久久一区二区三区精品-久久一区二区明星换脸-久久一区二区精品-久久一区不卡中文字幕-91精品国产爱久久久久久-91精品国产福利尤物免费

新GRE寫作名人素材庫:哥白尼

雕龍文庫 分享 時間: 收藏本文

新GRE寫作名人素材庫:哥白尼

  我們在新GRE寫作中要格外重視思維邏輯與論據論證,平時注意積累素材,多收集一些新GRE寫作論據論證例子。下面是小編為大家搜集的關于哥白尼的名人素材,希望能夠幫助大家更好地備考新GRE寫作,獲得新GRE寫作高分。

  哥白尼

  Copernicus, Nicolas 1473 -- 1543

  Astronomer and founder of the heliocentric ordering of the planets. Born on February 19, 1473, in Torun, Poland. He belonged to a family of merchants. His uncle, the bishop and ruler of Ermland, was the person to whom Copernicus owed his education, career, and security. Copernicus studied at the University of Cracow from 1491 to 1494. While he did not attend any classes in astronomy, it was during his student years there that Copernicus began to collect books on astronomy and mathematics. Some of these contain marginal notes by him dating back to that period, but it remains conjectural whether Copernicus had already made at that time a systematic study of the heliocentric theory.

  Copernicus returned to Torun in 1494, and in 1496, through the efforts of his uncle, he became a canon at Frauenburg, remaining in that office for the remainder of his life. Almost immediately Copernicus set out for Bologna to study canon law. In Bologna, Copernicus came under the influence of Domenico Maria de Novara, an astronomer known for his admiration of Pythagorean lore. There Copernicus also recorded some planetary positions, and he did the same in Rome, where he spent the Jubilee Year of 1500.

  In 1501 there followed a brief visit at home. His first official act as canon there was to apply for permission to spend 3 more years in Italy, which was granted him on his promise that he would study medicine. Copernicus settled in Padua, but later he moved to the University of Ferrara, where he obtained in 1503 the degree of doctor in canon law. Only then did he take up the study of medicine in Padua, prolonging his leave of absence until 1506.

  Upon returning to Ermland, Copernicus stayed in his uncles castle at Heilsberg as his personal physician and secretary. During that time he translated from Greek into Latin the 85 poems of Theophylactus Simacotta, the 7th-century Byzantine poet. The work, printed in Cracow in 1509, evidenced Copernicuss humanistic leanings. At this time Copernicus was also mulling over the problems of astronomy, and the heliocentric system in particular. The system is outlined in a short manuscript known as the Commentariolus, or small commentary, which he completed about 1512. Copies of it circulated among his friends eager to know the Sketch of Hypotheses Made by Nicolaus Copernicus on the Heavenly Motions, as Copernicus referred to his work. In it, right at the outset, there was a list of seven axioms, all of which stated a feature specific to the heliocentric system. The third stated in particular: All the spheres revolve about the sun as their midpoint, and therefore the sun is the center of the universe. The rest of the work was devoted to the elaboration of the proposition that in the new system only 34 circles were needed to explain the motion of planets.

  The Commentariolus produced no reaction, either in print or in letters, but Copernicuss fame began to spread. Two years later he received an invitation to be present as an astronomer at the Lateran Council, which had as one of its aims the reform of the calendar; he did not attend. His secretiveness only seemed to further his reputation. In 1522 the secretary to the King of Poland asked Copernicus to pass an opinion on De motu octavae spherae , just published by Johann Werner, a mathematician of some repute. This time he granted the request in the form of a letter in which he took a rather low opinion of Werners work. More important was the concluding remark of the letter, in which Copernicus stated that he intended to set forth elsewhere his own opinion about the motion of the sphere of stars. He referred to the extensive study of which parts and drafts were already very likely extent at that time.

  Copernicus could pursue his study only in his spare time. As a canon, he was involved in various affairs, including legal and medical, but especially administrative and financial matters. In fact, he composed a booklet in 1522 on the remedies of inflation, which then largely meant the preservation of the same amount of gold and silver in coins. For all his failure to publish anything in astronomy, to have his manuscript studies circulate, or to communicate with other astronomers, more and more was rumored about his theory, still on the basis of the Commentariolus.

