Coelogyne fimbriata Lindl. (Orchidaceae), a medicinal orchid, is mainly distributed in southern China, Cambodia, northeastern Indonesia, Laos, Malaysia, Thailand, and Vietnam (Clayton and Beaman, 2002). Because southern China is the northernmost edge of its distribution region, Chinese C. fimbriata populations are of particular concern because populations on distribution margins are most vulnerable to disturbance (Channell and Lomolino, 2000). Furthermore, in consideration of global climate change and habitat fragmentation, it is urgent to design effective conservation strategies for endangered natural orchid populations (Swarts and Dixon, 2009). Coelogyne fimbriata is an epiphytic or lithophytic orchid, which requires a dormancy period in winter. This species grows on its substrate with creeping and slender rhizomes. It can reproduce both sexually via seed and vegetatively by rhizomatic growth. Usually blooming in late summer, it produces one or two flowers on a scape. The flowers exhibit a type of pollinator deception in which the flower odor mimics food for foraging female wasps (Cheng et al., 2009).
Many studies have focused on the pollination syndromes of orchids (Tang et al., 2014); however, there is a lack of genetic information documented for this species. Because genetic information is important for the conservation and sustainable utilization of orchids (Gijbels et al., 2015), we developed microsatellite markers to allow studies of the genetic diversity, genetic structure, and mating system of C. fimbriata. In total, 15 polymorphic microsatellite loci were isolated and characterized to study genetic variation within this species clade. These highly polymorphic loci displayed high genetic variation and extensive usability in congeneric species, and may serve as a universal tool for orchid genetic studies.
METHODS AND RESULTS
A biotin-streptavidin capture method was employed to construct a microsatellite-enriched DNA library (Jiang et al., 2011). First, we extracted genomic DNA from silica gel-dried leaves of one C. fimbriata individual using a Plant Genomic DNA Extraction Kit (Tiangen, Beijing, China). The enzyme MseI (New England Biolabs, Beverly, Massachusetts, USA) was used to digest approximately 300 ng of genomic DNA in a 25-µL reaction volume for 2 h at 37°C. Fragments 200–1000 bp in length were then ligated to an MseI-adapter pair (F: 5′-TACTCAGGACTCAT-3′ and R: 5′-GACGATGAGTCCTGAG-3′). The ligation-digestion mixture was diluted with ultrapure water (1:4), and the diluted fragments were amplified using MseI-N primer (5′-GATGAGTCCTGAGTAAN-3′) in a 25-µL PCR reaction volume at 95°C for 5 min, followed by 23 cycles of 94°C for 30 s, 53°C for 1 min, and 72°C for 1 min. Next, to obtain microsatellite-enriched DNA fragments, the PCR products were hybridized with 5′-biotinylated (AC)15 probes. We used streptavidin-coated magnetic beads (Promega Corporation, Madison, Wisconsin, USA) to capture single-stranded DNA fragments containing microsatellites. The enriched products were amplified using MseI-N primers for 28 cycles. After the PCR products were purified using a multifunctional DNA Extraction Kit (Bioteke Corporation, Beijing, China), they were ligated into Escherichia coli strain DH5α with the pMD19-T vector (TaKaRa Biotechnology Co., Dalian, Liaoning, China).
We randomly selected and sequenced 249 positive clones using M13+/M13- primers on an ABI 3730 DNA Sequence Analyzer (Applied Biosystems, Foster City, California, USA). Of the 249 sequenced clones, 136 contained microsatellites. Twenty-four sequences were discarded because of short flanking regions for primer design. Finally, we designed 112 primer pairs using Premier 5.0 (PREMIER Biosoft International, Palo Alto, California, USA). We selected 28 individuals from Dawei Mountain, Yunnan Province, and 19 from Diaoluo Mountain, Hainan Province, China (Appendix 1), for PCR using these 112 primers. Of the 112 primers, 47 produced an expected band on 1% agarose gel, 40 failed to obtain amplification products, and 25 others produced multiple bands that were difficult to discriminate. To test for polymorphism, we used the M13(−21)-tailed primer method to fluorescently label alleles and PCR products, which were electrophoretically resolved using an ABI 3730 DNA Sequence Analyzer (Applied Biosystems) with an internal lane standard (GeneScan 500[−250] LIZ) (Schuelke, 2000). Microsatellite loci were amplified under the following conditions: 5 min of denaturation at 94°C; 30 cycles of 30 s at 94°C, 30 s at 53–65°C, and 30 s at 72°C; eight cycles of 30 s at 94°C, 30 s at 53°C, and 30 s at 72°C; and a final 10-min extension at 72°C. Allele binning and calling were conducted using GeneMapper 4.0 (Applied Biosystems), revealing 15 polymorphic loci.
