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Planetary Taxonomy
Planetary Taxonomy

... The IAU definition of planet can be solidified in three ways: 1) Replace “orbits the Sun” with “orbits a star” to make the definition applicable to exoplanets. exoplanets 2) Make the definition more rigorous by adopting an explicit criterion for dynamical dominance (such as a threshold on the direct ...
Desert Skies - Tucson Amateur Astronomy Association
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... retrograde motions of naked eye planets. We also had a presentation on carbon stars and double stars from JD Metzger and an observing list for September presented by Mary Turner. The efforts of those who stepped up to help us last month are greatly appreciated. We still have space in the October mee ...
The Geographic Position of a Celestial Body
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... slowly (tidal friction) and, moreover, fluctuates in an unpredictable manner due to random movements of matter within the earth's body (magma) and on the surface (water, air). Therefore, neither of both time scales is strictly uniform. Many astronomical applications, however, require a linear time s ...
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proposed path of the missing planet

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Celebrating the centennial of a celestial yardstick
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... had abundant volcanic activity (and may have some ongoing activity today), which is involved in concentrating such elements. Yet the amounts of these elements, their distribution, and many other factors are completely unknown. The MESSENGER spacecraft is studying Mercury’s composition from orbit, bu ...
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Astronomy Essay Questions

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... This book containing information about 2800 stars and 88 constellations is the result of an enormous work, begun by Prof. Helmut Werner shortly after the Second World War. This project of H. Werner, who was astronomer and member of the staff of the Carl Zeiss firm was continued after his death in 19 ...
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... Brahe and Kepler. But in their own time, these ideas were mere speculations that were overshadowed by Plato’s insistence upon a stationary earth and circular motion of stars and planets. Some of the important early astronomical speculations include the following: “Central fire” or “the hearth of Zeu ...
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... has evolved into a giant. If the star equals one solar mass, then it becomes a red giant. If the star equals 100 solar masses, then it will become a supergiant. In about 5 billion years, our sun will become a giant. Once the red giant’s core uses its supply of helium, it contracts even more. As the ...
How the Earth Moves Transcript
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... flourish in the Arabic world and in Asia, improving the instruments and equipment used to measure the position of cosmic bodies. The more precise measurements led to better compilations and catalogues of the night sky. A radical overhaul of our understanding of the relative position of cosmic bodies ...
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Astronomy Timeline
Astronomy Timeline

... 130 B.C. - Greek astronomer Hipparchus develops the first accurate star map and star catalogue, and a reliable method to predict solar eclipses 46 B.C. - Julius Caesar, after consulting the astronomer Sosigenes of Alexandria, introduces the Julian Calendar, a regular year of 365 days divided into 12 ...
low-res - Communicating Astronomy with the Public Journal
low-res - Communicating Astronomy with the Public Journal

... and hold together. If it weren’t for dark matter, our Galaxy would not exist as we know it, and human life would not have developed. Dark matter is more than five times as abundant as all the matter we have detected so far. As cosmologist Sean Carroll says, “Most of the ...
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Theoretical astronomy

Theoretical astronomy is the use of the analytical models of physics and chemistry to describe astronomical objects and astronomical phenomena.Ptolemy's Almagest, although a brilliant treatise on theoretical astronomy combined with a practical handbook for computation, nevertheless includes many compromises to reconcile discordant observations. Theoretical astronomy is usually assumed to have begun with Johannes Kepler (1571–1630), and Kepler's laws. It is co-equal with observation. The general history of astronomy deals with the history of the descriptive and theoretical astronomy of the Solar System, from the late sixteenth century to the end of the nineteenth century. The major categories of works on the history of modern astronomy include general histories, national and institutional histories, instrumentation, descriptive astronomy, theoretical astronomy, positional astronomy, and astrophysics. Astronomy was early to adopt computational techniques to model stellar and galactic formation and celestial mechanics. From the point of view of theoretical astronomy, not only must the mathematical expression be reasonably accurate but it should preferably exist in a form which is amenable to further mathematical analysis when used in specific problems. Most of theoretical astronomy uses Newtonian theory of gravitation, considering that the effects of general relativity are weak for most celestial objects. The obvious fact is that theoretical astronomy cannot (and does not try) to predict the position, size and temperature of every star in the heavens. Theoretical astronomy by and large has concentrated upon analyzing the apparently complex but periodic motions of celestial objects.
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