In praise of a favourite fossil site: the beach from Overstrand to Cromer, north Norfolk
Stephen K Donovan (UK)
If asked what is my favourite fossil collecting site, I would have to say the Farquhar’s Beach oyster bed on the south-central coast of Jamaica. I taught at the University of the West Indies for over 12 years and this locality was an easy drive. In my retirement I doubt if I will ever see it again – too far away and too expensive a trip – but it has a special place in my heart.
Who wouldn’t be fascinated by a bed 3.3m thick preserving articulated Neogene oysters in their life position, individual specimens being up to 400mm in length (Littlewood and Donovan, 1988; Donovan and Miller, 1999)? But, in truth, we all have our favourites, where we found a prize specimen or had a spark of realisation of a thought that proved informative. I could wax lyrical on many sites such as this.
If I had to choose a favourite site in the UK at present, my vote would have to be the north Norfolk coast between Overstrand and Cromer. There are notable sites in Norfolk that roll off the tongue, such as the Trimingham chalk, Happisburgh, the Cromer forest bed and the red chalk at Hunstanton, all of which are worthy and keep producing notable specimens. Overstrand to Cromer may not sit in the pantheon of Norfolk’s greatest sites, but it is because of its relative obscurity that it appeals. Holidaymakers apart, I have little competition from other collectors. I keep finding specimens that satisfy some of my personal interests, such as erratics, Cretaceous echinoids and modern borings.
Locality
This article is adapted from chapter 47 of my book, Hands-On Palaeontology: A Practical Manual, and chapter 20 of Fossils on the Seashore: Beachcombing and Palaeontology (see also my article, On the beach: Fossils on the Seashore).
The chalk and flint cobbles on the beach at Cromer and Overstrand are likely local in origin, derived mainly from offshore. The Chalk of north Norfolk extends from the Cenomanian to the Lower Maastrichtian (Burke et al., 2010, fig. 1); the latter is unusually young for the English Cretaceous succession (Peake and Hancock, 1961). Rafts of Chalk were thrust by glacial ice during the Pleistocene and are similarly Campanian–Maastrichtian based on fossil evidence (Burke et al., 2010, pp. 621–623).
The high ground in the field area is the Cromer Ridge, an east-west structure between Holt and Trimingham (Holt-Wilson, 2011, p. 18). Its origin was complex – during Pleistocene glaciations, glaciers ‘bulldozed’ superficial deposits to form the Ridge. Rafts of Chalk were intruded into these younger deposits by glaciers; and some Chalk rafts are seen between Overstrand and Cromer. Superficial deposits are prone to landslides and cliffs may be unstable, so take care.
The beach at Overstrand is about [NGR TH 249 410]; that at Cromer, east of the pier, is about [NGR TH 227 420] (Figs. 1 and 2). Although dominantly sandy, the beach also has numerous pebbles and cobbles, the majority of which are locally derived from the Upper Cretaceous, including cobbles of flint and, less commonly, chalk. The Cromer Museum is worth a visit, with a fine display of local geology and fossils.


Figured specimens are deposited in various museums except where not collected (see captions to Figs. 3-12). Museum prefixes are: Naturalis Biodiversity Center (sic), Leiden, the Netherlands (prefix RGM); Natuurhistorisch Museum Maastricht, the Netherlands (NHMM); and the Natural History Museum, London, UK (NHMUK).
What to look for
Or, more accurately, what I look for. This locality satisfies three of my interests: pre-Ice Age, fossiliferous erratics; Chalk fossils, particularly echinoids; and modern borings in Chalk erratics.
Pre-ice age, fossiliferous erratics (Fig. 3)
Glacial and fluvial erratics from this beach are mainly lithics (see The Northfolk Project: Erratics and stones on the beach). Fossiliferous erratics are rare, but include a crinoid columnal in a Derbyshire screwstone, RGM 544 455 (Donovan, 2010), and vertical burrows of possible Mississippian age (Donovan, 2011b, fig. 3).
RGM 544 455 (Fig. 3) is a chert pebble of unique morphology for this area, with moulds preserving the shapes of embedded crinoid fossils, assigned tentatively to Megistocrinus? globosus? (Phillips) and typically Palaeozoic. The only British Palaeozoic cherts rich in mouldic crinoid debris are Derbyshire screwstones (Mississippian).

