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0 Gravity, Rotation, Shape of the Earth 0.1 Inertia. Conservation laws
0 Gravity, Rotation, Shape of the Earth 0.1 Inertia. Conservation laws

... inertia depends on the direction of the axis. One should thus use the tensor of inertia. In a coordinate system with origin at the center of mass, there are three perpendicular axes, the principal axes of d’inertia, respective to which the moment of inertia is maximum, minimum, and intermediary. Not ...
Modeling the Solar System - American Museum of Natural History
Modeling the Solar System - American Museum of Natural History

... Use this lesson plan to create a moving model of relative planet speed. Preparation for the Investigation in the Beyond Planet Earth Exhibition From what students know about planets and space, along with what they observed in their models of the solar system, have them think about the challenges tha ...
because they reflect light from the sun.
because they reflect light from the sun.

... of light that we see in the night sky when a small chunk of interplanetary debris  burns up as it passes through our atmosphere.  If any part of a meteoroid survives the fall through the atmosphere and lands on  Earth, it is called a meteorite. ...
Lecture 2 - Origin of elements, classification
Lecture 2 - Origin of elements, classification

... Al2O3, TiO2, REE oxides), Fe and Ni metals – Further out, silicates form – Finally, ices (H2O, NH4, CH4, etc) form ...
Viking
Viking

... Asteroid: objects revolving around the sun that are too small and too numerous to be considered planets Asteroid belt: the region of the solar system between the orbits of Mars and Jupiter, where many asteroids are ...
Universal Gravitation
Universal Gravitation

... divided and cancelled out like terms we get… And this tells us the speed, vt, that we would need to travel in an orbit with radius, r, around an object with mass, mE. ...
Chapter 20 Questions
Chapter 20 Questions

... 11. What do we call the motion of a body as it orbits another body in space? 12. What do we call the time it takes for an object to revolve around the sun once? 13. What are the differences between prograde rotation and retrograde rotation? Which applies to the Earth? 14. Which planet is considered ...
reviewmtnoanswers1
reviewmtnoanswers1

... velocity is (change in position)/time elapsed acceleration is (change in velocity/time elapsed ...
The Solar System
The Solar System

... Nebular hypothesis – formation of solar system n  Recall the birth of stars! The sun is the nearest star to us. n  The process of formation of solar system in Nebular hypothesis ...
Life on Jovian Moons
Life on Jovian Moons

... bigger body (‘direct gravitational accumulation’) •  4 large moons, the ‘Galilean Moons’ ...
Study Guide Our Solar System Student Note: The upcoming test on
Study Guide Our Solar System Student Note: The upcoming test on

... and helium. The sun’s atmosphere includes the photosphere, the chromosphere and the corona. Each layer has unique properties. The photosphere is the inner layer which you see when you look at the sun. The chromosphere is the middle layer. The corona is the outer layer. The corona gradually thins int ...
vocabulary words to know
vocabulary words to know

... SQUEEZE YOUR ANSWERS into the little space given!! Staple your paper to the back of the study guide. 9. How did Galileo’s observations support the idea of a heliocentric system? 10. Why does Mercury have only a thin atmosphere? 11. How do astronomers explain that Venus rotates in the opposite direct ...
Investigation 3 for Dylan Nina and Shea
Investigation 3 for Dylan Nina and Shea

... • Thus, as planets get closer to the sun they change acceleration. • Uranus revolves every decade. • Every planet revolves counter clockwise. ...
Gravitation
Gravitation

... The NEW "r" that you see is simply a unit vector like I,j, & k-hat. A unit vector, remember, tells you the direction the force is going. In this case it means that it is between the two bodies is RADIAL in nature. The NEGATIVE SIGN is meant to denote that a force produces "bound" orbits. It is only ...
AP_Physics_C_-_Gravitation - St. Raymond High School for Boys
AP_Physics_C_-_Gravitation - St. Raymond High School for Boys

