Ecotourism in the small island Caribbean

Ecotourism-related strategies can serve to enhance the tourism industries of small Caribbean islands, which are presently dominated by a 3S (sea, sand, sun) product. In the first place, the principles of Alternative Tourism can be applied to 3S tourism in order to minimize negative environmental impacts. Secondly, diversionary ecotourism opportunities can be promoted to diversify the tourism product, thus providing a nature-oriented alternative to resort-based tourists. Thirdly, regional ecotourism, catering to ecotourists, can be fostered in mountainous interiors, peripheral islands, undeveloped coastlines, rural agricultural areas and in offshore reefs. A fourth strategy, exemplified by Dominica, entails a comprehensive ecotourism approach for destinations in which 3S tourism is undesired or unsuited.     

Transverse geochemical variations across the Antarctic Peninsula: Implications for the genesis of calc-alkaline magmas

Magnetic activity throughout the Antarctic Peninsula and the South Shetland Islands has been dominantly of a calc-alkaline nature for the last 200 Ma. Chemically, the plutonic and volcanic products are typical of a continental margin magmatic arc, similar to those from western South America. Within any one area, volcanic and plutonic rocks are compositionally indistinguishable, and all magmatic products show increasing SiO₂, and increasing K/Si, Rb/Si, Th/Si and to a lesser extent Ce/Si and La/Si ratios away from the proposed trench axis. The calc-alkaline basaltic compositions also have high large ion lithophile (LIL; e.g. K, Rb, Th)/high field strength (HFS; e.g. Zr, Nb, Ti) ratios relative to non-orogenic counterparts, and increasing LIL/HFS element ratios with increasing fractionation. It is proposed that the high LIL/HFS element ratios in basaltic and andesitic melts are primary features due to dehydration processes with the subducted slab and to fractionation of minor mineral phases from the melt. The increasing LIL/HFS element ratios in more acid rocks are probably due to removal of minor mineral phases from the melt. Although zone refining may contribute to the spatial variations across the peninsula, we have proposed that an enriched subcontinental mantle provides a viable alternative source for the observed K-h variations and for the increased LIL-element contents found in continental margin calc-alkaline magmas.     

Constraining groundwater flow,residence times,inter-aquifer mixing,and aquifer properties using environmental isotopes in the southeast Murray Basin,Australia

Environmental isotopes (particularly δ¹⁸O, δ²H, and δ¹³C values, ⁸⁷Sr/⁸⁶Sr ratios, and a¹⁴C) constrain geochemical processes, recharge distribution and rates, and inter-aquifer mixing in the Riverine Province of the southern Murray Basin. Due to methanogenesis and the variable δ¹³C values of matrix calcite, δ¹³C values are highly variable and it is difficult to correct ¹⁴C ages using δ¹³C values alone. In catchments where δ¹³C values, ⁸⁷Sr/⁸⁶Sr ratios, and major ion geochemistry yield similar a¹⁴C corrections, ∼15% of the C is derived from the aquifer matrix in the silicate-dominated aquifers, and this value may be used to correct ages in other catchments. Most groundwater has a¹⁴C above background (∼2 pMC) implying that residence times are <30 ka. Catchments containing saline groundwater generally record older ¹⁴C ages compared to catchments that contain lower salinity groundwater, which is consistent with evapotranspiration being the major hydrogeochemical process. However, some low salinity groundwater in the west of the Riverine Province has residence times of >30 ka probably resulting from episodic recharge during infrequent high rainfall episodes. Mixing between shallower and deeper groundwater results in ¹⁴C ages being poorly correlated with distance from the basin margins in many catchments; however, groundwater flow in palaeovalleys where the deeper Calivil–Renmark Formation is coarser grained and has high hydraulic conductivities is considerably more simple with little inter-aquifer mixing. Despite the range of ages, δ¹⁸O and δ²H values of groundwater in the Riverine Province do not preserve a record of changing climate; this is probably due to the absence of extreme climatic variations, such as glaciations, and the fact that the area is not significantly impacted by monsoonal systems.     

Distinguishing groundwater flow paths in different fractured-rock aquifers using groundwater chemistry: Dandenong Ranges, southeast Australia

Major ion geochemistry is used to qualitatively interpret groundwater residence times within an aquifer, and the extent of mixing between aquifers with distinctive mineralogy. In conjunction with hydraulic heads and stable isotope geochemistry, flow paths and inter-aquifer exchange are defined in a fractured-rock aquifer system in the Dandenong Ranges, southeast Australia. Stable isotopes indicate modern seasonal recharge throughout the system. At high elevations in the sub-catchment, which includes both marine Silurian-Devonian sedimentary and Tertiary basalt aquifers, Cl is derived primarily from cyclic salts, and differences in mineralogy result in groundwater from the basalt aquifer having higher TDS contents (123–262 mg/L) and (Ca+Mg)/Na ratios (0.9–1.3) than groundwater from the sedimentary aquifer (TDS: 55–79 mg/L; (Ca+Mg)/Na: 0.1–0.2). At low elevations, in areas of local groundwater discharge, the more regional flow system in the Silurian-Devonian sediments contains additional Cl from water–rock interaction and has distinctly higher TDS contents (517–537 mg/L). Differences in groundwater chemistry between the aquifers and between shallower and deeper flow systems highlights areas of inter-aquifer mixing. This is particularly important for aquifer vulnerability where groundwater quality in the deeper aquifer may be impacted by surface activities.