Thus,I presume that RGM 544 455 originated from the White Peak of Derbyshire. At least three Neogene formations in the Overstrand area are each known to contain a small proportion of clasts of Carboniferous cherts (Green and McGregor, 1990; Rose et al., 2001; Moorlock et al., 2002): the Wroxham Crag Formation; the Overstrand Formation; and the Holkham Till Member of the Holderness Formation.
Chalk fossils, particularly echinoids (Figs. 4C, D, 5C, D and 6-10)
Chalk is exposed offshore on the sea bed and as glaciotectonic rafts emplaced in the cliffs (see above). The beach is sandy, with many flint clasts and rather fewer cobbles of chalk. Fossiliferous clasts of the Cretaceous, both chalk and flints, include sponges (Donovan, 2022b; Figs. 4A, B, and 7 herein), belemnites (Donovan and Lewis, 2010; Figs. 4A, B, 8 and 9 herein) and echinoderms (such as Donovan, 2012, 2013; Figs. 4C, D. 5C, D, 6 and 10 herein).

Other echinoid species are few and rare (Donovan, 2012; Figs. 4C, D and 6 right). The diversity of Chalk echinoids is low. For example, until recently, I had never found a Micraster (Donovan, 2022a; Fig. 6 right herein) between Overstrand and Cromer. Echinocorys is not common, but is the most often encountered of the Chalk echinoids (Donovan, 2012; Figs. 5C, D, 6 left and 10), preserved as calcitic tests, and flint steinkerns (= internal moulds) and external moulds.Most likely, the large size and robust tests of Echinocorys make it more obvious,and is more likely to be preserved of the Chalk echinoids.

Flint is particularly common on this beach. Chalk is a white, fine-grained limestone with relatively minor occurrences of flint (= chert), a secondary deposit. The relative proportions of these rock types are reversed where they are reworked as beach clasts. Between Cromer and Overstrand, clasts are dominantly flint, and chalk is a minor component of the beach load. This is because flint is harder and more durable than chalk. Chalk clasts are ground down by flint in the coastal zone (Donovan, 2021b).

Sponges, many originally siliceous, are common in flint cobbles. A typical example is preserved as a well-rounded, elongate flint clast (Fig. 7). The sponge was possibly vase-shaped and likely oriented parallel to the long axis of the clast, whose shape it may have influenced during corrasion (that is, corrosion+abrasion). On one side of the sponge is a planispiral shell (Fig. 7), probably a serpulid worm (Proliserpula ampullaceal (J. de C. Sowerby); see Jäger, 2012).

A second specimen in flint is an incomplete belemnite rostrum preserved as an external mould, tapering towards a distal point (NHMM 2020 029; Fig. 8, right).The longitudinal section is off-centre. The rostrum is intensely bored close to the surface, with borings coarsely cast in flint. Borings are slender, straight to curved and apparently unbranched, but cross-cutting. Belemnites in flint are commonly incomplete, but are nonetheless easily identified as such. Although imperfect, the belemnites in Fig .8 (left) and 9 are likely Belemnitella sp.

Modern borings in Chalk erratics (Figs. 4A, B, 5, 11 and 12)
The three common borings found at this site are allochthonous, all marine and derived from offshore. They are similar to those that occur widely around the North Sea coast of England (Donovan et al., 2019; Donovan and Harper, 2025).


Caulostrepsis (Fig. 11) is a U-shaped boring, long and slender, with a central vane. It is produced by spionid polychaete worms of the genus Polydora (Bromley, 2004, p. 460). These borings have a figure-of-eight to slot shape in section. Gregarious accumulations commonly have borings of a similar size; solitary Caulostrepsis may be larger and inhabit oyster valves rather than lithic clasts (Donovan, 2017).

Entobia (Figs. 4A, B and 5C) is the product of boring sponges, principally members of the family Clionaidae. Differences in the style of preservation and changes to sponge colonies as they grow to maturity can radically change the form (Bromley and d’Alessandro, 1984). Surfaces are initially perforated by numerous apertures; shallow corrasion reveals the intricate three-dimensional structure of the sponge borings (Figs. 4A, B and 5C).
Gastrochaenolites (Figs. 5A, B, D, 11 and 12) is large and may be several centimetres in length. The boring is club-shaped. Most Gastrochaenolites are the spoor of endolithic bivalves (Kelly and Bromley, 1984). The club-shape is most clearly seen if a complete boring is cast in, for example, latex (Fig. 5B).

References
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