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Speed of Planets Google Document File
... 2. The dwarf planet Ceres orbits the Sun at an average distance of 2.8AU .Plot the point that would represent Ceres on the graph. What is the average speed of Ceres? 3. The dwarf planet Pluto orbits at an average distance from the Sun of 39.5 AU. Extrapolating from your graph, what is Pluto’s averag ...
... 2. The dwarf planet Ceres orbits the Sun at an average distance of 2.8AU .Plot the point that would represent Ceres on the graph. What is the average speed of Ceres? 3. The dwarf planet Pluto orbits at an average distance from the Sun of 39.5 AU. Extrapolating from your graph, what is Pluto’s averag ...
quarter 1 assessment review
... 3) Explain the Big Bang Theory (Use Key Words: singularity, space, time, matter, energy, elements, expansion, gases, background radiation) The theory that the universe began as a single point of matter, space, time and energy called singularity. This point exploded and began to spread into the expan ...
... 3) Explain the Big Bang Theory (Use Key Words: singularity, space, time, matter, energy, elements, expansion, gases, background radiation) The theory that the universe began as a single point of matter, space, time and energy called singularity. This point exploded and began to spread into the expan ...
Our Solar System
... What are Kuiper Belt objects? Class of icy bodies orbiting beyond Neptune. Found only in the outer Solar System (>30AU) Densities of 1.2 to 2 g/cc (mostly ices) Examples: Pluto & Eris (icy dwarf planets) Kuiper Belt Objects (30-50AU) Charon, Pluto’s large moon Sedna & Quaor: distant large icy bodi ...
... What are Kuiper Belt objects? Class of icy bodies orbiting beyond Neptune. Found only in the outer Solar System (>30AU) Densities of 1.2 to 2 g/cc (mostly ices) Examples: Pluto & Eris (icy dwarf planets) Kuiper Belt Objects (30-50AU) Charon, Pluto’s large moon Sedna & Quaor: distant large icy bodi ...
Solar System Formation
... of a cloud of dust and gas until a dense object forms (planetesimal). ...
... of a cloud of dust and gas until a dense object forms (planetesimal). ...
Facts of our solar system.
... Day and night • We have day and night because when we are facing the sun we have light so we have daytime and when we’re facing the other side we can’t see the sun so we get no light it, is all dark so it is night time. ...
... Day and night • We have day and night because when we are facing the sun we have light so we have daytime and when we’re facing the other side we can’t see the sun so we get no light it, is all dark so it is night time. ...
Distances in Space Vocabulary
... Astronomers have to use units of length MUCH bigger than usual. ...
... Astronomers have to use units of length MUCH bigger than usual. ...
The Solar System
... the strongest hurricane-force winds on Earth top out at about 110 meters, or (360 feet), per second. These super-fast winds, combined with heat rising from within the planet's interior, cause the yellow and gold bands visible in the atmosphere. ...
... the strongest hurricane-force winds on Earth top out at about 110 meters, or (360 feet), per second. These super-fast winds, combined with heat rising from within the planet's interior, cause the yellow and gold bands visible in the atmosphere. ...
What do you know about light?
... • As planets form, they become the dominant gravitational body in their orbit in the Solar System. • As they interact with other, smaller objects, they either consume them, or sling them away with their gravity. ...
... • As planets form, they become the dominant gravitational body in their orbit in the Solar System. • As they interact with other, smaller objects, they either consume them, or sling them away with their gravity. ...
Benchmark Number:
... A celestial body that appears as a fuzzy head usually surrounding a bright nucleus, that has a usually highly eccentric orbit, that consists primarily of ice and dust, and that often develops one or more long tails when near the sun. ...
... A celestial body that appears as a fuzzy head usually surrounding a bright nucleus, that has a usually highly eccentric orbit, that consists primarily of ice and dust, and that often develops one or more long tails when near the sun. ...
Earth and Its Place in the Solar System
... Earth and Its Place in the Solar System Study Guide Vocabulary (11 questions) Revolution Orbit Asteroid Lunar eclipse Phases Solar system Axis Planet Rotation Solar eclipse Comet Planets Label the planets on a diagram Tell how the inner planets are alike Compare two inner ...
