Huddart, D. & Glasser, N.F. 2007. Quaternary of Northern England. Geological Conservation Review Series No. 25, JNCC, Peterborough, ISBN 1 86107 490 5. The original source material for these web pages has been made available by the JNCC under the Open Government Licence 3.0. Full details in the JNCC Open Data Policy
Old Mere, Hornsea
N.F. Glasser
Introduction
Old Mere, Hornsea, in the East Riding of Yorkshire, is an important site for the study of both local and regional vegetation history and environmental change in the Holderness area during the Holocene Epoch. The importance of the site is twofold. Firstly, palynological analyses of cores obtained from the site have been used in compilation of a regional pollen stratigraphy for Holderness (Beckett, 1981). Secondly, comparisons between Old Mere, Hornsea and the much smaller nearby kettlehole at The Bog, Roos have been used to demonstrate the importance of local factors in pollen deposition and preservation. The main published work on this site is that of Beckett (1975, 1981), who obtained radiocarbon-dated cores from Old Mere, Hornsea and from The Bog, Roos (Beckett, 1977b). The differences in the pollen records from the two sites reflect the much stronger local influences on pollen deposition at Old Mere, Hornsea. This is primarily the result of a greater input from local streams into the lake because of the larger size of the catchment at Old Mere. The site also features in many reviews of the regional palaeoenvironmental history of this area of Holderness (Gilbertson, 1984a; Flenley 1984, 1987, 1990; Catt, 1991b; Van de Noort and Davies, 1993; Dinnin, 1995; Dinnin and Lillie, 1995b; Taylor, 1995; Greig, 1996; Lillie and Geary, 1999).
Description
Old Mere, Hornsea lies on the Holderness coast, immediately south of the town of Hornsea. The entire Holderness Plain is composed of glaciogenic sediments, including a variable thickness of diamicton, sand and gravel. Organic deposits and place names provide evidence that numerous former shallow lakes (meres) existed in Late-glacial and post-glacial times, especially in eastern Holderness. Their disappearance was largely the result of natural silting aided by medieval and later drainage (Sheppard, 1957). The only surviving open-water mere is that of Hornsea Mere. The GCR site at Old Mere, Hornsea is a dry depression of landscaped ground at c. 1 m OD, protected from the North Sea by a sea wall. The site occupies the eastern end of a pre-glacial valley, which extends westwards to Brandes-burton and includes the surviving Hornsea Mere, which is immediately inland of Old Mere itself
A transect of borings reported by Beckett (1981) revealed up to 14 m depth of lacustrine deposits in the Old Mere basin, comprising mainly clay and fine detritus mud
The upper 9.5 m of a core obtained by Beckett (1981) yielded sufficient pollen for palynological analysis and radiocarbon dating
HO-1 (9.45–8.95 m)
The pollen spectra are dominated by Betula (40–70%), Pinus (10%) and Gramineae (5–10%). Quercus, Ulmus and Alnus also occur in small amounts towards the top of this zone. Salix pollen is abundant at the base of this zone, but decreases upwards. The pollen of certain herbs, notably Filipendula, is present.
HO-2 (8.95–7.55 m)
The lower boundary of this zone is drawn where Corylus/Myrica pollen shows a sharp increase and Betula declines. Ulmus and Quercus also increase at the base of this zone. Corylus/Myrica pollen dominates, with values from 70% at the base to 40% at the top of this zone. Betula, Pinus, Ulmus and Quercus all contribute around 5–10%. Tilia cordata and Alnus pollen are present in small amounts. Very few herbs are present, apart from Gramineae and Cyperaceae pollen.
Depth in core (cm) | Description |
0.00–0.50 | Made ground |
0.50–1.40 | Sandy clay |
1.40–1.75 | Clayey detritus mud with organic matter |
1.75–9.30 | Fine detritus mud with no recognizable plant material |
9.30–12.30 | Silty clay with occasional organic matter |
12.30–12.60 | Clayey fine detritus mus with some silt |
12.60–13.80 | Gravelly clay |
HO-3 (7.55–4.40 m)
The base of this zone is marked by an increase in Alnus pollen to exceed 20%. Alnus contributes about 30% throughout the zone. Of the other trees, Betula and Pinus both decline from about 10% at the base to 2 or 3% at the top of the zone. Ulmus pollen values (5–10%) are also slightly higher at the base. Quercus, at 5–10% for much of this zone, increases to 15–20% near the top. Tilia cordata pollen values increase from minimal amounts to around 5% higher in this zone, and Fraxinus is sparsely present in the upper horizons. Corylus/Myrica pollen contributes 40%, decreasing to 20% at the top of the zone. Hedera pollen is consistently present in small amounts, whereas herb pollen is scarce.
