravitational attraction has squeezed material out of their cores c. They consists mostly of water d. They contain large qu ...
... 19. Compare the rings of Jupiter, Saturn, Uranus, and Neptune. 20. The low average densities of Jupiter and Saturn compared with Earth suggest that: a. They are hollow b. Their gravitational attraction has squeezed material out of their cores c. They consists mostly of water d. They contain large qu ...
Other tenants
... We have already mentioned that the planets with their satellites and rings are not the only bodies that occupy the Solar System. To start with, between the orbits of Mars and Jupiter, there is the Main Asteroid Belt that is not just a flat disc with rocks of different sizes and shapes as we usually ...
... We have already mentioned that the planets with their satellites and rings are not the only bodies that occupy the Solar System. To start with, between the orbits of Mars and Jupiter, there is the Main Asteroid Belt that is not just a flat disc with rocks of different sizes and shapes as we usually ...
Edible Solar System
... 2. Invite nine children to each hold a piece of fruit in front of the room. Ask all the children what the fruit might represent in a model of our solar system. (the planets) As a group, have the children work to arrange the children holding the fruit in the proper order, starting with the planet/fru ...
... 2. Invite nine children to each hold a piece of fruit in front of the room. Ask all the children what the fruit might represent in a model of our solar system. (the planets) As a group, have the children work to arrange the children holding the fruit in the proper order, starting with the planet/fru ...
Planet Name - TeacherWeb
... Title Page Title page showing a picture of the planet, its name, and a catchy phrase encouraging people to visit. ...
... Title Page Title page showing a picture of the planet, its name, and a catchy phrase encouraging people to visit. ...
Gravity (Chapter 11) Kepler`s Laws - FSU
... The mass, which enters the force law, is called inertial mass, F = mI a , whereas the mass, which enters the gravitational law, is called gravitational mass, F~12 ...
... The mass, which enters the force law, is called inertial mass, F = mI a , whereas the mass, which enters the gravitational law, is called gravitational mass, F~12 ...
9ol.ASTRONOMY 1 ... Identify Terms - Matching (20 @ 1 point each =...
... 9. Describe Saturn's rings: What are they made of, are there more than one, how big are the particles that make up the rings? (slide 27 – 29) 10. Describe the interior of Jupiter and draw a labeled sketch of a cross section through Jupiter. (see slide 5 Lecture) ...
... 9. Describe Saturn's rings: What are they made of, are there more than one, how big are the particles that make up the rings? (slide 27 – 29) 10. Describe the interior of Jupiter and draw a labeled sketch of a cross section through Jupiter. (see slide 5 Lecture) ...
Word Pro - Smvocab
... Fixed Stars - those stars and other heavenly bodies that maintain fixed patterns in the sky. Hypothesis - an unproved theory tentatively accepted to explain certain facts. Magnification - the apparent increase in size of an object viewed with a lens. Magnitude - the degree of brightness of a star. M ...
... Fixed Stars - those stars and other heavenly bodies that maintain fixed patterns in the sky. Hypothesis - an unproved theory tentatively accepted to explain certain facts. Magnification - the apparent increase in size of an object viewed with a lens. Magnitude - the degree of brightness of a star. M ...
Solar Nebula Theory
... Solar Nebula Theory Basic properties of the Solar System that need to be explained: 1. All planets orbit the Sun in the same direction as the Sun’s rotation 2. All planetary orbits are confined to the same general plane 3. Terrestrial planets form near the Sun, Jovian planets further out ...
... Solar Nebula Theory Basic properties of the Solar System that need to be explained: 1. All planets orbit the Sun in the same direction as the Sun’s rotation 2. All planetary orbits are confined to the same general plane 3. Terrestrial planets form near the Sun, Jovian planets further out ...
Power Point - Solar System
... Orbital path crosses Pluto’s Faint rings made of dust particles Composed of H, He, & Methane & a core of molten ...
... Orbital path crosses Pluto’s Faint rings made of dust particles Composed of H, He, & Methane & a core of molten ...
The Solar System Mr J and Miss Mac The Solar System is made up
... contains around 98% of all the material in the Solar System. The larger an object is, the more gravity it has. Because the Sun is so large, its powerful gravity attracts all the other objects in the Solar System towards it. At the same time, these objects, which are moving very rapidly, try to fly a ...
... contains around 98% of all the material in the Solar System. The larger an object is, the more gravity it has. Because the Sun is so large, its powerful gravity attracts all the other objects in the Solar System towards it. At the same time, these objects, which are moving very rapidly, try to fly a ...
File
... Smaller Members of the Solar System Asteroids • are composed of rock & metal. • Although they orbit the Sun, they are too small to be considered planets. • Most asteroids lie in the asteroid belt, located between Mars & Jupiter. ...
... Smaller Members of the Solar System Asteroids • are composed of rock & metal. • Although they orbit the Sun, they are too small to be considered planets. • Most asteroids lie in the asteroid belt, located between Mars & Jupiter. ...
Kepler`s Laws - Harnett County High Schools Wiki
... suggested Sun was center of solar system First time a sun-centered or “heliocentric” model was proposed In a heliocentric model, the inner planets move faster in their orbits than the outer planets do; as Earth bypasses a slower moving outer planet it appears the outer planet temporarily moves backw ...
... suggested Sun was center of solar system First time a sun-centered or “heliocentric” model was proposed In a heliocentric model, the inner planets move faster in their orbits than the outer planets do; as Earth bypasses a slower moving outer planet it appears the outer planet temporarily moves backw ...
planet - FieldStudy.com
... JUPITER: Jovian, largest planet, primarily H2 and He, rings, big red spot, winds and storms, lightning, most intense magnetosphere due to liquid metallic hydrogen, 11 times size of Earth, visited by Voyager and most recently by Galileo. IO – most volcanic object in solar system EUROPA – smoothest su ...
... JUPITER: Jovian, largest planet, primarily H2 and He, rings, big red spot, winds and storms, lightning, most intense magnetosphere due to liquid metallic hydrogen, 11 times size of Earth, visited by Voyager and most recently by Galileo. IO – most volcanic object in solar system EUROPA – smoothest su ...
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.