Palaeogeography, Palaeoclimatology, Palaeoecology
Cyclone frequency during the last 5000 years at Curacoa Island, north Queensland, Australia
Introduction
Although tropical cyclones are extreme events, they are elements of the natural climate of northern Australia. Well dated coastal sequences of cyclonic deposits can be used to assess the frequency of past cyclones and assist long term climatic prediction. Partial records of cyclone activity during the last 4000 years in northeast Queensland were reported from Curacoa Island and Princess Charlotte Bay by Chappell et al. (1983), and from Lady Eliot Island by Chivas et al. (1986). These studies did not detect any statistically significant variation of depositional events, but stratigraphic sampling and dating were not exhaustive. Others have claimed that the frequency of ridge-building events in northern Australia varied in the last 6000 years (Rhodes, 1980, Lees and Clements, 1987), but Chappell and Thom (1986) argued that the variations may have been caused by changes of sediment supply.
The present study is based on the beach-ridge and shingle spit complex at Curacoa Island in the Palm Group, Central Queensland, first described by Hopley (1968). Radiocarbon dates of coral fragments collected from shallow pits along a transect crossing the beach ridges were reported by Chappell et al. (1983); however, their pits were irregularly spaced and had too few dates to assess possible variations of ridge building events. Here, we examine two new transects in detail. Radiocarbon ages of 22 morphostratigraphic units were determined with multiple dates from each unit, and the series of dated deposits was analysed for trends or changes in frequency of depositional events.
Section snippets
Site physiography
Curacoa Island (18°40′S; 146°33′E) lies immediately north of Great Palm Island, 28 km offshore from Lucinda on the Queensland coast (Fig. 1). The island rises steeply from the sea; it is 3 km long, up to 0.8 km wide and the summit is 298 m above sea level. The long axis bears NNW. Narrow coral reefs slope away steeply from the shores, punctuated on the exposed eastern side by submerged promontories of very massive, isolated corals. To the east and southeast of the Palm Group, the Great Barrier Reef
Morphostratigraphy
Two transects across the shingle ridges were surveyed and levelled to mean sea level (MSL), which was established by recording the tide at the site and correlating to tide tables for Lucinda. Highest astronomical tide (HAT) is used here as a height datum for the shingle ridges, as Hopley and Harvey (1979) use HAT as a datum for cyclonic surges in north Queensland. Transect H1 was surveyed in July 1995 and was sampled from 32 hand-dug pits of 0.8–1.5 m depth. Transect H2 was described and sampled
Sampling and radiocarbon dating
Each storm deposit (SD) identified in a pit or trench exposure was sampled for radiocarbon dating. Fig. 3 shows sample points. Branching corals (mainly Acropora, Montipora and Pocillopora) that had well preserved corallite rims and fresh breakage surfaces were the preferred sampling material. Samples were examined for secondary infills under a dissecting microscope and were scanned by X-ray diffraction for secondary calcite. All samples used to establish the chronology reported here were clean
Storm deposit series and ages
Fig. 5 shows the sequence of SDs identified in the series of shingle ridges from transects H1 and H2. Twenty-two SDs shown in Fig. 5 were identified from the trenches on transect H2, and units observed in the pits on H1 were correlated with H2. Correlation of SDs underlying the seaward flanks and crests of major ridges was reasonably straightforward, but correlations between buried SDs were based their relationships to the surface units, as shown by buried groundsurfaces or key pumice deposits.
Geomorphologic history
The Curacoa spit has a foundation of carbonate-cemented boulder beach deposits containing scattered corals, which outcrops intertidally on the northern side of the spit, particularly towards its distal end (Fig. 2). Radiocarbon ages from cemented coral clasts show that the proto-spit formed around 6000 B.P. (Hopley, 1968). The spit has since grown higher through accretion of steep, narrow ridges of boulders and coarse coral, but the major change of the last 6000 years has been accumulation of a
Discussion and conclusions
The evidence described above shows that the rate of progradation and the frequency of SD accretion have not changed in the last 5000 years. This suggests that cyclone frequency has not varied, provided that the likelihood that cyclones produce SDs remains constant.
Deposition of a coral shingle SD requires prior development of the coral sources. If the time required for source regeneration after a cyclonic event is considerably longer than the average interval between cyclones, then variations of
Acknowledgements
This research was supported by a grant from the Australian National Greenhouse Advisory Committee (NGAC). Field site access was provided by the Palm Island Community. Ilona Horvath, Anna Chappell, Colin Campbell and Eugene Wallensky assisted the fieldwork; Steve Robertson guided MH in the radiocarbon dating laboratory. Mrs Lana Murray of the Australian Geological Survey Organisation did the cartography.
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