Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q17016801> ?p ?o }
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- Q17016801 subject Q15258555.
- Q17016801 subject Q8543131.
- Q17016801 abstract "Ghost craters on the planet Mercury have tectonic features such as graben and wrinkle ridges. These features were formed by extensional and contractional forces originating in tectonic processes such as uplift and global contraction. The combination of graben and wrinkle ridges inside ghost craters found on Mercury has not been observed on any of the other terrestrial planets.".
- Q17016801 thumbnail Ghost_craters_on_Mercury.png?width=300.
- Q17016801 wikiPageWikiLink Q111.
- Q17016801 wikiPageWikiLink Q128207.
- Q17016801 wikiPageWikiLink Q1499003.
- Q17016801 wikiPageWikiLink Q15258555.
- Q17016801 wikiPageWikiLink Q1592877.
- Q17016801 wikiPageWikiLink Q182539.
- Q17016801 wikiPageWikiLink Q188719.
- Q17016801 wikiPageWikiLink Q192810.
- Q17016801 wikiPageWikiLink Q193343.
- Q17016801 wikiPageWikiLink Q308.
- Q17016801 wikiPageWikiLink Q313.
- Q17016801 wikiPageWikiLink Q405.
- Q17016801 wikiPageWikiLink Q47089.
- Q17016801 wikiPageWikiLink Q55818.
- Q17016801 wikiPageWikiLink Q667575.
- Q17016801 wikiPageWikiLink Q8072.
- Q17016801 wikiPageWikiLink Q83296.
- Q17016801 wikiPageWikiLink Q8543131.
- Q17016801 comment "Ghost craters on the planet Mercury have tectonic features such as graben and wrinkle ridges. These features were formed by extensional and contractional forces originating in tectonic processes such as uplift and global contraction. The combination of graben and wrinkle ridges inside ghost craters found on Mercury has not been observed on any of the other terrestrial planets.".
- Q17016801 label "Ghost craters on Mercury".
- Q17016801 depiction Ghost_craters_on_Mercury.png.