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Unit 1
Unit 1

... Formation of Planetary Nebula ...
Chapter 9 Lecture 1
Chapter 9 Lecture 1

... Meteorites from Moon and Mars • A few meteorites arrive from the Moon and Mars • Composition differs from the asteroid fragments. • A cheap (but slow) way to acquire moon rocks and Mars rocks. • One Mars meteorite generated a stir when scientists claimed evidence for microscopic life in it. ...
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... Although close observation and returned samples left no doubt that almost all of the Moon’s craters resulted from impacts, and the rest of the solar system had been heavily bombarded as well, no one had ever witnessed a significant impact. That changed when a comet, appropriately co-discovered by Ge ...
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... time to move away from the region in which they were formed (and no time for the star formation region to run out of gas!) ...
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36040345-1 - Space Medicine Association

... By definition we tend to think of life today in terms of biological forms already familiar to us on earth. We call this "terrestrial" life, classified according to location, geobiolagy ~ 7 ~ = the earth). And to designate life processes which occur in the cosmos outside the earth, we propose the sim ...
Sample Midterm - IUPUI Physics
Sample Midterm - IUPUI Physics

... 17. A particular star has a B-V value of 0.9 at a distance of 12 parsecs. If a similar star were to be found at a distance of 1200 parsecs and you ignore absorption of light be dust then what would the B-V value of that star be? a) 90 b) 9 * 10-3 c) 1188.9 d) 0.9 18. In the core of the sun when two ...
Phys 214. Planets and Life
Phys 214. Planets and Life

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Stellar Evolution after the Main Sequence
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... supernova is an exploding star that can become three times as bright as the sun. When a supernova occurs. All the dust particles, gas, and Dupree collect up. Creating a Nebula. These Nebulas can create many stars like our sun. Some stars can be brighter then others. This is an example of a Supernova ...
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No Slide Title

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The following voc. are listed in the order that we received them in
The following voc. are listed in the order that we received them in

... Earth is illuminated; occurs when the Moon, Earth and Sun form a 90° angle. First Quarter – The phase of the Moon in which only the right half of the Moon’s side that faces Earth is illuminated; occurs when the Moon, Earth and Sun form a 90° angle. Planet- a massive, usually spherical space object t ...
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... • How long will the sun last if the energy is produced by burning coal? C+O2→CO2 – Life time = m(E/m)/L – E/m=9MJ/kg – 1500 years ...
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... You may have noticed that the dates corresponding to each zodiacal constellation are not the same as the dates commonly quoted for “star signs”. In the next Activity, we will investigate why this is so. Another question may have occurred to you: when the Sun is “in” Aquarius, for example, Aquarius ...
A Binary Mass-Orbit Nomenclature for Planetary Bodies
A Binary Mass-Orbit Nomenclature for Planetary Bodies

... These general ideas have led to problems as astronomy progressed. The largest satellite of a giant planet can easily match for size the smallest independently orbiting planet in the system; in our own Solar System, Ganymede and Titan are both larger than Mercury, though in terms of mass the planet i ...
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Formation and evolution of the Solar System



The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.
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