tire
... 3. The hottest planet due to a runaway greenhouse effect. 4. The furthest Jovian planet from the Sun. 5. Name of the space program that put the first humans on the Moon. 6. Formed by the impact of a Mars-sized body with proto-Earth. 7. The only moon in the solar system with a thick atmosphere. 8. A ...
... 3. The hottest planet due to a runaway greenhouse effect. 4. The furthest Jovian planet from the Sun. 5. Name of the space program that put the first humans on the Moon. 6. Formed by the impact of a Mars-sized body with proto-Earth. 7. The only moon in the solar system with a thick atmosphere. 8. A ...
Solar System Summary Sheet File
... Comets can be described as being dirty snowballs because they are mainly made up of ice and dust. As the comets approach the Sun they begin to warm up. The surface Ice begins to evaporate. The radiation pressure and solar wind (charged ions/particles) emitted by the Sun forces the water vapour to st ...
... Comets can be described as being dirty snowballs because they are mainly made up of ice and dust. As the comets approach the Sun they begin to warm up. The surface Ice begins to evaporate. The radiation pressure and solar wind (charged ions/particles) emitted by the Sun forces the water vapour to st ...
17.1 What is the solar system?
... 17.1 What is the solar system? • Today, we define the solar system as the sun and all objects that are gravitationally bound to the sun. • The solar system is roughly divided into the inner planets (Mercury, Venus, Earth, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and Neptune) • The ...
... 17.1 What is the solar system? • Today, we define the solar system as the sun and all objects that are gravitationally bound to the sun. • The solar system is roughly divided into the inner planets (Mercury, Venus, Earth, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and Neptune) • The ...
Components of the Solar System Learning Targets
... Venus hottest, greenhouse effect, dense atmosphere, rotates opposite of other planets, Earth’s sister (because of size only), layers, volcanic activity, longest day (day is longer than its year), no moons, Earth liquid water, one moon, layers, atmosphere, greenhouse effect, volcanic activity, only p ...
... Venus hottest, greenhouse effect, dense atmosphere, rotates opposite of other planets, Earth’s sister (because of size only), layers, volcanic activity, longest day (day is longer than its year), no moons, Earth liquid water, one moon, layers, atmosphere, greenhouse effect, volcanic activity, only p ...
Solar System Study Guide 1
... tilted like Uranus. Uranus is tilted so far that it is tipped over on its side! This gives Uranus a winter that lasts about 21 years! ...
... tilted like Uranus. Uranus is tilted so far that it is tipped over on its side! This gives Uranus a winter that lasts about 21 years! ...
Bella Nicole and Calli
... The Solar System began 5 billion years ago. There were 9 planets, but scientists think Pluto should not be considered a planet anymore. A solar system is the Sun and the group of planets and bodies that orbit around it. ...
... The Solar System began 5 billion years ago. There were 9 planets, but scientists think Pluto should not be considered a planet anymore. A solar system is the Sun and the group of planets and bodies that orbit around it. ...
Document
... of the Gods. It would take 11 earths lined up next to each other to get from one side of Jupiter to the other, it would also take 317 earths to equal Jupiter's mass. Jupiter's red spot is a gigantic storm that has been there for over 300 years! If Jupiter had 80 times ...
... of the Gods. It would take 11 earths lined up next to each other to get from one side of Jupiter to the other, it would also take 317 earths to equal Jupiter's mass. Jupiter's red spot is a gigantic storm that has been there for over 300 years! If Jupiter had 80 times ...
History of Astronomy – Modeling the Solar System Early Studies
... Showed that the Sun was much farther than the Moon from the Earth, using simple trigonometry of the angle between the Moon and the Sun at 1st Quarter. ...
... Showed that the Sun was much farther than the Moon from the Earth, using simple trigonometry of the angle between the Moon and the Sun at 1st Quarter. ...
PowerPoint Presentation - Planetary Configurations
... The Chaotic Early Solar System • Recent computer models are challenging earlier views that planets formed in an orderly way at their current locations • These models suggest that the jovian planets changed their orbits substantially, and that Uranus and Neptune could have changed places • These cha ...
... The Chaotic Early Solar System • Recent computer models are challenging earlier views that planets formed in an orderly way at their current locations • These models suggest that the jovian planets changed their orbits substantially, and that Uranus and Neptune could have changed places • These cha ...
quarter 1 assessment review
... c) Background Radiation – the radiation left over from the big bang can still be detected in space. d) Hydrogen and Helium – the abundance of these two elements suggests they were the first to be created after the BB ...
