Activity 1 The History and Scale of the Solar System
... plane of its disk.The individual stars you see dotting the night sky are just the ones nearest to Earth in the galaxy.When you view the Milky Way, you are “looking through” those nearest stars to see the more distant parts of the galaxy. In a sense, you are looking at our galaxy from the inside. In ...
... plane of its disk.The individual stars you see dotting the night sky are just the ones nearest to Earth in the galaxy.When you view the Milky Way, you are “looking through” those nearest stars to see the more distant parts of the galaxy. In a sense, you are looking at our galaxy from the inside. In ...
Model the Movements of the Planets
... can make a small model for his or her notebook. Teams of students can make larger models to hang on the wall. As described previously, move small pictures or symbols of the planets into their orbital locations every few days. Once a week is fine. Add one or more of the outer planets: Jupiter, Saturn ...
... can make a small model for his or her notebook. Teams of students can make larger models to hang on the wall. As described previously, move small pictures or symbols of the planets into their orbital locations every few days. Once a week is fine. Add one or more of the outer planets: Jupiter, Saturn ...
Making the Cards - Teaching Made Practical
... Choose 2 planets, and then compare and contrast them using the Venn Diagram. Then, write a short paragraph explaining the most important similarities and differences between the 2 planets. Planet:_______________________________ ...
... Choose 2 planets, and then compare and contrast them using the Venn Diagram. Then, write a short paragraph explaining the most important similarities and differences between the 2 planets. Planet:_______________________________ ...
1 When Is a Planet Not a Planet? The Story of Pluto
... burn away. The planets farthest from the Sun became the gas giants, Jupiter, Saturn, Uranus, and Neptune. Because astronomers still believed this theory about how our planets formed, they had a problem with Pluto. When it was first discovered in 1930, astronomers assumed Pluto was made of ice and ga ...
... burn away. The planets farthest from the Sun became the gas giants, Jupiter, Saturn, Uranus, and Neptune. Because astronomers still believed this theory about how our planets formed, they had a problem with Pluto. When it was first discovered in 1930, astronomers assumed Pluto was made of ice and ga ...
Powerpoint
... • Long ago water was dissociated by the solar radiation (unlike the earth, Mars has no ozone layer to shield the solar ultraviolet radiation) • no liquid water on surface, a little water combined with minerals in soil; polar caps (極冠) contain layers of frozen CO2 (dry ice) with frozen water beneath. ...
... • Long ago water was dissociated by the solar radiation (unlike the earth, Mars has no ozone layer to shield the solar ultraviolet radiation) • no liquid water on surface, a little water combined with minerals in soil; polar caps (極冠) contain layers of frozen CO2 (dry ice) with frozen water beneath. ...
Kepler`s Third Law - Faculty Web Pages
... Now we need to do the same for all the other planets. Stop time by pressing 7. Zoom out until Venus’ orbit just fits in your screen. Again mark Venus’ position on the screen and note the date in Table 1. Let time pass as fast as you want by pressing the Increase Time Speed button (or by pressing L) ...
... Now we need to do the same for all the other planets. Stop time by pressing 7. Zoom out until Venus’ orbit just fits in your screen. Again mark Venus’ position on the screen and note the date in Table 1. Let time pass as fast as you want by pressing the Increase Time Speed button (or by pressing L) ...
Asteroids
... Trojan Asteroids • The law of gravity permits an orbit around the sun exactly 60º ahead of and behind Jupiter, called Lagrange points. – Asteroids collect there – Several hundred Trojan asteroids locked to Jupiter L4 Trojans ...
... Trojan Asteroids • The law of gravity permits an orbit around the sun exactly 60º ahead of and behind Jupiter, called Lagrange points. – Asteroids collect there – Several hundred Trojan asteroids locked to Jupiter L4 Trojans ...
What is a terrestrial planet?
