The conductive cooling of planetesimals with temperature-dependent properties
Modelling the planetary heat transport of small bodies in the early Solar System allows us to understand the geological context of meteorite samples. Conductive cooling in planetesimals is controlled by thermal conductivity, heat capacity, and density, which are functions of temperature (T). We inve...
Главные авторы: | Murphy Quinlan, M, Walker, AM, Davies, CJ, Mound, JE, Muller, T, Harvey, J |
---|---|
Формат: | Journal article |
Язык: | English |
Опубликовано: |
American Geophysical Union
2021
|
Схожие документы
-
Chondrites as samples of differentiated planetesimals
по: Elkins Tanton, Linda T., и др.
Опубликовано: (2017) -
Unlocking planetesimal magnetic field histories: a refined, versatile model for thermal evolution and dynamo generation
по: Sanderson, HR, и др.
Опубликовано: (2024) -
Can planetesimals form by collisional fusion?
по: Mitra, D, и др.
Опубликовано: (2013) -
Detailed Calculations of the Efficiency of Planetesimal Accretion in the Core-accretion Model. III. The Contribution of Planetesimals beyond Saturn
по: Nader Haghighipour, и др.
Опубликовано: (2024-01-01) -
Possible Ribose Synthesis in Carbonaceous Planetesimals
по: Klaus Paschek, и др.
Опубликовано: (2022-03-01)