www.orbitalscale.com (also orbitalscale.net)
INTRODUCTION
The Orbital Scale of glacio-eustasy is constructed with stratons – chronostratigraphic units that are tuned by the long-eccentricity 405,000-year orbital cycle (0.405 Myr E-Cycle) (Figure 1, Matthews and Frohlich, 2002; Matthews and Al-Husseini. 2010), and referred to g2-g5 in the astronomical model of the Solar System (Laskar et al., 2004; Laskar, 2020). The E-cycle represents continuous changes of the Earth’s orbit around the Sun from nearly circular to elliptical, which are caused by the gravitational tug-of-war between Venus (g2) and Jupiter (g5) over the Earth’s position relative to the Sun.
Stratons have an average duration of c. 0.4 Myr and represent climate and glacio-eustatic cycles that correspond to transgressive-regressive (T-R) depositional sequences. Candidate stratons are interpreted throughout the Phanerozoic, and are generally referred to fourth-order sequences (e.g., Haq, 2014, 2018; Haq and Schutter, 2008; Simmons, 2020). Many candidate stratons are also referred to as high-frequency sequences or cycles, medium- or small-scale sequences or cycles, cycles or cycle sets, parasequences or parasequence sets, etc. In cases where these units are calibrated by empirical geologic time scales and have an average duration of c. 0.4 Myr they are most likely stratons. To avoid ambiguity resulting from the various synonyms for these sequences, the c. 0.4 Myr time-rock unit was named the “straton” (Matthews and Al-Husseini, 2010).
E-Cycles are numbered between the maxima of the 0.405 Myr sinusoidal component of the Fourier representation of eccentricity (Laskar et al., 2004; Laskar, 2020). Base/start Cycle E1 occurred at 192,125 years before present (Figure 1); base/start Cycle E2 at 0.0192125 + 0.405 Ma (million years before present), and base/start Cycle EN = .0192125 + N x 0.405 Ma (Hinnov, 2018). The 0.405 Myr E-Cycle is resolved by cyclostratigraphic analyses of rhythmic stratigraphic series and used to calibrate biozones and stages in the Astronomical Time Scale (ATS, e.g., Hinnov, 2018; Huang, 2018). It is referred to as the tuning fork or astronomical metronome of stratigraphy (Hinnov, 2018; Laskar, 2020).
Stratons are numbered as integers between the minima of eccentricity with base/start of Straton 1 calibrated at 371,000 years before present (Figure 1); base/start of Straton 2 is 0.371 + 0.405 Ma, and base/start Straton N is 0.371 + (N-1) × 0.405 Ma (Figure 2). The base/start of any straton differs by 23,625 years from the mid-point of an E-Cycle. For example base/start of Straton 1 at 0.371 Ma differs by 0.023625 Myr from the mid-point of E-Cycle 1 at 0.394625. Most chronostratigraphic calibrations carry uncertainties of ± 0.1 to ± 1.0 Myr that far exceed the difference of c. 0.02 Myr between mid-point E-cycles and base stratons.
Correlating an individual straton calibrated in astronomical time to a candidate fourth-order sequence dated in a biozone or stage is difficult because the latter are rarely dated to the numerical age resolution of a straton by radiometric and cyclostratigraphic techniques. This problem was addressed by considering how eccentricity variations cause groups of stratons to form T-R sequences that may be recognized as million-scale third-order sequences.
The first six Fourier terms of the eccentricity equation (Laskar et al., 2004) beat at periods of c. 0.1, 0.4 and 2.4 Myr (see Figs. 7 and 8 in Matthews and Frohlich, 2002). These beats produce sequences that are still too short to establish accurate correlations to sequences that are dated with accuracies that can be incorrect by several million years.
To extend the search for sequence architectures with much longer durations the periods of all 20 Fourier terms of the eccentricity equation (Laskar et al., 2004; see Table 1 in Matthews and Al-Husseini. 2010) were slightly rounded-off resulting in a tuned eccentricity that beats at 14.58 Myr, and contains 36 cycles of 0.405 Myr. The tuned eccentricity has a similar shape and magnitude to the unturned version, but its advantage is it repeats every 14.58 Myr and can be used in any Phanerozoic interval (see Fig. 5 in Matthews and Al-Husseini, 2010).
The time interval of 14.58 Myr defines an Orbiton (36 sets of stratons) bounded by significant lowstands. Orbiton 1 is predicted between sequence boundary SB 1 at 16.166 Ma and SB 0 (zero) at 1.586 Ma (Figure 2). Sequence boundaries represent the start of post-glacial sea-level rises (transgression). The interval between SB 1 at 1.586 Ma and SB 37 at 541.046 Ma consists of 37 orbitons, and the ages of SBs can be estimated by the arithmetical formula:
SB N = 1.586 + (N × 14.58) Ma
Orbitons contain three 4.86 Myr stratigraphic units named “dozons” consisting of sets of 12 stratons (named A, B and C in ascending order) that are also bounded by major lowstands (Figure 2). The 12 stratons in a dozon are named in ascending order as A-1 to A-12, B-1 to B-12, and C-1 to C-12. Stratons A-12, B-12 and C-12 typically consist of major lowstands and are capped by SBs.
