Endogenous Lunar Volatiles

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00025798%3A_____%2F23%3A10169342" target="_blank" >RIV/00025798:_____/23:10169342 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1515/9781501519895-020" target="_blank" >https://doi.org/10.1515/9781501519895-020</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1515/9781501519895-020" target="_blank" >10.1515/9781501519895-020</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Endogenous Lunar Volatiles

Popis výsledku v původním jazyce

The intrinsic properties of the elements and their resulting behavior in natural systems represent the underpinnings of geochemistry as a scientific discipline (Goldschmidt 1937). One of the most valuable intrinsic properties of an element is its volatility. The volatility of an element is most commonly expressed as a 50% condensation temperature, which corresponds to the temperature at which 50% of an element would have condensed from a gas of solar composition at nebular total pressure of 10-4 bars (e.g., Lodders 2003). Refractory elements are characterized by high condensation temperatures with the inverse being true for more volatile elements. Although condensation temperatures are widely used to understand elemental depletions in planetary materials, condensation from a nebular gas may not be the most relevant system for understanding volatile loss from planetary bodies or from the protolunar disk.

Název v anglickém jazyce

Endogenous Lunar Volatiles

Popis výsledku anglicky

The intrinsic properties of the elements and their resulting behavior in natural systems represent the underpinnings of geochemistry as a scientific discipline (Goldschmidt 1937). One of the most valuable intrinsic properties of an element is its volatility. The volatility of an element is most commonly expressed as a 50% condensation temperature, which corresponds to the temperature at which 50% of an element would have condensed from a gas of solar composition at nebular total pressure of 10-4 bars (e.g., Lodders 2003). Refractory elements are characterized by high condensation temperatures with the inverse being true for more volatile elements. Although condensation temperatures are widely used to understand elemental depletions in planetary materials, condensation from a nebular gas may not be the most relevant system for understanding volatile loss from planetary bodies or from the protolunar disk.

Druh

C - Kapitola v odborné knize

CEP obor

—

OECD FORD obor

10505 - Geology

Projekt

—

Návaznosti

V - Vyzkumna aktivita podporovana z jinych verejnych zdroju

Rok uplatnění

2023

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název knihy nebo sborníku

New Views of the Moon 2

ISBN

978-1-946850-11-9

Počet stran výsledku

58

Strana od-do

729-786

Počet stran knihy

869

Název nakladatele

MINERALOGICAL SOC AMER &amp; GEOCHEMICAL SOC

Místo vydání

Chantilly

Kód UT WoS kapitoly

001169611400017