  Not all the comments were flattering. Luther denounced Copernicus as the fool who will turn the whole science of astronomy upside down. In 1531 a satirical play was produced about him in Elbing, Prussia, by a local schoolmaster. In Rome things went better, for the time being at least. In 1533 John Widmanstad, a papal secretary, lectured on Copernicuss theory before Pope Clement VII and several cardinals. Widmanstads hand was behind the letter that Cardinal Schonberg sent in 1536 from Rome to Copernicus, urging him to publish his thoughts, or at least to share them with him.

  It was a futile request. Probably nobody knew exactly how far Copernicus had progressed with his work until Georg Joachim , a young scholar from Wittenberg, arrived in Frauenburg in the spring of 1539. When he returned to Wittenberg, he had already printed an account, known as the Narratio prima, of Copernicuss almost ready book. Rheticus was also instrumental in securing the printing of Copernicuss book in Nuremberg, although the final supervision remained in the care of Andrew Osiander, a Lutheran clergyman. He might have been the one who gave the work its title, De revolutionibus orbium coelestium, which is not found in the manuscript. But Osiander certainly had written the anonymous preface, in which Copernicuss ideas were claimed as mere hypotheses by their author, or convenient mathematical formalism that had nothing to do with the physical reality.

  The printed copy of his work, in six books, reached Copernicus only a few hours before his death on May 24, 1543. The physics of Copernicus was still Aristotelian and could not, of course, cope with the twofold motion attributed to the earth. But Copernicus could have done a better job as an observer. He added only 27 observations, an exceedingly meager amount, to the data he took over uncritically from Ptolemy and from more recent astronomical tables. The accuracy of predicting celestial phenomena on the basis of his system did not exceed the accuracy achieved by Ptolemy. Nor could Copernicus provide proof for the phases of Mercury and Venus that had to occur if his theory was true. The telescope was still more than half a century away. Again, Copernicus could only say that the stars were immensely far away to explain the absence of stellar parallax due to the orbital motion of the earth. Here, the observational evidence was not forthcoming for another 300 years. Also, while Ptolemy actually used only 40 epicycles, their total number in Copernicuss system was 84, hardly a convincing proof of its greater simplicity.

  Still, the undeniable strength of Copernicuss work lay in its appeal to simplicity. The rotation of the earth made unnecessary the daily revolution of thousands of stars. The orbital motion of the earth fitted perfectly with its period of 365 days into the sequence set by the periods of other planets. Most importantly, the heliocentric ordering of planets eliminated the need to think of the retrograde motion of the planets as a physical reality. In the tenth chapter of the first book Copernicus made the straightforward statement: In the center rests the sun. For who would place this lamp of a very beautiful temple in another or better place than this wherefrom it can illuminate everything at the same time.

  The thousand copies of the first edition of the book did not sell out, and the work was reprinted only three times prior to the 20th century. No great book of Western intellectual history circulated less widely and was read by fewer people than Copernicuss Revolutions. Nonetheless, it has come to be considered a seminal text of modern astronomy.

  希望小編整理的以上新GRE寫作論據論證關于哥白尼的文章對各位考生有所幫助,大家可以選擇幾段來進行背誦,在GRE作文里作為論據進行論證。此外,也可以在平時多搜集一些比較好的論據,來增加作文的含金量。

  

  我們在新GRE寫作中要格外重視思維邏輯與論據論證,平時注意積累素材,多收集一些新GRE寫作論據論證例子。下面是小編為大家搜集的關于哥白尼的名人素材,希望能夠幫助大家更好地備考新GRE寫作,獲得新GRE寫作高分。

  哥白尼

  Copernicus, Nicolas 1473 -- 1543

  Astronomer and founder of the heliocentric ordering of the planets. Born on February 19, 1473, in Torun, Poland. He belonged to a family of merchants. His uncle, the bishop and ruler of Ermland, was the person to whom Copernicus owed his education, career, and security. Copernicus studied at the University of Cracow from 1491 to 1494. While he did not attend any classes in astronomy, it was during his student years there that Copernicus began to collect books on astronomy and mathematics. Some of these contain marginal notes by him dating back to that period, but it remains conjectural whether Copernicus had already made at that time a systematic study of the heliocentric theory.

