Occurrence of Leaf Blight on Cosmos Caused by Alternaria cosmosa in Korea

Article information

Plant Pathol J. 2015;31(1):78-82
Publication date (electronic) : 2015 March 31
doi : https://doi.org/10.5423/PPJ.NT.09.2014.0095
1Department of Plant Protection, College of Agriculture, Yangtze University, Jingzhou 434025, China
2Department of Applied Biology, College of Agriculture and Life Sciences, Chungnam National University, Daejeon 305-764, Korea
3Division of Applied Bioscience & Biotechnology, College of Agriculture & Life Sciences, Chonnam National University, Gwangju 500-757, Korea
4Ginseng Resources Institute, Korea Ginseng Corp., Daejeon 305-805, Korea
*Corresponding author. Phone) +82-42-821-5762, FAX) +82-42-823-8679, E-mail) shunyu@cnu.ac.kr, hblee@jnu.ac.kr
Received 2014 September 24; Revised 2014 November 24; Accepted 2014 November 29.

Abstract

In 2011, a leaf blight disease was observed on cosmos (Cosmos bipinnatus) leaves in Nonsan, Korea. The causal pathogen was isolated and identified based on morphological and molecular approaches. Morphological characteristics of the pathogen matched well with the Alternaria cosmosa and also easily distinguishable from Alternaria zinniae reported from cosmos seeds by producing branched beak. Phylogenetically, the pathogen could not be distinguished from A. passiflorae based on the sequence analysis of a combined data set of Alt a1 and gpd genes. However, A. passiflorae was distinguished from the present species by having conidiophores with 4 to 5 conidiogenous loci. The results indicate that the present Alternaria species is A. cosmosa. Pathogenicity tests revealed that the isolate was pathogenic to the leaves of Cosmos bipinnatus. This is the first report of Alternaria blight disease caused by A. cosmosa on cosmos in Korea.

Cosmos bipinnatus, known as the garden cosmos or Mexican aster, is a half-hardy annual herbaceous plant native to Mexico. The species belonging to the family Asteraceae offers flowers of solitary red, white, pink or purple color blooms (Dubey and Singh, 2011). The cosmos has been widely cultivated as a valuable ornamental plant since its first introduction in Korea in 1938 (Park, 2009). Now, it is commonly to be found in plant gardens and along the sides of road or river in Korea. Fruits and aerial parts of the plant are useful as traditional herbal medicine to reduce various diseases such as jaundice, intermittent fever, and splenomegaly (Jang et al., 2008). Jang et al. (2008) reported that the cosmos flowers showed a significant antioxidant activity and protective effect against oxidative DNA damage

Anthracnose, powdery mildew and white smut diseases of Cosmos bipinnatus have been reported in Korea caused by Colletotrichum acutatum, Podosphaer fusca and Entyloma cosmic, respectively (Park et al., 2012). Cho (2004) isolated a large-spored Alternaria containing narrow-taper long beak from C. bipinnatus in Gongju and Naju, Korea, in 2000. The Alternaria species was considered as a new species based on the morphological and molecular characteristics. However, the author did not assign scientific name of the pathogen. Soon afterwards, a new species of Alternaria, A. cosmosa Y.L. Li & W.S. Wu was reported from cosmos seeds in Taiwan on the basis of conidial morphology, which showed a specific pathogenicity on Cosmos bipinnatus and C. sulphureus (yellow cosmos) (Wu and Li, 2005). Simmons (2007) summarized his results of a lifetime study on Alternaria taxonomy based on morphology and described 275 species totally. But he did not include the species in his publication because he unsuccessfully obtained the ex-type material of A. cosmosa for the comparison with the other morphologically similar taxa. Meanwhile, Alternaria danida on Ageratum houstonianum is suggested as a similar taxon for A. cosmosa (Simmons, 2007).

In 2011, a large-spored Alternaria was isolated again from blight leaves of Cosmos bipinnatus in Nonsan, Korea. The morphological characteristics were identical to previously reported species of Alternaria (Cho, 2004). The objective of the present study was to report a new Alternaria disease of Cosmos bipinnatus in Korea and to identify the causal pathogen based on morphological and molecular approaches.

Symptoms and isolation of the fungus

Blight symptoms on lower leaves of Cosmos bipinnatus were observed during the period of August–September 2011 in Nonsan, Chungnam, Korea (Fig. 1A). Infected leaves showed small and brown necrotic spots along with leaf discoloring. The necrotic lesions were enlarged gradually, finally resulting in the leaf blight and defoliation. The diseased leaves were cut and placed in a moist Petri dish for conidial sporulation. Pure cultures (including CNU 111459) of the Alternaria species were obtained by single spore isolation method. Another isolate (CNU 3437) of Alternaria sp. collected in 2000 (Cho, 2004) and preserved in the Culture Collection of Chungnam National University (CNU) in Korea was also used in this study. The new isolates were deposited in the CNU Culture Collection, and the Korean Agricultural Culture Collection (KACC) in Suwon, Korea.