HO-4 (4.40–2.55 m)
The lower boundary of this zone is drawn where Ulmus pollen values fall below 5%. Alnus (40%) and Quercus (10–20%) dominate the arboreal pollen, with Pinus and Ulmus present in small amounts. Betula pollen values lie around 5%. Tilia cordata pollen drops to around 2% near the base of the zone, but exceeds 5% at higher levels. Fraxinus is present in small amounts only in the lower half of this zone. Corylus/Myrica pollen values are consistently at 25–35%. At the base of the zone there is a slight increase in herb pollen values, notably of Gramineae; Plantago lanceolata, Rumex acetosa and Artemisia also occur. The increase in herb pollen is not maintained in the higher levels of the zone.
HO-5 (2.55–1.55 m)
The base of this zone is marked by a rise in the values of herbs, especially Gramineae and Plantago lanceolata, and a decline in Tilia cordata. Alnus (20–40%) and Quercus (5–20%) dominate the arboreal pollen, with small amounts of Betula, Pinus, Ulmus, Tilia cordata and Fraxinus. Corylus/Myrica pollen values decline from 30% to 5% through this zone. Herb pollen increases throughout the zone to reach 50% of the total dry-land pollen at the top of the profile. There also are significant amounts of pollen of Cerealia type (Cyperaceae, Artemisia, Liguliflorae and Chenopodiaceae) and a range of other herb pollen taxa in small quantities.
Interpretation
The stratigraphical evidence suggests that changes within the Old Mere throughout much of the Late Devensian and Holocene were only minor (Beckett, 1981). The Late-Glacial clay deposits and fine detritus mud that fills much of the basin are indicative of deposition in open water conditions. The absence of pollen of submerged and floating-leaved macrophytes from much of pollen zones HO-2 and HO-3 suggests that the throughflow of water was too rapid to allow the establishment of much aquatic vegetation and/or that the water depth was considerable. On the assumption that the raised shore lines of Hornsea Mere represent the water depth in zone HO-3, this suggests a water depth of around 7.5 m (Beckett, 1981). The increase in aquatic pollen during pollen zones HO-4 and HO-5 points to a shallowing of the water or reduction in stream flow. The uppermost deposits suggest that the mere may have dried out rapidly, with no time for a regular hydroseral sequence, as in the kettlehole at The Bog, Roos. The upper horizons of detritus mud contain successively more inwashed clay, perhaps representing human activity. These are overlain by deposits of sand, interpreted as blown sand from the coastal dune systems. Beckett (1981) suggests that the mere dried up sometime around 2000 years BP. The presence of freshwater ostracods in the clayey upper horizons of the Old Mere demonstrates that the site was not inundated by the sea for any length of time (Robinson, 1972).
Beckett (1981) proposed five regional pollen assemblage zones for the Plain of Holderness based on the palynological analyses from Old Mere, Hornsea and The Bog, Roos. These follow the local pollen zones described above.
HO-1 Betula–Pinus assemblage zone
This zone is dominated by arboreal pollen, notably Betula with some Pinus. A range of herb types, notably Filipendula, also is present. Radiocarbon dating places this assemblage zone in the early Holocene, immediately above the Late Devensian–Holocene boundary.
HO-2 Corylus/Myrica–Ulmus assemblage zone
This zone is dominated by Corylus/Myrica pollen, with plentiful pollen of Betula, Pinus, Ulmus and Quercus and little herb pollen. A radiocarbon date of 8507 ± 55 years BP was obtained for this pollen zone (Beckett, 1975).
HO-3 Alnus–Ulmus assemblage zone
This zone is dominated by arboreal pollen, chiefly Alnus, but also with abundant Ulmus and Quercus and some Corylus/Myrica pollen. Herb pollen is scarce. This zone is bracketed by radiocarbon dates of 8507 ± 55 years BP from the top of HO-2 and a date of 5099 ± 50 years BP
HO-4 Alnus–Quercus assemblage zone
This zone is dominated by arboreal pollen including Alnus and Quercus. Ulmus pollen is scarce. Small amounts of herb pollen occur, notably Gramineae, Plantago lanceolata and Chenopodiaceae. The base of this zone is dated to 5099 ± 50 years BP (Beckett, 1975).
HO-5 Alnus–Gramineae assemblage zone
This zone contains abundant herb pollen. Alnus dominates the arboreal pollen, with smaller amounts of Betula and Quercus. Many herb pollen types are present, notably Gramineae, Plantago lanceolata, and Cerealia type. Dates for the start and end of this zone are unclear, but radiocarbon dates indicate that this pollen zone includes the time spanning 3120 ± 105 years BP to 3433 ± 110 years BP.
Conclusions
Old Mere, Hornsea has yielded a radiocarbon-dated pollen sequence from the Late Devensian–early Holocene boundary to c. 2000 years BP The pollen record from Old Mere, Hornsea is important in defining the regional pollen assemblages for Holderness, of which five regional pollen zones have been recognized. The pollen record from Old Mere is very different to that obtained from nearby at The Bog at Roos, where the pollen spectra are swamped by local pollen produced from the rapidly changing bog surface.