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Constellations and Distances to Stars
Constellations and Distances to Stars

... • Stars within the same constellation are not necessarily close. They could appear to be almost touching and actually be one trillion kilometers apart. Very few stars are gravitationally bound to one another. • One way to know when a star is close to our solar system is to measure parallax. • Parall ...
Unit Lesson Plan – Atomic Structure
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... 24. 6.49 In recent years, scientists have discovered hundreds of planets orbiting other stars. Some of these planets are in orbits that are similar to that of earth, which orbits the sun(Msun = 1.99 × 1030 kg) at a distance of1.50 × 1011 m, called 1 astronomical unit (1 au).Others have extreme orbi ...
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... Precession of the Northern Pole Star The star Polaris, which is currently close to the North Celestial Pole, appears to be stationary while other stars appear to rotate around it as the Earth turns daily on its axis [see Star Trail photograph.] However, the specific star that is the North Star varie ...
Piscataway High School - Piscataway Township Schools
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Astronomy - Dalriada at dalriada.org.uk
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... word for wanderer because they seem to wander among the stars. They are very difficult to explain on a geocentric basis, although Ptolemy tried hard in the 2nd century A.D. His Ptolemaic system was finally blown away by Copernicus (1473-1543) who developed a comprehensive heliocentric model, and all ...
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... In 1995 GPS (Global Positioning System) was the first system of geolocation by satellite to become operational. Developed by the Americans during the Cold War it was originally a military invention but it has since revolutionised civilian life too. Its applications are numerous and varied: maritime ...
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... Read Section 16-1 on pages 344-348 of SP to help you answer the following questions: 22. The life cycle of stars are generally measured in ________________ of years. 23. What is meant by a nebula? Particles in a nebula join together and form clumps. These clumps attract each other with the force of ...
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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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