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... 5. Blow it up (probably not a good idea) H. Outside the Belt 1. Several hundred _______ asteroids are in a 1:1 orbital lock w/ Jupiter (2 comets) 2. They are found at __________ points – Joseph Lagrange (1772) a. ___ pts. are in synch w/ a planet b. Trojans only found at L4 & L5: ____ 0 in front of ...
... 5. Blow it up (probably not a good idea) H. Outside the Belt 1. Several hundred _______ asteroids are in a 1:1 orbital lock w/ Jupiter (2 comets) 2. They are found at __________ points – Joseph Lagrange (1772) a. ___ pts. are in synch w/ a planet b. Trojans only found at L4 & L5: ____ 0 in front of ...
Jupiter: The Giant Planet
... Jupiter is the fifth planet from the Sun and is the largest one in the solar system. If Jupiter were hollow, more than one thousand Earths could fit inside. It also contains more matter than all of the other planets combined. There is a ring system, but it is very faint and is totally invisible from ...
... Jupiter is the fifth planet from the Sun and is the largest one in the solar system. If Jupiter were hollow, more than one thousand Earths could fit inside. It also contains more matter than all of the other planets combined. There is a ring system, but it is very faint and is totally invisible from ...
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... New Moon - The Moon's unilluminated side is facing the Earth. The Moon is not visible (except during a solar eclipse). Waxing Crescent - The Moon appears to be partly but less than one-half illuminated by direct sunlight. The fraction of the Moon's disk that is illuminated is increasing. First Quart ...
... New Moon - The Moon's unilluminated side is facing the Earth. The Moon is not visible (except during a solar eclipse). Waxing Crescent - The Moon appears to be partly but less than one-half illuminated by direct sunlight. The fraction of the Moon's disk that is illuminated is increasing. First Quart ...
Table of contents Overview of the Solar System
... means that its axis of spin is almost pointing at the Sun. A theory is that Uranus might have collided with another planet-sized body after it was formed. Due to this, it has extreme seasons not like any other planet in the Solar System. The season are roughly 20 years long, which means that for alm ...
... means that its axis of spin is almost pointing at the Sun. A theory is that Uranus might have collided with another planet-sized body after it was formed. Due to this, it has extreme seasons not like any other planet in the Solar System. The season are roughly 20 years long, which means that for alm ...
The booklet - Cosmos
... means that its axis of spin is almost pointing at the Sun. A theory is that Uranus might have collided with another planet-sized body after it was formed. Due to this, it has extreme seasons not like any other planet in the Solar System. The season are roughly 20 years long, which means that for alm ...
... means that its axis of spin is almost pointing at the Sun. A theory is that Uranus might have collided with another planet-sized body after it was formed. Due to this, it has extreme seasons not like any other planet in the Solar System. The season are roughly 20 years long, which means that for alm ...
Planets: a brief tour
... • Highly elongated orbit causes it to occasionally travel inside the orbit of Neptune, where it resided from 1979 thru February 1999 • Moon (Charon) discovered in 1978 • Average temperature is -210ºC ...
... • Highly elongated orbit causes it to occasionally travel inside the orbit of Neptune, where it resided from 1979 thru February 1999 • Moon (Charon) discovered in 1978 • Average temperature is -210ºC ...
Planet Jupiter
... were a container, over 1400 planets the size of Earth could fit inside. The picture above is the first colour picture taken of Jupiter. We can also see Europa, one of Jupiter’s moons, which is approximately t he same size as Earth; imagine how small we are! Jupiter is a large gas planet where clouds ...
... were a container, over 1400 planets the size of Earth could fit inside. The picture above is the first colour picture taken of Jupiter. We can also see Europa, one of Jupiter’s moons, which is approximately t he same size as Earth; imagine how small we are! Jupiter is a large gas planet where clouds ...
The Planets and the Sun
... such as the sun is a ______. The path the orbit object takes around the sun is its _____. Small asteroidsorbit the sun in a rocky objects, known as _____ comets are path between Mars and Jupiter. _____, small space objects made of ice, dust, and gases, orbit the sun, too. The sun and all of the obje ...
... such as the sun is a ______. The path the orbit object takes around the sun is its _____. Small asteroidsorbit the sun in a rocky objects, known as _____ comets are path between Mars and Jupiter. _____, small space objects made of ice, dust, and gases, orbit the sun, too. The sun and all of the obje ...
