O-25 HAIMEA ALTA AND HAIMEA OVUMSERPENTIS,WHAT’S THE DIFFERENCE?Deborah-Ann C. Rowe<strong>Department</strong> <strong>of</strong> Geography <strong>and</strong> Geology, Mona<strong>The</strong> oligopygoids are a group <strong>of</strong> irregular echinoidsunique to the Eocene <strong>of</strong> the Caribbean <strong>and</strong>adjacent regions. <strong>The</strong>se echinoids are the sister group to the clypeasteroids (=s<strong>and</strong> dollars), <strong>and</strong> arerepresented by a number <strong>of</strong> species in the genera Haimea Michelin <strong>and</strong> Oligopygus de Loriol. Bothgenera are locally common in the Eocene <strong>of</strong> Jamaica. <strong>The</strong> difficulty in distinguishing betweenspecies within the genus Haimea has long been documented. Two species are locally common withinthe Middle-Upper Eocene Swanswick Formation, but they cannot always easily be differentiated.Without taking measurements, the only feature that can be used to distinguish Haimea alta (Arnold<strong>and</strong> Clark) from Haimea ovumserpentis (Guppy) is the greater height <strong>of</strong> H. alta. This method issubjective <strong>and</strong> is reliable only in those cases where the test <strong>of</strong> H. alta is highly inflated, as that <strong>of</strong> H.ovumserpentis can also be inflated as well. H. alta may be so inflated as to resemble a fossilized golfball, whereas H. ovumserpentis is generally lower, more elongate <strong>and</strong> pentagonal in outline. Kier’s“Revision <strong>of</strong> the Oligopygoid Echinoids” (1967, Smithsonian Miscellaneous Contributions, vol.152, no. 2, 147 pp.) gives an outline <strong>of</strong> the morphological details which may be used to differentiatebetween the two species, including the shorter petal length <strong>and</strong> greater number <strong>of</strong> ambulacral platesbeyond the petals <strong>of</strong> H. alta. In an attempt to find other ways <strong>of</strong> telling the two species apart, 17measurements each have been made <strong>of</strong> 112 better preserved specimens <strong>of</strong> Haimea from an echinoidlocality in the Swanswick Formation at Beecher Town, in the parish <strong>of</strong> St. Ann, Jamaica. Based onthese measurements, bivariate statistical analyses were carried out in order to seek out the bestmeans <strong>of</strong> identifying each species. Using scatter diagrams <strong>and</strong> regression analysis, the parameters <strong>of</strong>test length, test height, <strong>and</strong> width <strong>and</strong> height <strong>of</strong> peristome, were found to be the most suitable to tellthe two species apartO-26 CRETACEOUS TO EOCENE EVOLUTIONOF CENTRAL JAMAICASimon Mitchell<strong>Department</strong> <strong>of</strong> Geography <strong>and</strong> Geology, Mona<strong>The</strong> Central Inlier exposes a suite <strong>of</strong> latest Cretaceous to Paleocene rocks that formed part <strong>of</strong> anextinct volcanic isl<strong>and</strong> arc system. Detailed mapping <strong>of</strong> the inlier has resulted in a new underst<strong>and</strong>ing<strong>of</strong> the geological history <strong>of</strong> Jamaica. <strong>The</strong> 1 st phase <strong>of</strong> active arc volcanism is represented by <strong>and</strong>esiticlavas, associated volcaniclastic sediments, <strong>and</strong> minor porphyritic basaltic dykes. This complex wasuplift <strong>and</strong> deeply eroded prior to the deposition <strong>of</strong> an inportant onlapping sedimentary successioncomprising the Slippery Rock <strong>and</strong> Guinea Corn formations. Sedimentary analysis <strong>of</strong> this successiondemonstrates the presence <strong>of</strong> a carbonate platform succession <strong>of</strong> restricted rudist-bearing carbonatefacies with associated shallow water clastics deposited closer to l<strong>and</strong>. Renewed volcanism in thePaleocene (with a probable hiatus at the Cretaceous-Tertiary boundary) saw extensive marine <strong>and</strong>terrestrial deposition <strong>of</strong> volcaniclastic s<strong>and</strong>stones <strong>and</strong> conglomerates which culminated in ignimbriteemplacement. This sedimentary succession was strongly deformed by tectonics in the early Eocenewith the formation <strong>of</strong> steep to vertical fold limbs associated with south-westerly verging folds <strong>and</strong>associated thrusting. After a period <strong>of</strong> renewed erosion, the deposition <strong>of</strong> the Yellow LimestoneGroup marked the first stage in the development <strong>of</strong> an extensive carbonate platform that persistedfrom Eocene to Miocene time.44
