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... Explaining the Characteristics of the Solar System 1. The orbits of the planets lie in the same plane because the rotating solar nebula collapsed into a disk, and the planets formed in that disk. Objects are co-eval (4.) 2. The division into small inner and giant outer planets rests upon the amoun ...
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... it has a thick atmosphere that consists of mostly the carbon dioxide (96%), a known greenhouse gas. On Venus the carbon dioxide gas lets in the visible light from the Sun. This visible light hits the surface which gets heated up and produces infrared light. The infrared light cannot pass through the ...
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... axis as it is moving along its orbit. In doing so, it varies the alignment with the Sun and this entails an additional time to reach the same Earth-Sun orientation once again; this does not occur for the other stars that are so distant that they can be considered fixed. When measuring a year, things ...
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... 8. Over the course of one year, the speed of the orbit of Earth around the Sun... (A) Does not change at all (B) Changes by a small amount (less than ten percent) (C) Changes by a large amount (greater than ten percent) ...
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... 1632: "Dialogo Dei Massimi Sistemi" (In Italian! Not Latin! For the common people!) He published his masterpiece, Dialogue on the Two Chief World Systems, in which he had two people, one representing the view of Ptolemy and other the view of Copernicus, present their arguments before an intelligent ...
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... changes in the orbit of Uranus led Alexis Bouvard to deduce that its orbit was subject to gravitational perturbation by an unknown planet. Neptune was subsequently observed by Johann Galle within a degree of the position predicted by Urbain Le Verrier, and its largest moon, Triton, was discovered sh ...
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... Saturn is similar to Jupiter in some ways. While its mass is lower (95 Earth masses), it is still able to sustain severe amounts of hydrogen and helium. The surface temperature (134 K at 1 bar level) is lower than Jupiter’s, so more helium was able to condensate; thus leading to a slightly lower hel ...
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... point to the end of the zeros. For 2.99 800 000, there are eight places. This means the power of base 10 has an exponent of 8, written as 108. Step 3: Delete the zeroes. The number written in scientific notation is 2.998 × 108 m/s. Write the following numbers in scientific notation: 1. the distance ...
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... Here G is Newton’s gravitational constant, P is the orbital period and a is the distance between the two objects. If you use G = 6.67x10-11 m3/(kg x s2), then you want P in units of seconds and a in units of meters. If M2 is MUCH SMALLER than M1, this formula gives you a way to measure M1 (you just ...
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The red planet is called Mars The sun is our closest star. Laika was

... In 1590 the first star was discovered. Scientists do not count Pluto as a planet. Saturn is also known as the ringed planet. Venus is the hottest planet in the solar system. Uranus is four times the size of Earth. Mercury is the closest planet to the sun. All life on Earth depends on the sun. By Cha ...
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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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