![Models of the solar system](http://s1.studyres.com/store/data/008591892_1-a4acf2cc5088e9355d5ae62d6dc51f6a-300x300.png)
Chapter 9 Notes
... 37._________________. Earth is one of the 38.________________ planets that move around the 39.________________. A 40.__________________ is a large body in space that moves around a 41.________________. A 42._______________ does not produce 43._______________ of its own. Earth and 44.________________ ...
... 37._________________. Earth is one of the 38.________________ planets that move around the 39.________________. A 40.__________________ is a large body in space that moves around a 41.________________. A 42._______________ does not produce 43._______________ of its own. Earth and 44.________________ ...
Overview of Solar System - FLASH Center for Computational Science
... system,” and the rings are analogous to a scaled-down version of the asteroid belts in our own solar system (which we will discuss in just a moment). ...
... system,” and the rings are analogous to a scaled-down version of the asteroid belts in our own solar system (which we will discuss in just a moment). ...
Lesson 1 For students of Geography, 2 course. Subject: THE SOLAR
... of the telescope in Hilland, Galileo built one of his own and was able to add four new bodies to the system: the brighter of the moons (or satellites) that revolve around Jupiter. Since Galileo’s time telescopic improvements have made possible the discovery of many more members of the sun’s family. ...
... of the telescope in Hilland, Galileo built one of his own and was able to add four new bodies to the system: the brighter of the moons (or satellites) that revolve around Jupiter. Since Galileo’s time telescopic improvements have made possible the discovery of many more members of the sun’s family. ...
Solar System Scale Activity
... other ‘large’ objects from its orbital zone; hence it is now called a “dwarf planet”. Pluto’s unique orbit: Pluto’s orbital path around the Sun is very far being circular, its ellipQcal orbit is much ...
... other ‘large’ objects from its orbital zone; hence it is now called a “dwarf planet”. Pluto’s unique orbit: Pluto’s orbital path around the Sun is very far being circular, its ellipQcal orbit is much ...
Exploring the Solar System
... planet's orbit (P = how long it takes the planet to go around the Sun), then you can determine that planet's distance from the Sun (a = the semi-major axis of the planet's orbit). ...
... planet's orbit (P = how long it takes the planet to go around the Sun), then you can determine that planet's distance from the Sun (a = the semi-major axis of the planet's orbit). ...
Chapter8- Jovian Planet Systems
... hydrosulfide gas, and other sulfur and phosphorous compounds ...
... hydrosulfide gas, and other sulfur and phosphorous compounds ...
Scale Distances in the Solar System
... out other ‘large’ objects from its orbital zone, hence it is now called a “dwarf planet”. Pluto’s unique orbit: Pluto’s orbital path around the Sun is very far being circular, its elliptical orbit is much more eccentric than the eight planets. At times, Pluto is 49 AU from the Sun and at other times ...
... out other ‘large’ objects from its orbital zone, hence it is now called a “dwarf planet”. Pluto’s unique orbit: Pluto’s orbital path around the Sun is very far being circular, its elliptical orbit is much more eccentric than the eight planets. At times, Pluto is 49 AU from the Sun and at other times ...
Visit www.sciencea-z.com www.sciencea-z.com
... The solar system is our home in space. It’s special to us because it’s where we live. Understanding our solar system and how it formed might give us clues about other solar systems. Let’s take an imaginary flight through the solar system. We’ll start at the center: the Sun. As we move away from the ...
... The solar system is our home in space. It’s special to us because it’s where we live. Understanding our solar system and how it formed might give us clues about other solar systems. Let’s take an imaginary flight through the solar system. We’ll start at the center: the Sun. As we move away from the ...
planets - Personal.psu.edu
... • Radius: 71,500 km (112 times Earth’s) • Density: 1300 kg/m3—cannot be rocky or metallic as inner planets are • Rotation rate: Problematic, as Jupiter has no solid surface; different parts of atmosphere rotate at different rates • From magnetic field, rotation period is 9 hr, 55 min ...
