Planet Distance from sun (in km) Distance in scientific notation Mercury 57‚909‚000 5.7909*10^7 Venus 108‚200‚000 1.082*10^8 Earth 149‚600‚000 1.496*10^8 Mars 227‚940‚000 2.2794*10^8 Jupiter 778‚400‚000 7.784*10^8 Saturn 1‚423‚600‚000 1.4236*10^9 Uranus 2‚867‚000‚000 2.867*10^9 Neptune 4‚488‚400‚000 4.4884*10^9 (dont
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of the retinue of objects that orbit the Sun‚ most of the mass is contained within eight (8) relatively solitary planets whose orbits are almost circular and contained within a nearly-flat disc called the ecliptic plane. The four smaller inner planets; Mercury‚ Venus‚ Earth and Mars‚ also called the terrestrial planets‚ are primarily composed of rock and metal. The four outer planets‚ Jupiter‚ Saturn‚ Uranus and Neptune‚ also called the gas giants‚ are composed largely of hydrogen and helium and
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was discovered in September 1845. It was discovered by means of mathematics before being seen through a telescope. It began in 1843 when John Adams‚ a young English astronomer and mathematician‚ began working to find thew location of the unknown planet. Adams predicted the planned would be about 1.6 billion kilometres farther from the sun then Uranus. That’s when he completed his work in September 1845. Also Urbain Leverriar‚ unknown to Adams‚ began working on the same project. By mid-1846‚ Leverriar
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understand the planet and atmosphere of Earth’s neighbor. Yet‚ Pioneer 10 had three primary goals: make in situ measurements of Jupiter‚ study the asteroid belt‚ and investigate the planetary medium. The first‚ to make in situ measurements of Jupiter‚ included taking measurements of and understanding the planet’s atmosphere‚ take close-up images of the planet‚ and continue on to fly past Saturn. For the second goal‚ the asteroid belt is the circular groupings of asteroids and small planets in
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Ptolemaic system is a geocentric cosmology assuming that the Earth is stationary and the centre of the universe. Ptolemy’s model showed that planets revolved around a point and that point revolved around another point which was earth. In order to explain the motion of the planets‚ Ptolemy combined eccentricity with an epicyclic model where he assumed the planets moved on a small sphere or circle‚ called an epicycle‚ that moved on a larger sphere or circle‚ called a deferent. The rotation around the
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everything was revealed to him. The little prince took much care of his planet. He doesn’t want anything destroyed his home. One day‚ a rose appeared on his planet. For him‚ it is the most beautiful creature ever. He fell in love with it but he caught the rose lied to him. So he decided to leave her and not to trust the rose anymore. To cure his loneliness‚ he went to the other planets to explore. He found himself in the near planet where he met the king who’s clad in royal purple and ermine‚ which
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Early Western Scientists Brittany M. Singleton Honors 201 Newberry College Early Western Scientists The Renaissance era is known to be the era of “rebirth”. This “rebirth” began in Italy in the fourteenth century and spread north‚ including England‚ to other countries by the sixteenth century (Anonymous C 2013). The Renaissance was more than just a reawakening‚ this time period brought new discoveries both geographically and intellectually. Renaissance thinkers often associated
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Mythological aspect of the astronomy are mostly covered on the northern hemisphere‚ which includes the 12 zodiac constellations and some other constellations. The zodiac constellations formed an imaginary circle which the sun‚ moon‚ and seven of the nine planets orbited in the space‚ for example the Taurus which symbolizes the bull which describe zeus‚ and the form he took when he carried off the phoenician maiden‚ Europa. The other constellations are the constellations located out of the imaginary circle
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formulated by the Greek philosopher Ptolemy around 140 AD. The sun‚ moon‚ planets and stars all revolved around the earth in circular orbits. Back then‚ everyone “knew” that the earth stood still at the center of the universe. But there were problems with this model. Although the stars move smoothly through the heavens along fixed circular orbits‚ the planets do not. They wander among the other stars (which is where the term “planet” came from; it means “wanderer” in Greek). Their speed varies‚ their
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[2] The planets The research expands to include the terrestrial planets‚ and their satellites. This involves the physics of the interior‚ the geology of the planet or satellite surface‚ the surface morphology‚ and studying their tectonics‚ mineralogy and dating. Observing the outer planets and their satellites includes studying formation and evolution. This method of observation and study involves remote sensing at all wavelengths and in situ measurements. Planet formation and planet evolution
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