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太阳星云

n.solar nebula
网络nebular hypothesis; Near-collision theory; Sar Nebula

太阳星云

太阳星云

英-汉网络释义

太阳星云

solar nebula

太阳星云（Solar Nebula）通过凝聚和吸积形成太阳、太阳系内天体的气团和弥散的固体物质。大约50亿年前开始塌缩，后来形 …

nebular hypothesis

Near-collision theory

什么意思... ... The collision theory 碰撞理论 Near-collision theory 太阳星云 hard sphere collision theory 刚性球碰撞理论 ...

Sar Nebula

...、甲烷、氨以及〝岩石〞，这和太阳系形成当时，原始 太阳星云(Sar Nebula)的组成非常类似。土星的内部非常类似木星， …

2

When the Sun ignited in the solar nebula , hydrogen , helium and other volatile materials were evaporated in the area near the Sun .

当太阳在太阳星云被点燃时，临近太阳附近的氢、氦和其他易挥发物质都成为蒸汽。

3

Formation ages of Ca-Al -rich inclusions and chondrules may speculate the time-scale of evolution of the early solar nebula.

原始球粒陨石中富钙 -铝包体和球粒的形成年龄，可作为早期太阳星云演化的时标；

4

Asteroids are the rocky remains from the collapse of a solar nebula .

小行星是从太阳星云崩溃的岩石遗迹。

5

Chondrules are spherical bodies formed early during the formation of the solar nebula.

陨石是在太阳星云的形成早期形成的球形机构

6

Most of this matter was pulled to the center of the nebula .

大部分气尘云物质凝聚到太阳星云中心。

7

The earth developed from a planetary embryo in the solar nebula into the third planet of our solar system .

地球在早期的太阳星云中由行星胎成长为太阳系的第三颗行星。

8

Our solar system arose from a large, rotating cloud of interstellar debris called the solar nebula .

太阳系是星际碎片太阳星云中的大团旋转云演变而生的。

9

Condensation age of solar nebula

太阳星云凝聚年龄

10

Homogenization of the isotopic composition in the solar nebula

太阳星云同位素组成均一化

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