“2016年IOAA理论第2题-土卫六上的气体”的版本间的差异

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Gas particles in a planetary atmosphere have a wide distribution of speeds. If the r.m.s. (root mean square)
 
Gas particles in a planetary atmosphere have a wide distribution of speeds. If the r.m.s. (root mean square)
 
thermal speed of particles of a particular gas exceeds 1/6 of the escape speed, then most of that gas will
 
thermal speed of particles of a particular gas exceeds 1/6 of the escape speed, then most of that gas will
escape from the planet. What is the minimum atomic weight (relative atomic mass), 𝐴min, of an ideal
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escape from the planet. What is the minimum atomic weight (relative atomic mass), 𝐴<sub>min</sub>, of an ideal
 
monatomic gas so that it remains in the atmosphere of Titan?
 
monatomic gas so that it remains in the atmosphere of Titan?
  
 
Given, mass of Titan 𝑀<sub>T</sub> = 1.23 × 10<sup>23</sup> kg, radius of Titan 𝑅<sub>T</sub> = 2575 km, surface temperature of
 
Given, mass of Titan 𝑀<sub>T</sub> = 1.23 × 10<sup>23</sup> kg, radius of Titan 𝑅<sub>T</sub> = 2575 km, surface temperature of
 
Titan 𝑇<sub>T</sub> = 93.7 K.
 
Titan 𝑇<sub>T</sub> = 93.7 K.
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[[分类:热学]]

2019年9月11日 (三) 17:24的版本

英文题目

(T2) Gases on Titan

Gas particles in a planetary atmosphere have a wide distribution of speeds. If the r.m.s. (root mean square) thermal speed of particles of a particular gas exceeds 1/6 of the escape speed, then most of that gas will escape from the planet. What is the minimum atomic weight (relative atomic mass), 𝐴min, of an ideal monatomic gas so that it remains in the atmosphere of Titan?

Given, mass of Titan 𝑀T = 1.23 × 1023 kg, radius of Titan 𝑅T = 2575 km, surface temperature of Titan 𝑇T = 93.7 K.