1.10.1.2.SS - WordPress.com
... outermost planets, Uranus and Neptune, are composed largely of substances with relatively high melting points (compared with hydrogen and helium), called ices, such as water, ammonia and methane, and are often referred to separately as "ice giants". ...
... outermost planets, Uranus and Neptune, are composed largely of substances with relatively high melting points (compared with hydrogen and helium), called ices, such as water, ammonia and methane, and are often referred to separately as "ice giants". ...
CHAPTER 1 Planets of the Solar System
... Who is in the Sun’s family? The family includes the Sun, its eight planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune), and the five known dwarf planets (Ceres, Pluto, Makemake, Haumea, and Eris). In the image above, relative sizes of the Sun, planets, and dwarf planets and t ...
... Who is in the Sun’s family? The family includes the Sun, its eight planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune), and the five known dwarf planets (Ceres, Pluto, Makemake, Haumea, and Eris). In the image above, relative sizes of the Sun, planets, and dwarf planets and t ...
CHAPTER 1 Planets of the Solar System
... Who is in the Sun’s family? The family includes the Sun, its eight planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune), and the five known dwarf planets (Ceres, Pluto, Makemake, Haumea, and Eris). In the image above, relative sizes of the Sun, planets, and dwarf planets and t ...
... Who is in the Sun’s family? The family includes the Sun, its eight planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune), and the five known dwarf planets (Ceres, Pluto, Makemake, Haumea, and Eris). In the image above, relative sizes of the Sun, planets, and dwarf planets and t ...
Summative Assessment 1
... 3. Which planet has the most satellites (moons)? 4. Which planet is coldest? 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 ...
... 3. Which planet has the most satellites (moons)? 4. Which planet is coldest? 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 ...
Volcanoes and Igneous Activity Earth
... • Discovered in 1930 • Highly elongated orbit causes it to occasionally travel inside the orbit of Neptune, where it resided from 1979 thru February 1999 • Moon (Charon) discovered in 1978 • Average temperature is -210ºC ...
... • Discovered in 1930 • Highly elongated orbit causes it to occasionally travel inside the orbit of Neptune, where it resided from 1979 thru February 1999 • Moon (Charon) discovered in 1978 • Average temperature is -210ºC ...
The Planets in our Solar System
... Saturn and Jupiter Composition: Liquid hydrogen and other elements (outer mantle), slushy layer of icy compounds of water, methane, and ammonia (inner mantle), and an icy & rocky (core) Red light is absorbed by methane, which is why this planet is blue-green in color Sunlight strength: 1% of Earth’s ...
... Saturn and Jupiter Composition: Liquid hydrogen and other elements (outer mantle), slushy layer of icy compounds of water, methane, and ammonia (inner mantle), and an icy & rocky (core) Red light is absorbed by methane, which is why this planet is blue-green in color Sunlight strength: 1% of Earth’s ...
EARTH-CENTERED MODELS OF THE SOLAR SYSTEM
... The planets in order from biggest to smallest are: Jupiter, Saturn, Uranus, Neptune, Earth, Venus, Mars, Mercury. ...
... The planets in order from biggest to smallest are: Jupiter, Saturn, Uranus, Neptune, Earth, Venus, Mars, Mercury. ...
Astrobiologie: De speurtocht naar leven in het universum
... Development of groundand space based telescopes space missions, laboratory simulations, design of dedicated instrumentation and robotic tools ...
... Development of groundand space based telescopes space missions, laboratory simulations, design of dedicated instrumentation and robotic tools ...
The Solar System
... Test your knowledge about the solar system by filling out a quiz. Just click on the check mark and it will take you to the quiz. ...
... Test your knowledge about the solar system by filling out a quiz. Just click on the check mark and it will take you to the quiz. ...
solar system
... crucial position in our solar system, which makes this planet such an ideal place for us to live. Students may also consider how small our entire world is compared to some of our fellow planets, the Sun, and the vastness of space. For some students, this perspective might provide a sense of scale fo ...
... crucial position in our solar system, which makes this planet such an ideal place for us to live. Students may also consider how small our entire world is compared to some of our fellow planets, the Sun, and the vastness of space. For some students, this perspective might provide a sense of scale fo ...
Final exam
... orbit (with aphelion at or outside Jupiter, some got out as far as 50,000 AU "Dirty snowballs" mostly ice and some rock ...
... orbit (with aphelion at or outside Jupiter, some got out as far as 50,000 AU "Dirty snowballs" mostly ice and some rock ...
Nice model
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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).