About: http://webisa.webdatacommons.org/205783244

Property	Value
http://www.w3.org/1999/02/22-rdf-syntax-ns#type	http://www.w3.org/ns/prov#Entity
http://www.w3.org/ns/prov#value	Because changes in air temperature take time to propagate into the subsurface, the amount of cooling depends mostly on the thermal properties of the top metre or so of the Martian surface.
http://www.w3.org/ns/prov#wasQuotedFrom	all-geo.org