Fig. 1

Alternaria leaf blight on Cosmos bipinnatus and colony of the causal fungus. (A) discolored and necrotic symptoms on leaves of C. bipinnatus. (B) obverse (left) and reverse (right) of colony grown on potato dextrose agar at 25°C for 7 days.

Morphological characteristics

The isolate CNU 111459 was grown on potato dextrose agar (PDA; Difco, Montreal, Canada) incubated at 25°C in the dark. Colony diameters were measured after 7 days of incubation and other characteristics such as texture, color and pigmentation were also recorded. The isolate was also cultured on potato carrot agar (PCA: 20 g white potato, 20 g carrot, and 20 g agar in 1 l) under fluorescent lights (8/16 light/dark) at 22°C to induce sporulation (Simmons, 2007). Randomly selected conidia (50) from 7-day-old cultures were used to obtain conidial measurements and photograph was taken using an OLYMPUS BX50 light microscope (OLYMPUS, Tokyo, Japan) with an Artcam 300MI digital camera (ARTRAY, Tokyo, Japan).

The colonies on PDA were cotton or woolly, effuse, white or pale to dark grey; reverse yellow to orange, secreting a yellow pigment into the medium, 65–74 mm in diameter (Fig. 1B). Conidiophores on PCA were simple, erect or curved, septate (1–7), pale brown, smooth-walled, usually only one pigmented terminal conidiogenous site, measuring 25–120 (−140)×4.5–8.5 μm (Fig. 2A, 2B). Conidia were solitary, straight or slightly curved, mostly long obclavate, olivaceous brown to dark yellowish brown, smooth-walled, rostrate, tapering towards a long beak; conidium body 60–130 (−140)×5–15 (−22) μm, with 2–13 (−16) transeverse septa, 1–4 longitudinal septa; beaks narrowly filamentous, filiform, sub hyaline to pale brown, often branched once, twice or more, 50–200 (−220) μm long, 2–3 μm wide, with 0–8 septa (Fig. 2C).

Fig. 2

Conidial morphology of the present isolate CNU 111459 from Cosmos bipinnatus. (A) sporulation patterns, (B) conidiophores, (C) conidia. Scale bars = 50 μm.

The cultural, conidial and sporulation characteristics of the present Alternaria species was identical with the species described by Cho (2004) in Korea and A. cosmosa reported by Wu and Li in Taiwan (2005) even though there were some variation in the size of conidia (Table 1). Some morphological characteristics of Alternaria (e.g., color, size, shape of conidia, and sporulation patterns) that are used for identification sometimes overlap among species and vary depending on the cultural conditions (e.g., temperature and substrate) (Simmons and Roberts, 1993).

Alternaria species used for phylogenetic analyses

The first report of A. cosmosa was from cosmos seeds (Wu and Li, 2005). Richardson (1979) also reported another Alternaria species, A. zinniae, from cosmos seeds. But A. zinniae is easily differentiated from the present Alternaria species by producing unbranched beak. Morphologically, the present Alternaria species was distinct to A. carthami and similar with A. agripestis and A. passiflorae (Table 2). However, A. agripestis differed from the present species by having ornamented conidial body, and A. passiflorae distinguished from the present species by having conidiophores with 4 to 5 conidiogenous loci (Simmons, 2007). Simmons (2007) mentioned that A. cosmosa and A. danida are morphologically similar species. However, conidial beak tip of A. danida is possible to convert into a secondary conidiophore yielding a chain of two conidia, the morphological phenomenon was not observed among the present A. cosmosa isolates, and not described by Wu and Li (2005).

Morphological comparison among the present Alternaria species and the other related species

Phylogenetic analysis

Genomic DNA of the present isolates (CNU 3437 and CNU 111459) was extracted using a modified protocol of Park et al. (2005). Fragments containing Alternaria allergen a 1 (Alt a1) gene and glyceraldehyde-3-phosphate dehydrogenase (gpd) gene were amplified with primers Alt-a1-for & Alt-a1-rev (Hong et al., 2005), and gpd1 & gpd2 (Berbee et al., 1999), respectively. PCR products were purified using a Wizard PCR prep kit (Promega, Madison, WI, USA) and sequenced using commercial sequencing service provider (Macrogen, Seoul, Korea). Resultant sequences were deposited in GenBank (Table 1), from which the molecular sequences for the other species were retrieved and included in the study. A pair-wise alignment of all sequences was completed using the ClustalX program (Thompson et al., 1997). Phylogenetic relationships of a combined dataset were estimated by a maximum likelihood analysis using the RAxML program (Stamatakis et al., 2008).

PCR amplification resulted DNA fragments in size of 452 and 564 bp from Alt a1 and gpd genes, respectively. The present Alternaria isolates CNU 111459, CNU 3437 and A. passiflorae could not be differentiated by the sequences of these two genes (Fig. 3). Phylogenetic analysis of the dataset revealed that the present Alternaria species was closely related to A. carthami and A. agripestis, genetically distant to A. danida which was accordance to the results of Lawrence et al. (2013).

