| Literature DB >> 24865774 |
Gemma V Clucas1, Michael J Dunn2, Gareth Dyke3, Steven D Emslie4, Ron Naveen5, Michael J Polito6, Oliver G Pybus7, Alex D Rogers7, Tom Hart7.
Abstract
Climate change is a major threat to global biodiversity. Antarctic ecosystems are no exception. Investigating past species responses to climatic events can distinguish natural from anthropogenic impacts. Climate change produces 'winners', species that benefit from these events and 'losers', species that decline or become extinct. Using molecular techniques, we assess the demographic history and population structure of Pygoscelis penguins in the Scotia Arc related to climate warming after the Last Glacial Maximum (LGM). All three pygoscelid penguins responded positively to post-LGM warming by expanding from glacial refugia, with those breeding at higher latitudes expanding most. Northern (Pygoscelis papua papua) and Southern (Pygoscelis papua ellsworthii) gentoo sub-species likely diverged during the LGM. Comparing historical responses with the literature on current trends, we see Southern gentoo penguins are responding to current warming as they did during post-LGM warming, expanding their range southwards. Conversely, Adélie and chinstrap penguins are experiencing a 'reversal of fortunes' as they are now declining in the Antarctic Peninsula, the opposite of their response to post-LGM warming. This suggests current climate warming has decoupled historic population responses in the Antarctic Peninsula, favoring generalist gentoo penguins as climate change 'winners', while Adélie and chinstrap penguins have become climate change 'losers'.Entities:
Mesh:
Year: 2014 PMID: 24865774 PMCID: PMC4034736 DOI: 10.1038/srep05024
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1Sample locations across the Scotia Arc.
Insert shows the location of the map relative to the Antarctic continent and South America. Gentoo penguin sample locations are shown with circles, chinstrap penguin colonies with triangles and Adélie penguin colonies with squares. Each sample location is coloured independently, and is consistent with Figure 2. The archipelago names are given in green. The map was produced by TH with help from Dr. Heather Lynch using ArcGIS and modified in ArcSoft® PhotoStudio.
mtDNA diversity and neutrality test results for each species and sub-species
| n | NH | NP | H (SD) | π (SD) | Fu's | Tajima's | |
|---|---|---|---|---|---|---|---|
| Gentoo penguin | 249 | 110 | 58 | 0.981 (0.003) | 0.023 (0.012) | −0.726 | |
| 91 | 40 | 22 | 0.955 (0.009) | 0.008 (0.005) | −1.222 | ||
| 158 | 70 | 48 | 0.984 (0.003) | 0.012 (0.007) | |||
| Chinstrap penguin | 166 | 116 | 46 | 0.987 (0.004) | 0.006 (0.004) | ||
| Adélie penguin | 122 | 115 | 128 | 0.999 (0.001) | 0.016 (0.008) |
n, number of individuals sequenced; NH, number of haplotypes; NP, number of polymorphic sites; H, haplotype diversity; π, nucleotide diversity; SD, standard deviation.
*denotes significance at α = 0.05;
**denotes significance at α = 0.01;
***denotes significance at α = 0.001.
Figure 2Median-joining haplotype networks for gentoo (a), chinstrap (b) and Adélie penguins (c).
The area of each pie chart represents the number of haplotypes as shown by the scale at the bottom. Star contraction has been applied to the chinstrap penguin haplotype network and so some of the terminal nodes are not displayed. The representatives of the “Ross Sea” and “Antarctic” lineages (with GenBank accession numbers) are indicated on the Adélie network. Colours represent the populations where the haplotype was sampled, according to symbols on Figure 1. Black scale bar shows one mutation in gentoo and chinstrap penguins; blue scale bar shows one mutation in Adélie penguins; broken line shows 25 mutational steps. Photographic images belong to TH.
Figure 3Bayesian skyline plots showing the change in effective female population size for each species and sub-species.
Solid lines show the median estimate; dotted lines show the 95% highest posterior density interval. Solid vertical line shows the mean tMRCA for the population, whilst the projection is made to the upper limit of the 95% highest posterior density interval of the tMRCA. The bottom panel shows the Antarctic temperature anomaly (the difference from the average of the last 1000 years) as estimated from the EPICA Dome C ice core54.