... Earth and Its Place in the Solar System Study Guide Vocabulary (11 questions) Revolution Orbit Asteroid Lunar eclipse Phases Solar system Axis Planet Rotation Solar eclipse Comet Planets Label the planets on a diagram Tell how the inner planets are alike Compare two inner ...
File
... radiation from the Sun releases the gases and particles in the comet • The wind from the Sun pushes the gases and particles away, this forms a comet tail ...
... radiation from the Sun releases the gases and particles in the comet • The wind from the Sun pushes the gases and particles away, this forms a comet tail ...
Ch 20: A Family of Planets
... Outer Planets Differ greatly in size and composition from inner planets All outer planets (except Pluto) are gas giants – Large – No solid surface – All have rings ...
... Outer Planets Differ greatly in size and composition from inner planets All outer planets (except Pluto) are gas giants – Large – No solid surface – All have rings ...
Science – Chapter 9, Lesson 1 telescope – a tool that makes far
... 3. ***Pluto – small and made of rocks and frozen gases with one moon and no rings asteroid – piece of rock that orbits the sun (can be as small as a grain or as large as California) asteroid belt – an area between inner planets and outer planets ...
... 3. ***Pluto – small and made of rocks and frozen gases with one moon and no rings asteroid – piece of rock that orbits the sun (can be as small as a grain or as large as California) asteroid belt – an area between inner planets and outer planets ...
Solar System – Odds & Ends - Saint Paul Public Schools
... Jupiter, Saturn, Uranus, Neptune, and Pluto are planets. No scientific basis. 2) Historical plus: Mercury through Pluto are planets, as is any newly discovered object larger than Pluto. But why is Pluto’s size the cutoff? ...
... Jupiter, Saturn, Uranus, Neptune, and Pluto are planets. No scientific basis. 2) Historical plus: Mercury through Pluto are planets, as is any newly discovered object larger than Pluto. But why is Pluto’s size the cutoff? ...
Solar System - ppt
... The nebula had been slowly rotating, but began to collapse to its center. The nebula’s rotational speed increased which flattened the nebula into a more disk-like shape. As the cloud continued to collapse in on itself, a large massive ...
... The nebula had been slowly rotating, but began to collapse to its center. The nebula’s rotational speed increased which flattened the nebula into a more disk-like shape. As the cloud continued to collapse in on itself, a large massive ...
Space Section 13.1 pages 400-403 The universe is everything that
... http://www.astropix.com/HTML/C_SPRING/URSAS.HTM Objects in our solar system ...
... http://www.astropix.com/HTML/C_SPRING/URSAS.HTM Objects in our solar system ...
Solar system - Science 504
... when the earth is in the middle . A solar eclipse is when the moon is in the middle . ...
... when the earth is in the middle . A solar eclipse is when the moon is in the middle . ...
Nice model
![](https://commons.wikimedia.org/wiki/Special:FilePath/Lhborbits.png?width=300)
The Nice model (/ˈniːs/) is a scenario for the dynamical evolution of the Solar System. It is named for the location of the Observatoire de la Côte d'Azur, where it was initially developed, in Nice, France. It proposes the migration of the giant planets from an initial compact configuration into their present positions, long after the dissipation of the initial protoplanetary gas disk. In this way, it differs from earlier models of the Solar System's formation. This planetary migration is used in dynamical simulations of the Solar System to explain historical events including the Late Heavy Bombardment of the inner Solar System, the formation of the Oort cloud, and the existence of populations of small Solar System bodies including the Kuiper belt, the Neptune and Jupiter Trojans, and the numerous resonant trans-Neptunian objects dominated by Neptune. Its success at reproducing many of the observed features of the Solar System means that it is widely accepted as the current most realistic model of the Solar System's early evolution, though it is not universally favoured among planetary scientists. One of its limitations is reproducing the outer-system satellites and the Kuiper belt (see below).