Fig. 3

Maximum likelihood tree of the present Alternaria species from Cosmos bipinnatus based on a combined dataset of Alt a1 and gpd gene sequences. Bootstrap values are shown above branches. The bar indicates nucleotide substitutions per site.

Although the present Alternaria species could be delimited from A. passiflorae based on the phylogenetic analysis in the study, the morphology of conidial body and condiophore was an obvious delimitation characteristic. Hence, the present Alternaria isolates CNU 111459 and CNU 3437 were all confirmed as Alternaria cosmosa Y.L. Li & W.S. Wu (2005). This is the first report of Alternaria blight caused by A. cosmosa on Cosmos bipinnatus in Korea.

Pathogenicity

The pathogenicity of the species was conducted by spraying conidial suspension (1×105 conidia/ml) to the detached surface-sterilized leaves. Necrotic spots were induced after two to three days and enlarged the size with age (data not shown). Conidia of A. cosmosa were re-isolated from the diseased leaves. A. cosmosa were pathogenic to Cosmos bipinnatus and C. sulphureus (yellow cosmos), which is readily infected the lower leaves of yellow cosmos and caused brownish spots (Wu et al., 2007). During our observation in Korea, the causal disease was also commonly found on the lower leaves of C. bipinnatus.

Acknowledgment

This study was supported by a grant from the National Institute of Biological Resources (NIBR), funded by the Ministry of Environment (MOE) of the Republic of Korea.

References

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Article information Continued

Fig. 1

Alternaria leaf blight on Cosmos bipinnatus and colony of the causal fungus. (A) discolored and necrotic symptoms on leaves of C. bipinnatus. (B) obverse (left) and reverse (right) of colony grown on potato dextrose agar at 25°C for 7 days.

Fig. 2

Conidial morphology of the present isolate CNU 111459 from Cosmos bipinnatus. (A) sporulation patterns, (B) conidiophores, (C) conidia. Scale bars = 50 μm.

Fig. 3

Maximum likelihood tree of the present Alternaria species from Cosmos bipinnatus based on a combined dataset of Alt a1 and gpd gene sequences. Bootstrap values are shown above branches. The bar indicates nucleotide substitutions per site.

Table 1

Alternaria species used for phylogenetic analyses

Species Isolate GenBank accession No.

Alt a 1 gpd
A. agripestis CBS 577.94 JQ646440 JQ646356
A. carthami CBS 635.80 JQ646421 JQ64633
A. cichorii CBS 102.33 JQ646424 JQ646340
A. cirsinoxia CBS 113261 JQ646435 JQ646351
A. cosmosa CNU 3437 KM655806 KM655808
A. cosmosa CNU 111459 KM655807 KM655809
A. cretica CBS 109164 JQ646426 JQ646342
A. cyphomandrae CBS 109155 JQ646444 JQ646360
A. danida EGS 07–029 JQ646420 JQ646336
A. dichondrae CBS 199.74 JQ646441 JQ646357
A. grandis CBS 109158 JQ646425 JQ646341
A. hawaiiensis CBS 630.93 JQ646436 JQ646352
A. linicola CBS 103.46 JQ646447 JQ646363
A. multirostrata CBS 712.68 JQ646446 JQ646362
A. passiflorae CBS 113.38 JQ646437 JQ646353
A. porri ATCC 58175 AY563296 AY278806
A. protenta CBS 116696 JQ646419 JQ646335
A. scorzonerae CBS 478.83 JQ646418 JQ646334
A. solani EGS 44–098 GQ180096 GQ180080
A. solani-nigri CBS 113403 JQ646417 JQ646333
A. subcylindrica CBS 109161 JQ646429 JQ646345
A. tomatophila EGS 42–156 GQ180101 GQ180085

Table 2

Morphological comparison among the present Alternaria species and the other related species

Species Conidial body Beak (μm) Culture media Temperature References

Size (μm) Transverse septa
A. agripestis 80–110 × 11–18 8–11 190–260 PCA 22°C Simmons (2007)
A. carthami 75–90 × 17–22 8–10 150–200 V8A 22°C Simmons (2007)
A. danida 95–120 × 23–26 6–11 175–250 (>250) V8A 22°C Simmons (2007)
CNU 111459 60–130 (−141) × 5–15 (−22) 2–13 (−16) 50–200 (−220) PCA 22°C In the study
CNU 3437 50–100 × 12–18 6–13 75–163 V8A 20°C Cho (2004)
A. cosmosa 50–110 × 15–25 7–12 112.5–287.5 V8A 25°C Wu and Li (2005)
50–100 × 15–22.5 6–11 137.5–287.5 PCA 25°C Wu and Li (2005)
A. passiflorae 70–115 × 16–22 7–10 (>10) 100–220 V8A 22°C Simmons (2007)