Days and Years (Sessions I and II) Days and
... planets and inner planets move around the Sun but at different distances? (The outer planets have a much farther distance to travel than the inner planets.) Would you call the marching band model a good one to use to represent what happens in our Solar System as planets revolve around the Sun? Why? ...
... planets and inner planets move around the Sun but at different distances? (The outer planets have a much farther distance to travel than the inner planets.) Would you call the marching band model a good one to use to represent what happens in our Solar System as planets revolve around the Sun? Why? ...
Solar System/Planet Formation
... Most planets have low obliquity Large outer planets have ~solar composition Small inner planets enriched in heavy elements Impact craters on virtually every planetary body “Debris” in asteroid belt, Kuiper belt Meteorites have common age: ~4.6 Ga ...
... Most planets have low obliquity Large outer planets have ~solar composition Small inner planets enriched in heavy elements Impact craters on virtually every planetary body “Debris” in asteroid belt, Kuiper belt Meteorites have common age: ~4.6 Ga ...
File
... c. _________ (!) methane on surface d. Similar to ___________ Earth (?) e. *Low surface _________ (1/7 gE) f. 10 x more gas -- 60% > pressure 3. Frigid -- ____ K surface C. Medium-sized moons 1. __ of 6 ________ locked 2. Similar densities - unlike Jupiter’s 3. _____ -- largest, but only 1/30th Mm 4 ...
... c. _________ (!) methane on surface d. Similar to ___________ Earth (?) e. *Low surface _________ (1/7 gE) f. 10 x more gas -- 60% > pressure 3. Frigid -- ____ K surface C. Medium-sized moons 1. __ of 6 ________ locked 2. Similar densities - unlike Jupiter’s 3. _____ -- largest, but only 1/30th Mm 4 ...
The Formation of Uranus and Neptune in the Jupiter
... and Saturn. In addition to the planetary-size objects, we included a trans-Saturnian disk of smaller objects stretching from 10 to 60 AU . In Series II and III, we investigated the evolution of a system where Jupiter grows rst. In Series II, we studied the behavior of four 15M cores distributed be ...
... and Saturn. In addition to the planetary-size objects, we included a trans-Saturnian disk of smaller objects stretching from 10 to 60 AU . In Series II and III, we investigated the evolution of a system where Jupiter grows rst. In Series II, we studied the behavior of four 15M cores distributed be ...
Solar System Trading Cards, Jr. Edition
... Solar System Trading Cards, Jr. Edition • www.nasa.gov ...
... Solar System Trading Cards, Jr. Edition • www.nasa.gov ...
planetinvasionwebquest[1]. - teachingandlearningwithtech
... What is the size of the planet? What is the length of days and years? Find 3 interesting facts about Jupiter. Find at least 1 similarity and one 1 difference between Jupiter and Earth. http://starchild.gsfc.nasa.gov/docs/StarChild/solar_system_level1/j upiter.html http://www.enchantedlearning.com/su ...
... What is the size of the planet? What is the length of days and years? Find 3 interesting facts about Jupiter. Find at least 1 similarity and one 1 difference between Jupiter and Earth. http://starchild.gsfc.nasa.gov/docs/StarChild/solar_system_level1/j upiter.html http://www.enchantedlearning.com/su ...
Workbook IP
... relationship and attributes of objects in the solar system. Understand and correctly use unit vocabulary. Using a table, identify physical properties of the components of the Solar System (i.e., planets, dwarf planets. comets, asteroids, meteors) ...
... relationship and attributes of objects in the solar system. Understand and correctly use unit vocabulary. Using a table, identify physical properties of the components of the Solar System (i.e., planets, dwarf planets. comets, asteroids, meteors) ...
Classroom activity
... autumnal equinoxes, dates when the day and night are of equal length in both hemispheres. In the Southern Hemisphere the seasons are the opposite. This can be easily seen in this model. At the end of the activity, students should be able to tell you that we have seasons because of the Earth’s tilt o ...
