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Asteroids Comets and Meteoriods 2015
Asteroids Comets and Meteoriods 2015

... comet It was discovered by Edmund Halley in 1682. Its orbital period is 76 years. The last appearance in 1986. (2062) ...
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... in six comets from the Oort cloud yielded a mean D/H ratio of (2.96 6 0.25) 3 1024. The D/H value in carbonaceous chondrites, (1.4 6 0.1) 3 1024, together with dynamical simulations, led to models in which asteroids were the main source of Earth’s water7, with #10 per cent being delivered by comets. ...
The Asteroid Belt - peterboroughastronomy.com
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... The first thing we should establish is the difference between an asteroid and a comet. In the very simplest terms an asteroid is a chunk of rock that orbits the Sun and is within our solar system. A comet is a giant dirty snowball that is pulled in from a very distant area called the Oort Cloud. Thi ...
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... What are Trojan Asteroids, and where are they located? (Where are the regular asteroids, for that matter?) What probes have visited Jupiter and when? Which comet crashed into Jupiter, and when? How far away from Jupiter are its four main moons? (use Jupiter’s diameter = 1) What is Jupiter’s mass com ...
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... farther out than the Kuiper belt. The Oort Cloud is a very sparse sphere of comets thought to encircle the solar system out to a distance of about 50,000 AU. Occasionally objects from the ...
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... A large body of small objects orbiting (the short period comets <200 years) the Sun in a radial zone extending outward from the orbit of Neptune (30 AU) to about 100 AU. Pluto maybe the biggest of the Kuiper Belt object. Oort Cloud Long Period Comets (period > 200 years) seems to come mostly from a ...
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... How many asteroids are there? 26 very large asteroids have been discovered, which is probably most of the big ones; but, there are still millions of smaller ones that we have yet to see because they are too tiny, only a mile or so across. If we stuck all the asteroids together, how big would the new ...
Problem Set 3 Solutions Problem 1: D
Problem Set 3 Solutions Problem 1: D

... where Ri is the initial mass of the cloud, Rf is the radius of the Sun, and Ri  Rf . About half this energy is radiated away and contributes to the luminosity, but let’s not worry about factors of order unity since we’re already making lots of approximations. The luminosity is then ...
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Oort cloud



The Oort cloud (/ˈɔrt/ or /ˈʊərt/) or Öpik–Oort cloud, named after Dutch astronomer Jan Oort and Estonian astronomer Ernst Öpik, is a theoretical spherical cloud of predominantly icy planetesimals believed to surround the Sun at a distance of up to around 100,000 AU (2 ly). This places it at almost half of the distance to Proxima Centauri, the nearest star to the Sun, and in interstellar space. The Kuiper belt and the scattered disc, the other two reservoirs of trans-Neptunian objects, are less than one thousandth as far from the Sun as the Oort cloud. The outer limit of the Oort cloud defines the cosmographical boundary of the Solar System and the region of the Sun's gravitational dominance.The Oort cloud is thought to comprise two regions: a spherical outer Oort cloud and a disc-shaped inner Oort cloud, or Hills cloud. Objects in the Oort cloud are largely composed of ices, such as water, ammonia, and methane.Astronomers conjecture that the matter composing the Oort cloud formed closer to the Sun and was scattered far into space by the gravitational effects of the giant planets early in the Solar System's evolution. Although no confirmed direct observations of the Oort cloud have been made, it may be the source of all long-period and Halley-type comets entering the inner Solar System, and many of the centaurs and Jupiter-family comets as well. The outer Oort cloud is only loosely bound to the Solar System, and thus is easily affected by the gravitational pull both of passing stars and of the Milky Way itself. These forces occasionally dislodge comets from their orbits within the cloud and send them towards the inner Solar System. Based on their orbits, most of the short-period comets may come from the scattered disc, but some may still have originated from the Oort cloud.
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