आइज्याक न्युटन: Difference between revisions

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{{Infobox scientist
|name = सर आइज्याक न्युटन
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'''सर आइज्याक न्युटन''', [[Fellow of the Royal Society|FRS]] (ज्यानुवरी ४, सन् १६४३ {{ndash}} मार्च ३१, सन् १७२७ {{smaller|<nowiki>[</nowiki>[[Old Style and New Style dates|OS]]: 25 December 1642{{ndash}} 20 March 1727<nowiki>]</nowiki>}})<ref name="OSNS"/> छम्ह अंग्रेज फिजिसिस्ट, गणितज्ञ, खगोलशास्त्री, प्राकृतिक दार्शनिक, अल्केमिस्ट, व धर्मशास्त्री ख। वय्कः मानव इतिहासय् दकले प्रभावशाली मनुय् छम्ह ख।
'''सर आइज्याक न्युटन''', [[Fellow of the Royal Society|FRS]] (4 January 1643 {{ndash}} 31 March 1727 {{smaller|<nowiki>[</nowiki>[[Old Style and New Style dates|OS]]: 25 December 1642{{ndash}} 20 March 1727<nowiki>]</nowiki>}})<ref name="OSNS"/> was an [[English people|English]] [[physicist]], [[mathematician]], [[Astronomy|astronomer]], [[Natural philosophy|natural philosopher]], [[Alchemy|alchemist]], and [[Theology|theologian]] and one of the most influential men in human history. His ''[[Philosophiæ Naturalis Principia Mathematica]]'', published in 1687, is by itself considered to be among the most influential books in the [[history of science]], laying the groundwork for most of [[classical mechanics]]. In this work, Newton described [[law of universal gravitation|universal gravitation]] and the three [[Newton's laws of motion|laws of motion]] which dominated the scientific view of the [[physical universe]] for the next three centuries. Newton showed that the motions of objects on [[Earth]] and of [[celestial mechanics|celestial]] bodies are governed by the same set of natural laws by demonstrating the consistency between [[Kepler's laws of planetary motion]] and his theory of gravitation, thus removing the last doubts about [[heliocentrism]] and advancing the [[scientific revolution]].
 
== लिधंसा ==
{{लिधंसा}}