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Slide 1 - NMSU Astronomy
Slide 1 - NMSU Astronomy

... we left the Sun! • Earth is the only planet in the Solar System to have liquid on its surface. It is also the largest rocky planet. ...
Gravitation
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... is so far from the sun that it does not reflect much sunlight. You cannot see it from Earth without using a telescope. Uranus is different from the other planets because it is “tipped” on its side. As shown in the figure below, the north and south poles of Uranus point almost directly at the sun. Th ...
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... orbiting (M), but not on the object’s mass (m). ...
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... Sun. What do you notice about the sizes of the orbits? Compare the orbits near the Sun with those farther away from the Sun. If you were the commander of a spacebus that traveled among the planets, would you rather travel between the Inner Planets (Mercury, Venus, Earth, Mars) or the Outer Planets ( ...
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... Inner planets have metallic cores and rocky surfaces like mountains, canyons, and craters. ...
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... really does not have a surface (you would sink into the liquid icy center) • Atmospheric features: Contains mostly ...
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Program List 2016-17 - Northern Stars Planetarium

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... Helium is the second most abundant element at 7.8% in terms of number of atoms and 25% in terms of mass. The sun is 0.1% other elements. The sun makes up 99.9% of the mass of our solar system. The sun is not a liquid or a solid. It is a plasma - a mixture of atomic nuclei and free electrons. ...
UNIT C - apel slice
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... plants and animals die, they decay, or rot. Some that died long ago became fossil fuels, such as oil, that people use today. Have you ever noticed that the sun seems to move across the sky? The sun is actually stationary, while the Earth revolves around A There are many ways to classify stars. A sta ...
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... crossing of the meridian by evenly spaced “clock stars” ...
Planets: a brief tour
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Scaling the Solar System
Scaling the Solar System

... 2. Cut the Remaining Part into 10 Equal Parts  Take 5 parts and combine them with the ball in the Saturn box.  Combine 2 parts to put into the Neptune box.  Put 2 parts into the Uranus box. 3. Cut the Remaining Part into 4 Equal Parts  Take 3 parts and combine them with the ball in the Saturn bo ...
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... 1. Annual changes are the result of Earth’s orbital motion around the Sun. 2. The plane in which earth orbits about the sun is called the ecliptic. 3. At one point the earth’s axis is tilted toward the sun while the other is tipped away42 from the sun. ...
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... between the Earth and the Moon is stronger than the force between the Earth and the Sun. Even though the Sun has such a great mass, the shorter distance between the Earth and the Moon makes the force between the Earth and the Moon much stronger than the force between the Earth and the Sun. Gravity & ...
Chapter 19
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... Kepler’s first discovery, or first law of motion, came from his careful study of the movement of the planet Mars. He discovered that the planet did not move in a circle around the sun, but in an elongated circle called an ellipse. An ellipse is a closed curve in which the sum of the distance from th ...
Chapter 19
Chapter 19

... Kepler’s first discovery, or first law of motion, came from his careful study of the movement of the planet Mars. He discovered that the planet did not move in a circle around the sun, but in an elongated circle called an ellipse. An ellipse is a closed curve in which the sum of the distance from th ...
27.1 Review - geraldinescience
27.1 Review - geraldinescience

... May 14­11:07 AM ...
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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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