英语词汇“protoplanet”的意思、用法、释义、翻译、读音、例句、短语、词组-英语词典

是什么意思

原行星；

英英释义

Protoplanet

Protoplanets are large planetary embryos that originate within protoplanetary discs and have undergone internal melting to produce differentiated interiors. They are believed to form out of kilometer-sized planetesimals that attract each other gravitationally and collide.

以上来源于:Wikipedia

学习怎么用

双语例句

用作名词(n.)

In the meantime the protoplanet cores were proceeding to consolidate.
在此期间，原行星的核开始凝成。

权威例句

Protoplanet
Protoplanet
Protoplanet
Protoplanet Migration by Nebula Tides ☆
Giant gaseous protoplanet formation?
Formation of Protoplanet Systems and Diversity of Planetary Systems
The Formation of Protoplanet Systems and the Diversity of Planetary Systems
Scattering of Planetesimals by a Protoplanet: Slowing Down of Runaway Growth
Evolution of the Solar Nebula. IV. Giant Gaseous Protoplanet Formation
Gas Giant Protoplanet Formation: Disk Instability Models with Detailed Thermodynamics and Varied Artificial Viscosity
Reversing type II migration: resonance trapping of a lighter giant protoplanet
A vaporization model for iron/silicate fractionation in the Mercury protoplanet
Global hydromagnetic simulations of a planet embedded in a dead zone: gap opening, gas accretion and formation of a protoplanetary jet

单词	protoplanet
释义	protoplanet 听听怎么读英 [pr??t?'pl?n?t] 美 [pro?t?'pl?n?t] 是什么意思 n. 原行星；英英释义 Protoplanet Protoplanets are large planetary embryos that originate within protoplanetary discs and have undergone internal melting to produce differentiated interiors. They are believed to form out of kilometer-sized planetesimals that attract each other gravitationally and collide. 以上来源于:Wikipedia 学习怎么用双语例句用作名词(n.) In the meantime the protoplanet cores were proceeding to consolidate. 在此期间，原行星的核开始凝成。权威例句 Protoplanet Protoplanet Protoplanet Protoplanet Migration by Nebula Tides ☆ Giant gaseous protoplanet formation? Formation of Protoplanet Systems and Diversity of Planetary Systems The Formation of Protoplanet Systems and the Diversity of Planetary Systems Scattering of Planetesimals by a Protoplanet: Slowing Down of Runaway Growth Evolution of the Solar Nebula. IV. Giant Gaseous Protoplanet Formation Gas Giant Protoplanet Formation: Disk Instability Models with Detailed Thermodynamics and Varied Artificial Viscosity Reversing type II migration: resonance trapping of a lighter giant protoplanet A vaporization model for iron/silicate fractionation in the Mercury protoplanet Global hydromagnetic simulations of a planet embedded in a dead zone: gap opening, gas accretion and formation of a protoplanetary jet
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