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Phylogeography of the planktonic shrimp Lucifer hanseni Nobili 1905 in the Indo-Malayan Archipelago

Published online by Cambridge University Press:  24 February 2016

Mary Mar Noblezada*
Affiliation:
Atmosphere and Ocean Research Institute, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa 277-8564, Japan The Marine Science Institute, University of the Philippines Diliman, Velasquez St., 1101 Quezon City, Philippines OceanBio Laboratory, Division of Biological Sciences, College of Arts and Sciences, The University of Philippines Visayas, 5023 Miagao, Iloilo, Philippines
Hiroomi Miyamoto
Affiliation:
Tohuku National Fisheries Research Institute, Fisheries Research Agency, 3-27-5 Shinhama, Shiogama 985-0001, Japan
Wilfredo L. Campos
Affiliation:
OceanBio Laboratory, Division of Biological Sciences, College of Arts and Sciences, The University of Philippines Visayas, 5023 Miagao, Iloilo, Philippines
Fatimah MD. Yusoff
Affiliation:
Department of Aquaculture, Faculty of Agriculture, Institute of Bioscience, Universiti Putra Malaysia, 43400 UPM, Serdang, Selangor, Malaysia
Shuhei Nishida
Affiliation:
Atmosphere and Ocean Research Institute, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa 277-8564, Japan
*
Correspondence should be addressed to:M.M. Noblezada, Atmosphere and Ocean Research Institute, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa 277-8564, Japan email: mmpnoblezada@gmail.com
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Abstract

Using partial sequences of two mitochondrial genes, cytochrome c oxidase subunit I (COI) and 12S ribosomal RNA (12S rRNA), and one nuclear gene, 28S ribosomal RNA (28S rRNA), we investigated population genetics of the holoplanktonic shrimp Lucifer hanseni Nobili, 1905 in the Indo-Malayan Archipelago (IMA), encompassing Andaman Sea, Malacca Strait, Gulf of Thailand, Borneo Island, Philippines (hereafter collectively referred to as the Thailand-Malaysia-Philippine area: TMP), Celebes Sea (CS), and the waters near islands in the Western Pacific (WP) including Palau, Papua New Guinea and Solomon Islands. The samples from the TMP showed the highest number of haplotypes. Significant phylogeographic structure was found in the L. hanseni populations (ΦST = 0.832 for COI, 0.159 for 12S rRNA, 0.783 for 28S rRNA). The total number of haplotypes was 46 in COI, 28 in 12S rRNA and 23 in 28S rRNA. The haplotype network analyses revealed two major clades for COI (subgroups: TMP + CS, WP) and for 12S rRNA and 28S rRNA (TMP, CS + WP). The CS and WP populations appeared isolated from the TMP populations. The samples from the CS showed low genetic diversity compared with the other samples at both haplotype and nucleotide levels, suggesting that the population CS experienced bottleneck events. This is the first demonstration of significant genetic structure of a holoplanktonic metazoan in IMA, which is suggested to be synergistically influenced by historical events (vicariance) and contemporary oceanographic circulations and corroborates the results of previous studies on other benthic/demersal animals with mero-planktonic phases.

Information

Type
Research Article
Copyright
Copyright © Marine Biological Association of the United Kingdom 2016 
Figure 0

Fig. 1. Map showing sampling locations of Lucifer hanseni in the Indo-Malayan Archipelago. White dots represent collection sites presented in details in Table 1. Grey areas indicate the shoreline during the Pleistocene low sea-level stands (100 m below the present-day level, according to Voris, 2000). Black arrows indicate major ocean currents across the region, and dotted arrows show seasonally reversing currents. Indonesian Throughflow (ITF), North Equatorial Current (NEC), North Equatorial Counter Current (NECC), New Guinea Coastal Current (NGCC), and South Equatorial Current (SEC).

Figure 1

Table 1. Sampling stations of Lucifer hanseni.

Figure 2

Table 2. List of PCR and sequencing primers used in the molecular analysis of Lucifer hanseni.

Figure 3

Fig. 2. Bayesian tree based on sequences of COI (A) 12S rRNA (B) and 28S rRNA (C) of Lucifer hanseni. Numerical values are Bayesian posterior probabilities (left) and maximum likelihood bootstrap values (right). For easy visualization, we have displayed the tree based on mitochondrial gene COI as a phylogram and those based on mitochondrial gene 12S rRNA and nuclear gene 28S rRNA as ultrametric trees.

Figure 4

Fig. 3. Geographic distribution (A) and median joining network (B) of COI haplotypes of Lucifer hanseni. Shading indicates the frequency of occurrence of each haplotype. The numbers inside or at the side of each circle and the colour represent the unique haplotype corresponding to the legend. The circle size is proportional to the frequency of occurrence, ranging from 1–46. The black nodes denote the mutational step.

Figure 5

Table 3. Genetic diversity statistics and tests of selective neutrality for Lucifer hanseni (DNA regions: COI, 12S rRNA, 28S rRNA). Number of individuals sequenced (Nind), number of haplotypes (NH), number of polymorphic sites per population (NP), haplotype diversity (HD), and nucleotide diversity (π).

Figure 6

Table 4. Geographic distribution, frequency distribution and number of haplotypes of Lucifer hanseni for: (a) COI, (b) 12S rRNA, and (c) 28S rRNA. Shaded are haplotypes shared between stations and/or between areas.

Figure 7

Table 5. Pairwise ΦST distances between areas for Lucifer hanseni. Asterisks indicate significance level (P) calculated from 10,000 permutations: * for P < 0.001.

Figure 8

Fig. 4. Geographic distribution (A) and median-joining network (B) of 12S rRNA haplotypes of Lucifer hanseni. Shading indicates the frequency of occurrence of each haplotype. The numbers inside or at the side of each circle and the colour represent the unique haplotype corresponding to the legend. The circle size is proportional to the frequency of occurrence, ranging from 1–28. The black nodes denote the mutational step.

Figure 9

Fig. 5. Geographic distribution (A) and median-joining network (B) of 28S rRNA haplotypes of Lucifer hanseni. Shading indicates the frequency of occurrence of each haplotype. The numbers inside or at the side of each circle and the colour represent the unique haplotype corresponding to the legend. The circle size is proportional to the frequency of occurrence, ranging from 1–23.

Figure 10

Table 6. Pairwise ΦST distances between major clades for Lucifer hanseni. DNA regions: COI, 12SrRNA, 28SrRNA. * Indicates significant differences for P < 0.001.