... released a list of 1235 extrasolar planet candidates, Io and Europa are also satellites that have internal including six that were "Earth-size" or "super-Earthstructures similar to that of terrestrial planets. In the size" (i.e. less than 2 Earth radii) and which were located within their stars' hab ...
... released a list of 1235 extrasolar planet candidates, Io and Europa are also satellites that have internal including six that were "Earth-size" or "super-Earthstructures similar to that of terrestrial planets. In the size" (i.e. less than 2 Earth radii) and which were located within their stars' hab ...
FREE Sample Here
... A. A large asteroid impact occurred, which resulted in environmental change that led to the death of the dinosaurs. B. They began to slowly go extinct. C. A massive volcanic eruption resulted in global cooling, which killed the dinosaurs. D. The extinction of the dinosaurs 65 million years ago remai ...
... A. A large asteroid impact occurred, which resulted in environmental change that led to the death of the dinosaurs. B. They began to slowly go extinct. C. A massive volcanic eruption resulted in global cooling, which killed the dinosaurs. D. The extinction of the dinosaurs 65 million years ago remai ...
Vagabonds of the Solar System
... – the fuzzy, luminous ball produced by the liberated gas and dust as the comet near the Sun – Typically 1 million km in diameter – The visible head of the comet ...
... – the fuzzy, luminous ball produced by the liberated gas and dust as the comet near the Sun – Typically 1 million km in diameter – The visible head of the comet ...
Solar_System_2013 Page 1
... Earth experiences these due to the moons gravity pulling on its oceans. A B C D ...
... Earth experiences these due to the moons gravity pulling on its oceans. A B C D ...
A Brief History of Planetary Science
... system is made up of many small icy bodies Kuiper Belt extends from 30-500 AU formed from left over planetesimals at the edge of the solar system ...
... system is made up of many small icy bodies Kuiper Belt extends from 30-500 AU formed from left over planetesimals at the edge of the solar system ...
Planets Power Point
... 3,660,000,000 miles from Sun; no other planet is as far from Sun Pluto found in 1930 because it was pulling Neptune out of orbit can only guess what it's like must be ice cold with solid, dense center, may have one moon think it's 2,000 miles in diameter, smallest planet & is why we now call it a dw ...
... 3,660,000,000 miles from Sun; no other planet is as far from Sun Pluto found in 1930 because it was pulling Neptune out of orbit can only guess what it's like must be ice cold with solid, dense center, may have one moon think it's 2,000 miles in diameter, smallest planet & is why we now call it a dw ...
The Solar System Powerpoint
... big does a planet need to be to become a full-fledged planet instead of a dwarf? You might think the minimum size requirement is arbitrary, but the size cutoff is actually based on other properties of the object and its history in the Solar System. Both planets and dwarf planets orbit the Sun, not o ...
... big does a planet need to be to become a full-fledged planet instead of a dwarf? You might think the minimum size requirement is arbitrary, but the size cutoff is actually based on other properties of the object and its history in the Solar System. Both planets and dwarf planets orbit the Sun, not o ...
Solar System - Bellevue ISD
... big does a planet need to be to become a full-fledged planet instead of a dwarf? You might think the minimum size requirement is arbitrary, but the size cutoff is actually based on other properties of the object and its history in the Solar System. Both planets and dwarf planets orbit the Sun, not o ...
... big does a planet need to be to become a full-fledged planet instead of a dwarf? You might think the minimum size requirement is arbitrary, but the size cutoff is actually based on other properties of the object and its history in the Solar System. Both planets and dwarf planets orbit the Sun, not o ...
1 Patterns in the Solar System (Chapter 18)
... Considering the nebular origin of the solar system, suggest a reason why the orbits of the planets are nearly all on the same plane of the ecliptic. In other words, think about the way in which the solar system formed and describe any aspects or characteristics that may have caused the planets to be ...
... Considering the nebular origin of the solar system, suggest a reason why the orbits of the planets are nearly all on the same plane of the ecliptic. In other words, think about the way in which the solar system formed and describe any aspects or characteristics that may have caused the planets to be ...
