Dynamics of the hindgut microbiota of the Japanese honey bees (Apis cerana japonica) throughout the overwintering period

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Microbiology

Introduction

The gut microbiota of honey bees plays a critical role in their health (Raymann & Moran, 2018), including decomposing dietary compounds (Engel, Martinson & Moran, 2012), producing short-chain fatty acids (SCFAs) as an energy source (Zheng et al., 2017), degrading potentially toxic plant metabolites (Motta et al., 2022), inhibiting the growth of honey bee pathogens (Wu et al., 2014), and stimulating the immune system (Kwong, Mancenido & Moran, 2017; Motta & Moran, 2024). Disruption of the gut microbiota composition due to antibiotic treatment and pesticide exposure causes dysbiosis, leading to host mortality (Raymann, Shaffer & Moran, 2017; Motta & Moran, 2024).

During winter, honey bees survive the severe cold environment in a metabolically and physically active state that is essential for ensuring the colony’s survival until the following spring (Moeller, 1977; Doeke, Frazier & Grozinger, 2015). Cold stress is a major cause of individual and colony mortality in honey bees and also increases the risk of disease and infection outbreaks (Doeke, Frazier & Grozinger, 2015; Xu et al., 2017). During overwintering, feeding is essentially limited to food stored within the colony (pollen, bee bread, and honey). To cope with the surrounding cold stress, the honey bees must maintain the temperature of the colony’s outer edge and core by vigorously vibrating their flight muscles to generate heat (Doeke, Frazier & Grozinger, 2015). The gut microbiota of overwintering honey bees has been increasingly recognized for its beneficial role in survival during the overwintering period. Most studies have focused on the Western honey bees (Apis mellifera), reporting an increase in gut bacteria abundance during this period (Kešnerová et al., 2020) along with changes in gut microbiota composition (Bleau et al., 2020; Kešnerová et al., 2020; Liu et al., 2021; Castelli et al., 2022; Li et al., 2022; Brar et al., 2025). These findings suggest that gut bacteria may play crucial roles in energy absorption and immune function, thereby substantially contributing to survival during the overwintering period.

The Apis genus is naturally distributed across Asia, Europe, and Africa (Ji, 2021). The Western honey bees are widely distributed worldwide, including their native regions of Europe, Africa, and the Middle East, while Eastern honey bees (Apis cerana) are found throughout South, Southeast, and East Asia (Ji, 2021). Compared to Western honey bees, Eastern honey bees exhibit superior cold tolerance and are better adapted to surviving the harsh overwintering period (Li et al., 2012; Xu et al., 2017). In consideration of the advantageous role of the gut microbiota in the overwintering process of honey bees, we hypothesized that the gut microbiota plays a significant role in enabling Eastern honey bees to tolerate cold stress and successfully overwinter. Characterizing the hindgut microbiota of overwintering honey bees will help narrow down the candidate bacteria beneficial for survival under cold and harsh environments, providing novel insights into the symbiotic relationships between honey bees and their hindgut microbiota.

This study focused on the Japanese honey bees (Apis cerana japonica), a subspecies of the Eastern honey bee that is native to Japan. The aim was to develop a comprehensive inventory of the hindgut microbiota of A. c. japonica using high-throughput sequencing of the V3–V4 region of the bacterial 16S rRNA gene. In addition, we compared the composition of the hindgut microbiota before, during, and after the overwintering period to identify distinctive microbial features associated with successful overwintering.

Materials and Methods

Sample collection

The study samples were collected from four A. c. japonica colonies in Ibaraki, Japan. Two colonies were maintained by our laboratory at the National Institute of Environmental Studies in Tsukuba City, while the other two were managed by local beekeepers in Tsukuba City and Inashiki District, respectively. We sampled 30 foragers from each colony using a net with clean plastic cups over three periods: October 2022 (before overwintering, BO group), December 2022 (during overwintering, OW group), and March 2023 (after overwintering, AO group) (Table 1). The total number of samples was 360 (30 honey bees per colony × four colonies × three periods). All samples were immediately placed on ice after collection and stored at −80 °C until DNA extraction.