... c) Background Radiation – the radiation left over from the big bang can still be detected in space. d) Hydrogen and Helium – the abundance of these two elements suggests they were the first to be created after the BB ...
The Solar System
... planets. Dwarf planets such as, Ceres and Eris and Pluto are named dwarf planets because they do not have enough gravitational force to put them in a circular orbit around the sun and they don't have enough gravity to be clear of debris. 5 Clarify what is meant by a terrestrial planet? Terrestrial p ...
... planets. Dwarf planets such as, Ceres and Eris and Pluto are named dwarf planets because they do not have enough gravitational force to put them in a circular orbit around the sun and they don't have enough gravity to be clear of debris. 5 Clarify what is meant by a terrestrial planet? Terrestrial p ...
Chapter 23
... As speed of rotation increased the center of the disk began to flatten out Matter became more concentrated in the center, where the sun eventually formed. Planets began to form as matter started to collide and clump together Baby planets called planetesimals began to form ...
... As speed of rotation increased the center of the disk began to flatten out Matter became more concentrated in the center, where the sun eventually formed. Planets began to form as matter started to collide and clump together Baby planets called planetesimals began to form ...
The Solar System
... • Most scientist accept the Nebular Theory, or Nebular Model, as the best supported explanation • It explains why… – Planets are so far apart – In the same plane – orbit in the same direction ...
... • Most scientist accept the Nebular Theory, or Nebular Model, as the best supported explanation • It explains why… – Planets are so far apart – In the same plane – orbit in the same direction ...
Planets orbit the Sun at different distances.
... in the western sky in the early evening, you have probably seen the planet Venus. Even if you live in a city, you may have seen Mars, Jupiter, or Saturn but thought that you were seeing a star. Mercury is much more difficult to see. You need a telescope to see the large but distant planets Uranus an ...
... in the western sky in the early evening, you have probably seen the planet Venus. Even if you live in a city, you may have seen Mars, Jupiter, or Saturn but thought that you were seeing a star. Mercury is much more difficult to see. You need a telescope to see the large but distant planets Uranus an ...
Level :3ASS3-4 School Year: 2009/2010 English
... Our solar system consists of an average star we call the Sun, the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto. It includes also the satellites of the planets; numerous comets, asteroids, and meteoroids. The moon is the satellite rotating around the Erath and the ...
... Our solar system consists of an average star we call the Sun, the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto. It includes also the satellites of the planets; numerous comets, asteroids, and meteoroids. The moon is the satellite rotating around the Erath and the ...
Topic 9/10
... Satellite- any object in space orbiting a larger object Inertia- things in motion will remain in motion unless acted upon by an equal and opposite force Asteroid- rocky objects up to 600 miles across, there is a belt b/t Mars and Jupiter Meteor- falling star Comet- icy objects caught in highly ellip ...
... Satellite- any object in space orbiting a larger object Inertia- things in motion will remain in motion unless acted upon by an equal and opposite force Asteroid- rocky objects up to 600 miles across, there is a belt b/t Mars and Jupiter Meteor- falling star Comet- icy objects caught in highly ellip ...
The Solar System: Unit 3 Review/Study Guide
... bodies lack atmosphere and have weak surface gravity. The largest of the small bodies are known as dwarf planets. A dwarf planet is a celestial body that orbits the sun and is round because of its own gravity, but it does not have the mass to have cleared other bodies out of its orbit around the sun ...
... bodies lack atmosphere and have weak surface gravity. The largest of the small bodies are known as dwarf planets. A dwarf planet is a celestial body that orbits the sun and is round because of its own gravity, but it does not have the mass to have cleared other bodies out of its orbit around the sun ...
direct - grade 4High peaks elementary
... appears to be moving from east to west, however, Earth is moving, not the sun. planets and other bodies orbit around the sun Earth rotates on its axis as it revolves around the sun, this causes day and night. Earth’s axis is tilted which causes seasons. Gravitational forces affect all matter in the ...
... appears to be moving from east to west, however, Earth is moving, not the sun. planets and other bodies orbit around the sun Earth rotates on its axis as it revolves around the sun, this causes day and night. Earth’s axis is tilted which causes seasons. Gravitational forces affect all matter in the ...
Universe and Solar System
... numbers---Scientists use it to explain distances in space due to their large size Look at pg. 626 ...
... numbers---Scientists use it to explain distances in space due to their large size Look at pg. 626 ...
Formation and evolution of the Solar System
The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.