... autumnal equinoxes, dates when the day and night are of equal length in both hemispheres. In the Southern Hemisphere the seasons are the opposite. This can be easily seen in this model. At the end of the activity, students should be able to tell you that we have seasons because of the Earth’s tilt o ...
Giant Planets
... Saturn’s rings are made of chunks of water ice the size of a building or smaller. Larger chunks, considered to be tiny moons, orbit within the rings. Saturn’s main rings are very bright. The outermost ring is three times as wide as the planet, but it is usually too faint to see. Saturn’s rings have ...
... Saturn’s rings are made of chunks of water ice the size of a building or smaller. Larger chunks, considered to be tiny moons, orbit within the rings. Saturn’s main rings are very bright. The outermost ring is three times as wide as the planet, but it is usually too faint to see. Saturn’s rings have ...
Chapter 12 (in pdf)
... • Kuiper belt comets formed in the Kuiper belt: flat plane, aligned with the plane of planetary orbits, orbiting in the same direction as the planets. • Oort cloud comets were once closer to the Sun, but they were kicked out there by gravitational interactions with jovian planets: spherical distri ...
... • Kuiper belt comets formed in the Kuiper belt: flat plane, aligned with the plane of planetary orbits, orbiting in the same direction as the planets. • Oort cloud comets were once closer to the Sun, but they were kicked out there by gravitational interactions with jovian planets: spherical distri ...
Earth-like worlds on eccentric orbits - Physics
... The semi-major axis a and orbital period P were set to 1n0 AU and 365 days, respectively, for all of our model runs and solar luminosity was varied to simulate climates at different locations within the HZ. For simplicity, we also fixed the tilt of the spin axis, continental topography and atmospher ...
... The semi-major axis a and orbital period P were set to 1n0 AU and 365 days, respectively, for all of our model runs and solar luminosity was varied to simulate climates at different locations within the HZ. For simplicity, we also fixed the tilt of the spin axis, continental topography and atmospher ...
Pluto
... Phases: Be sure to include the sun in your drawing and the words: new moon, waxing crescent, first quarter, waxing gibbous, full moon, waning gibbous, last quarter, waning crescent. Include what phase the moon will be in on May 24. ...
... Phases: Be sure to include the sun in your drawing and the words: new moon, waxing crescent, first quarter, waxing gibbous, full moon, waning gibbous, last quarter, waning crescent. Include what phase the moon will be in on May 24. ...
A Brief History of Planetary Science
... Needed new definition when rest of solar system was discovered with telescopes ...
... Needed new definition when rest of solar system was discovered with telescopes ...
Remnants of Rock and Ice (Chapter 12)
... If we arrange the asteroids by their average distance from the Sun, or period, then we see gaps Orbital periods of objects in gaps are simple fractions of Jupiter’s 12 year orbit Caused by orbital resonances (Draw on board) ...
... If we arrange the asteroids by their average distance from the Sun, or period, then we see gaps Orbital periods of objects in gaps are simple fractions of Jupiter’s 12 year orbit Caused by orbital resonances (Draw on board) ...
Powerpoint - BU Imaging Science
... If we arrange the asteroids by their average distance from the Sun, or period, then we see gaps Orbital periods of objects in gaps are simple fractions of Jupiter’s 12 year orbit Caused by orbital resonances (Draw on board) ...
... If we arrange the asteroids by their average distance from the Sun, or period, then we see gaps Orbital periods of objects in gaps are simple fractions of Jupiter’s 12 year orbit Caused by orbital resonances (Draw on board) ...
Lab 3: The Galilean Revolution
... If your planet is Jupiter, you will measure the orbit of Ganymede. If your planet is Saturn, you will measure the orbit of Titan. If your planet is Uranus, you will measure the orbit of Oberon. If your planet is Neptune, you will measure the orbit of Triton. For each of your successful observations: ...
