000006824 001__ 6824
000006824 005__ 20240217081315.0
000006824 0247_ $$2DOI$$a10.34133/space.0075
000006824 037__ $$aSCART-2024-0084
000006824 100__ $$aGillmann, Cedric 
000006824 245__ $$aInterior Controls on the Habitability of Rocky Planets
000006824 260__ $$c2024
000006824 500__ $$aGold Open Access
000006824 520__ $$aNo matter how fascinating and exotic other terrestrial planets are revealed to be, nothing generates more excitement than announcements regarding their habitability. From the observation of Mars to present-day efforts toward Venus and the characterization of exoplanets, the search for life, or at least environments that could accommodate life, has been a major drive for space exploration. So far, we have found no other unquestionably habitable world besides Earth. The conditions of the habitability of terrestrial planets have proved elusive, as surface conditions depend on the complex interplay of many processes throughout the evolution of a planet. Here, we review how the interior of a rocky planet can drive the evolution of its surface conditions and atmosphere. Instead of listing criteria assumed to be critical for life, we discuss how the bulk-silicate planet can affect the onset, continuation, and cessation of habitability. We then consider how it can be observed, and current efforts toward this end.
000006824 536__ $$aFED-tWIN STELLA/$$cFED-tWIN STELLA/$$fFED-tWIN STELLA
000006824 594__ $$aNO
000006824 700__ $$aHakim, Kaustubh 
000006824 700__ $$aLourenco, Diogo L.
000006824 700__ $$aQuanz, Sascha P.
000006824 700__ $$aSossi, Paolo A.
000006824 773__ $$c0075$$pSpace: Science & Technology$$v4$$y2024
000006824 8560_ $$fkaustubh.hakim@ksb-orb.be
000006824 85642 $$ahttps://spj.science.org/doi/10.34133/space.0075
000006824 8564_ $$s2469447$$uhttp://publi2-as.oma.be/record/6824/files/Gillmann2024Review.pdf
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000006824 8564_ $$s22616$$uhttp://publi2-as.oma.be/record/6824/files/Gillmann2024Review.jpg?subformat=icon-180$$xicon-180
000006824 905__ $$apublished in
000006824 980__ $$aREFERD