Planetary Order
... When the teacher and students are finished with the lecture portion of the lesson, the students can then start the activity which is creating the Planetary Playing Cards. The Planetary Playing Cards are a handout that the teacher must pass out to students. Students will be creating 11 cards, one ...
... When the teacher and students are finished with the lecture portion of the lesson, the students can then start the activity which is creating the Planetary Playing Cards. The Planetary Playing Cards are a handout that the teacher must pass out to students. Students will be creating 11 cards, one ...
Jupiter`s Moons - cloudfront.net
... small irregularly shaped moons orbiting close to Jupiter. They are probably the source of the material for Jupiter’s rings. Since 1999 45 more smaller moons were discovered orbiting far from Jupiter and are either captured asteroids or the result of collisions. ...
... small irregularly shaped moons orbiting close to Jupiter. They are probably the source of the material for Jupiter’s rings. Since 1999 45 more smaller moons were discovered orbiting far from Jupiter and are either captured asteroids or the result of collisions. ...
1 GS106 Lab 1 and 2 Answer Key READING QUESTIONS Four
... Outer Planets (Jupiter, Saturn, Uranus, Neptune): large diameter, less dense, cooler surface temperatures Which Planet Would Float in Water? - Saturn Jupiter Day = 9.9 Earth Hours Venus Day = 5832.5 Earth Hours Earth Years comprising a Jupiter year? = 11.9 Earth Yrs 2 planets with 90% of mass in Sol ...
... Outer Planets (Jupiter, Saturn, Uranus, Neptune): large diameter, less dense, cooler surface temperatures Which Planet Would Float in Water? - Saturn Jupiter Day = 9.9 Earth Hours Venus Day = 5832.5 Earth Hours Earth Years comprising a Jupiter year? = 11.9 Earth Yrs 2 planets with 90% of mass in Sol ...
Mercury The planet Mercury looks a little bit like Earth`s moon. Like
... beyond that orbit. From 1979 until early 1999, Pluto had actually been the eighth planet from the sun. Then, on Feb. 11, 1999, it crossed Neptune's path and once again became the solar system's most distant planet — until it was demoted to dwarf planet status. Pluto will stay beyond Neptune for 228 ...
... beyond that orbit. From 1979 until early 1999, Pluto had actually been the eighth planet from the sun. Then, on Feb. 11, 1999, it crossed Neptune's path and once again became the solar system's most distant planet — until it was demoted to dwarf planet status. Pluto will stay beyond Neptune for 228 ...
Solar System - Joy Senior Secondary School
... • It is the 8th planet from the sun. • It is Uranus’ twin although it is a little smaller. • It is named after the roman god of the sea. ...
... • It is the 8th planet from the sun. • It is Uranus’ twin although it is a little smaller. • It is named after the roman god of the sea. ...
Name: Category: 30 points 20 points 10 points 0 points Accurate
... Your child has been assigned to complete a solar system project. He/She may choose one of the choices below to complete. The project will be due no later than November 10, 2016. If your child completes their project earlier than this date, they are more than welcome to turn it in. ...
... Your child has been assigned to complete a solar system project. He/She may choose one of the choices below to complete. The project will be due no later than November 10, 2016. If your child completes their project earlier than this date, they are more than welcome to turn it in. ...
Using an Orrery – teachers` guide
... “morning stars” or “evening stars” respectively. The outer planets (those farther from the Sun than Earth) may be seen at different times depending on their position. If used with the orrery set up with today’s longitudes, this method gives an approximate guide to which planets one could see tonight ...
... “morning stars” or “evening stars” respectively. The outer planets (those farther from the Sun than Earth) may be seen at different times depending on their position. If used with the orrery set up with today’s longitudes, this method gives an approximate guide to which planets one could see tonight ...
The interiors of Planets
... • An obvious question is - what is the maximum size a planet can have? To figure this out, first imagine that we are building a cold planet up in size. • Initially, ...
... • An obvious question is - what is the maximum size a planet can have? To figure this out, first imagine that we are building a cold planet up in size. • Initially, ...
Chapter 9 - WordPress.com
... Has Earth’s Magnetic field ever switched polarity? Yes, 9 times in the last 35 million years, last reversal was about 30,000 years ago. What are the four basic processes that shape surface geology? Impact cratering, volcanism, tectonics, and erosion. Describe the surface features of the terrestrial ...
... Has Earth’s Magnetic field ever switched polarity? Yes, 9 times in the last 35 million years, last reversal was about 30,000 years ago. What are the four basic processes that shape surface geology? Impact cratering, volcanism, tectonics, and erosion. Describe the surface features of the terrestrial ...
