Multi-isotope analysis of mammal bones provides environmental context for the adoption of agriculture in the Tehuacan Valley of Mexico. [PDF]
Somerville AD +9 more
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A probable ancient nearshore zone in southern Utopia on Mars unveiled from observations at the Zhurong landing area. [PDF]
Wu B +14 more
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Geologic Constraints on the Formation and Evolution of Saturn's Mid-Sized Moons. [PDF]
Rhoden AR +9 more
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A tale of two planets: Disparate evolutionary models for Mars inferred from radiogenic isotope compositions of Martian meteorites. [PDF]
Borg LE, Kruijer TS.
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Reduced contribution of sulfur to the mass extinction associated with the Chicxulub impact event. [PDF]
Rodiouchkina K +9 more
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El Niño modulated Holocene hydroclimate extremes as a dipolar pattern of droughts in northeastern China and floods in southwestern China. [PDF]
Fan J +8 more
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Volcanism-induced collapse and recovery of the Atlantic meridional overturning circulation under glacial conditions. [PDF]
Vettoretti G +10 more
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New crater calibrations for the lunar crater-age chronology
Earth and Planetary Science Letters, 2014Abstract Measuring the spatial density of craters emplaced on geologic units is the primary method used for remotely estimating ages of solar system surfaces. The calibration for this method, which enables conversion of crater density to absolute age, comes from Apollo and Luna lunar samples for which absolute radiometric ages have been determined ...
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Crater size-frequency distributions and a revised Martian relative chronology
Icarus, 1988A relative plotting technique is applied to Viking 1:2M photomosaics of 25,826 Martian craters of diameter greater than 8 km and age younger than that of the Martian surface. The size-frequency distribution curves are calculated and analyzed in detail, and the results are presented in extensive tables and maps.
Nadine G Barlow
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Cratering Chronology and the Evolution of Mars
Space Science Reviews, 2001Results by Neukum et al. (2001) and Ivanov (2001) are combined with crater counts to estimate ages of Martian surfaces. These results are combined with studies of Martian meteorites (Nyquist et al., 2001) to establish a rough chronology of Martian history.
Hartmann, W.K., Neukum, G.
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