Skip to main content
National Science Review logoLink to National Science Review
. 2021 Apr 12;8(6):nwab063. doi: 10.1093/nsr/nwab063

High-precision geochronological constraints on the duration of ‘Dinosaur Pompeii’ and the Yixian Formation

Yuting Zhong 1,2, Magdalena H Huyskens 3, Qing-Zhu Yin 4,, Yaqiong Wang 5, Qiang Ma 6,7, Yi-Gang Xu 8,9,
PMCID: PMC8288181  PMID: 34691675

SUMMARY

High-precision U-Pb zircon ages of 125.755 ± 0.061 Ma and 124.122 ± 0.048 Ma, respectively, represent the onset and termination of Yixian Formation in the Jin-Yang basin, bracketing its duration to 1.633 ± 0.078 Myr.


The Early Cretaceous Jehol Biota, renowned for its exceptionally well-preserved volcanic-influenced ecosystem, was buried in lacustrine and occasionally fluvial sediments. This includes, notably, the Huajiying, Yixian and Jiufotang Formations in northern Hebei and western Liaoning and equivalent ash-interbedding sediments in neighboring areas [1–3] (Fig. 1). It harbors many evolutionarily significant taxonomies, e.g. feathered dinosaurs, early birds, mammals and flowering plants, representing one of the most diversified terrestrial biotas of the Mesozoic [1,2,4].

Figure 1.

Figure 1.

(A) The schematic geological map of western Liaoning Province (modified from Wang et al. [3]) with the sampling locations. (B) Early Cretaceous stratigraphic columns in northern Hebei and western Liaoning. Three formations, in italics, namely Huajiying, Yixian and Jiufotang Formations, are the main hosts of the Jehol Biota. (C) Composite stratigraphic column (modified from Zhou et al. [4]) and the sampling horizons of the Yixian Formation. (D) A summary plot comparing literature age data (Supplementary Table S1) with our new U-Pb CA-ID-IRMS results for the Yixian Formation. The 40Ar/39Ar dates are corrected using the decay constant of Renne et al. [9] and all reported uncertainties are in 2σ. Red circles denote U-Pb ages obtained in this study, with the full systematic uncertainties (uncertainty Z) for comparison with 40Ar/39Ar dates. (E) Ranked-age plots for single zircon U-Pb analyses for CY18–20, CY17–17, CY17–18 and CY17–9.

The evolutionary radiation of the Jehol Biota can be broadly divided into three phases [5], with the first phase limited to a small area in northern Hebei (Huajiying Formation), the second phase expanding to western Liaoning (Yixian Formation), marking the greatest diversification, and the third phase (Jiufotang Formation) representing the widest distribution. Accordingly, it is crucial to precisely determine the timing and duration of the Yixian Formation. Despite considerable efforts in the past two decades attempting to achieve this goal, the published results (Fig. 1D) are confusing and inadequate. (i) Despite its lowermost stratigraphic locations [3], the existing ages of the Lujiatun Unit (LJT Unit) are younger than those of the immediate overlying Lower Lava Unit. The ages of the upper Yixian Formation are younger than the overlying Jiufotang Formation. It therefore casts serious doubt on the robustness of these dating results. (ii) Although most of the published ages of the Yixian Formation, with the exception of those for the LJT Unit, define an overall decrease in age following the stratigraphic column from bottom to top, the ages within individual units do not always show a consistency in stratigraphically upward deceasing trend. These problems may stem either from inaccurate stratigraphic information of some dated samples, or from inconsistency of inter-laboratory analyses, between different dating methods (i.e. 40Ar/39Ar and U-Pb dating by either laser ablation or secondary ion probe), and relatively large analytical uncertainties, which are inadequate for the purpose of establishing a chronostratigraphic framework. We therefore use a U-Pb chemical abrasion-isotope dilution-isotope ratio mass spectrometry (CA-ID-IRMS) dating technique with a typical analytical precision <0.05% to date single zircons from volcanic tuff layers collected from the top (CY18–20), middle (CY17–17) and bottom (CY17–18 and CY17–9) of the Yixian Formation in the Jin-Yang basin (Fig. 1C), in order to tightly constrain its absolute age and duration.

The new CA-ID-IRMS ages show significant improvement in analytical precision compared with literature data (Fig 1D and E). Our new ages collectively provide very tight constraints on the onset at 125.755 ± 0.061 Ma (CY17–9) and termination at 124.122 ± 0.048 Ma (CY18–20) of the Yixian Formation, respectively, bracketing its duration to 1.633 ± 0.078 Myr. It is significantly shorter than the previous broad range estimates of ∼2–7 Myr [6]. The fossil preservation in the LJT Unit is often referred to as the ‘Chinese Pompeii’ for dinosaurs and other fossils, due to rapidly deposited catastrophic pyroclastic flows [7]. Our new age constraints with the extraordinarily short duration of the LJT Unit (<71 ± 86 Kyr) support the sudden nature of the deposition event(s) that preserved fossils in three-dimensional structures with gestures.