Table 1:
Detailed information on sampling in this study.
Period1) Sampling date Colony ID Location2) DNA sample ID
BO 10/19/2022 H Tsukuba city, Ibaraki, Japan H10-1, H10-2, H10-3
10/27/2022 I Inashiki district, Ibaraki, Japan I10-1, I10-2, I10-3
10/20/2022 T NIES T10-1, T10-2, T10-3
10/20/2022 X NIES X10-1, X10-2, X10-3
OW 12/19/2022 H Tsukuba city, Ibaraki, Japan H12-1, H12-2. H12-3
12/18/2022 I Inashiki district, Ibaraki, Japan I12-1, I12-2. I12-3
12/19/2022 T NIES T12-1, T12-2. T12-3
12/19/2022 X NIES X12-1, X12-2. X12-3
AO 3/15/2023 H Tsukuba city, Ibaraki, Japan H3-1, H3-2, H3-3
3/16/2023 I Inashiki district, Ibaraki, Japan I3-1, I3-2, I3-3
3/7/2023 T NIES T3-1, T3-2, T3-3
3/7/2023 X NIES X3-1, X3-2, X3-3
DOI: 10.7717/peerj.20050/table-1

Notes:

BO, Before overwintering; OW, during overwintering; AO, after overwintering.
NIES, National Institute for Environmental Studies (Tsukuba, Ibaraki, Japan).

DNA extraction

After thawing the honey bees on ice, they were surface-sterilized by immersing them in 70% ethanol for 30 s, followed by rinsing with ultrapure water for 30 s. The hindguts, including the pylorus, ileum, and rectum, were carefully removed on ice using sterile forceps. Ten hindguts were pooled into 2.0 mL sterile tubes containing TE buffer (10 mmol L−1 Tris-HCl and 1 mmol L−1 EDTA-2Na, pH 8.0) supplemented with 5% (v/v) Triton X-100 (MP Biomedicals, Irvine, CA, USA) and glass beads (1.0 mm diameter). The hindguts were disrupted by three cycles of crushing at 3,200 rpm for 30 s using Beads Crusher µT-12 (Taitec, Saitama, Japan) and 30 s of cooling on ice. The homogenates were centrifuged at 6,000× g for 10 min to sediment debris. Total bacterial DNA was extracted from 180 μL of the resulting supernatant using the DNeasy Blood and Tissue Kit (Qiagen, Hilden, Germany) according to the manufacture’s instructions. The DNA concentration of the 36 samples (three replicates per colony × four colonies × three sampling periods) was measured using a NanoDrop One spectrophotometer (Thermo Fisher Scientific, Waltham, MA, USA).

High-throughput sequencing of the V3–V4 region of the bacterial 16S rRNA gene

The bacterial V3–V4 hypervariable regions of the 16S rRNA gene were amplified using a universal primer set comprising 341F (5′-ACACTCTTTCCCTACACGACGCTCTTCCGATCT-NNNNN-CCTACGGGNGGCWGCAG-3′) and 805R (5′-GTGACTGGAGTTCAGACGTGTGCTCTTCCGATCT-NNNNN-GACTACHVGGGTATCTAATCC-3′). These primers include adapter sequences compatible with the Illumina library preparation workflow and are specific to the amplification of the bacterial V3–V4 regions. Polymerase chain reaction (PCR) was performed using template DNA (5 ng µl−1) with Blend Taq Plus polymerase (Toyobo, Osaka, Japan) following the manufacturer’s instructions. The PCR cycling conditions were initial denaturation at 94 °C for 2 min, followed by 30 cycles of denaturation at 94 °C for 30 s, annealing at 55 °C for 30 s, and extension at 72 °C for 30 s. The resulting PCR amplicons were verified by 1.5% agarose gel electrophoresis at 100 V for 25 min, stained with ethidium bromide, and visualized under UV illumination. The PCR amplicons were sent to Bioengineering Lab. Co., Ltd. (Kanagawa, Japan) for sequencing. The amplicons were purified using AMPure XP Beads (Beckman Coulter, Brea, CA, USA), and the DNA concentrations were measured using a Synergy H1 multimode microplate reader (Agilent Technologies, Santa Clara, CA, USA) and a QuantiFluor dsDNA System (Promega, Madison, WI, USA). Library preparation was performed using the purified amplicons with dual-index barcoding to enable sample multiplexing. After determining the library concentrations as described above, quality checking was performed using a dsDNA 915 Reagent kit (Agilent Technologies) on a Fragment Analyzer System (Agilent Technologies). Each library was pooled at an equimolar concentration and underwent 300 bp paired-end sequencing using MiSeq Reagent Kit v3 (Illumina, San Diego, CA, USA) on a MiSeq benchtop sequencer (Illumina).

