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英語(yǔ)人>網(wǎng)絡(luò)例句>Kepler's law 相關(guān)的網(wǎng)絡(luò)例句
Kepler's law相關(guān)的網(wǎng)絡(luò)例句

查詢(xún)?cè)~典 Kepler's law

與 Kepler's law 相關(guān)的網(wǎng)絡(luò)例句 [注:此內(nèi)容來(lái)源于網(wǎng)絡(luò)日韩三级亚洲三级,僅供參考]

After some treatment of centripetal force, he deduces Kepler's third law.

在向心力的一些論述之后,他推出了開(kāi)普勒的第三定律国产精品欧美亚洲韩国日本不卡。

He would give a book worth 40 shillings to anyone who could deduce Kepler's laws from the inverse-square law.

Christopher Wren打賭如果有人能用平方反比定律推論開(kāi)普勒定律,他就會(huì)將一本價(jià)值40先令的書(shū)送給這個(gè)人中国熟妇性视频一区。

Kepler's laws of Newton discovered the law of gravitation 10000 l ^ D has laid the foundation, then to the law of gravity, in turn, amended the third Kepler principle, namely, the ratio of 32 to strictly say no is a constant with the planets related to the quality of the l ^ D.

開(kāi)普勒定律為牛頓發(fā)現(xiàn)萬(wàn)l^D有引力定律奠定了基礎(chǔ)日日爱自拍com,而后,萬(wàn)有引力定律反過(guò)來(lái)又修正了開(kāi)普勒第三定律www.色色色色色色色色色,即比值32嚴(yán)格說(shuō)不為常數(shù)而與行星l^D的質(zhì)量有關(guān)www日免费看。

In many ways, Galileo was a more modern thinker than Kepler (Galileo's contemporary) or Newton (whose single greatest accomplishment, apart from the invention of calculus, was the explanation of Kepler's three laws of planetary motion and their implications for the law of universal gravitation).

在許多方面,比起刻卜勒或牛頓(除了發(fā)明微積分外AV影院网站,牛頓的最大成就在於解釋刻卜勒行星三大運(yùn)動(dòng)定律18岁以内禁看黄色视频,以及它們?cè)谌f(wàn)有引力定律上的蘊(yùn)意),伽利略是更現(xiàn)代的思想家日韩不卡视频毛片。

Kepler's third law gave a more specific hint about the nature of the force.

開(kāi)普勒第三定律給出了一個(gè)關(guān)于力的本質(zhì)的更為具體的說(shuō)明免费看毛片视频在线播放。

Kepler's second law means that a planet's orbital speed changes with its distance from the sun.

開(kāi)普勒第二定律指行星的軌道速度與其和太陽(yáng)的距離。

To understand the increasing sizes of the circles according as the celestial body moves farther away from the sun, one has to be aware of Kepler's second law of planetary motion.

為了解各界日益增加的大小根據(jù)作為移動(dòng)的天體遠(yuǎn)離太陽(yáng)欧美熟妇白嫩大屁黑人啪啪,人們必須意識(shí)到開(kāi)普勒的行星運(yùn)動(dòng)第二定律日韩三级欧美一区中文。

Sitting before the computer, a process that lasts effectively for years may take place in a few seconds, the Kepler's and Newton's law are understood in a shorter time.

坐在計(jì)算機(jī)前邊,持續(xù)多年的一個(gè)處理過(guò)程可以在幾分鐘之內(nèi)發(fā)生人人操,人人舔人人干,開(kāi)普勒和牛頓的理論在短時(shí)間內(nèi)就會(huì)被理解男人天堂精品自拍。

Each planet speeds up when it is nearer the Sun and travels more slowly when it is far from the Sun (this is Kepler's Second Law of Planetary Motion).

各個(gè)行星加速當(dāng)它太陽(yáng)是更近的并且慢慢地旅行當(dāng)它在離太陽(yáng)很遠(yuǎn)的地方(這是星球運(yùn)動(dòng)Kepler's 第二法律)。

As a result of Kepler's second law, the celestial body needs a longer time to pass through a sign in the zodiac when the celestial body is remote from the sun than when the celestial body is nearby the sun.

作為開(kāi)普勒第二定律的結(jié)果免费狼友,天體需要較長(zhǎng)的時(shí)間來(lái)通過(guò)星座中的天體時(shí)在线加勒比无码专区,從遠(yuǎn)程比太陽(yáng)的天體時(shí),附近是太陽(yáng)的跡象99riAV日日久。

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