The Solar System - Henry County Schools
... http://lasp.colorado.edu/education/outerplan ets/orbit_simulator/ • The planets in our solar system differ in size, composition (rock or gas), surface and atmospheric conditions, and distance from the sun. ...
... http://lasp.colorado.edu/education/outerplan ets/orbit_simulator/ • The planets in our solar system differ in size, composition (rock or gas), surface and atmospheric conditions, and distance from the sun. ...
Exam# 2 Review (Draft)
... •What are the lunar maria (mare) and what caused them? •How do we explain the presence of Earth’s magnetic field •What are the two conditions that may explain the formation of magnetic field in a planet? •Does the Earth meet these two conditions? •What causes the terrestrial aurora? Describe the pro ...
... •What are the lunar maria (mare) and what caused them? •How do we explain the presence of Earth’s magnetic field •What are the two conditions that may explain the formation of magnetic field in a planet? •Does the Earth meet these two conditions? •What causes the terrestrial aurora? Describe the pro ...
Chapter 3: Our Solar System
... Jupiter and Saturn to have suitably “hardened” electronic systems so that could withstand the intense radiation belts that exist around these planets. An aid to SETI (The Search for Extra-Terrestrial Intelligence) The most sensitive and sophisticated SETI program ever undertaken was Project Phoenix ...
... Jupiter and Saturn to have suitably “hardened” electronic systems so that could withstand the intense radiation belts that exist around these planets. An aid to SETI (The Search for Extra-Terrestrial Intelligence) The most sensitive and sophisticated SETI program ever undertaken was Project Phoenix ...
Lecture18
... – Violent winds and convective turbulence would mix any lifebearing gas quickly over extremes of temperasture & pressure. – Although the sunlight is very weak, internal heat is available. – They are very difficult to explore! ...
... – Violent winds and convective turbulence would mix any lifebearing gas quickly over extremes of temperasture & pressure. – Although the sunlight is very weak, internal heat is available. – They are very difficult to explore! ...
Chapter 19 The Solar System Overview
... Comet- a small body of ice, rock, and cosmic dust that follows an elliptical orbit that gives off gas and dust in the form of a tail as it passes close to the sun. Satellites orbit planets, comets are prob. composed of material left over from the formation of the solar system. Most asteroids can be ...
... Comet- a small body of ice, rock, and cosmic dust that follows an elliptical orbit that gives off gas and dust in the form of a tail as it passes close to the sun. Satellites orbit planets, comets are prob. composed of material left over from the formation of the solar system. Most asteroids can be ...
the sun
... Comet- a small body of ice, rock, and cosmic dust that follows an elliptical orbit that gives off gas and dust in the form of a tail as it passes close to the sun. Satellites orbit planets, comets are prob. composed of material left over from the formation of the solar system. Most asteroids can be ...
... Comet- a small body of ice, rock, and cosmic dust that follows an elliptical orbit that gives off gas and dust in the form of a tail as it passes close to the sun. Satellites orbit planets, comets are prob. composed of material left over from the formation of the solar system. Most asteroids can be ...
Fun Fact: Venus rotates backward compared with mist other planets
... The Sun The sun is in the center of the solar system. It is also, the biggest object in the solar system. The sun is one of the many, many stars in the universe. ...
... The Sun The sun is in the center of the solar system. It is also, the biggest object in the solar system. The sun is one of the many, many stars in the universe. ...
File
... Host: Welcome! Today we will see which planets are the best in the solar system. We have nine contestants – eight planets and a dwarf planet – who will compete for awards. Each planet will tell us about itself and why it is unique among the planets. When all the planets have spoken, the judges will ...
... Host: Welcome! Today we will see which planets are the best in the solar system. We have nine contestants – eight planets and a dwarf planet – who will compete for awards. Each planet will tell us about itself and why it is unique among the planets. When all the planets have spoken, the judges will ...
Nice model
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).