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Tempestite in Estonia (Silurian dolomite).

Tempestites are studied throughout sedimentary geology and paleotempestology, they are storm deposits that can be recognized throughout the rock record. The deposit gets its meaning from the word tempest which simply means a violent storm, the tempestite describes the preservation and physical representation of a violent storm event (tempest) within the rock record. Tempestites can be preserved within a multitude of sedimentological environments, including delta systems, estuarian systems, coastal environments, deep sea environments, and even fresh water lacustrine environments. Tempesites most often form in wave dominated delta systems and are preserved within the sedimentological record below fair weather wave base and above storm weather wave base.[1] They are commonly characterized by hummocky cross stratified beds that have an erosive base, and can form under combined flow regimes.[2] This erosive base is often seen in the form of gutter casts.


Tempestites had been identified in the rock record for a long time, however the exact sequence of sedimentary structures that are commonly seen in the rock record, known as the idealized sequence, wasn't described until 1979 by Dott and Bourgeois. This idealized sequence follows the order of a hummocky cross stratified layer (H) often with sole markings on the base, followed by a planar laminated layer (F) synonymous to the lower place bed, followed by a cross laminated layer (X) preserved as ripple marks in plan view, and finally topped with a muddy layer (M) which is generally interpreted to be caused by suspensions settling of finer material during the waning period of the storm. Each one of these sedimentary structures can be affected by bioturbation, when organisms living in the sediment at the time burrow through it. Bioturbation, can be a great indicator of the depth of the water column the tempestite was deposited in, in a given study area, through the use if ichnology, as certain organisms will only persist at certain depths and will generate unique markings within the sedimentary structures that can be identified. However too much bioturbation can wipe out the preservation of the sedimentary structures and essentially making the bed massive, making the confident interpretation of a tempestite much more difficult for geologists.[2] Tempestites can also amalgamate due to their erosive bases and this will cause for portions of the idealized H-F-X-M sequence to repeat, as each storm event has eroded down into the sediment that was deposited by the last, and incorporating that sediment into its own deposit.[3]

Significance and Usage[edit]

Tempestite deposits are very useful for aiding in paleoecological and paleogeographical interpretations. As storms that generate tempestite deposits can only form in between 5 degrees and 20 degrees north and south latitude (with even the largest 1000 year storm only being preserved upwards of 35 degrees latitude), accurate recognition of a tempestite deposit within the rock record allows for confident interpretation of a range of latitudes. Since hummocky cross stratification forms during the combined flow and waning oscillatory flow current regimes, the preserved amplitudes of their hummocks and swales are reflective of the storm intensity. Once it is understood where the deposit in question was deposited relative to the paleo-shoreline, which can usually be done using the ichnological data preserved in the same location, the hummock amplitudes/wavelengths, grainsize (decreases with increase in paleo water depth), and bedding thickness (decreases with increase in paleo water depth) can be used to estimate the storm intensity/energy. An understanding of the intensity of past storms has large implications for our understanding of how storm intensity might change with climate change occurring today. During the Cretaceous, CO2 levels were much higher and the global temperature was much higher. With an understanding of how storm intensity changed throughout this time period towards today, we can begin to understand how it will change with our changing climate.[4]

Tempestite deposits are also highly sought after petroleum reservoirs, as they are large laterally continuous sheet like deposits that have the potential to hold high volumes of petroleum with good permeability and porosity.


  1. ^ Paul M. Myrow (1), John B. Southard (1996). "Tempestite Deposition". SEPM Journal of Sedimentary Research. 66. doi:10.1306/d426842d-2b26-11d7-8648000102c1865d. ISSN 1527-1404.
  2. ^ a b Bourgeois, Joanne; Dott, R. H. (1982-08-01). "Hummocky stratification: Significance of its variable bedding sequences". GSA Bulletin. 93 (8): 663–680. Bibcode:1982GSAB...93..663D. doi:10.1130/0016-7606(1982)93<663:HSSOIV>2.0.CO;2. ISSN 0016-7606.
  3. ^ Long, D Gf (2007-03-01). "Tempestite frequency curves: a key to Late Ordovician and Early Silurian subsidence, sea-level change, and orbital forcing in the Anticosti foreland basin, Quebec, Canada". Canadian Journal of Earth Sciences. 44 (3): 413–431. Bibcode:2007CaJES..44..413L. doi:10.1139/e06-099. ISSN 0008-4077.
  4. ^ Li, Fengjie; Yang, Yuchuan; Li, Junwu; Yang, Chengjin; Dai, Tingyong; Zhao, Junxing; Yi, Haisheng (October 2014). "Lacustrine tempestite and its geological significance in the Cenozoic study of the Qaidam Basin". Journal of Asian Earth Sciences. 92: 157–167. Bibcode:2014JAESc..92..157L. doi:10.1016/j.jseaes.2014.06.020. ISSN 1367-9120.