  Copernicus returned to Torun in 1494, and in 1496, through the efforts of his uncle, he became a canon at Frauenburg, remaining in that office for the remainder of his life. Almost immediately Copernicus set out for Bologna to study canon law. In Bologna, Copernicus came under the influence of Domenico Maria de Novara, an astronomer known for his admiration of Pythagorean lore. There Copernicus also recorded some planetary positions, and he did the same in Rome, where he spent the Jubilee Year of 1500.

  In 1501 there followed a brief visit at home. His first official act as canon there was to apply for permission to spend 3 more years in Italy, which was granted him on his promise that he would study medicine. Copernicus settled in Padua, but later he moved to the University of Ferrara, where he obtained in 1503 the degree of doctor in canon law. Only then did he take up the study of medicine in Padua, prolonging his leave of absence until 1506.

  Upon returning to Ermland, Copernicus stayed in his uncles castle at Heilsberg as his personal physician and secretary. During that time he translated from Greek into Latin the 85 poems of Theophylactus Simacotta, the 7th-century Byzantine poet. The work, printed in Cracow in 1509, evidenced Copernicuss humanistic leanings. At this time Copernicus was also mulling over the problems of astronomy, and the heliocentric system in particular. The system is outlined in a short manuscript known as the Commentariolus, or small commentary, which he completed about 1512. Copies of it circulated among his friends eager to know the Sketch of Hypotheses Made by Nicolaus Copernicus on the Heavenly Motions, as Copernicus referred to his work. In it, right at the outset, there was a list of seven axioms, all of which stated a feature specific to the heliocentric system. The third stated in particular: All the spheres revolve about the sun as their midpoint, and therefore the sun is the center of the universe. The rest of the work was devoted to the elaboration of the proposition that in the new system only 34 circles were needed to explain the motion of planets.

  The Commentariolus produced no reaction, either in print or in letters, but Copernicuss fame began to spread. Two years later he received an invitation to be present as an astronomer at the Lateran Council, which had as one of its aims the reform of the calendar; he did not attend. His secretiveness only seemed to further his reputation. In 1522 the secretary to the King of Poland asked Copernicus to pass an opinion on De motu octavae spherae , just published by Johann Werner, a mathematician of some repute. This time he granted the request in the form of a letter in which he took a rather low opinion of Werners work. More important was the concluding remark of the letter, in which Copernicus stated that he intended to set forth elsewhere his own opinion about the motion of the sphere of stars. He referred to the extensive study of which parts and drafts were already very likely extent at that time.

  Copernicus could pursue his study only in his spare time. As a canon, he was involved in various affairs, including legal and medical, but especially administrative and financial matters. In fact, he composed a booklet in 1522 on the remedies of inflation, which then largely meant the preservation of the same amount of gold and silver in coins. For all his failure to publish anything in astronomy, to have his manuscript studies circulate, or to communicate with other astronomers, more and more was rumored about his theory, still on the basis of the Commentariolus.

  Not all the comments were flattering. Luther denounced Copernicus as the fool who will turn the whole science of astronomy upside down. In 1531 a satirical play was produced about him in Elbing, Prussia, by a local schoolmaster. In Rome things went better, for the time being at least. In 1533 John Widmanstad, a papal secretary, lectured on Copernicuss theory before Pope Clement VII and several cardinals. Widmanstads hand was behind the letter that Cardinal Schonberg sent in 1536 from Rome to Copernicus, urging him to publish his thoughts, or at least to share them with him.

