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GAIA A Stereoscopic Census of our Galaxy
GAIA A Stereoscopic Census of our Galaxy

Ancient Egyptian Astronomy
Ancient Egyptian Astronomy

... Aryabhatta - was born in 476 A.D., and is widely recognized as the father of Indian astronomy. When he was about 25 years old, he presented astronomical and mathematical theories in which the Earth was taken to be spinning on its axis and the periods of the planets were given with respect to the Sun ...
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... is a star that can only be seen in the daytime, but the moon can be seen sometimes at night and sometimes during the day. Students know there are more stars in the sky than anyone can count, but they are not scattered evenly, and they are not all the same in brightness or color. Students know the su ...
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... – More than half of the stars in the sky are either binary stars or members of multiple-star systems. – Astronomers are able to identify binary stars through several methods. • Accurate measurements can show that its position shifts back and forth as it orbits the center of mass. • In an eclipsing b ...
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Orbital Motion and Energy 28. What is the gravitational field strength

... 3. On Earth, the maximum speed without skidding for a car on a level circular curved track of radius 40 m is 15 m/s. This car and track are then transported to another planet for the Indy Galactic 500. The maximum speed without skidding is now 8.4 m/s. What is the value of the acceleration due to gr ...
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How does gravity work? - Plus Maths

... compared to that experienced by the much less massive Earth. That's why the Sun remains more or less stationary, while the Earth is forced on an orbit around it. Newton's theory of gravity, published in 1687, is remarkably accurate when it comes to most practical purposes, and went unchallenged for ...
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... We still have to answer the question of Pluto’s status. Is Pluto a planet or not? In the early 2000s Caltech’s Mike Brown discovered small objects in the outer reaches of the Solar System, well beyond Neptune’s orbit. One of these objects turned out to be about the size of Pluto. The new object was ...
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53.3 A New View of Gravity • What is gravity?

... (with circumferences increasingly less than 21fr) near the bottom of the bowl, showing that gravity becomes stronger and 1'+te curvature of spacetime becomes greater as we ap­ proach the Sun's surface. (Notice that the curvature does not continue to increase with depth inside the Sun, because the st ...
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Predicting Sky Dome Appearance on Earth

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Chapter 2: Discovering the Universe for Yourself

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Discovery of a candidate inner Oort cloud planetoid

... From a four month baseline the orbital elements are still uncertain, but positions for the 2002 season can be predicted with reasonable accuracy. A search of the Skymorph database of NEAT observations shows that high-quality images were obtained surrounding the predicted location of our object from ...
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... Earth. Such synchronous rotation is common among ...
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... • or the stars are not uniformly distributed • or it is not static (or two or all of these might be true). Today, it is generally accepted that the universe is not infinite, and that it is expanding rather than static. The Cosmological Principle states that the universe has a generally uniform app ...
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... 2. A chest is 2.5 cubits in length and 1.5 cubits in width and height. Given that a cubit is equivalent to 17.7 in., find the volume of the chest. 3. What is the speed in miles per hour of a beam of light traveling at 3.00 x 108 m/s? 4. Many highways have a speed limit of 55 mi/h. Is this speed grea ...
Astronomy 730 / Galaxies
Astronomy 730 / Galaxies

... zb. At t = t0 the boundary conditions are that σz(R, t0) = σz(0, t0) exp(−R/2hR) and hz(R, t0) = constant. If we take σz(R0,t0) = 20 km/s, we know that hz(R, t0) = 350 pc, again based on the old stars in the thin disk in the solar neighborhood. (c) Equate σz(R, t0) = σz(0, t0) exp(-R/2hR) with σz(R, ...
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... A) It contains between 100 billion and 1 trillion stars. B) Our solar system is located very close to the center of the Milky Way Galaxy. C) The galaxy is about 100,000 light-years in diameter. D) One rotation of the galaxy takes about 200 million years. Answer: B 25) Which of the following correctl ...
Dr Conor Nixon Fall 2006
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... per second to energy, the 4x1026 watts needed to power the Sun is released. This is miniscule compared to the mass of the Sun! • Working out the details took several more decades of work… • The Sun is 99% composed of hydrogen and helium, so the source was probably in those materials. • The crucial o ...
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The Milky Way Galaxy

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Scale the Universe - Crystal Ball Science
Scale the Universe - Crystal Ball Science

Mathematics in Art and Architecture GEM1518K
Mathematics in Art and Architecture GEM1518K

... Even though it is now known that this ancient model of a stationary Earth is incorrect, you can still use this model because it is a convenient way to predict the motions of the stars and planets relative to a location on the Earth. A star's apparent brightness is actually determined by its distance ...
Solar System Formation
Solar System Formation

... on geologic maps to show different types or ages of rocks. The geologic events in an area and the weathering and erosion that has taken place will determine what types and ages of rock are present. Geologic maps can be very specific, showing many types of rocks and using shorter age distinctions, or ...
10 New Constellations
10 New Constellations

< 1 ... 50 51 52 53 54 55 56 57 58 ... 369 >

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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