... The NEW "r" that you see is simply a unit vector like I,j, & k-hat. A unit vector, remember, tells you the direction the force is going. In this case it means that it is between the two bodies is RADIAL in nature. The NEGATIVE SIGN is meant to denote that a force produces "bound" orbits. It is only ...
Queen`s Observatory Multimedia Guide
Queen`s Observatory Multimedia Guide

... Queen’s Observatory Multimedia Guide (1) DVDs: ...
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... Now tell students that they will represent their group’s object by choosing appropriate items from different “planet stations.” One station has a variety of round objects – they can look for something to represent their planet’s size, on the same scale where a grape represents Earth. The second stat ...
Gravitation PPT
Gravitation PPT

... The NEW "r" that you see is simply a unit vector like I,j, & k-hat. A unit vector, remember, tells you the direction the force is going. In this case it means that it is between the two bodies is RADIAL in nature. The NEGATIVE SIGN is meant to denote that a force produces "bound" orbits. It is only ...
lagrange - The Institute of Mathematical Sciences
lagrange - The Institute of Mathematical Sciences

... ensured that their orbits were cleared of almost all other planetary material. The asteroid belt is thought to be planetary material which was not allowed to collapse into a “planet” because of the gravitational influence of the massive planet Jupiter. Earlier it was thought to be a planet broken up ...
What is a Planet
What is a Planet

... There are 3 Dwarf Planets in our Solar System; Pluto, Eris (found in the Kupier Belt) and a very large asteroid called Ceres. What is a Planet? – In 2006 the International Astronomical Union define a planet as an object that orbits the sun with sufficient mass and gravity. – Dwarf Planets orbit the ...
Comets…
Comets…

... •Stars – motion due to earth’s rotation. Position of stars do not change significantly over history, although astronomy can measure their motion ...
ppt
ppt

... indicates a fairly new surface No organic molecules have been detected on surface, but we don’t know about under the ice sheet Possibility of subsurface ocean due to heat from tidal heating of the planet caused by Jupiter ...
Atmosphere
Atmosphere

... are all found in the Kupier Belt) and a very large asteroid called Ceres. What is a Planet? – In 2006 the International Astronomical Union define a planet as an object that orbits the sun with sufficient mass and gravity to pull itself into sphere and clear its “neighborhood” of other objects. – Dwa ...
1_31_planetary calculator
1_31_planetary calculator

... The students will come forward with scales they want to use to make a model of the Solar System. Example of scales they might think of: • The earth is 5 cm diameter and everything is scaled accordingly. • The size of the Earth as unit to make a Solar System hands-on model. • The distance of the Eart ...
Section 1 Formation of the Solar System Chapter 27
Section 1 Formation of the Solar System Chapter 27

... rotation the spin of a body on its axis • Each complete rotation takes about one day. • The Earth rotates from west to east. At any given moment, the hemisphere of Earth that faces the sun experiences daylight. At the same time, the hemisphere of Earth that faces away from the sun experiences nightt ...
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Earth's rotation



Earth's rotation is the rotation of the planet Earth around its own axis. The Earth rotates from the west towards east. As viewed from North Star or polestar Polaris, the Earth turns counter-clockwise.The North Pole, also known as the Geographic North Pole or Terrestrial North Pole, is the point in the Northern Hemisphere where the Earth's axis of rotation meets its surface. This point is distinct from the Earth's North Magnetic Pole. The South Pole is the other point where the Earth's axis of rotation intersects its surface, in Antarctica.The Earth rotates once in about 24 hours with respect to the sun and once every 23 hours 56 minutes and 4 seconds with respect to the stars (see below). Earth's rotation is slowing slightly with time; thus, a day was shorter in the past. This is due to the tidal effects the Moon has on Earth's rotation. Atomic clocks show that a modern-day is longer by about 1.7 milliseconds than a century ago, slowly increasing the rate at which UTC is adjusted by leap seconds.
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