Planetary Temperatures in the Presence of an Inert, Nonradiative Atmosphere

Nicol John Leslie ()
Additional contact information
Nicol John Leslie: Department of Physics, James Cook University of North Queensland, Townville, Australia

Quaestiones Geographicae, 2020, vol. 39, issue 3, 69-85

Abstract: This study considers solid planets at about 300 K and an inert atmosphere having no interaction with associated radiation. Processes considered include transfer of energy from the surface skin to underlying layers depending on thermal properties. Temperatures of the surface depend on the rates of transfer of energy between soil layers. The atmosphere is warmed at base by contact with the surface, convection and turbulence distributing higher temperatures through the air. Comparisons between theoretical and measured temperatures show a close similarity. Mean planetary temperatures are calculated, depending on thermal parameters and the intensity of light/radiation from the particular solar system.

Keywords: planet; inert atmosphere; temperatures; capacity/conductivity; soil; air (search for similar items in EconPapers)
Date: 2020
References: View complete reference list from CitEc
Citations:

Downloads: (external link)
https://doi.org/10.2478/quageo-2020-0024 (text/html)

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:vrs:quageo:v:39:y:2020:i:3:p:69-85:n:5

DOI: 10.2478/quageo-2020-0024

Access Statistics for this article

Quaestiones Geographicae is currently edited by Andrzej Kostrzewski

More articles in Quaestiones Geographicae from Sciendo
Bibliographic data for series maintained by Peter Golla ().