Cargando…

Venus nightside surface temperature

First global map of Venus nightside surface temperature using Akatsuki infrared measurements reveals hot Venus surface with an average surface temperature of about 698 K. Surface temperatures do not show any significant variation with changing latitudes because only a small amount (~2.5%) of solar e...

Descripción completa

Detalles Bibliográficos
Autor principal: Singh, D.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2019
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6362074/
https://www.ncbi.nlm.nih.gov/pubmed/30718759
http://dx.doi.org/10.1038/s41598-018-38117-x
_version_ 1783392817832263680
author Singh, D.
author_facet Singh, D.
author_sort Singh, D.
collection PubMed
description First global map of Venus nightside surface temperature using Akatsuki infrared measurements reveals hot Venus surface with an average surface temperature of about 698 K. Surface temperatures do not show any significant variation with changing latitudes because only a small amount (~2.5%) of solar energy reaches the surface. Surface temperatures are relatively colder at higher altitude regions as compared to lower altitude regions. However, the major temperature variation on Venus surface is governed by various lithospheric heat transport mechanisms. On a global scale, surface temperatures show a spatial variation of about 230 K.
format Online
Article
Text
id pubmed-6362074
institution National Center for Biotechnology Information
language English
publishDate 2019
publisher Nature Publishing Group UK
record_format MEDLINE/PubMed
spelling pubmed-63620742019-02-06 Venus nightside surface temperature Singh, D. Sci Rep Article First global map of Venus nightside surface temperature using Akatsuki infrared measurements reveals hot Venus surface with an average surface temperature of about 698 K. Surface temperatures do not show any significant variation with changing latitudes because only a small amount (~2.5%) of solar energy reaches the surface. Surface temperatures are relatively colder at higher altitude regions as compared to lower altitude regions. However, the major temperature variation on Venus surface is governed by various lithospheric heat transport mechanisms. On a global scale, surface temperatures show a spatial variation of about 230 K. Nature Publishing Group UK 2019-02-04 /pmc/articles/PMC6362074/ /pubmed/30718759 http://dx.doi.org/10.1038/s41598-018-38117-x Text en © The Author(s) 2019 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.
spellingShingle Article
Singh, D.
Venus nightside surface temperature
title Venus nightside surface temperature
title_full Venus nightside surface temperature
title_fullStr Venus nightside surface temperature
title_full_unstemmed Venus nightside surface temperature
title_short Venus nightside surface temperature
title_sort venus nightside surface temperature
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6362074/
https://www.ncbi.nlm.nih.gov/pubmed/30718759
http://dx.doi.org/10.1038/s41598-018-38117-x
work_keys_str_mv AT singhd venusnightsidesurfacetemperature