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Chapter 4 The Solar System
Chapter 4 The Solar System

... Others are discovered through the periodic dimming of the parent star’s luminosity. ...
Homework 4 1 Chapter 3 October 4, 2011
Homework 4 1 Chapter 3 October 4, 2011

... warmer only the rock and metal could condense and eventually form planets made of those materials. But, farther away the hydrogen and helium condensed as well, so planets in that region are composed of these elements as well (in fact their composition is dominated by these elements since they were m ...
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... extending to about 50,000 AU Kuiper belt: On orderly orbits from 30-100 AU in disk of solar system ...
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... a. about a hundred million years b. 5 billion years c. 5000 years d. 500,000 years e. greater than 10 billion years 3. Most of the extrasolar planets that have been discovered orbiting stars besides the sun are a. on nearly circular orbits, not what was expected. b. large jovian-like planets with di ...
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... Formation of Solar System • Solar Nebula Theory (18th century) – Solar System originated from a rotating, disk-shaped cloud of gas and dust • Modern theory is that the Solar System was born from an interstellar cloud (an enormous rotating cloud of gas and dust) ...
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... so the even lower semi-major axis of 2012 VP113 makes tides extremely unlikely. If the inner Oort cloud objects were created from the gravitational tide within our Sun’s birth cluster, the low semi-major axis of 2012 VP113 constrains the birth cluster to have been a moderate 10,000 solar masses per ...
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Homework #9 - Solutions - Department of Physics and Astronomy

... in intergalactic space (beyond the halo) We would expect to see only old extreme population II stars (and possibly population III stars which are predicted to exist but have not been conclusively observed). e) in the galactic bulge Population II since there is little gas and dust for new star format ...
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... that the bright band on the night sky known as the Milky Way might consist of distant stars. Aristotle (384–322 BC), however, believed the Milky Way to be caused by "the ignition of the fiery exhalation of some stars which were large, numerous and close together" and that the "ignition takes place i ...
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... Pluto (high inclination of orbit). Proof of period of high collision evident on moon ...
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... The Formation of the Solar System  There are nine outstanding properties of our solar system that any formation theory must be able to explain. In your table groups, see how many you can come up with. ...
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... mi) is a unit of length which is well known in the United States. It is also known as a statute mile, and is equivalent to 5280 feet or 1760 yards. The kilometer is not as well understood. Those currently studying the metric system in school or having recently completed their schooling, can probably ...
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... planet that was destroyed in a massive collision long ago. The second theory is that asteroids are material that never formed a planet. In fact, if the estimated total mass of all asteroids was gathered into a single object, the object would be less than 932 miles across -- less than half the diamet ...
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... point A sweeps over a certain area as the planet moves to point B in a given time interval. A line from the Sun to a planet at point C will sweep over the same area as the planet moves to point D during the same time interval. The time required to move from point A to point B is the same as the time ...
Monday, October 19 - Otterbein University
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... directions of revolution of planets about Sun is the same, and is the same as the direction of the Sun's rotation directions of rotation of planets about their axes is also mostly in the same direction as the Sun's (exceptions: Venus, Uranus, Pluto) most moons revolve around their planets in the sam ...
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... Origin and Evolution of Comets Comets originate from very great distances The aphelia of new comets are typically ~50,000 AU This clustering of aphelia was first noted by Dutch astronomer Jan Oort in 1950 He then proposed an idea for the origin of those comets, which is still accepted by most astro ...
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... Part of Kuiper Belt and influences other orbits Show gif: http://www.universetoday.com/wpcontent/uploads/2016/03/Planet_Nine_animation.gif Video here with more info if interested: • http://www.universetoday.com/133555/planet-9-cantrun-forever-two-asteroids-give-clues/ ...
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... Unlike the other small bodies in the solar system, comets have been known since antiquity. There are Chinese records of Comet Halley going back to at least 240 BC. The famous Bayeux Tapestry, which commemorates the Norman Conquest of England in 1066, depicts an apparition of Comet Halley. As of 1995 ...
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... belt lies in the plane of the ecliptic at distances between 30 and 500 AU from the Sun • It is thought to contain many tens of thousands of comet nuclei ...
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... From dust grains to planets Our protoplanetary disk probably lasted “only” a few million years before being absorbed or blown away by the Sun, but most of the planet formation could be completed during that time. Our parent cloud was mostly made of gaseous hydrogen and helium, which are the main con ...
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The NEW Solar System

... years that was centered around the planet Jupiter rather than the Sun. However, the Sun’s gravitational influences caused enough wobble in the comet’s orbit that astronomers were able to predict, observe and analyze a collision between a comet and a planet for the first time in modern history. With ...
A Brief History of Planetary Science
A Brief History of Planetary Science

... Pluto and Charon are in a close, tidally locked orbit ...
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here

... of glowing diffuse gas, which may be 100,000 km across.  A dust tail, blown off by the radiation from the ...
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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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