The impact of orbitally-driven changes in solar insolation on “greenhouse” climates

Mathematics – Logic

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[4910] Paleoceanography / Astronomical Forcing

Scientific paper

We seek to determine the link between climate change and eccentricity-scale lithologic cycles found in early Paleogene deep-sea sediments. Through a multi proxy investigation of cyclic lithologic variations recorded at Shatsky Rise (NW Pacific Ocean, Ocean Drilling Program Leg 198), we test the hypotheses that orbital variations in solar insolation caused changes in wind intensity and aridity in dust source regions as well as the corrosiveness of global deep ocean waters. During the study interval at ~58Ma, Shatsky Rise was in the central tropical Pacific, situated far from any existing shoreline so that any terrigenous silicate material that reached the location likely was windblown dust. Variations in the grain size and flux of eolian material delivered to the open ocean are used as a proxy for atmospheric circulation patterns and vigor, and changes in the aridity and/or vegetation cover of dust source regions, respectively. We have determined the grain size and dust accumulation rates over eight consecutive 100 kyr eccentricity cycles. Median grain sizes ranged from 8.7Φ to 8.4Φ over the interval, suggesting relative wind intensity changes of 30-60%, but with no resolvable orbital periodicity. In contrast, 232Th (a proxy for continentally derived material) and sedimentological analyses indicate dust fluxes to Shatsky Rise varied on eccentricity timescales, with maximum accumulation occurring during eccentricity maxima. 232Th concentrations in the bulk sediment indicate that the entire detrital fraction is continentally derived and not authigenic. The calculated 232Th fluxes (0.9 -17.4 mg/cm2/kyr) agree well with sediment dust mass accumulation rates determined using traditional chemical extraction techniques (2.9 to 15.9 mg/cm2/kyr). Nd and Sr isotopic values of the “eolian” sediment fraction were less and more radiogenic than coeval seawater, respectively, supporting the assumption the material was derived from the continents and is not authigenic (average ɛNd(t) = -10.0 and 87Sr/86Sr = 0.70906). The pacing of dust flux variations with eccentricity changes suggests that continental aridity is controlled by cyclic changes in solar insolation. Carbonate mass accumulation rates across the 8 eccentricity cycles exhibit a small range of 0.54 to 0.79 g/cm2/kyr. While intervals of increased dust accumulation during maximum eccentricity may “dilute” the total calcium carbonate accumulation, these can only account for a small fraction of the total carbonate change. Thus, the remaining difference in carbonate content must have been driven by coincident changes in carbonate accumulation. We analyzed the Nd isotopic composition of fossil fish debris to track potential changes in water mass composition that may have contributed to cyclic variations in seafloor corrosiveness. Preliminary results show a small range in ɛNd(t) of fish teeth -3.9 to -2.9, however a slight trend in the isotopic data suggests the possibility of orbitally-paced changes in water mass, with more radiogenic Nd coinciding with intervals of greater carbonate accumulation.

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