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nebular theory - Marcia`s Science Teaching Ideas
nebular theory - Marcia`s Science Teaching Ideas

... 8. Inner protoplanets - most of their lightweight gases are boiled away, Outer protoplanets - the lightweight gases did not boil away so the appear much larger Why? because of the heat from the nearby sun 9. Moons (Protomoons) 10. Perhaps one of Neptune's moons broke away or was pushed by an impact) ...
PlanetTour
PlanetTour

... European space agency http://www.esa.int/export/SPECIALS/Mars_Express/ ...
Introduction to the Solar System
Introduction to the Solar System

... The ancient Greeks believed that Earth was at the center of the universe, as shown in Figure 1.1. This view is called the geocentric model of the universe. Geocentric means "Earth-centered." In the geocentric model, the sky, or heavens, are a set of spheres layered on top of one another. Each object ...
A Sense of Scale - Young Scientists Journal
A Sense of Scale - Young Scientists Journal

... Majoris, a supermassive black hole is currently theorised to have a maximum size of 10AU (VY has diameter 9AU, where one Astronomical Unit is the distance from Earth to the Sun). However, while only a little larger, it is far more massive; although the star is estimated to be around 20 times as mass ...
Document
Document

... The Universe has lots of motion The spinning of the Earth causes the rising and setting of the Sun and stars The revolution of the Earth around the Sun determines the year The tilt of the Earth determines the seasons The spinning, revolution and tilt determine the part of the sky which is visible Yo ...
Worksheet 1
Worksheet 1

... d. small icy bodies in the extreme outer parts of the Solar System that are disturbed into orbits that bring them closer to the Sun e. luminous clouds in the Earth’s upper atmosphere created when a small asteroid is captured by the Earth’s gravitational force 27. The asteroid belt lies between the o ...
fall_2000_final
fall_2000_final

... E. the comet nears aphelion. 39. The Moon’s orbit is slightly inclined to Earth’s orbit. This explains A. why the Sun moves along the ecliptic. B. why we never see the lunar far side. C. why we see the Moon sometimes during the day. D. why earthshine occurs. E. why a solar eclipse doesn’t occur ever ...
star guide 2013
star guide 2013

... clouds in the atmosphere and dark regions of exposed rock on the surface. Beyond Mars lies the gas giant Jupiter, the largest planet in the Solar System. Viewed through a telescope the planet’s disc appears crossed by dark belts. A huge storm known as the Great Red Spot can also be seen. This is two ...
Slide 1
Slide 1

The Solar System - Wayne State University
The Solar System - Wayne State University

Gnomon V26 No2.pub - The Association for Astronomy Education
Gnomon V26 No2.pub - The Association for Astronomy Education

... Union has properly classified Pluto as an object belonging to a different class from the main solar planets. This provides a unique opportunity to teach about the formation and nature of the solar system. It is important to teach that, when Pluto was discovered a few decades ago, it was assumed to b ...
U - Net Start Class
U - Net Start Class

... Sunspots-areas on the sun that are cooler than the rest of the sun. ...
1_31_planetary calculator
1_31_planetary calculator

... speeds and at different distances from the Sun. This activity makes students realize how big these differences are and how important it is to choose an adequate scale for sizes, distances and revolution periods, to represent the Solar System. With ”Eyes on the Solar System” software and a hands-on m ...
The Inner Planets
The Inner Planets

Terrestrial Planets
Terrestrial Planets

...  All planets except Venus and Uranus have prograde rotation  The sun contains all the mass  The planets (especially Jupiter and Saturn) contain most of the angular momentum in the solar system  Abundance gradient. Inner solar system is poor in light volatile gases such as H, He, but rich in Fe & ...
astr221lect2x
astr221lect2x

... • Sidereal year: Time for Earth to complete one orbit of Sun • Tropical year: Time for Earth to complete one cycle of seasons • Tropical year is about 20 ...
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Name

... Base your answers to question 5 on the diagram in below. The diagram shows Earth revolving around the Sun. Letters A, B, C, and D represent Earth’s location in its orbit on the first day of the four seasons. Aphelion (farthest distance from the Sun) and perihelion (closest distance to the Sun) are l ...
STARS AND PLANETS: A NEW SET OF MIDDLE SCHOOL
STARS AND PLANETS: A NEW SET OF MIDDLE SCHOOL

... Scale Model Solar System activities are commonly used at levels ranging elementary [1] to college [2] for the purpose of helping students visualize their “place in space”. Star and Planets (for grades 6-8) expands upon the idea of a Scale Model Solar System to include the sizes and distance of stars ...
File
File

... ____2. The earth has seasons because _________________. a. The gravitational pull of the Moon b. The Earth is tilted on its axis 23.5  c. The Earth changes temperature ...
Asteroids, Comets, Meteors…what`s the difference
Asteroids, Comets, Meteors…what`s the difference

... Asteroids, Comets, Meteors…what’s the difference? Astronomy Name: ...
What did ancient civilizations achieve in astronomy?
What did ancient civilizations achieve in astronomy?

... hypothesis accordingly. But, since it was not permissible to ignore, those eight minutes pointed the road to a complete reformation in astronomy. ...
Planetary Parachute
Planetary Parachute

... created to model our solar system as it orbits the sun. The Planetary Parachute can be used as a cooperative educational activity that provides a variety of movement skills integrated with science and math concepts. It provides a “hands-on” activity in which the students can see, feel, and interact ...
20.1 A Solar System is Born
20.1 A Solar System is Born

... 3. Planetesimals begin to form within the swirling disk. 4. As the largest planetesimals grown in size, their gravity attracts more gas and dust. 5. Smaller planetesimals collide with the larger ones, and planets begin to grow 6. A star is born, and the remaining gas and dust are blown out of the ne ...
Planetary Science - Laboratory for Atmospheric and Space Physics
Planetary Science - Laboratory for Atmospheric and Space Physics

... Planetary science focuses on many aspects of solar system objects, from their deep interiors to the distant influences of a planet’s gravitational or magnetic field far from the planet’s surface. LASP planetary scientists study data from ground, telescope, and space-based instruments to understand t ...
Davis Planetarium
Davis Planetarium

... Time returns, November 3 – don’t forget to turn your clocks back one hour before you go to bed on Saturday, November 2! Comet ISON in conjunction with the Sun, November 28 – You’ll likely hear more about this comet as it makes its way around the Sun. Comet ISON is new to our sky and the show it may ...
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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.
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