Some argue that the Jianshangou (JSG) and LJT Units are stratigraphically equivalent primarily based on prior chronological data [8]. However, the two units show considerably different petrographic facies, mineralogical characteristics and geochemical compositions (Supplementary Texts 1 and 2), suggesting that the two units represent separate depositional events. The difference in the two units is further confirmed by the younger age of CY17–17 from the JSG Unit than that of the LJT Unit. The ages of the LJT and JSG Units are resolvable given the extraordinary precision achieved in this study, with the JSG Unit being sequentially deposited later than the LJT Unit, in agreement with their stratigraphic relationship observed in the field and cores [3].

The refined duration of the Yixian Formation also yields important insights on the duration of the JSG lacustrine deposits. The sedimentary cyclicity was interpreted as periodic lake-level fluctuations plausibly caused by climatic changes that in turn may be orbitally forced Milankovitch cycles [3,10]. If so, our study effectively rules out the lacustrine cyclostratigraphy documented in part of the Yixian Formation being driven by orbital eccentricity, but more likely obliquity or precession signals. Our new data indicate that the entire Yixian Formation is only 1.633 ± 0.078 Myr maximum, which means that the JSG Unit within the Yixian Formation should be <1.633 Myr. This would clearly exclude the possibility of interpreting the 2 m cycle as a 100 Kyr eccentricity cycle for a 41 m JSG Unit. It is possible that the sedimentation rates of lacustrine environments between the studied outcrops and drill cores are highly variable, and obtaining accurate Milankovitch cycle signals from the terrestrial sediments remains a challenging goal without further high-resolution geochronological constraints.

Supplementary Material

nwab063_Supplemental_File

Contributor Information

Yuting Zhong, State Key Laboratory of Isotope Geochemistry, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, China; CAS Center for Excellence in Deep Earth Science, China.

Magdalena H Huyskens, Department of Earth and Planetary Sciences, University of California at Davis, USA.

Qing-Zhu Yin, Department of Earth and Planetary Sciences, University of California at Davis, USA.

Yaqiong Wang, State Key Laboratory of Palaeobiology and Stratigraphy, Nanjing Institute of Geology and Palaeontology and Center for Excellence in Life and Paleoenvironment, Chinese Academy of Sciences, China.

Qiang Ma, State Key Laboratory of Isotope Geochemistry, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, China; State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences, China University of Geosciences, China.

Yi-Gang Xu, State Key Laboratory of Isotope Geochemistry, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, China; CAS Center for Excellence in Deep Earth Science, China.

FUNDING

This work was supported by the National Natural Science Foundation of China (41688103 and 41873018) and the Strategic Priority Research Program (B) of the Chinese Academy of Sciences (XDB18000000). This is contribution No. IS-3022 from GIGCAS.

Conflict of interest statement. None declared.

REFERENCES

  • 1. Zhou ZH. Natl Sci Rev 2014; 1: 543–59. 10.1093/nsr/nwu055 [DOI] [Google Scholar]
  • 2. Pan YH, Sha JG, Zhou ZHet al. Cretac Res 2013; 44: 30–8. 10.1016/j.cretres.2013.03.007 [DOI] [Google Scholar]
  • 3. Wang YQ, Olsen PE, Sha JGet al. Palaeogeogr Palaeoclimatol Palaeoecol 2016; 464: 110–33. 10.1016/j.palaeo.2016.06.043 [DOI] [Google Scholar]
  • 4. Zhou ZH, Barrett PM, Hilton J. Nature 2003; 421: 807–14. 10.1038/nature01420 [DOI] [PubMed] [Google Scholar]
  • 5. Zhou ZH, Wang Y, Xu Xet al. The Jehol Biota: an exceptional window into Early Cretaceous terrestrial ecosystems. In: Nicholas F (ed.). Terrestrial Conservation Lagerstätten: Windows into the Evolution of Life on Land. Edinburgh: Dunedin Academic Press, 2017, 169–214. [Google Scholar]
  • 6. Chang SC, Zhang HC, Renne PRet al. Palaeogeogr Palaeoclimatol Palaeoecol 2009; 280: 94–104. 10.1016/j.palaeo.2009.06.021 [DOI] [Google Scholar]
  • 7. Jiang BY, Harlow GE, Wohletz Ket al. Nat Commun 2014; 5: 3151. 10.1038/ncomms4151 [DOI] [PubMed] [Google Scholar]
  • 8. Chang SC, Gao KQ, Zhou CFet al. Palaeogeogr Palaeoclimatol Palaeoecol 2017; 487: 399–406. 10.1016/j.palaeo.2017.09.026 [DOI] [Google Scholar]
  • 9. Renne PR, Mundil R, Balco Get al. Geochim Cosmochim Acta 2010; 74: 5349–67. 10.1016/j.gca.2010.06.017 [DOI] [Google Scholar]
  • 10. Wu HC, Zhang SH, Jiang GQet al. Palaeogeogr Palaeoclimatol Palaeoecol 2013; 385: 221–8. 10.1016/j.palaeo.2013.05.017 [DOI] [Google Scholar]

Associated Data

This section collects any data citations, data availability statements, or supplementary materials included in this article.

Supplementary Materials

nwab063_Supplemental_File

Articles from National Science Review are provided here courtesy of Oxford University Press

RESOURCES