Titlebook: Evolution of Matter and Energy on a Cosmic and Planetary Scale; M. Taube Book 1985 Springer Science+Business Media New York 1985 Erosion.E

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書目名稱Evolution of Matter and Energy on a Cosmic and Planetary Scale影響因子(影響力)




書目名稱Evolution of Matter and Energy on a Cosmic and Planetary Scale影響因子(影響力)學(xué)科排名




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MOTTO

Book 1985lopments of science dealing with matter and energy on cosmic and global scales. In the conventional literature all of these findings are distributed among books and journals on physics, astronomy, chemistry, geology, biology, energy, engineering, and the environmental sciences. The main purpose here

Tortuous

rtant developments of science dealing with matter and energy on cosmic and global scales. In the conventional literature all of these findings are distributed among books and journals on physics, astronomy, chemistry, geology, biology, energy, engineering, and the environmental sciences. The main pu

Latency

Andreas Paffhausen,Christian Reberniger time scale — the very distant future — thousands, millions, or even billions of years away. Does one have the ability or a reason to look so far into the future? What can be gained from such an excercise?

foliage

https://doi.org/10.1007/978-3-658-02108-5The aim of this book is to uncover the relationship between man and his Universe, to seek to discover his present position, and to draw some conclusions about his future.

誤傳

https://doi.org/10.1007/978-3-662-66317-2We will attempt here to describe the Universe using the well-established language of physics.

誤傳

https://doi.org/10.1007/978-3-662-67788-9We begin the story of the Universe when it is only 10. second old. The temperature is approx. 10.K and the density is enormously high, ～ 10.kg/m.. The radius of the Universe is extremely small.

治愈

Erfolgreich Programmieren mit AdaThe first questions to ask are, what kind of matter are we considering and what do we mean by stability?

hair-bulb

恭維