Kepler`s Laws Notes
... CofM, r becomes greater, so must become smaller for L to stay the same. A classic analogy of conservation of angular momentum is that of the figure skater. If a skater is spinning with arms out, and then brings arms inwards towards the body (center of mass), the arms’ r is decreased. For L to rema ...
... CofM, r becomes greater, so must become smaller for L to stay the same. A classic analogy of conservation of angular momentum is that of the figure skater. If a skater is spinning with arms out, and then brings arms inwards towards the body (center of mass), the arms’ r is decreased. For L to rema ...
Planet Project Jupiter
... Distance from the sun It is approximately 4.95 Astronomical units away. It is the fifth planet from the sun. ...
... Distance from the sun It is approximately 4.95 Astronomical units away. It is the fifth planet from the sun. ...
View PDF
... The sun is the central and largest body in the solar system. The sun’s warming of the Earth and tilt of the Earth on its axis have an importan t connection to the seasons. Earth’s motion is the basis for measuring time. Objects in the sky move in regular and predictable patterns around the Sun. The ...
... The sun is the central and largest body in the solar system. The sun’s warming of the Earth and tilt of the Earth on its axis have an importan t connection to the seasons. Earth’s motion is the basis for measuring time. Objects in the sky move in regular and predictable patterns around the Sun. The ...
The Detection and Properties of Planetary Systems
... collapses into a disk. Jets and other mechanisms provide a means to remove angular momentum ...
... collapses into a disk. Jets and other mechanisms provide a means to remove angular momentum ...
Planets and Moons
... What are moons? Moons are like little planets that encircle the real planets. Usually, they are much smaller than planets. Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. 63 for Jupiter). ...
... What are moons? Moons are like little planets that encircle the real planets. Usually, they are much smaller than planets. Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. 63 for Jupiter). ...
Melbourne Solar System Trail.pub
... 10. Pluto, discovered in 1930, is a tiny world smaller than Earth. Charon, one of its three moons, is half the size of Pluto. Beyond Neptune are thousands of asteroids of ice and rock left over from when the planets were formed called ‘Kuiper Belt’. In 2005 a Kuiper Belt Object or ‘KBO’ larger than ...
... 10. Pluto, discovered in 1930, is a tiny world smaller than Earth. Charon, one of its three moons, is half the size of Pluto. Beyond Neptune are thousands of asteroids of ice and rock left over from when the planets were formed called ‘Kuiper Belt’. In 2005 a Kuiper Belt Object or ‘KBO’ larger than ...
SC.5.E.5.1, SC.5.E.5.3, SC.4.E.5.4
... ). Now you will measure how long it takes each planet to orbit the Sun. Notice that the date shown below the simulation is today’s date. Drag an arrow from the left of the Gizmo and place it next to Mercury. Click Play. When Mercury completes one orbit (reaches the arrow), click Pause. Record Today’ ...
... ). Now you will measure how long it takes each planet to orbit the Sun. Notice that the date shown below the simulation is today’s date. Drag an arrow from the left of the Gizmo and place it next to Mercury. Click Play. When Mercury completes one orbit (reaches the arrow), click Pause. Record Today’ ...
star (yes, the sun is really a star)
... hot it is, both on the surface and in the sun’s middle parts (let’s just say you’d fry if you got anywhere near it)! You’ll also discover what the sun’s made of, as well as how it got its start way back at the beginning of our solar system’s history. And, you can find out ...
... hot it is, both on the surface and in the sun’s middle parts (let’s just say you’d fry if you got anywhere near it)! You’ll also discover what the sun’s made of, as well as how it got its start way back at the beginning of our solar system’s history. And, you can find out ...
C1: The Inner Planets of the Solar System
... from above the North pole of the Sun. What is unusual about the rotation of Venus? a. Venus does not rotate. b. The spin axis of Venus is almost parallel to the ecliptic plane. c. Venus rotates in the same direction as the rest of the planets. d. Venus rotates in the opposite direction to all other ...
... from above the North pole of the Sun. What is unusual about the rotation of Venus? a. Venus does not rotate. b. The spin axis of Venus is almost parallel to the ecliptic plane. c. Venus rotates in the same direction as the rest of the planets. d. Venus rotates in the opposite direction to all other ...