... If your planet is Jupiter, you will measure the orbit of Ganymede. If your planet is Saturn, you will measure the orbit of Titan. If your planet is Uranus, you will measure the orbit of Oberon. If your planet is Neptune, you will measure the orbit of Triton. For each of your successful observations: ...
Closest ever exoplanet is potentially habitable
... atmosphere and water may still be present. Under certain conditions, which remain hypothetical, the planet may even harbor liquid water on its surface and have an environment potentially favorable to life. Their findings can be accessed online. By definition, this is the closest exoplanet to Earth e ...
... atmosphere and water may still be present. Under certain conditions, which remain hypothetical, the planet may even harbor liquid water on its surface and have an environment potentially favorable to life. Their findings can be accessed online. By definition, this is the closest exoplanet to Earth e ...
Chapter8- Jovian Planet Systems
... • All of the Jovian planets have ring systems, including Jupiter. • Saturn’s rings are the most prominent and spectacular. They ...
... • All of the Jovian planets have ring systems, including Jupiter. • Saturn’s rings are the most prominent and spectacular. They ...
The Solar System - Thomas County Schools
... • The planets are divided into two groups – The inner planets are smaller, closer to the sun, and have rocky surfaces (Mercury, Venus, Earth, Mars) – The outer planets are larger, farther from the sun and do not have solid surfaces (Jupiter, Saturn, Uranus, Neptune) ...
... • The planets are divided into two groups – The inner planets are smaller, closer to the sun, and have rocky surfaces (Mercury, Venus, Earth, Mars) – The outer planets are larger, farther from the sun and do not have solid surfaces (Jupiter, Saturn, Uranus, Neptune) ...
second grade - Math/Science Nucleus
... effect) making the surface of Venus the hottest in the Solar System, about 750oK. Venus rotates very slowly, taking 243 days to complete one turn. It is named for the Roman goddess of love. Earth is a little more than 12,000 kilometers in diameter. It differs from the other planets because it has l ...
... effect) making the surface of Venus the hottest in the Solar System, about 750oK. Venus rotates very slowly, taking 243 days to complete one turn. It is named for the Roman goddess of love. Earth is a little more than 12,000 kilometers in diameter. It differs from the other planets because it has l ...
Moon Hunt
... 10. The planet Mars will probably be the next in line for a visit from Earthlings. On the back of this paper give 5 facts about each of Mars’ Moons. ...
... 10. The planet Mars will probably be the next in line for a visit from Earthlings. On the back of this paper give 5 facts about each of Mars’ Moons. ...
The Solar System: The Sun and the Planets
... planets such as incredibly hot Venus, desert-like Mars, and monster-sized Jupiter. In the night sky, the planets appear as only bright points of light because they are so far away. The four planets nearest the Sun are Mercury, Venus, Earth, and Mars. These small, rocky planets are considered part of ...
... planets such as incredibly hot Venus, desert-like Mars, and monster-sized Jupiter. In the night sky, the planets appear as only bright points of light because they are so far away. The four planets nearest the Sun are Mercury, Venus, Earth, and Mars. These small, rocky planets are considered part of ...
Tides, Moons, Rings, and Pluto
... A planet within the solar system is a celestial body that 1. Orbits the Sun 2. Is massive enough for its self- gravity to give it a nearly ...
... A planet within the solar system is a celestial body that 1. Orbits the Sun 2. Is massive enough for its self- gravity to give it a nearly ...
Lining Up the Planets - Math-4326
... A person or school purchasing this AIMS activity is hereby granted permission to make up to 200 copies of any portion of it, provided these copies will be used for educational purposes and only at one school site. Workshop or conference presenters may make one copy of a purchased activity for each p ...
... A person or school purchasing this AIMS activity is hereby granted permission to make up to 200 copies of any portion of it, provided these copies will be used for educational purposes and only at one school site. Workshop or conference presenters may make one copy of a purchased activity for each p ...