![es1 solar system computer lab](http://s1.studyres.com/store/data/014242395_1-85863895486fe5b283fde6597bfa2520-300x300.png)
es1 solar system computer lab
... Follow the instructions to launch a probe to Mars. Try it a few times. If you keep missing Mars use the hint button for assistance but you should try first without this tool. Describe the challenge in deciding on a launch date. How long did it take for your shuttle to reach Mars? Quit out of the bro ...
... Follow the instructions to launch a probe to Mars. Try it a few times. If you keep missing Mars use the hint button for assistance but you should try first without this tool. Describe the challenge in deciding on a launch date. How long did it take for your shuttle to reach Mars? Quit out of the bro ...
Grade 3: Solar System
... • Teacher will assign individual or small groups of students to be a specific planet, or the sun within the solar system. • Each group or student will be given a ball of string, four planet marker cards, and a planet information card that tells them the length of string they should cut which will re ...
... • Teacher will assign individual or small groups of students to be a specific planet, or the sun within the solar system. • Each group or student will be given a ball of string, four planet marker cards, and a planet information card that tells them the length of string they should cut which will re ...
Lesson #5: Ch 3, Section 3, The Inner Planets
... This lesson went well because the students are generally interested in the solar system, especially when Earth is involved. They have great insight into the solar system and I feel that this project will allow them to dive deeper into the solar system and showcase their skills in two ways instead of ...
... This lesson went well because the students are generally interested in the solar system, especially when Earth is involved. They have great insight into the solar system and I feel that this project will allow them to dive deeper into the solar system and showcase their skills in two ways instead of ...
solar system websearch
... system and _______________ is the largest planetary moon. F. Saturn is known for its __________. Saturn's largest moon is called _____________________. ...
... system and _______________ is the largest planetary moon. F. Saturn is known for its __________. Saturn's largest moon is called _____________________. ...
3 The Outer Planets
... is so far from the sun that it does not reflect much sunlight. You cannot see it from Earth without using a telescope. Uranus is different from the other planets because it is “tipped” on its side. As shown in the figure below, the north and south poles of Uranus point almost directly at the sun. Th ...
... is so far from the sun that it does not reflect much sunlight. You cannot see it from Earth without using a telescope. Uranus is different from the other planets because it is “tipped” on its side. As shown in the figure below, the north and south poles of Uranus point almost directly at the sun. Th ...
A Planetary Overview
... oddball world. One of its 3 moons is half its size (Charon). It will be visited by spacecraft in 2015. • Soon in the 1990s other objects out where Pluto lived were being discovered. One of these, Eris, was found to be a little larger than Pluto • In 2006, the phrase “dwarf planet” was defined for th ...
... oddball world. One of its 3 moons is half its size (Charon). It will be visited by spacecraft in 2015. • Soon in the 1990s other objects out where Pluto lived were being discovered. One of these, Eris, was found to be a little larger than Pluto • In 2006, the phrase “dwarf planet” was defined for th ...
Planets - WordPress.com
... Earth's size — that its core should have cooled off long ago. The discovery in 2007 by Earth-based radar observations that Mercury's core may still be molten could help explain its magnetism, though the solar wind may play a role in dampening the planet’s magnetic field ...
... Earth's size — that its core should have cooled off long ago. The discovery in 2007 by Earth-based radar observations that Mercury's core may still be molten could help explain its magnetism, though the solar wind may play a role in dampening the planet’s magnetic field ...
File - Mrs. Oakley`s Weebly
... is made up of matter and energy. Galaxies are composed of stars, gas, dust, dark matter, and solar systems. Our Solar System is contained in a galaxy known as the Milky Way. Until the mid-1600s, people believed in the geocentric model: that Earth (geo) was the center (centric) of the universe. It wa ...
... is made up of matter and energy. Galaxies are composed of stars, gas, dust, dark matter, and solar systems. Our Solar System is contained in a galaxy known as the Milky Way. Until the mid-1600s, people believed in the geocentric model: that Earth (geo) was the center (centric) of the universe. It wa ...
© Space Explorers, Inc.
... over half the surface of Mars is desert-like. Scientists now believe there are large amounts of water trapped below the surface. The Asteroid Belt lies between Mars and Jupiter. The belt is composed mainly of small (compared to planets!) solid pieces of rock. The largest is Ceres, which is 623 miles ...
... over half the surface of Mars is desert-like. Scientists now believe there are large amounts of water trapped below the surface. The Asteroid Belt lies between Mars and Jupiter. The belt is composed mainly of small (compared to planets!) solid pieces of rock. The largest is Ceres, which is 623 miles ...
Jupiter - pridescience
... when Jupiter passes directly in front of the sun. They are made of small rocks and dust, and they are dark in color. ...
... when Jupiter passes directly in front of the sun. They are made of small rocks and dust, and they are dark in color. ...
Solar System - Bishop Seabury Academy
... as iron in the liquid state • The stronger fields of the Jovian planets are generated by liquid metallic hydrogen or by water with ionized molecules dissolved in it ...
... as iron in the liquid state • The stronger fields of the Jovian planets are generated by liquid metallic hydrogen or by water with ionized molecules dissolved in it ...
