Section 14.4 Outer Planets
... Uranus’s Moons Voyager 2 obtained clear, high-resolution images of each of the five large moons of Uranus known at the time: Miranda, Ariel, Umbriel, Titania, and Oberon . The two largest, Titania and Oberon, are about 1,600 kilometres (1,000 miles) in diameter, roughly half the size of Earth's Moo ...
... Uranus’s Moons Voyager 2 obtained clear, high-resolution images of each of the five large moons of Uranus known at the time: Miranda, Ariel, Umbriel, Titania, and Oberon . The two largest, Titania and Oberon, are about 1,600 kilometres (1,000 miles) in diameter, roughly half the size of Earth's Moo ...
Orbits of Planets and Moons
... 2. Planets closer to the sun have smaller, faster orbital paths. 3. Planets farther away from the sun have longer, slower orbital paths. ...
... 2. Planets closer to the sun have smaller, faster orbital paths. 3. Planets farther away from the sun have longer, slower orbital paths. ...
Chapter 24 Vocabulary link - Flushing Community Schools
... the nucleus. We have a famous one that orbits the Sun every 76 years. ...
... the nucleus. We have a famous one that orbits the Sun every 76 years. ...
4th-grade-science-lesson-plan
... cones representing the planets and the distance they are from the sun. *For best results have this outside 2. Give each child a space jam card 3. Have students get into groups so that there is one student with each planet. (If there are more than 8 students per group, hand out the introduction cards ...
... cones representing the planets and the distance they are from the sun. *For best results have this outside 2. Give each child a space jam card 3. Have students get into groups so that there is one student with each planet. (If there are more than 8 students per group, hand out the introduction cards ...
Planets-in-solar
... Many of the moons of our solar system are as intriguing as the planets. Earth's Moon holds many clues to the formation of our home world and rest of the solar system and offers a potential starting point for humanity to extend its reach deeper into space. Jupiter's Europa and Ganymede harbor signs o ...
... Many of the moons of our solar system are as intriguing as the planets. Earth's Moon holds many clues to the formation of our home world and rest of the solar system and offers a potential starting point for humanity to extend its reach deeper into space. Jupiter's Europa and Ganymede harbor signs o ...
Planet Card Game - Space Awareness
... for some time. Neptune has a very thin ring system and at least 14 moons. ...
... for some time. Neptune has a very thin ring system and at least 14 moons. ...
The Planet Walk Brochure - Take it on the walk for fun on the go
... To begin, visit the Sun station on the corner of 5th Avenue and “G” Street. The map will guide you. Then proceed down 5th Avenue, following the signs to each of the four inner planet stations: Mercury, Venus, Earth, and Mars. If you’re up for more, you can continue the Planet Walk along the Tony Kno ...
... To begin, visit the Sun station on the corner of 5th Avenue and “G” Street. The map will guide you. Then proceed down 5th Avenue, following the signs to each of the four inner planet stations: Mercury, Venus, Earth, and Mars. If you’re up for more, you can continue the Planet Walk along the Tony Kno ...
PHYS 185 Chapter 5 Highlights 1. Definition of a planet a. Who: The
... ii. Eris in 2003 – larger than Pluto and has a moon Dysnomia. So you can’t define a planet based on it having a moon, unless you make Eris a planet. iii. Sedna in 2004 - 3X further out than Pluto, bigger than Quaoar iv. more than 1000 objects found that are at least 1/2 the size of Pluto, some of th ...
... ii. Eris in 2003 – larger than Pluto and has a moon Dysnomia. So you can’t define a planet based on it having a moon, unless you make Eris a planet. iii. Sedna in 2004 - 3X further out than Pluto, bigger than Quaoar iv. more than 1000 objects found that are at least 1/2 the size of Pluto, some of th ...
supplemental educational materials PDF
... Astronomers are concerned that they might send the New Horizons spacecraft on a collision course with some space debris. They are counting on the spacecraft to send back amazing pictures of our faraway dwarf neighbor, and they do not want New Horizons to be destroyed before it makes its observations ...
... Astronomers are concerned that they might send the New Horizons spacecraft on a collision course with some space debris. They are counting on the spacecraft to send back amazing pictures of our faraway dwarf neighbor, and they do not want New Horizons to be destroyed before it makes its observations ...
Planets Order, Characteristics, and Orbits
... how objects in A the solar system are in . regular and predictable motions that explain such phenomena as days, years, seasons, eclipses, tides and moon cycles. ...
... how objects in A the solar system are in . regular and predictable motions that explain such phenomena as days, years, seasons, eclipses, tides and moon cycles. ...
Best of the Solar System Handout.
... over 300 km long, and up to 8 km deep. The three brown circles on the left are very large volcanoes about 300 km across, larger than any volcano on Earth. You cannot see as many craters on Mars as you can see on the Moon or Mercury. MARS - Viking Lander 1 View of the Surface This scene from the surf ...
... over 300 km long, and up to 8 km deep. The three brown circles on the left are very large volcanoes about 300 km across, larger than any volcano on Earth. You cannot see as many craters on Mars as you can see on the Moon or Mercury. MARS - Viking Lander 1 View of the Surface This scene from the surf ...
Exploring Our Solar System: A Journey
... planet. The surface of the Earth is estimated to only be about 100 million years old • Most of the Earth’s mass, is found in its liquid mantel layer just below the crust ...
... planet. The surface of the Earth is estimated to only be about 100 million years old • Most of the Earth’s mass, is found in its liquid mantel layer just below the crust ...
Quiz on Solar System study guide with key
... • Know how the shape of the orbits of the planets (more circular) generally compare to the shape of comets’ orbits (more elliptical) • Know that a comet’s speed in its orbit is faster closer to the sun and slower farther from the sun • Know that comets originate from either the Kuiper belt or the Oo ...
... • Know how the shape of the orbits of the planets (more circular) generally compare to the shape of comets’ orbits (more elliptical) • Know that a comet’s speed in its orbit is faster closer to the sun and slower farther from the sun • Know that comets originate from either the Kuiper belt or the Oo ...
Astronomy Study Guide ACADEMIC
... 9. Where is Pluto located and why is he no longer a planet? 10. Venus is called Earth’s twin planet. Why? What do they have in common? 11. How do astronomers explain that Venus rotates in the opposite direction from most planets and moons? What is the vocabulary word for that type of rotation? 12. N ...
... 9. Where is Pluto located and why is he no longer a planet? 10. Venus is called Earth’s twin planet. Why? What do they have in common? 11. How do astronomers explain that Venus rotates in the opposite direction from most planets and moons? What is the vocabulary word for that type of rotation? 12. N ...
Glossary
... Mars- It is the fourth planet from the Sun. In some ways it’s like our Earth. Mars has volcanoes, valleys and sandy desert. Mercury- It is the closest planet to the Sun. It is a barren rocky planet and its surface is covered with huge holes or craters where rocks called meteorites have crashed into ...
... Mars- It is the fourth planet from the Sun. In some ways it’s like our Earth. Mars has volcanoes, valleys and sandy desert. Mercury- It is the closest planet to the Sun. It is a barren rocky planet and its surface is covered with huge holes or craters where rocks called meteorites have crashed into ...
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).