Factors affecting the distribution of rock-lobster larvae (Panulirus longipes cygnus), with reference to variability of plankton-net catches

One of the major problems in the quantitative study of the distribution of larvae of the western rock lobster Panulirus longipes cygnus George, is the high variability in planktonnet catches taken at night, even when replicate hauls are made at a single station. Some of the possible causes of this variability are considered. The density of early and late-stage phyllosoma larvae caught at the surface at night showed no direct relationship to either temperature or salinity. Early-stage phyllosoma larvae were equally well represented at the surface under all light conditions encountered at night. In contrast, the density of late-stage phyllosoma larvae at the surface was, on an average, four times greater on dark nights than on bright moonlight nights. The mean density for all phyllosoma stages decreased rapidly with depth, i.e., from 0.70/1000 m³ at the surface to 0.04/1000 m³ at 25 to 35 m, indicating that the vertical movements at night are not very extensive. The density of early-stage phyllosoma larvae in the surface at night showed no relationship to micronekton biomass (measured as wet weight). Density of late-stage phyllosoma larvae at the surface at night increased slightly, but significantly, with increase of micronekton biomass, possibly indicating similar behavioural responses to light or some other factor(s). The distribution of cast exuviae of final-stage phyllosoma larvae indicated that metamorphosis to the puerulus phase can occur more than 100 miles (161 km) from shore. Moreover, 80% of the puerulus larvae caught were within 80 miles (129 km) of the shore. Mean densities of puerulus larvae taken at and below the surface at night were 0.04/1000 m³ and 0.10/1000 m³, respectively, although total numbers were low. This evidence indicates that, after metamorphosis, the puerulus larvae return to the coastal environment at some subsurface depth.