THE INNER PLANETS
... • Uranus is about 4 times the diameter of Earth, but is still much smaller than Jupiter and Saturn. Uranus is a very far from the sun, making it colder than Saturn, and is surrounded by a group of thin, flat rings that are much darker than Saturn’s ...
... • Uranus is about 4 times the diameter of Earth, but is still much smaller than Jupiter and Saturn. Uranus is a very far from the sun, making it colder than Saturn, and is surrounded by a group of thin, flat rings that are much darker than Saturn’s ...
Lecture 15 - Physics 1025 Introductory Astronomy
... volcano which kept growing in one place. The largest canyon was not cut by water; it is a tectonic crack. But there are many signs of copious water on Mars at an earlier time, river beds and channels that could only have been made by water. So Mars appears to have had a thick atmosphere and running ...
... volcano which kept growing in one place. The largest canyon was not cut by water; it is a tectonic crack. But there are many signs of copious water on Mars at an earlier time, river beds and channels that could only have been made by water. So Mars appears to have had a thick atmosphere and running ...
Chapter 23: The Solar System Review Terrestrial Jovian Which
... 2. Small rocky bodies mostly found between the orbits of Mars and Jupiter 3. This planet gets very hot due to a very thin atmosphere, and it has similar features to Earth’s moon. 4. The third planet from the sun and the fifth largest planet. 5. A small particle that travels through space that is giv ...
... 2. Small rocky bodies mostly found between the orbits of Mars and Jupiter 3. This planet gets very hot due to a very thin atmosphere, and it has similar features to Earth’s moon. 4. The third planet from the sun and the fifth largest planet. 5. A small particle that travels through space that is giv ...
Planets and Moons
... What are moons? Moons are like little planets that encircle the real planets. Usually, they are much smaller than planets. Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. 63 for Jupiter). ...
... What are moons? Moons are like little planets that encircle the real planets. Usually, they are much smaller than planets. Planets can have no moons (like Mercury and Venus), one moon (like Earth) or up to a very large number of moons (e.g. 63 for Jupiter). ...
Formation of the Solar System
... • Most of the water started out as comets—icy bodies--got too close to the ________ ________________________ early Earth. • Because of the heat, the water _____________ and became part of the ___________________. • As Earth cooled, the water _________________ and fell as ...
... • Most of the water started out as comets—icy bodies--got too close to the ________ ________________________ early Earth. • Because of the heat, the water _____________ and became part of the ___________________. • As Earth cooled, the water _________________ and fell as ...
Chapter 23 Vocabulary
... 1. solar system- system of nine planets and many other objects that orbit our sun 2. inner planets- the four solid, rocky planets closest to the sun; Mercury, Venus, Earth, and Mars 3. Mars- in our solar system, the fourth planet from the sun 4. Jupiter- in our solar system, the fifth planet from th ...
... 1. solar system- system of nine planets and many other objects that orbit our sun 2. inner planets- the four solid, rocky planets closest to the sun; Mercury, Venus, Earth, and Mars 3. Mars- in our solar system, the fourth planet from the sun 4. Jupiter- in our solar system, the fifth planet from th ...
ExamView - Untitled.tst - Newark Catholic High School
... ____ 13. Evidence suggests that ____ originate in the Oort Cloud located beyond the orbit of Pluto. a. comets c. meteoroids b. asteroids d. meteorites ____ 14. ____ is the largest planet in the solar system, is the fifth planet from the Sun, and has colorful clouds. One of its 17 moons is the most v ...
... ____ 13. Evidence suggests that ____ originate in the Oort Cloud located beyond the orbit of Pluto. a. comets c. meteoroids b. asteroids d. meteorites ____ 14. ____ is the largest planet in the solar system, is the fifth planet from the Sun, and has colorful clouds. One of its 17 moons is the most v ...
Class 32
... The composition of the cores of all four Jovian planets is expected to be very similar despite their large range of size and density. Jupiter and Saturn are large enough to have metallic hydrogen and to have liquid cores of rock, metal and H compounds. The cores of Uranus and Neptune are relatively ...
... The composition of the cores of all four Jovian planets is expected to be very similar despite their large range of size and density. Jupiter and Saturn are large enough to have metallic hydrogen and to have liquid cores of rock, metal and H compounds. The cores of Uranus and Neptune are relatively ...
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).