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Resumen Se ha utilizado geoquímica de iones mayores para interpretar cualitativamente los tiempos de residencia del agua subterránea dentro de un acuífero, y el grado de mezcla entre acuíferos con mineralogía característica. De manera conjunta con presiones hidráulicas y geoquímica de isótopos estables, se han definido trayectorias de flujo e intercambio entre acuíferos en un sistema de acuífero de roca fracturada en las Sierras Dandenong, sureste de Australia. Los isótopos estables indican recarga estacional moderada a través del sistema. A elevaciones altas en la sub-cuenca que incluye acuíferos sedimentarios Silúrico-Devónicos y acuíferos basálticos Terciarios, Cl se deriva principalmente de sales cíclicas. Las diferencias en mineralogía resultan en agua subterránea del acuífero basáltico que tiene mayores contenidos TDS (123–262 mg/L) y mayor relación (Ca+Mg)/Na (0.9–1.3) que el agua subterránea de los acuíferos sedimentarios (TDS:55–79 mg/L; (Ca+Mg)/Na: 0.1–0.2). A elevaciones bajas, en áreas de recarga local de agua subterránea, el sistema de flujo más regional en los sedimentos Silúrico-Devónicos contiene Cl adicional que se deriva de la interacción roca-agua y típico contenido TDS más alto (517–537 mg L). Las diferencias en la química del agua subterránea entre los acuíferos y entre los sistemas de flujo más profundo y más somero resalta áreas de mezcla entre acuíferos. Esto es particularmente importante para la vulnerabilidad del acuífero donde la calidad del agua subterránea en el acuífero más profundo puede ser impactada por las actividades superficiales.

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Résumé Les ions majeurs sont utilisés pour interpréter quantitativement les temps de résidence des eaux souterraines dans les aquifères, et létendue des zones de mélange entre les aquifères de différentes minéralogies. En regard de la répartition des charges hydrauliques et des informations données par les isotopes stables, les écoulements et les échanges inter-aquifères sont définis dans un aquifère fracturé dans le Dandenong Ranges, SE de lAustralie. Les isotopes stables indiquent des recharges modernes et saisonnières à travers le système aquifère. A haute altitude dans le sous-bassin versant, qui inclut des sédiments du Siluro-Dévonien et des basaltes du Tertiaire, le chlore est dabord dérivé des sels cycliques, et des différences minéralogiques dans les eaux souterraines sont observées selon laquifère : basalte tertiaire (TDS: 123–262 mg/L; Ca+Mg/Ca: 0.9 à 1.3) et sédiments primaires (TDS: 55–79 mg/L; Ca+Mg/Ca: 0.1–0.2). Aux basses altitudes, dans les zones locales de décharge des eaux souterraines, les écoulements les plus régionaux possèdent des teneurs plus élevées en Chlore en provenance des interactions eau—roche, et des TDS plus élevées (515–537 mg/L). Des différences dans la chimie des eaux souterraines entre les aquifères et entre les systèmes découlement de surface et les écoulements profonds mettent en lumière les zones de mélange inter-aquifère. Ceci est particulièrement important pour la définition de la vulnérabilité où la qualité des eaux souterraines en profondeur peuvent subir les impacts des activités de surface.

     

Unusual comets (?) as observed from the Hubble Space Telescope

In separate projects, the Hubble Space Telescope has been used to assess the nature of 3 unusual objects: Chiron, Pholus and P/Shoemaker-Levy 9. This paper will compare these objects and discuss how the unique capabilities of the HST may be used to address the issue of cometary activity in each. Chiron, which has exhibited obvious cometary characteristics for several years, might have a bound dust coma that is unresolvable from the ground. In an attempt to directly observe this bound coma, we have obtained a series of images of Chiron with the HST Planetary Camera. Inner coma structure out to 0.2 has been detected. From these observations we infer a low bulk nucleus density for Chiron. Both HST and ground-based images of 5145 Pholus have been obtained to search for evidence of activity. The ground-based data give the most sensitive limits; however, it is shown that the WFPC-2 on HST can give limits 2–3 orders of magnitude more sensitive than conventional ground-based limits. Finally, as part of a collaborative effort, we have been obtaining HST observations of SL9 in order to determine the fragment sizes and to assess their nature (i.e., cometary vs. asteroid). Both ground-based observations from the UH 2.2m telescope on Mauna Kea and HST observations show that the near-nucleus dust is redder than the sun. While FOS spectra did not detect OH emission, the WFPC-2 HST data show that the inner coma remained very circular from July 1993 up until 2 weeks prior to impact, implying continued production of dust.