Seebens, Hanno and Blackburn, Tim M. and Dyer, Ellie E. and Genovesi, Piero and Hulme, Philip E. and Jeschke, Jonathan M. and Pagad, Shyama and Pyšek, Petr and van Kleunen, Mark and Winter, Marten and Ansong, Michael and Arianoutsou, Margarita and Bacher, Sven and Blasius, Bernd and Brockerhoff, Eckehard G. and Brundu, Giuseppe and Capinha, César and Causton, Charlotte E. and Celesti-Grapow, Laura and Dawson, Wayne and Dullinger, Stefan and Economo, Evan P. and Fuentes, Nicol and Guénard, Benoit and Jäger, Heinke and Kartesz, John and Kenis, Marc and Kühn, Ingolf and Lenzner, Bernd and Liebhold, Andrew M. and Mosena, Alexander and Moser, Dietmar and Nentwig, Wolfgang and Nishino, Misako and Pearman, David and Pergl, Jan and Rabitsch, Wolfgang and Rojas-Sandoval, Julissa and Roques, Alain and Rorke, Stephanie and Rossinelli, Silvia and Roy, Helen E. and Scalera, Riccardo and Schindler, Stefan and Štajerová, Kateřina and Tokarska-Guzik, Barbara and Walker, Kevin and Ward, Darren F. and Yamanaka, Takehiko and Essl, Franz (2018) 'Global rise in emerging alien species results from increased accessibility of new source pools.', Proceedings of the National Academy of Sciences., 115 (10). E2264-E2273.
Our ability to predict the identity of future invasive alien species is largely based upon knowledge of prior invasion history. Emerging alien species—those never encountered as aliens before—therefore pose a significant challenge to biosecurity interventions worldwide. Understanding their temporal trends, origins, and the drivers of their spread is pivotal to improving prevention and risk assessment tools. Here, we use a database of 45,984 first records of 16,019 established alien species to investigate the temporal dynamics of occurrences of emerging alien species worldwide. Even after many centuries of invasions the rate of emergence of new alien species is still high: One-quarter of first records during 2000–2005 were of species that had not been previously recorded anywhere as alien, though with large variation across taxa. Model results show that the high proportion of emerging alien species cannot be solely explained by increases in well-known drivers such as the amount of imported commodities from historically important source regions. Instead, these dynamics reflect the incorporation of new regions into the pool of potential alien species, likely as a consequence of expanding trade networks and environmental change. This process compensates for the depletion of the historically important source species pool through successive invasions. We estimate that 1–16% of all species on Earth, depending on the taxonomic group, qualify as potential alien species. These results suggest that there remains a high proportion of emerging alien species we have yet to encounter, with future impacts that are difficult to predict.
|Full text:||(AM) Accepted Manuscript|
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|Publisher Web site:||https://doi.org/10.1073/pnas.1719429115|
|Date accepted:||03 January 2018|
|Date deposited:||18 June 2019|
|Date of first online publication:||05 February 2018|
|Date first made open access:||18 June 2019|
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