second grade - Math/Science Nucleus
... should be a shape of a planet on a stick for each of the students (3 of each planet). 2. This lab works best outdoors. Divide the class into groups of eleven or more. Explain the lab to the students. Tell them that their groups will compete to see who can "measure" the relative distances of the plan ...
... should be a shape of a planet on a stick for each of the students (3 of each planet). 2. This lab works best outdoors. Divide the class into groups of eleven or more. Explain the lab to the students. Tell them that their groups will compete to see who can "measure" the relative distances of the plan ...
Outer Planets
... Saturn’s Radiation •Saturn radiates between 1.5 and 2.5 times as much energy as it receives from the sun. •Similar to Jupiter, it obtains sources of internal heat. •It has a weak magnetic field. ...
... Saturn’s Radiation •Saturn radiates between 1.5 and 2.5 times as much energy as it receives from the sun. •Similar to Jupiter, it obtains sources of internal heat. •It has a weak magnetic field. ...
ASTR 241 syllabus Barnes
... This course introduces students to the Solar System as an arena for physics, and teaches them to solve Solar System problems by applying basic physical laws. Students passing this course will be able to calculate orbital trajectories of planets and other objects, evaluate surface temperatures for pl ...
... This course introduces students to the Solar System as an arena for physics, and teaches them to solve Solar System problems by applying basic physical laws. Students passing this course will be able to calculate orbital trajectories of planets and other objects, evaluate surface temperatures for pl ...
Rotation and Revolution of the Earth-PPT
... This is a model of the sun’s light as it strikes the earth. ...
... This is a model of the sun’s light as it strikes the earth. ...
Possibilities for life elsewhere in the Solar System In our fifth
... Tides on the Earth are caused primarily by the gravity of the Moon, and secondarily by the gravity of the Sun. Basically, the part of the ocean that faces the Moon is closer to it than the Earth on average. Therefore, that part is pulled more strongly, leading to water that is slightly raised, i.e., ...
... Tides on the Earth are caused primarily by the gravity of the Moon, and secondarily by the gravity of the Sun. Basically, the part of the ocean that faces the Moon is closer to it than the Earth on average. Therefore, that part is pulled more strongly, leading to water that is slightly raised, i.e., ...
File
... • The center of the nebula became more dense and the temperature increased. • The Sun formed from nuclear reactions in the center of the nebula. • Material farther away from the center of the nebula formed a disk and began to clump together, eventually becoming planets. ...
... • The center of the nebula became more dense and the temperature increased. • The Sun formed from nuclear reactions in the center of the nebula. • Material farther away from the center of the nebula formed a disk and began to clump together, eventually becoming planets. ...
The Planets and Their Moons
... Adrastea, Thebe, Callirrhoe, Themisto, Kalyke, Iocaste, Erinome, Harpalyke, Isonoe, Praxidike, Megaclite, Taygete, Chaldene, Autonoe, Thyone, Hermippe, Eurydome, Sponde, Pasithee, Euanthe, Kale, Orthosie, Euporie, Aitne, plus others yet to receive names ...
... Adrastea, Thebe, Callirrhoe, Themisto, Kalyke, Iocaste, Erinome, Harpalyke, Isonoe, Praxidike, Megaclite, Taygete, Chaldene, Autonoe, Thyone, Hermippe, Eurydome, Sponde, Pasithee, Euanthe, Kale, Orthosie, Euporie, Aitne, plus others yet to receive names ...
conjunction and opposition
... The sequence of pictures below show the occultation of Jupiter behind the moon ...
... The sequence of pictures below show the occultation of Jupiter behind the moon ...
To Jupiter … and Beyond! - Five Star Publications, Inc.
... 14-year mission by plunging into the dense atmosphere of Jupiter. Moving at more than 100,000 miles per hour, it was crushed, disintegrated and lost forever. But that little spacecraft taught us much about Jupiter. Never fear, your spaceship will not have the same fate. When you get to Jupiter, you ...
... 14-year mission by plunging into the dense atmosphere of Jupiter. Moving at more than 100,000 miles per hour, it was crushed, disintegrated and lost forever. But that little spacecraft taught us much about Jupiter. Never fear, your spaceship will not have the same fate. When you get to Jupiter, you ...
Chapter 6 Lecture 4
... Earth’s moon was probably created when a big planetesimal slammed into the newly forming Earth. Other large impacts may be responsible for other exceptions like rotation of Venus and Uranus ...
... Earth’s moon was probably created when a big planetesimal slammed into the newly forming Earth. Other large impacts may be responsible for other exceptions like rotation of Venus and Uranus ...
Comet Hayukatake
... does for the tail of a comet. • In the outer solar system the volatiles are in the form of ice. Ices can stick together and make larger bodies. • Jupiter originally was a mixture of rocky material and ice. It grew large enough to be able to hold onto hydrogen and helium. It ...
