here
... • Final conclusion was: – orbits of planets are just like any other object accelerating in a gravitational field (gun bullet physics) ...
... • Final conclusion was: – orbits of planets are just like any other object accelerating in a gravitational field (gun bullet physics) ...
4-H or - Waushara County UW-Extension
... TALK IT OVER What is a solar system? o Planets, moons, comets, asteroids, minor planets, dust and gases What does the sun do for us? What does it give us? What shape is the sun? o Round/spherical What color does it look like? o Yellow, but it is actually white How many planets are in the s ...
... TALK IT OVER What is a solar system? o Planets, moons, comets, asteroids, minor planets, dust and gases What does the sun do for us? What does it give us? What shape is the sun? o Round/spherical What color does it look like? o Yellow, but it is actually white How many planets are in the s ...
The Jovian Planets
... Jupiter’s interior generates more heat energy than it receives from the Sun Astronomers believe that Jupiter’s tremendous gravitational pull is causing elements such as He to collapse into the core. The movement of the elements is believed to be the source of the heat. As planets form they shrink as ...
... Jupiter’s interior generates more heat energy than it receives from the Sun Astronomers believe that Jupiter’s tremendous gravitational pull is causing elements such as He to collapse into the core. The movement of the elements is believed to be the source of the heat. As planets form they shrink as ...
The Jovian Planets
... Jupiter’s interior generates more heat energy than it receives from the Sun Astronomers believe that Jupiter’s tremendous gravitational pull is causing elements such as He to collapse into the core. The movement of the elements is believed to be the source of the heat. As planets form they shrink as ...
... Jupiter’s interior generates more heat energy than it receives from the Sun Astronomers believe that Jupiter’s tremendous gravitational pull is causing elements such as He to collapse into the core. The movement of the elements is believed to be the source of the heat. As planets form they shrink as ...
Jupiter by Jessie Ann and Rosalyn
... Jupiter has high speed winds that whip by at more than 400 mph! These winds are trapped in the planet's wide bands of latitude. Each band has a slightly different chemical make-up and temperature from the others. This gives it a color which is different from surrounding bands. The light colored band ...
... Jupiter has high speed winds that whip by at more than 400 mph! These winds are trapped in the planet's wide bands of latitude. Each band has a slightly different chemical make-up and temperature from the others. This gives it a color which is different from surrounding bands. The light colored band ...
PATTERNS OF MASS AND DENSITY IN THE SOLAR SYSTEM
... Why are the inner and outer planets densities so different? Consider both what you found out on your graph and also what you know about composition to support your statements ...
... Why are the inner and outer planets densities so different? Consider both what you found out on your graph and also what you know about composition to support your statements ...
File
... 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 other planet ...
... 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 other planet ...
AOD Example
... • Mark the line from the Earth to Sol (use a ruler) and determine the configurations of all the planets. Most planets will be between configurations. Use Starry Night to find the ecliptic longitudes. • Staple your print outs to this page to hand in. ...
... • Mark the line from the Earth to Sol (use a ruler) and determine the configurations of all the planets. Most planets will be between configurations. Use Starry Night to find the ecliptic longitudes. • Staple your print outs to this page to hand in. ...
Facts and figures on the sun and planets
... (99.8% of mass of solar system) • Density: 1.41 (water = 1) • Composition (by mass): Hydrogen: 73%, Helium: 25%, ...
... (99.8% of mass of solar system) • Density: 1.41 (water = 1) • Composition (by mass): Hydrogen: 73%, Helium: 25%, ...
Our Solar System
... A large mass at the centre of a solar system that produces heat and light…………….. A cluster of billions of stars, held together by gravity…………….. Gravitational Force per unit mass. Measured in newtons per kg…………….. The force of attraction between all objects…………….. The force acting on an object due t ...
... A large mass at the centre of a solar system that produces heat and light…………….. A cluster of billions of stars, held together by gravity…………….. Gravitational Force per unit mass. Measured in newtons per kg…………….. The force of attraction between all objects…………….. The force acting on an object due t ...
Dark anomalies called on the surface of the Sun allowed early
... Pluto was recently demoted from planet to “dwarf” planet status. Which of the following reasons best explains why its classification was changed? a. Pluto does not have enough gravity to put itself into a spherical shape. Only spherical celestial bodies are now considered planets. b. Pluto actually ...
... Pluto was recently demoted from planet to “dwarf” planet status. Which of the following reasons best explains why its classification was changed? a. Pluto does not have enough gravity to put itself into a spherical shape. Only spherical celestial bodies are now considered planets. b. Pluto actually ...
Science Lesson Plan: Our Solar System: I Wonder? (I 1-‐D-‐R)
... 6. What is Our Solar System. NASA Education. [Online] NASA, April 9, 2009. [Cited: September 22, 2011.] http://www.nasa.gov/audience/forstudents/k-‐4/stories/what-‐is-‐the-‐solar-‐system.html. 7. Libbey, Ted. Gustav Holst's ...
... 6. What is Our Solar System. NASA Education. [Online] NASA, April 9, 2009. [Cited: September 22, 2011.] http://www.nasa.gov/audience/forstudents/k-‐4/stories/what-‐is-‐the-‐solar-‐system.html. 7. Libbey, Ted. Gustav Holst's ...
Sorting the Solar System
... Eris is a Dwarf Planet with a moon called Dysnomia. It is more massive than Pluto and orbits the Sun three times farther. It was discovered in 2005 and caused a stir after initially being described as the 10th planet. Eros was the first near-Earth asteroid discovered. It is also one of the largest. ...
... Eris is a Dwarf Planet with a moon called Dysnomia. It is more massive than Pluto and orbits the Sun three times farther. It was discovered in 2005 and caused a stir after initially being described as the 10th planet. Eros was the first near-Earth asteroid discovered. It is also one of the largest. ...
Planets and Dwarf Planets - Super Teacher Worksheets
... This is a very exciting time. New objects in space are still being discovered! Scientists say there will likely be more dwarf planets announced in the next few years. What will be the name of the next dwarf planet? What name would you choose? ...
... This is a very exciting time. New objects in space are still being discovered! Scientists say there will likely be more dwarf planets announced in the next few years. What will be the name of the next dwarf planet? What name would you choose? ...
Earth`s Formation – Tutorial Script
... solar winds fiercest (solar winds are very hot, charged particles that escape off the sun’s surface at high speeds). Uncompacted gases and low-density elements, including molecules like water, would have been blown outward to the outer solar system where they accreted there to form the gaseous plane ...
... solar winds fiercest (solar winds are very hot, charged particles that escape off the sun’s surface at high speeds). Uncompacted gases and low-density elements, including molecules like water, would have been blown outward to the outer solar system where they accreted there to form the gaseous plane ...
Schoolyard Solar System 5E Lesson Plan
... 3. Tell students as teams or groups they will create their own one to ten billion scale model of the Solar System outdoors. The students will need to take with them their worksheet, a pencil, and a book or something solid to support the worksheet while they write. 4. Take the class outside to walk t ...
... 3. Tell students as teams or groups they will create their own one to ten billion scale model of the Solar System outdoors. The students will need to take with them their worksheet, a pencil, and a book or something solid to support the worksheet while they write. 4. Take the class outside to walk t ...
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).