<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>1405-3322</journal-id>
<journal-title><![CDATA[Boletín de la Sociedad Geológica Mexicana]]></journal-title>
<abbrev-journal-title><![CDATA[Bol. Soc. Geol. Mex]]></abbrev-journal-title>
<issn>1405-3322</issn>
<publisher>
<publisher-name><![CDATA[Sociedad Geológica Mexicana A.C.]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1405-33222025000100110</article-id>
<article-id pub-id-type="doi">10.18268/bsgm2025v77n1a021124</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Atmospheric influence on lithosphere formation during cooling of a global magma ocean]]></article-title>
<article-title xml:lang="es"><![CDATA[Influencia atmosférica en la formación de la litosfera durante el enfriamiento de un océano magmático global]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Carapia-Pérez]]></surname>
<given-names><![CDATA[Miguel Ángel]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Cañón-Tapia]]></surname>
<given-names><![CDATA[Edgardo]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,Centro de Investigación Científica y de Educación Superior de Ensenada División de Ciencias de la Tierra ]]></institution>
<addr-line><![CDATA[Ensenada B.C.]]></addr-line>
<country>México</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>00</month>
<year>2025</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>00</month>
<year>2025</year>
</pub-date>
<volume>77</volume>
<numero>1</numero>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S1405-33222025000100110&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S1405-33222025000100110&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S1405-33222025000100110&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[ABSTRACT The history of the cooling and solidification of the magma ocean produced after the large Moon-forming impact on Earth remains ill-constrained. The most commonly accepted scenario invokes a greenhouse effect of the atmosphere preventing the formation of a solid lithosphere before the complete solidification of the magma ocean from below. In this work we reexamine the cooling history of the planet after the impact, solving the 1D heat diffusion equation in spherical coordinates using the pdepe solver of Matlab for different atmospheric conditions that are compatible with a large impact event. Lithosphere formation is constrained by the time it takes for the atmosphere to drop below 1400°K when the conditions are adequate for solidifying a peridotite melt. Our results indicate that the Earth could have had a different thermal evolution than what has been commonly considered until now in most models of Earth&#8217;s evolution.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[RESUMEN La historia de enfriamiento y solidificación del océano de magma producido después del gran impacto de la formación de la Luna en la Tierra continúa incierta. El escenario más ampliamente aceptado invoca un efecto invernadero de la atmósfera que impide la formación de una litosfera sólida antes de que el océano de magma se solidifique por completo desde abajo. En este trabajo re-examinamos la historia de enfriamiento del planeta después del impacto resolviendo la ecuación de difusión de calor 1D en coordenadas esféricas utilizando el solucionador pdepe de Matlab para diferentes condiciones atmosféricas que son compatibles con un evento de gran impacto. La formación de litosfera está limitada por el tiempo que tarda la atmósfera en descender por debajo de los 1400°K cuando las condiciones son adecuadas para la solidificación de una peridotita fundida. Nuestros resultados indican que la Tierra podría haber tenido una evolución térmica diferente a la que comúnmente se ha considerado hasta ahora en la mayoría de los modelos de evolución de la Tierra.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[magma ocean]]></kwd>
<kwd lng="en"><![CDATA[thermal model]]></kwd>
<kwd lng="en"><![CDATA[atmosphere]]></kwd>
<kwd lng="en"><![CDATA[early Earth]]></kwd>
<kwd lng="es"><![CDATA[océano de magma]]></kwd>
<kwd lng="es"><![CDATA[modelo térmico]]></kwd>
<kwd lng="es"><![CDATA[atmósfera]]></kwd>
<kwd lng="es"><![CDATA[Tierra primitiva]]></kwd>
</kwd-group>
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