C3 - C4 vegetation composition of Wolfe Creek Meteorite Crater, Western Australia: implications for a paleoecological reconstruction

Matthew Wooller and Marilyn Fogel

Geophysical Laboratory, Carnegie Institution of Washington, 5152 Broad Branch Road, NW Washington DC, 20015-1305, US

Changes in environmental conditions, including the concentration of atmospheric CO2, disturbance, temperature, aridity and salinity, can influence the competitive balance between C3 and C4 plants. C3 and C4 plants posses diagnostic carbon stable isotope ratios, and d 13C data from dated sediments are frequently used to reconstruct C3 and C4 vegetation dynamics. Records of this type are lacking from Northern and Western Australia. A Late-Quaternary record from Wolfe Creek Meteorite Crater in Western Australia shows d 13Corganic values between -25 and -16‰. The present vegetation at the crater’s center consists of species tolerating saline (15-19 ppt) conditions, including Acacia ampliceps (d 13C = -25.9‰), Flaveria australasica (d 13C -13.0‰), Atriplex sp. (d 13C -11.0‰), sedges (d 13C = -9.6‰) and halophytic microbes (-14‰), while that at the outer edge is related to aridity and includes the C4 grass Triodia pungens (-11.8‰). In addition to salinity and aridity the present species distribution is related to the nutrient (nitrogen) status of the subrate. d 15N values from plants at the crater’s center are high (~10‰) relative to those values from plants at the edge (~0‰). These findings illustrate how complicated both modern and past C3 and C4 dynamics can be and highlight the need for additional habitat proxies, for example phytoliths, to distinguish C4-like d 13C values from saline, arid and microbial habitats.