Terrestrial or Inner Planets
... there is little such liquid material in the planet’s interior or that the liquid is not in a state of motion ...
... there is little such liquid material in the planet’s interior or that the liquid is not in a state of motion ...
time and origins power point
... Observations are indirect We were not there to see it What we can see is very slow So… – we do not try to produce a solar nebula model that exactly describes our Solar System and the planetary orbits and their masses – rather we look for a model that describes the characteristic properties of the pl ...
... Observations are indirect We were not there to see it What we can see is very slow So… – we do not try to produce a solar nebula model that exactly describes our Solar System and the planetary orbits and their masses – rather we look for a model that describes the characteristic properties of the pl ...
Solar System Webquest
... things made up to help describe the night sky _ help us tell which stars are which ______________________ 6. Why do we see different constellations throughout the year? _because the earth moves in relation to the sky 7. Define (Click on ZOOM Astronomy and then glossary): a. light year -_ the distanc ...
... things made up to help describe the night sky _ help us tell which stars are which ______________________ 6. Why do we see different constellations throughout the year? _because the earth moves in relation to the sky 7. Define (Click on ZOOM Astronomy and then glossary): a. light year -_ the distanc ...
ppt
... • Its mountains are much taller than those on Earth reaching heights of 16 km (52,000 feet) • Io appears to be a rocky silicate rich body that has a dense Fe/FeS core that extends halfway to the surface with a partially melted silicate-rich mantle, and a thin rocky crust. ...
... • Its mountains are much taller than those on Earth reaching heights of 16 km (52,000 feet) • Io appears to be a rocky silicate rich body that has a dense Fe/FeS core that extends halfway to the surface with a partially melted silicate-rich mantle, and a thin rocky crust. ...
The most important questions to study for the exam
... frozen surface, as deduced from ice-flow patterns on spacecraft images and their inferred movement. If so, what would be the source of heating that keeps this water from freezing? • Solar radiation, which at Jupiter's orbital distance is easily capable of melting ice. • Tidal distortion and stress c ...
... frozen surface, as deduced from ice-flow patterns on spacecraft images and their inferred movement. If so, what would be the source of heating that keeps this water from freezing? • Solar radiation, which at Jupiter's orbital distance is easily capable of melting ice. • Tidal distortion and stress c ...
FAR, FAR AWAY - Museum of Science and Industry
... EXPERIMENT: SOLAR SYSTEM SCALE MODEL AND JETPACK ...
... EXPERIMENT: SOLAR SYSTEM SCALE MODEL AND JETPACK ...
The Planets
... 4. We would almost surely not survive on Venus, firstly, because of the scorching temperature. As described in Q#3, Venus’ atmosphere causes the temperatures to rise to even higher than 470 degrees Celsius. The probes that have landed on Venus never lasted more than 2 hours against the heat. Also, V ...
... 4. We would almost surely not survive on Venus, firstly, because of the scorching temperature. As described in Q#3, Venus’ atmosphere causes the temperatures to rise to even higher than 470 degrees Celsius. The probes that have landed on Venus never lasted more than 2 hours against the heat. Also, V ...
Solar System Weather
... obtained an atmosphere, while others do not. Why is it that some planets have a thicker atmosphere than others? These answers will be included in our final report. Much research has been done to acquire knowledge of these planets. Our plan is to develop a paper that includes all of the planets and t ...
... obtained an atmosphere, while others do not. Why is it that some planets have a thicker atmosphere than others? These answers will be included in our final report. Much research has been done to acquire knowledge of these planets. Our plan is to develop a paper that includes all of the planets and t ...
Pluto Not A Planet
... Pluto has always been an “oddball” when it was considered a planet. Its composition is like a comet's. It is said that its elliptical orbit is tilted 17 degrees from the orbits of the other planets and is only 0.07 times the mass of the other celestial objects found in its orbit, so it does not mee ...
... Pluto has always been an “oddball” when it was considered a planet. Its composition is like a comet's. It is said that its elliptical orbit is tilted 17 degrees from the orbits of the other planets and is only 0.07 times the mass of the other celestial objects found in its orbit, so it does not mee ...
Lesson 5 - Introduction to the Solar System
... were considered to be planets for more than half a century, after which they became too numerous and were all demoted and reclassified as asteroids. However, Ceres was once again promoted and reclassified as a dwarf planet in 2006. Asteroid belt We continue to discover new asteroids, both in and out ...
... were considered to be planets for more than half a century, after which they became too numerous and were all demoted and reclassified as asteroids. However, Ceres was once again promoted and reclassified as a dwarf planet in 2006. Asteroid belt We continue to discover new asteroids, both in and out ...
The Outer Solar System Chapter 7:
... • Virtually no surface features visible from Earth • ~ 65 % of size of Earth’s Moon • Highly elliptical orbit; coming occasionally closer to the sun than Neptune ...
... • Virtually no surface features visible from Earth • ~ 65 % of size of Earth’s Moon • Highly elliptical orbit; coming occasionally closer to the sun than Neptune ...
How Big is our Solar System?
... One mini-marshmallow or other round object 0.4 - 0.5 inches in diameter ...
... One mini-marshmallow or other round object 0.4 - 0.5 inches in diameter ...
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).