O-27 PHASE TRANSITIONS AND ORDERING PHENOMENA INAMPHIPHILICMONOLAYERS AT THE AIR/WATER INTERFACEWillem Mulder<strong>Department</strong> <strong>of</strong> <strong>Chemistry</strong>, Mona<strong>The</strong> surface activity <strong>of</strong> molecules such as lipids, proteins <strong>and</strong> fatty acids is associated with their dualcharacter; that is, one part is hydrophobic (“water-fearing”) <strong>and</strong> the other part is hydrophilic(“water-loving”). Such molecules are also called “amphiphiles”. <strong>The</strong> primary requirement for anamphiphile to be surface-active is that the balance between hydrophilic <strong>and</strong> hydrophobic parts besuch that the molecule has its lowest free energy when it is adsorbed at an interface between twoimmiscible bulk phases (water/oil or water/air). <strong>The</strong> amphiphile will then be present as amonomolecular film. Examples include the surfactant films in microemulsions, Langmuir filmsformed by spreading amphiphilic molecules on a water surface, the dense (Langmuir-Blodgett) films<strong>of</strong> chain molecules on solid supports, or the two lipid monolayers facing each other in biologicalmembranes.<strong>The</strong> most common experiment performed on Langmuir monolayers is the determination <strong>of</strong> surfacepressure vs. area isotherms using a film balance 1 . <strong>The</strong> surface pressure Π is defined as the differencebetween the surface tension γ0 <strong>of</strong> <strong>pure</strong> water <strong>and</strong> the surface tension γ<strong>of</strong> the surface covered by themonolayerΠ = γ0 − γ (1)A barrier can be slid across the water surface to change the area accessible to a fixed amount <strong>of</strong>surface-active material. <strong>The</strong> surface pressure can be measured by determining the force on a floatseparating the monolayer from a clean water surface. A typical Π-A isotherm for a <strong>pure</strong> fatty acid orphospholipid is shown in the figure, where two regions can be discerned in which different surfacephases coexist. At large areas the amphiphile behaves like a two-dimensional gas. Upon compressiona plateau is reached, marking the onset <strong>of</strong> 2D condensation <strong>of</strong> the gas into a so-called liquidexp<strong>and</strong>ed(LE) phase. At the end <strong>of</strong> the plateau the entire monolayer is in the LE phase. On furthercompression the lateral pressure again increases steeper until the start <strong>of</strong> a second transition regionwhere the LE phase condenses into a liquid-condensed (LC) phase which is associated withincreased chain ordering. At the end <strong>of</strong> the LE/LC coexistence region there is another steep increasein pressure until the collapse pressure is reached, which marks the transformation to more stablethree-dimensional (micellar) phases.<strong>The</strong> formation <strong>of</strong> LC from LE in the second coexistence region (sometimes called the “maintransition”) can be followed by fluorescence microscopy if one adds a small amount <strong>of</strong> surface activefluorescent dye which is less soluble in the LC compared to the LE phase. Alternatively, one can usethe more recently developed non-invasive technique known as Brewster angle microscopy. <strong>The</strong>micrographs obtained with both techniques reveal that the LC phase exists in the form <strong>of</strong> isolateddomains (sizes ~10µm) which, in the case <strong>of</strong> chiral amphiphiles, change their shape from circles viaellipses to stripes, spirals, triskelions, etc. <strong>The</strong>se have been established to represent equilibriumshapes <strong>and</strong> the result <strong>of</strong> a competition between lateral electrostatic repulsion between the polar (orcharged) head groups <strong>of</strong> surfactants <strong>and</strong> (anisotropic) line tension.45
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Todd G. A., Daniels M. J. and Callo
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