  It was a futile request. Probably nobody knew exactly how far Copernicus had progressed with his work until Georg Joachim , a young scholar from Wittenberg, arrived in Frauenburg in the spring of 1539. When he returned to Wittenberg, he had already printed an account, known as the Narratio prima, of Copernicuss almost ready book. Rheticus was also instrumental in securing the printing of Copernicuss book in Nuremberg, although the final supervision remained in the care of Andrew Osiander, a Lutheran clergyman. He might have been the one who gave the work its title, De revolutionibus orbium coelestium, which is not found in the manuscript. But Osiander certainly had written the anonymous preface, in which Copernicuss ideas were claimed as mere hypotheses by their author, or convenient mathematical formalism that had nothing to do with the physical reality.

  The printed copy of his work, in six books, reached Copernicus only a few hours before his death on May 24, 1543. The physics of Copernicus was still Aristotelian and could not, of course, cope with the twofold motion attributed to the earth. But Copernicus could have done a better job as an observer. He added only 27 observations, an exceedingly meager amount, to the data he took over uncritically from Ptolemy and from more recent astronomical tables. The accuracy of predicting celestial phenomena on the basis of his system did not exceed the accuracy achieved by Ptolemy. Nor could Copernicus provide proof for the phases of Mercury and Venus that had to occur if his theory was true. The telescope was still more than half a century away. Again, Copernicus could only say that the stars were immensely far away to explain the absence of stellar parallax due to the orbital motion of the earth. Here, the observational evidence was not forthcoming for another 300 years. Also, while Ptolemy actually used only 40 epicycles, their total number in Copernicuss system was 84, hardly a convincing proof of its greater simplicity.

  Still, the undeniable strength of Copernicuss work lay in its appeal to simplicity. The rotation of the earth made unnecessary the daily revolution of thousands of stars. The orbital motion of the earth fitted perfectly with its period of 365 days into the sequence set by the periods of other planets. Most importantly, the heliocentric ordering of planets eliminated the need to think of the retrograde motion of the planets as a physical reality. In the tenth chapter of the first book Copernicus made the straightforward statement: In the center rests the sun. For who would place this lamp of a very beautiful temple in another or better place than this wherefrom it can illuminate everything at the same time.

  The thousand copies of the first edition of the book did not sell out, and the work was reprinted only three times prior to the 20th century. No great book of Western intellectual history circulated less widely and was read by fewer people than Copernicuss Revolutions. Nonetheless, it has come to be considered a seminal text of modern astronomy.

  希望小編整理的以上新GRE寫作論據論證關于哥白尼的文章對各位考生有所幫助,大家可以選擇幾段來進行背誦,在GRE作文里作為論據進行論證。此外,也可以在平時多搜集一些比較好的論據,來增加作文的含金量。

  

主站蜘蛛池模板: 欧美一区永久视频免费观看 | 日韩精品久久久免费观看夜色 | 91亚洲综合 | 国产欧美另类久久精品91 | 亚洲午夜在线观看 | 亚洲综合一二三区 | 全球成人网 | 分享一个无毒不卡免费国产 | 国产深夜福利视频网站在线观看 | 久久欧美成人精品丝袜 | 日本黄色大片在线播放视频免费观看 | 毛片免费看网站 | 欧美三级中文字幕 | 手机看片国产欧美日韩高清 | 欧美一区不卡二区不卡三区 | 亚洲综合精品一区二区三区中文 | 国产成人毛片 | 本道久久综合88全国最大色 | 手机在线视频一区 | 成年人网站在线观看免费 | 狠狠色狠狠色狠狠五月ady | 中文字幕日韩精品亚洲七区 | 成人国产精品一级毛片天堂 | 久久久不卡国产精品一区二区 | 国产精品亚洲高清一区二区 | 久久久免费精品 | 亚洲精品国产免费 | 日韩欧美在线一级一中文字暮 | 亚洲精品第一第二区 | 日韩女人做爰大片 | 欧美成人免费观看久久 | 国产小视频在线高清播放 | 日韩亚洲天堂 | 免费又黄又爽又猛大片午夜 | a级毛片免费观看网站 | 国产在线高清视频 | 男女性关系视频免费观看软件 | 澳门一级毛片手机在线看 | 免费国产成人高清在线观看不卡 | gv手机在线观看 | 久久成人a毛片免费观看网站 |