The magnitudes of sea-level fluctuations and grouping patterns of stratons in third-order sequences vary significantly depending on prevailing conditions on Earth (e.g., continent-ocean configuration, ocean and atmospheric circulation, size of ice-prone polar continents, level of greenhouse gases, etc.). Similarly the types of glacial scenarios can range from stable ice caps with sea-level fluctuations of 10–20 m, to mid-size ice caps with very pronounced lowstands and sea-level changes of 40–50 m. Ice caps can be stuck for a long time and eventually transition to minimum ice caps (Matthews and Al-Husseini, 2010; Ruebsam and Al-Husseini, 2021).
The orbital scale predicts each straton may have a unique sea-level magnitude such that stratigraphic discontinuities can occur between any two stratons, or a group of several stratons. The most prominent discontinuities (stratigraphic unconformity) are most likely to occur between Stratons 5 and 6, 8 and 9, and 11 and 12; several unconformities may also occur within Stratons 6 and 12. The positions of prominent discontinuities imply dozons consist of a lower c. 2.03 Myr third-order sequence (from base-up Stratons 1 to 5), and an upper third-order c. 2.83 Myr sequence (Stratons 6 to 12) (Figure 2).
The orbital scale predicts the main flooding surface/interval (MFS, MFI) occurs in Straton 2 in the lower 2.03 Myr T-R sequence of a dozon. The sequence architecture of the upper 2.83 Myr T-R sequence is more complicated and will depend on the choice of parameters. Typically it will consist of a 1.21 Myr T-R sequence (Stratons 6 to 8) with an MFS in Stratons 7 or 8, and a 1.62 Myr T-R sequence (Stratons 9 to 12) with an MFS in upper Stratons 9 or 10.
Al-Husseini, M.I., Ruebsam, W. 2020. Interpreting Phanerozoic δ13C patterns as periodic glacio-eustatic sequences. In: Montenari, M. (Ed.), Stratigraphy and Timescales. Vol. 5. Elsevier, p. 42–105.
Haq, B.U., 2014. Cretaceous eustasy revisited. Global Planetary Change, v. 113, p. 44–58.
Haq, B.U., 2018. Jurassic sea level variations: a reappraisal. GSA Today (Geol. Soc.) v. 28, p. 4–10.
Haq, B.U., Schutter, S.R., 2008. A chronology of Paleozoic Sea-level changes. Science, v. 322, p. 64–68.
Hinnov, L., 2018. Cyclostratigraphy and astrochronology in 2018. In: Montenari, M. (Ed.), Stratigraphy and Timescales, vol. 3. Elsevier, p. 4–80.
Huang, C., 2018. Astronomical Time Scale for the Mesozoic. In: Montenari, M. (Ed.), Stratigraphy and Timescales. Vol. 3. Elsevier, p. 81–150.
Laskar, J., 2020. Chapter 4. Astrochronology. In: Gradstein, F.M., Ogg, J.G., Schmity, M.D., Ogg, G.M. (Eds.), Geological Time Scale 2020, Elsevier, p. 130–158.
Laskar, J., P. Robutal, F. Joutel, M. Gastineau, A. Correia Levrard, B., 2004. A long term numerical solution for the insolation quantities of the Earth. Astronomy and Astrophysics, v. 428, p. 261–285.
Matthews, R.K., Frohlich, C., 2002. Maximum flooding surface and sequence boundaries: Comparisons between observation and orbital forcing in the Cretaceous and Jurassic (65-190 Ma). GeoArabia, v. 7, no. 3, p. 503–538.
Matthews, R.K., Al-Husseini, M.I., 2010. Orbital-forcing glacio-eustasy: A sequence-stratigraphic time scale. GeoArabia, v. 15, no. 3, p. 155–167.
Ruebsam, W., Al-Husseini, M.I., 2021. Orbitally synchronized late Pliensbachian–early Toarcian glacio-eustatic and carbon-isotope cycles. Palaeogeography, Palaeoclimatology, Palaeoecology, v. 577.
Simmons, M.D., 2020. Chapter 13. Phanerozoic Eustasy. In: Gradstein, F.M., Ogg, J.G., Schmity, M.D., Ogg, G.M. (Eds.), Geological Time Scale 2020, Elsevier, p. 357–400.
For further information please contact:
Dr. Moujahed Al-Husseini
Website managed and designed by Arnold Egdane
Copyright © Moujahed Al-Husseini 2020. All Rights Reserved.