... • Radius: 71,500 km (112 times Earth’s) • Density: 1300 kg/m3—cannot be rocky or metallic as inner planets are • Rotation rate: Problematic, as Jupiter has no solid surface; different parts of atmosphere rotate at different rates • From magnetic field, rotation period is 9 hr, 55 min ...
Defrosting North Polar Dunes
... Like the other three "gas giant" planets -- Jupiter, Saturn and Uranus -- Neptune has no solid surface. Its atmosphere contains hydrogen and helium with enough methane to give it a bluish tint. Winds on Neptune blow faster than on any other planet. The discoveries of Neptune and its largest moon, Tr ...
... Like the other three "gas giant" planets -- Jupiter, Saturn and Uranus -- Neptune has no solid surface. Its atmosphere contains hydrogen and helium with enough methane to give it a bluish tint. Winds on Neptune blow faster than on any other planet. The discoveries of Neptune and its largest moon, Tr ...
Planets - Calgary Islamic School OBK
... Any object that doesn't meet this 3rd criteria is considered a dwarf planet. And so, Pluto is a dwarf planet. There are still many objects with similar size and mass to Pluto jostling around in its orbit. And until Pluto crashes into many of them and gains mass, it will remain a dwarf planet. ...
... Any object that doesn't meet this 3rd criteria is considered a dwarf planet. And so, Pluto is a dwarf planet. There are still many objects with similar size and mass to Pluto jostling around in its orbit. And until Pluto crashes into many of them and gains mass, it will remain a dwarf planet. ...
A105 Stars and Galaxies
... The Sun entered an interstellar cloud of mixed plasma and gas about 103-105 years ago The directions of motion of the Sun and the cloud suggest that our Solar System will be in this cloud for the next million years The surrounding interstellar cloud will shrink the heliosphere to a smaller radiu ...
... The Sun entered an interstellar cloud of mixed plasma and gas about 103-105 years ago The directions of motion of the Sun and the cloud suggest that our Solar System will be in this cloud for the next million years The surrounding interstellar cloud will shrink the heliosphere to a smaller radiu ...
3,2,1 Planetarium Lane
... complete the card. I would stop here for day 2. Meet with each group to determine where its planet should hang in relation to the sun image. You can use these approximations for distance from the sun: Mercury—58.9 million km, Venus—108.2 million km, Earth—149.6 million km, Mars—227.8 million km, Jup ...
... complete the card. I would stop here for day 2. Meet with each group to determine where its planet should hang in relation to the sun image. You can use these approximations for distance from the sun: Mercury—58.9 million km, Venus—108.2 million km, Earth—149.6 million km, Mars—227.8 million km, Jup ...
Jupiter
... surrounding ones. Called the Great Red Spot, it has been likened to a great hurricane and is caused by tremendous winds that develop above the rapidly spinning planet. Winds blow counterclockwise around this disturbance at about 250 miles per hour. Hurricanes on Earth rarely generate winds ...
... surrounding ones. Called the Great Red Spot, it has been likened to a great hurricane and is caused by tremendous winds that develop above the rapidly spinning planet. Winds blow counterclockwise around this disturbance at about 250 miles per hour. Hurricanes on Earth rarely generate winds ...
Nebula Theory
... rocks on Earth and meteorites to test the amount of (parent isotope) compared to the amount of ...
... rocks on Earth and meteorites to test the amount of (parent isotope) compared to the amount of ...
MoonsRings
... The Galilean Moons Galileo saw 4 major moons around Jupiter. Each of them is rather different. The surfaces of Io and Europa are rather young, Ganymede and Callisto have lots of craters. The outer 3 have icy surfaces. The moons keep one face towards Jupiter due to tides. ...
... The Galilean Moons Galileo saw 4 major moons around Jupiter. Each of them is rather different. The surfaces of Io and Europa are rather young, Ganymede and Callisto have lots of craters. The outer 3 have icy surfaces. The moons keep one face towards Jupiter due to tides. ...
Nice model
![](https://commons.wikimedia.org/wiki/Special:FilePath/Lhborbits.png?width=300)
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).