| one publication added to basket [259018] | Eccentricity and obliquity paced carbon cycling in the Early Triassic and implications for post-extinction ecosystem recovery
Fu, W.; Jiang, D.-y.; Montañez, I.P.; Meyers, S.R.; Motani, R.; Tintori, A. (2016). Eccentricity and obliquity paced carbon cycling in the Early Triassic and implications for post-extinction ecosystem recovery. NPG Scientific Reports 6(27793): 7 pp. http://dx.doi.org/10.1038/srep27793
In: Scientific Reports (Nature Publishing Group). Nature Publishing Group: London. ISSN 2045-2322; e-ISSN 2045-2322, more
|   |
| Authors | | Top |
- Fu, W.
- Jiang, D.-y.
- Montañez, I.P.
|
- Meyers, S.R.
- Motani, R.
- Tintori, A.
|
|
| Abstract |
The timing of marine ecosystem recovery following the End Permian Mass Extinction (EPME) remains poorly constrained given the lack of radiometric ages. Here we develop a high-resolution carbonate carbon isotope (d13Ccarb) record for 3.20 million years of the Olenekian in South China that defines the astronomical time-scale for the critical interval of major evolutionary and oceanic events in the Spathian. d13Ccarb documents eccentricity modulation of carbon cycling through the period and a strong obliquity signal. A shift in phasing between short and long eccentricity modulation, and amplification of obliquity, is nearly coincident with a 2% decrease in seawater d13CDIC, the last of a longer-term stepped decrease through the Spathian. The mid-Spathian shift in seawater d13CDIC to typical thermocline values is interpreted to record a major oceanic reorganization with global climate amelioration. Coincidence of the phasing shift with the first occurrence of marine reptiles (248.81 Ma), suggests that their invasion into the sea and the onset of a complex ecosystem were facilitated by restoration of deep ocean ventilation linked mechanistically to a change in the response of the oceanic carbon reservoir to astronomical forcing. Together these records place the first constraints on the duration of the post-extinction recovery to 3.35 myr. |
|
