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1 Markets I: The Ecosystem and Exchange-Traded Markets市场在线 2 Markets II: Rates, FX and Credit市场在线 3 Markets III: Commodities, Energy and Crypto市场在线 4 Quantitative Methods方法在线 5 Derivatives and Volatility衍生品在线 6 Rates, Credit, XVA and Risk利率、信用与风险在线 7 Research Craft: Predictors, Backtests, Measurement, Portfolios研究在线 8 Strategies I: Equities and Futures策略在线 9 Strategies II: Volatility, Relative Value, Macro and the Bank Desks策略在线 10 Microstructure and Execution交易执行在线 11 Market Making and High-Frequency Trading做市在线 12 Machine Learning for Markets机器学习在线 13 Low-Latency Software技术在线 14 Networks, Hardware and Trading Infrastructure技术在线 15 Research, Data and Risk Platforms技术在线 16 The Desk and the Firm公司运营在线 17 The Industry: Firms, Roles and Careers职业发展在线 18 Interviews I: Maths, Probability and Speed职业发展在线 19 Interviews II: Markets, Trading Games and the Final Round职业发展在线 20 Interviews III: Code职业发展在线

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Earth and Space Sciences · 术语表

什么是 Condensation temperature, condensation sequence？

又称： condensation temperature · condensation sequence

Definition 2.3 University Earth and Space Sciences — Year 2 · 第 2 章 — Planet Formation and Meteorites

The condensation temperature of an element in a cooling gas of given composition and pressure is the temperature at which half of it has passed into solids at chemical equilibrium (the 50 per cent condensation temperature; the temperature at which its first solid appears is the appearance temperature). The condensation sequence is the order in which the elements and their solid compounds appear as the gas cools.

solid	formula	appears at (K)
corundum	$\ce{Al2O3}$	1677
hibonite	$\ce{CaAl12O19}$	1659
perovskite	$\ce{CaTiO3}$	1593
spinel	$\ce{MgAl2O4}$	1397
iron–nickel metal	$\ce{Fe}$ , with $\ce{Ni}$ , $\ce{Co}$ , $\ce{Cr}$	1357
forsterite	$\ce{Mg2SiO4}$	1354
schreibersite	$\ce{Fe3P}$	1248
troilite	$\ce{FeS}$	704
magnetite	$\ce{Fe3O4}$	371
water ice	$\ce{H2O}$	182
ammonia hydrate	$\ce{NH3.H2O}$	131
methane clathrate	$\ce{CH4.7H2O}$	78

Table 2.1. The condensation sequence of a gas of solar-system composition at

10^{-4}

bar: the temperature at which each solid first appears. Sodium and potassium enter feldspar; nickel, cobalt and chromium dissolve in the metal. Data: Lodders (2003).

The 50 per cent condensation temperatures of 36 elements in a gas of solar-system composition at 10-4 bar, coloured by Lodders’ volatility groups (oxygen: as water ice; carbon: as methane clathrate and ice). Data: Lodders (2003). — The 50 per cent condensation temperatures of 36 elements in a gas of solar-system composition at $10^{-4}$ bar, coloured by Lodders’ volatility groups (oxygen: as water ice; carbon: as methane clathrate and ice). Data: Lodders (2003).

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