Table 1.
Characteristics of 15 polymorphic microsatellite markers developed for Coelogyne fimbriata.
Characteristics of the 15 polymorphic microsatellite loci developed for C. fimbriata are shown in Table 1. An additional 32 monomorphic loci are described in Appendix 2. Each polymorphic locus had two to 17 alleles, with a mean of 5.1. At the population level, the observed and expected heterozygosities were calculated with GenAlEx 6.5 (Peakall and Smouse, 2012) and ranged from 0.000 to 1.000 and from 0.000 to 0.867, respectively (Table 2). FSTAT 2.9.2.3 (Goudet, 1995) was used to analyze linkage disequilibrium and Hardy-Weinberg equilibrium (HWE). No significant linkage disequilibrium at any locus was detected for either population. However, significant deviation from HWE was found for most loci in the two populations (Table 2), which may be indicative of strong clonality. Signs of null alleles were detected in the loci CF1-11, CF1-51, and CF2-126 with MICRO-CHECKER 2.2.3 (van Oosterhout et al., 2004).
Two wild C. ovalis Lindl. populations (Appendix 1) were used to test the cross-compatibility and polymorphism of the 15 microsatellite loci. This testing was performed because C. ovalis and C. fimbriata have been visually confused as the same species, with no clear differences shown in studies of pollinaria or other morphological characters (Pelser et al., 2000). However, many researchers do recognize C. fimbriata and C. ovalis as separate species (Govaerts, 1999; Wu and Hong, 2009; George and George, 2011). In our results, 11 of 15 loci could obtain clear PCR products and 10 showed moderate to high levels of polymorphism, with the exception of one locus (CF2-147). No significant linkage disequilibrium was detected in C. ovalis populations; however, significant deviation from HWE was found in these populations at most loci (Table 2). Signs of null alleles were detected in the CF1-26, CE1-120, CF2-126, and CF2-172 loci. In addition, cross-amplification of 15 polymorphic loci was conducted on another five related species (n = 5 for each species): C. cumingii Lindl., C. eberhardtii Gagnep., C. mayeriana Rchb. f., C. peltastes Rchb. f., and C. velutina de Vogel; these samples were collected from living plants at Shanghai Chenshan Botanical Garden (Appendix 1). Four to eight loci were successfully amplified in all five Coelogyne species (Table 3).
Table 2.
Characteristics of 15 polymorphic microsatellite loci in Coelogyne fimbriata and C. ovalis populations, respectively.a
CONCLUSIONS
In the current study, although a majority of the developed loci showed monomorphism (68.1%), 15 polymorphic loci were identified in C. fimbriata. These polymorphic loci are valuable for orchid population genetic studies. For example, these markers can be used to characterize the clonal structure of C. fimbriata to estimate seed and pollen flow at a fine scale. Furthermore, these polymorphic loci can provide more information, such as genetic diversity indices, which are important for the conservation and management of the species.
Table 3.
Amplification of 15 microsatellite loci developed for Coelogyne fimbriata in five other Coelogyne species.
ACKNOWLEDGMENTS
The authors thank Ming-Zhong Huang for providing the Hainan plant materials for the polymorphism analysis. This work was supported by funds from the Shanghai Landscaping Administrative Bureau (F122432) and the Chinese Academy of Sciences (WKT053).