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Tidal Evolution of Close-In Extra-Solar Planets
Tidal Evolution of Close-In Extra-Solar Planets

October 2014 - Newbury Astronomical Society
October 2014 - Newbury Astronomical Society

... A star like our Sun will spend a few million years in its very active pre-main sequence phase then settle into its normal life. The luminosity of the star is compared with our Sun on the vertical scale on the left (therefore our Sun is classified as 1). The absolute magnitude is shown on the vertica ...
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... As many as seven eclipses may occur during a calendar year. Four may be lunar, and three may be solar or vice versa. However, total eclipses of the sun and the moon occur infrequently. Solar and lunar eclipses do not occur during every lunar orbit. This is because the orbit of the moon is not in the ...
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... We predict how a remote observer would see the brightness variations of giant planets similar to those in our Solar System as they orbit their central stars. We model the geometry of Jupiter, Saturn and Saturn’s rings for varying orbital and viewing parameters. Broadband scattering properties for th ...
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... written down without *any* context whatsoever (e.g., for 1a, writing “164.85 years”, and nothing else), take off 1/3 of the points. One point off per question for inappropriately high precision (which usually means more than 2 significant figures in this homework). However, no points off for calcula ...
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... with water. Capricornus lies furthest west and is therefore the first of the four to rise in the evening, there is just one Messier object in Capricornus the globular cluster M30. The cluster is visible in binoculars and small telescopes. M30 lies a little over 3 degrees east of zeta (ζ) Capricorni. ...
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... b. Compare the similarities and differences of planets to the stars in appearance, position, and number in the night sky. c. Explain why the pattern of stars in a constellation stays the same, but a planet can be seen in different locations at different times. d. Identify how technology is used to o ...
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... the solar system after their first pass through the planetary region, mainly as a result of Jovian perturbations. Hence, by significantly reducing the population of returning objects, Jupiter lowers the chance of one of these cosmic bullets striking the Earth. However, in recent years, it has become ...
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slides - Relativity Group

... Origin of the Asteroids • From their composition, size, and location, asteroids support the solar nebula hypothesis and are thought to be fragments of planetesimals • For this connection to be established, differentiation needed to occur in large asteroids • Fragmentation of these early large astero ...
Astronomy - Bemidji State University
Astronomy - Bemidji State University

... arrangement of glass lenses to magnify objects. This arrangement provided limited magnification--up to 30 times for Galileo--and a narrow field of view; Galileo could see no more than a quarter of the moon's face without repositioning his telescope. In 1704, Sir Isaac I\lewton announced a new concep ...
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Definition of planet



The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies. Greek astronomers employed the term asteres planetai (ἀστέρες πλανῆται), ""wandering stars"", for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different objects, from the Sun and the Moon to satellites and asteroids.By the end of the 19th century the word planet, though it had yet to be defined, had become a working term applied only to a small set of objects in the Solar System. After 1992, however, astronomers began to discover many additional objects beyond the orbit of Neptune, as well as hundreds of objects orbiting other stars. These discoveries not only increased the number of potential planets, but also expanded their variety and peculiarity. Some were nearly large enough to be stars, while others were smaller than Earth's moon. These discoveries challenged long-perceived notions of what a planet could be.The issue of a clear definition for planet came to a head in 2005 with the discovery of the trans-Neptunian object Eris, a body more massive than the smallest then-accepted planet, Pluto. In its 2006 response, the International Astronomical Union (IAU), recognised by astronomers as the world body responsible for resolving issues of nomenclature, released its decision on the matter. This definition, which applies only to the Solar System, states that a planet is a body that orbits the Sun, is massive enough for its own gravity to make it round, and has ""cleared its neighbourhood"" of smaller objects around its orbit. Under this new definition, Pluto and the other trans-Neptunian objects do not qualify as planets. The IAU's decision has not resolved all controversies, and while many scientists have accepted the definition, some in the astronomical community have rejected it outright.
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