The Certification Exam
... Should, recommended, should not, not recommended • There may exist valid reasons in particular circumstances to ignore a particular item, but the full implications must be understood and carefully weighed before choosing a different course ...
... Should, recommended, should not, not recommended • There may exist valid reasons in particular circumstances to ignore a particular item, but the full implications must be understood and carefully weighed before choosing a different course ...
Observing the Solar System
... know these planets by the names the ancient Romans later gave them: Mercury, Venus, Mars, Jupiter, and Saturn. Most early Greek astronomers believed the universe to be perfect, with Earth at the center. The Greeks thought that Earth is inside a rotating dome they called the celestial sphere. Since g ...
... know these planets by the names the ancient Romans later gave them: Mercury, Venus, Mars, Jupiter, and Saturn. Most early Greek astronomers believed the universe to be perfect, with Earth at the center. The Greeks thought that Earth is inside a rotating dome they called the celestial sphere. Since g ...
Webquest – Answer Key
... 15. List the 2 planet that have the greatest density? Earth and Mercury. Are they inner or outer planets? inner. 16. Why are the outer planets less dense than the inner planets? The outer planets are less dense because they don't have water on them and the rocky planets tend to have more water. Also ...
... 15. List the 2 planet that have the greatest density? Earth and Mercury. Are they inner or outer planets? inner. 16. Why are the outer planets less dense than the inner planets? The outer planets are less dense because they don't have water on them and the rocky planets tend to have more water. Also ...
Newton`s Gravity Applied (PowerPoint)
... It is ‘weightless’. But a push from you will not move it much! It still has all its mass. When you push it, the reaction force (remember Newton’s 3rd law) will push back on you. You move as a result. ...
... It is ‘weightless’. But a push from you will not move it much! It still has all its mass. When you push it, the reaction force (remember Newton’s 3rd law) will push back on you. You move as a result. ...
The Solar System - Solon City Schools
... Rotates every 16.1 hours. Revolves around the sun every 165 years. Thick atmosphere of hydrogen & helium. 13 moons (Triton). Temperature -200oC. Has an ring system. Had a Great Dark Spot that has since disappeared. ...
... Rotates every 16.1 hours. Revolves around the sun every 165 years. Thick atmosphere of hydrogen & helium. 13 moons (Triton). Temperature -200oC. Has an ring system. Had a Great Dark Spot that has since disappeared. ...
Getting to Know: Formation of Our Solar System
... Why do the planets orbit the Sun? The matter in the solar nebula rotated around its center. As the solar nebula collapsed, matter began rotating more quickly. Over time, this motion caused the solar nebula to flatten into a disk-like shape with the Sun at the center. The planets formed from the mat ...
... Why do the planets orbit the Sun? The matter in the solar nebula rotated around its center. As the solar nebula collapsed, matter began rotating more quickly. Over time, this motion caused the solar nebula to flatten into a disk-like shape with the Sun at the center. The planets formed from the mat ...
Mars` Moons
... Some asteroids cross Earth’s orbit and eventually collide with Earth Ceres is the largest asteroid There are several types of asteroids Meteorites are solid objects from space that reach the Earth’s surface Most meteorites are from asteroids, a few are from Mars and the Moon. Most meteors ...
... Some asteroids cross Earth’s orbit and eventually collide with Earth Ceres is the largest asteroid There are several types of asteroids Meteorites are solid objects from space that reach the Earth’s surface Most meteorites are from asteroids, a few are from Mars and the Moon. Most meteors ...
Discover the planets of our solar system In 90 minutes through the
... The Solar System consists of the Sun and the astronomical objects gravitationally bound in orbit around it, all of which formed from the collapse of a giant molecular cloud approximately 4.6 billion years ago. Of the many objects that orbit the Sun, most of the mass is contained within eight relativ ...
... The Solar System consists of the Sun and the astronomical objects gravitationally bound in orbit around it, all of which formed from the collapse of a giant molecular cloud approximately 4.6 billion years ago. Of the many objects that orbit the Sun, most of the mass is contained within eight relativ ...
8.1_Formation of the Universe
... Mother = Mars Just = Jupiter Sold = Saturn Us = Uranus Nine = Neptune Pizzas = Pluto (*Not a planet anymore) ...
... Mother = Mars Just = Jupiter Sold = Saturn Us = Uranus Nine = Neptune Pizzas = Pluto (*Not a planet anymore) ...
Goal: To understand what the Kuiper Belt is, and why it is
... • Pluto is tilted by 120 degrees. Yes, that is more that tipped over. • Like Venus, Pluto rotates backwards. ...
... • Pluto is tilted by 120 degrees. Yes, that is more that tipped over. • Like Venus, Pluto rotates backwards. ...
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).