Abstract. Cenozoic stable carbon (δ13C) and oxygen (δ18O)
isotope ratios of deep-sea foraminiferal calcite co-vary with the 405 kyr
eccentricity cycle, suggesting a link between orbital forcing, the climate
system, and the carbon cycle. Variations in δ18O are partly
forced by ice-volume changes that have mostly occurred since the Oligocene.
The cyclic δ13C–δ18O co-variation is found in
both ice-free and glaciated climate states, however. Consequently, there
should be a mechanism that forces the δ13C cycles
independently of ice dynamics. In search of this mechanism, we simulate the
response of several key components of the carbon cycle to orbital forcing in
the Long-term Ocean-atmosphere-Sediment CArbon cycle Reservoir model
(LOSCAR). We force the model by changing the burial of organic carbon in the
ocean with various astronomical solutions and noise and study the response
of the main carbon cycle tracers. Consistent with previous work, the
simulations reveal that low-frequency oscillations in the forcing are
preferentially amplified relative to higher frequencies. However, while
oceanic δ13C mainly varies with a 405 kyr period in the
model, the dynamics of dissolved inorganic carbon in the oceans and of
atmospheric CO2 are dominated by the 2.4 Myr cycle of eccentricity.
This implies that the total ocean and atmosphere carbon inventory is strongly
influenced by carbon cycle variability that exceeds the timescale of the
405 kyr period (such as silicate weathering). To test the applicability of
the model results, we assemble a long (∼22 Myr) δ13C and
δ18O composite record spanning the Eocene to Miocene
(34–12 Ma) and perform spectral analysis to assess the presence of the
2.4 Myr cycle. We find that, while the 2.4 Myr cycle appears to be
overshadowed by long-term changes in the composite record, it is present as
an amplitude modulator of the 405 and 100 kyr eccentricity cycles.