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Astronomy Final Study Guide – Name: **This will be the biggest test
Astronomy Final Study Guide – Name: **This will be the biggest test

... 24. How are apparent and absolute brightness different? ...
Earth Science 24.3 The Sun
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... Orbit is a regular, repeating path that one object in space takes as it revolves around another one. All orbits are elliptical, which means they are an ellipse, similar to an oval. These orbits result from gravitational forces ...
Grand Tour Worksheet - School District of La Crosse
Grand Tour Worksheet - School District of La Crosse

... 1. WHEN WAS THE LAST VISIT FOR HALLEY’S COMET? 2. Comets mat very well be what? 3. Are new comets predictable? 4. How often does Halley’s Comet return? 5. Where does Halley’s spend most of its time? 6. How long has Halley’s been observed? ...
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A Tour of our Solar System
A Tour of our Solar System

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Lecture 2 - The University Centre in Svalbard
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Geography 06b
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... curved path, which is not uniformly curved. If the earth moves such a high constant speed on a non-uniformly curved path, then the earth will go outside of the elliptical path, because a body can move with a constant speed on a uniformly curved path. According to the curve, speed is adjusted to move ...
Dec 2017 - What`s Out Tonight?
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AP Physics Multiple Choice Practice – Gravitation 1. Each of five

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... on the Earth that came from Mars. One fell in Nakhla, Egypt, in 1911. It weighed 10 kg. The most famous one (ALH84001) was discovered in the Allan Hills of Antarctica. It is dated to be 4.5 billion years old. In a remarkable paper published in 1996, geologists claimed that this meteorite had evidenc ...
Jan 2011 Regents
Jan 2011 Regents

... **W and Y are high tides because it is the moon’s gravitational pull that causes tidal changes. X and Y will experience low tides until those locations rotate into the appropriate positions.(approx 6 hours later)** ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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