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Astronomy 1 Study Guide Key 16
Astronomy 1 Study Guide Key 16

... Moon – planet – main sequence star – red giant – supergiant – solar system – galaxy – universe 2. How do we measure distance in space? light year, parsec, or astronomical units 3. If a supernova is 400 light years away, it would take 400 years for us to see it. 4. If a distance is not as large as a ...
notes_chapter1 - Auburn University
notes_chapter1 - Auburn University

... Condensed nebulae formed flattened accretion discs Heat and mass from collapse ignited nuclear fusion and heavy elements were produced Stellar Wind = stream of atoms emitted by a star during its lifetime (solar wind) ...
Unit E - Topic 1.0 Notes
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... Gurson to measure the angle between the Moon and any given star • Early Telescope (late 16th century): invented in the late 16th century and it allowed astronomers such as Galileo to discover details about Earth's closet planetary neighbors and the relative size and distance of what laid beyond Eart ...
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... 15. What are the sources of energy which keep the center of Earth warm? 16. Describe the structure of the core and mantle of Earth. 17. How is crust created and destroyed on Earth? 18. What are the two different (although related) processes that create mountains on Earth? 19. What are the primary ch ...
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... a. Gravitational energy from the Sun must be greater than the kinetic energy of the planets b. Kinetic energy of the planets must be greater than the gravitational energy of the Sun c. The kinetic (orbital) and gravitational energies of the Sun and the planets must ...
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... The universe is estimated to be over 10 billion years old. The universe is composed of galaxies, stars, planets, asteroids, comets, and meteors, each having different properties. Our solar system exists within the Milky Way galaxy. The known components of our solar system are the Sun, four terrestri ...
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Key 3 - UNLV Physics

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chapter4 - Empyrean Quest Publishers

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... – relative size of earth and moon from lunar eclipse – relative size of moon and sun from solar eclipse • knew sun was much bigger than earth • presumably this led him to heliocentric model ...
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... Star: An object so massive that nuclear fusion is triggered in its interior, and thus it shines. Planet: Too small trigger nuclear fusion, these relatively large objects orbit a star. Moon: Solid objects that orbit planets. Asteroid: Small bodies of rock and/or metal that have their own orbit around ...
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... Earth in meteorites. • Organic material is carbon based compounds and is part of all life as we know it. • It may have been lightning that made these compounds become “alive”. • Water was necessary for life to evolve and this may have come from comets • Oxygen in the atmosphere was given off by earl ...
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... and Sun which banished two thousand year old beliefs. His discoveries of moons orbiting the planet Jupiter, and of the phases of Venus provided evidence for the sun-centered model. He also found that there were far more stars than was previously believed. Copernicus’ model gained acceptance, and wit ...
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... The word retrograde applies to the apparent backward motion of a planet. An old encyclopedia of astrology describes this retrograde motion as "…the effect of a slow-moving train as viewed from another train traveling parallel to it but at a more rapid rate, wherein the slower train appears to be mov ...
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... --Earth is the third planet orbiting the sun. --The moon orbits the Earth. I can describe why planet Earth is so unique and special. -Earth is the perfect distance from the sun to sustain life. -It has oxygen. -It has water in liquid form. I can explain why life on Earth is dependent on the Sun. -Th ...
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... object is less than that? • It can still coalesce under forces of selfgravity, magnetic fields, etc. ...
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... Planets are plentiful The first planet orbiting another Sun-like star was discovered in 1995. We now know of 209 (Feb 07). Including several stars with more than one planet - true planetary systems ...
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Acquaintance with solar system. By Edgaras Montvila 6D

... Uranus is named after the ancient Greek deity of the sky Uranus, the father of Cronus (Saturn ) and grandfather of Zeus( Jupiter). Surface temperature varies from –197.2 °C to ? °C. Uranus has a ring system. The planet system has a unique configuration among those of the planets because its axis of ...
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Planetary habitability



Planetary habitability is the measure of a planet's or a natural satellite's potential to develop and sustain life. Life may develop directly on a planet or satellite or be transferred to it from another body, a theoretical process known as panspermia. As the existence of life beyond Earth is unknown, planetary habitability is largely an extrapolation of conditions on Earth and the characteristics of the Sun and Solar System which appear favourable to life's flourishing—in particular those factors that have sustained complex, multicellular organisms and not just simpler, unicellular creatures. Research and theory in this regard is a component of planetary science and the emerging discipline of astrobiology.An absolute requirement for life is an energy source, and the notion of planetary habitability implies that many other geophysical, geochemical, and astrophysical criteria must be met before an astronomical body can support life. In its astrobiology roadmap, NASA has defined the principal habitability criteria as ""extended regions of liquid water, conditions favourable for the assembly of complex organic molecules, and energy sources to sustain metabolism.""In determining the habitability potential of a body, studies focus on its bulk composition, orbital properties, atmosphere, and potential chemical interactions. Stellar characteristics of importance include mass and luminosity, stable variability, and high metallicity. Rocky, terrestrial-type planets and moons with the potential for Earth-like chemistry are a primary focus of astrobiological research, although more speculative habitability theories occasionally examine alternative biochemistries and other types of astronomical bodies.The idea that planets beyond Earth might host life is an ancient one, though historically it was framed by philosophy as much as physical science. The late 20th century saw two breakthroughs in the field. The observation and robotic spacecraft exploration of other planets and moons within the Solar System has provided critical information on defining habitability criteria and allowed for substantial geophysical comparisons between the Earth and other bodies. The discovery of extrasolar planets, beginning in the early 1990s and accelerating thereafter, has provided further information for the study of possible extraterrestrial life. These findings confirm that the Sun is not unique among stars in hosting planets and expands the habitability research horizon beyond the Solar System.The chemistry of life may have begun shortly after the Big Bang, 13.8 billion years ago, during a habitable epoch when the Universe was only 10–17 million years old. According to the panspermia hypothesis, microscopic life—distributed by meteoroids, asteroids and other small Solar System bodies—may exist throughout the universe. Nonetheless, Earth is the only place in the universe known to harbor life. Estimates of habitable zones around other stars, along with the discovery of hundreds of extrasolar planets and new insights into the extreme habitats here on Earth, suggest that there may be many more habitable places in the universe than considered possible until very recently. On 4 November 2013, astronomers reported, based on Kepler space mission data, that there could be as many as 40 billion Earth-sized planets orbiting in the habitable zones of Sun-like stars and red dwarfs within the Milky Way. 11 billion of these estimated planets may be orbiting Sun-like stars. The nearest such planet may be 12 light-years away, according to the scientists.
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