Data analysis

To generate amplicon sequence variants (ASVs), DADA2 ver. 1.16 (Callahan et al., 2016) in RStudio software ver. 2023.12.0 + 369 was used for trimming and filtering the paired-end FASTQ reads data obtained following MiSeq high-throughput sequencing. Low-quality distributions and primers from each forward and reverse sequence were trimmed using parameters set to truncLen = c(290, 230) and trimLeft = c(17,21), respectively, and then the sequences were filtered using maxN = 0, maxEE = c(2,2), and truncQ = 2 parameters. Next, the forward and reverse reads were merged, after which chimeras and short reads (<400 bp) were discarded. The taxonomic classification of representative ASVs from phylum to genus level was assigned using the SILVA ver. 138.1 prokaryotic SSU database (Quast et al., 2013) as a reference dataset. Before downstream analysis, ASVs that were unclassified at the phylum level and were assigned as non-bacteria groups (e.g., chloroplasts and mitochondria) were manually removed.

To standardize sequencing depth at minimum read count across samples, abundance-based read resampling was performed using the rrarefy function of the vegan package ver. 2.6.4 (Oksanen et al., 2023) among all samples. Rarefaction curves were generated using the rarecurve function of the vegan package and the ggplot2 package ver. 3.4.2 (Wickham, 2016). The Coverage function in the entropart package ver. 1.6.12 (Marcon & Hérault, 2015) was used to calculate coverage and evaluate whether the sequencing depth was sufficient to fully represent the bacterial communities in each sample before and after rarefaction. After pooling ASVs at the lowest taxonomic level (bacterial genus), the bacterial community composition at the phylum and genus levels was visualized for each sample as bar plots using ggplot2. Taxa with a relative abundance of <1% across all samples were grouped and represented as “Others”.

Bacterial genera with a relative abundance >1% across all samples were defined as the core hindgut bacteria of Apis cerana japonica. All ASVs assigned to these core genera underwent similarity searches against the bacterial 16S rRNA gene sequence database in EzBioCloud (Yoon et al., 2017) to identify the closest related species.

Non-metric multidimensional scaling (NMDS) plot was generated based on Bray–Curtis dissimilarity using the metaMDS function from the vegan package and visualized using the ggplot2 package, in order to assess the β-diversity of the hindgut microbiota at the ASV level across the three time periods.

Statistical analysis

To detect differences in the hindgut microbial compositions among the three periods, we performed pairwise comparisons using permutational multivariate analysis of variance (PERMANOVA) based on the Bray–Curtis dissimilarity index with 9,999 permutations using the pairwise.adonis function of the pairwiseAdonis package ver. 0.4.1 (Martinez, 2020).

To investigate the effect of sampling period on the abundance of core bacterial genera, a generalized linear mixed model (GLMM) analysis was conducted, assuming a Poisson distribution with a log link function, using the glmer function from the lme4 package ver. 1.1.32 (Bates et al., 2015). The read count of each core bacterial genus was set as the response variable, with sampling period as a fixed effect and colony as a random effect. P-values < 0.05 were considered statistically significant for all comparisons.

Results

Sequence dataset overview

The high-throughput sequencing generated 1,381,026 raw reads (mean ± SD: 38,362 ± 5,199) from all samples. After trimming and filtering, 1,098,689 high-quality reads (mean ± SD: 30,519 ± 3,678) remained (Table S1), clustering into 260 ASVs (mean ± SD: 59 ± 10). Next, all nonbacterial reads were removed from all samples, and a read count-based cutoff was applied to match the minimum read count (21,808), resulting in a final dataset of 241 ASVs (mean ± SD: 54 ± 8). The rarefaction curves for each sample plateaued at the minimum read depth (Fig. S1), and the estimated coverage was exceeded 99% for all samples (Table S2), indicating that the sequencing depth was sufficient to identify most of the hindgut bacteria in the study samples.

