FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2010204035> ?p ?o ?g. }

• W2010204035 endingPage "184" @default.
• W2010204035 startingPage "173" @default.
• W2010204035 abstract "Impact events that produce large craters primarily occurred early in the Solar System’s history because the largest bolides were remnants from planetary formation. Determining when large impacts occurred on a planetary surface such as Mars can yield clues to the flux of material in the early inner Solar System which, in turn, can constrain other planetary processes such as the timing and magnitude of resurfacing and the history of the martian core dynamo. We have used a large, global planetary database in conjunction with geomorphologic mapping to identify craters superposed on the rims of 78 larger craters with diameters D ⩾ 150 km on Mars, ≈78% of which have not been previously dated in this manner. The densities of superposed craters with diameters larger than 10, 16, 25, and 50 km, as well as isochron fits were used to derive model crater ages of these larger craters and basins from which we derived an impact flux. In discussing these ages, we point out several internal inconsistencies of crater-age modeling techniques and chronology systems and, all told, we explain why we think isochron-fitting is the most reliable indicator of an age. Our results point to a mostly obliterated crater record prior to ∼4.0 Ga with the oldest preserved mappable craters on Mars dating to ∼4.3–4.35 Ga. We have used our results to constrain the cessation time of the martian core dynamo which we found to have occurred between the formation of Ladon and Prometheus basins, approximately 4.06–4.09 Ga. We also show that, overall, surfaces on Mars older than ∼4.0–4.1 Ga have experienced >1 km of resurfacing, while those younger than ∼3.8–3.9 Ga have experienced significantly less." @default.
• W2010204035 created "2016-06-24" @default.
• W2010204035 creator A5015258205 @default.
• W2010204035 creator A5068556726 @default.
• W2010204035 creator A5078848129 @default.
• W2010204035 creator A5090591484 @default.
• W2010204035 date "2013-07-01" @default.
• W2010204035 modified "2023-10-09" @default.
• W2010204035 title "Large impact crater histories of Mars: The effect of different model crater age techniques" @default.
• W2010204035 cites W1624814720 @default.
• W2010204035 cites W1664327713 @default.
• W2010204035 cites W1858416843 @default.
• W2010204035 cites W1959451655 @default.
• W2010204035 cites W1969484083 @default.
• W2010204035 cites W1982079946 @default.
• W2010204035 cites W1994090879 @default.
• W2010204035 cites W2006113258 @default.
• W2010204035 cites W2008227807 @default.
• W2010204035 cites W2012337099 @default.
• W2010204035 cites W2016262209 @default.
• W2010204035 cites W2018463199 @default.
• W2010204035 cites W2019294046 @default.
• W2010204035 cites W2023997504 @default.
• W2010204035 cites W2042371405 @default.
• W2010204035 cites W2045323482 @default.
• W2010204035 cites W2047917504 @default.
• W2010204035 cites W2050031805 @default.
• W2010204035 cites W2054153857 @default.
• W2010204035 cites W2059652784 @default.
• W2010204035 cites W2063135069 @default.
• W2010204035 cites W2065782610 @default.
• W2010204035 cites W2071017935 @default.
• W2010204035 cites W2074515519 @default.
• W2010204035 cites W2082069995 @default.
• W2010204035 cites W2090280768 @default.
• W2010204035 cites W2093662773 @default.
• W2010204035 cites W2096632126 @default.
• W2010204035 cites W2113865155 @default.
• W2010204035 cites W2118529717 @default.
• W2010204035 cites W2119685988 @default.
• W2010204035 cites W2129023561 @default.
• W2010204035 cites W2131693788 @default.
• W2010204035 cites W2142545238 @default.
• W2010204035 cites W2145892001 @default.
• W2010204035 cites W2148026027 @default.
• W2010204035 cites W2153889975 @default.
• W2010204035 cites W2171672780 @default.
• W2010204035 cites W4241035732 @default.
• W2010204035 cites W4243063327 @default.
• W2010204035 cites W4362213396 @default.
• W2010204035 doi "https://doi.org/10.1016/j.icarus.2013.03.019" @default.
• W2010204035 hasPublicationYear "2013" @default.
• W2010204035 type Work @default.
• W2010204035 sameAs 2010204035 @default.
• W2010204035 citedByCount "121" @default.
• W2010204035 countsByYear W20102040352013 @default.
• W2010204035 countsByYear W20102040352014 @default.
• W2010204035 countsByYear W20102040352015 @default.
• W2010204035 countsByYear W20102040352016 @default.
• W2010204035 countsByYear W20102040352017 @default.
• W2010204035 countsByYear W20102040352018 @default.
• W2010204035 countsByYear W20102040352019 @default.
• W2010204035 countsByYear W20102040352020 @default.
• W2010204035 countsByYear W20102040352021 @default.
• W2010204035 countsByYear W20102040352022 @default.
• W2010204035 countsByYear W20102040352023 @default.
• W2010204035 crossrefType "journal-article" @default.
• W2010204035 hasAuthorship W2010204035A5015258205 @default.
• W2010204035 hasAuthorship W2010204035A5068556726 @default.
• W2010204035 hasAuthorship W2010204035A5078848129 @default.
• W2010204035 hasAuthorship W2010204035A5090591484 @default.
• W2010204035 hasConcept C121332964 @default.
• W2010204035 hasConcept C127313418 @default.
• W2010204035 hasConcept C138774019 @default.
• W2010204035 hasConcept C17409809 @default.
• W2010204035 hasConcept C179537507 @default.
• W2010204035 hasConcept C2776219924 @default.
• W2010204035 hasConcept C2778600265 @default.
• W2010204035 hasConcept C2780472129 @default.
• W2010204035 hasConcept C487381 @default.
• W2010204035 hasConcept C539450922 @default.
• W2010204035 hasConcept C8058405 @default.
• W2010204035 hasConcept C83260615 @default.
• W2010204035 hasConcept C87355193 @default.
• W2010204035 hasConceptScore W2010204035C121332964 @default.
• W2010204035 hasConceptScore W2010204035C127313418 @default.
• W2010204035 hasConceptScore W2010204035C138774019 @default.
• W2010204035 hasConceptScore W2010204035C17409809 @default.
• W2010204035 hasConceptScore W2010204035C179537507 @default.
• W2010204035 hasConceptScore W2010204035C2776219924 @default.
• W2010204035 hasConceptScore W2010204035C2778600265 @default.
• W2010204035 hasConceptScore W2010204035C2780472129 @default.
• W2010204035 hasConceptScore W2010204035C487381 @default.
• W2010204035 hasConceptScore W2010204035C539450922 @default.
• W2010204035 hasConceptScore W2010204035C8058405 @default.
• W2010204035 hasConceptScore W2010204035C83260615 @default.
• W2010204035 hasConceptScore W2010204035C87355193 @default.
• W2010204035 hasIssue "1" @default.

• next