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    <AnnotationProperty rdf:about="http://purl.obolibrary.org/obo/IAO_0000115"/>
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    <!-- http://purl.obolibrary.org/obo/ENVO_01000639 -->

    <Class rdf:about="http://purl.obolibrary.org/obo/ENVO_01000639">
        <rdfs:label xml:lang="en">planetary structural layer</rdfs:label>
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    <!-- http://purl.obolibrary.org/obo/ENVO_01000641 -->

    <Class rdf:about="http://purl.obolibrary.org/obo/ENVO_01000641">
        <rdfs:label xml:lang="en">planetary core</rdfs:label>
        <rdfs:subClassOf rdf:resource="http://purl.obolibrary.org/obo/ENVO_01000639"/>
        <oboInOwl:hasBroadSynonym>core</oboInOwl:hasBroadSynonym>
        <rdfs:comment>&quot;Not to be confused with planetary core in the core accretion theory, referring to a central accretionary body surrounded by a halo of dust and gas which serves to trap debris and increase the rate of accretion..&quot; WIkipedia:Planetary_core. This class is meant to be applicable accross planets. Earth&#39;s core would be an instance. The &quot;layer&quot; aspect of cores may be problematic.</rdfs:comment>
        <ns2:IAO_0000115>A planetary core is the innermost structural layer or layers of a planet. The core may be entirely liquid, entirely solid, or have both liquid and solid parts.</ns2:IAO_0000115>
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