... does for the tail of a comet. • In the outer solar system the volatiles are in the form of ice. Ices can stick together and make larger bodies. • Jupiter originally was a mixture of rocky material and ice. It grew large enough to be able to hold onto hydrogen and helium. It ...
Pocket Planetarium V17N3.indd
... lower in the west at nightfall. As a result, the ringed planet will be visible for an increasingly shorter period in the evening. Note how the gap between Venus and Saturn diminishes as the weeks go by: From September 16 to 19, the two planets are less than 4 degrees apart. The ringed planet continu ...
... lower in the west at nightfall. As a result, the ringed planet will be visible for an increasingly shorter period in the evening. Note how the gap between Venus and Saturn diminishes as the weeks go by: From September 16 to 19, the two planets are less than 4 degrees apart. The ringed planet continu ...
Revolving Planets Lesson Plan
... sidewalk chalk, draw one circle (the sun) with 8 concentric circles surrounding it. Label each circle as follows, starting with the one closest to the sun and moving outwards: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. (See “Solar System Diagram” for an example.) ...
... sidewalk chalk, draw one circle (the sun) with 8 concentric circles surrounding it. Label each circle as follows, starting with the one closest to the sun and moving outwards: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. (See “Solar System Diagram” for an example.) ...
The two-and-a-half-hour school program experience is one of the
... Water Is Life in the Samuel Oschin Planetarium. The 30minute program in the Observatory’s grand 75-foot planetarium theater introduces students to the beauty and wonder of the night sky using both the most sophisticated star projector in the world and a stunning, all-dome digital laser projection sy ...
... Water Is Life in the Samuel Oschin Planetarium. The 30minute program in the Observatory’s grand 75-foot planetarium theater introduces students to the beauty and wonder of the night sky using both the most sophisticated star projector in the world and a stunning, all-dome digital laser projection sy ...
Unit 3, Chapter 2 Quiz
... Earth for thousands of years. Uranus was only discovered by telescope in 1781. Why can humans see Mercury using only their eyes, while they need telescopes to look at Uranus? a) Mercury is made so hot by the Sun that it glows. b) Mercury is much closer to Earth than Uranus. c) Mercury shines by its ...
... Earth for thousands of years. Uranus was only discovered by telescope in 1781. Why can humans see Mercury using only their eyes, while they need telescopes to look at Uranus? a) Mercury is made so hot by the Sun that it glows. b) Mercury is much closer to Earth than Uranus. c) Mercury shines by its ...
The Planets and Solar System Objects - Coca
... Aurora Borealis - Charged particles guided by Earth's magnetic field toward the North Pole, which hit our atmosphere causing it to glow. Northern Lights: Aurora Australis - southern lights Magnetosphere - region around the Earth in which the magnetic field keeps out charged particles flowing from th ...
... Aurora Borealis - Charged particles guided by Earth's magnetic field toward the North Pole, which hit our atmosphere causing it to glow. Northern Lights: Aurora Australis - southern lights Magnetosphere - region around the Earth in which the magnetic field keeps out charged particles flowing from th ...
(the inner and outer planets).
... •Pluto is small compared to the other outer planets. •Pluto is composed of rock compared to the “gas giants.” •Pluto does not have any rings. ...
... •Pluto is small compared to the other outer planets. •Pluto is composed of rock compared to the “gas giants.” •Pluto does not have any rings. ...
Earth-Sun Relationships - Los Angeles Mission College
... • Billions of galaxies – so far apart that measured in light years (1 light year = 6 trillion miles; speed of light is 186,000 mps) • The closest galaxy to ours is 75,000 light years away • Some of these distant systems are similar to our own Milky Way Galaxy, while others are quite different These ...
... • Billions of galaxies – so far apart that measured in light years (1 light year = 6 trillion miles; speed of light is 186,000 mps) • The closest galaxy to ours is 75,000 light years away • Some of these distant systems are similar to our own Milky Way Galaxy, while others are quite different These ...
FOSS Planetary Science Glossary 1 FOSS Planetary
... Orientation: The positioning of something, or the position or direction in which something lies. Origin: A starting point or place. Parallel: When lines, planes, or curved surfaces are always the same distance apart and never meet. Pattern: A regular or repeating form, order, or arrangement. Phase: ...
... Orientation: The positioning of something, or the position or direction in which something lies. Origin: A starting point or place. Parallel: When lines, planes, or curved surfaces are always the same distance apart and never meet. Pattern: A regular or repeating form, order, or arrangement. Phase: ...
Orrery
An orrery is a mechanical model of the solar system that illustrates or predicts the relative positions and motions of the planets and moons, usually according to the heliocentric model. It may also represent the relative sizes of these bodies; but since accurate scaling is often not practical due to the actual large ratio differences, a subdued approximation may be used instead. Though the Greeks had working planetaria, the first orrery that was a planetarium of the modern era was produced in 1704, and one was presented to Charles Boyle, 4th Earl of Orrery — whence came the name. They are typically driven by a clockwork mechanism with a globe representing the Sun at the centre, and with a planet at the end of each of the arms.