Hindgut microbiota composition

The composition at the phylum and genus levels for each period were described for those taxa with a relative abundance >1% across all samples, while those with a relative abundance <1% were grouped as “Others” (Fig. 1). At the phylum level, the hindgut microbiota of A. c. japonica was dominated by Actinobacteriota (0.4–13.1%), Bacteroidota (11.7–36.3%), Firmicutes (9.2–33.9%), and Proteobacteria (35.2–68.6%), collectively accounting for >99.9% of the relative abundance. At the genus level, six bacterial genera, namely Apibacter (11.6–36.3%), Bifidobacterium (0.2–13.1%), Bombilactobacillus (0.3–13.6%), Gilliamella (26.6–59.8%), Lactobacillus (6.9–28.2%), and Snodgrassella (0.7–22.4%) predominated, accounting for >96% of the hindgut microbiota in all three periods and all samples. The relative abundance of “Unclassified”, of which sequences were not assigned at the genus level, and “Others” was 0.0–5.4% and 0.0–12.1%, respectively. The details of relative abundance at the phylum and genus levels are listed in Tables S3S6.

Hindgut microbiota composition of the Japanese honey bees (Apis cerana japonica) sampled for each period at the (A) phylum and (B) genus levels.

Figure 1: Hindgut microbiota composition of the Japanese honey bees (Apis cerana japonica) sampled for each period at the (A) phylum and (B) genus levels.

BO, before overwintering; OW, during overwintering; AO, after overwintering.

Further examination of the six major bacterial genera revealed that, except for genus Bifidobacterium, many ASVs assigned to the core genera exhibited sequence similarities with type strains in the EzBioCloud database (Yoon et al., 2017) below the 98.7% threshold, which is commonly used to distinguish closely related species (Chun et al., 2018) (Table 2). Notably, 90% (27/30) of the ASVs assigned to Gilliamella showed this pattern, followed by Snodgrassella (65%, 13/20), Bombilactobacillus (60%, 3/5), Apibacter (53.8%, 7/13), and Lactobacillus (41.6%, 5/12), suggesting potentially novel bacterial species within the hindgut microbiota of A. c. japonica.

Table 2:
List of BLAST results against the EzBioCloud 16S rRNA database of ASVs assigned to the six core bacteria genera in the hindgut of the Japanese honey bees (Apis cerana japonica).
Assigned genus ASV ID 1) Length (bp) Top-hit taxon (strain level) 2) Accession ID Similarity (%)
Apibacter ASV1 423 Apibacter sp. B3924 WINM01000002 100
ASV16 423 Apibacter mensalis R-53146T LIVM01000008 99.5
Apibacter sp. B3924 WINM01000002 99.5
ASV9 423 Apibacter mensalis R-53146T LIVM01000008 99.8
Apibacter sp. B3924 WINM01000002 99.8
ASV32 423 Apibacter sp. B3924 WINM01000002 99.8
ASV33 423 Apibacter mensalis R-53146T LIVM01000008 100
ASV118 423 Apibacter sp. B3924 WINM01000002 96.2
ASV76 426 Apibacter sp. B3924 WINM01000002 97.9
ASV133 409 Apibacter mensalis R-53146T LIVM01000008 91.0
Apibacter sp. B3924 WINM01000002 91.0
ASV151 425 Apibacter sp. B3924 WINM01000002 97.6
ASV254 423 Apibacter sp. B3924 WINM01000002 90.6
ASV280 423 Apibacter sp. B3924 WINM01000002 91.0
ASV174 431 Apibacter mensalis R-53146T LIVM01000008 90.5
ASV279 422 Apibacter sp. B3924 WINM01000002 99.6
Bifidobacterium ASV51 408 Bifidobacterium indicum JCM 1302T LC071807 100
ASV11 410 Bifidobacterium sp. 7101 AWUN01000009 100
Bombilactobacillus ASV34 432 Bombilactobacillus mellifer Bin4NT JX099543 99.8
ASV47 431 Uncultured Firmicutes bacterium D08062C1 HM215046 98.1
ASV169 430 Uncultured Firmicutes bacterium D08062C1 HM215046 89.4
ASV12 429 Bombilactobacillus mellis Hon2T KQ033880 100
ASV23 431 Uncultured Firmicutes bacterium D08062C1 HM215046 98.4
Lactobacillus ASV6 428 Lactobacillus panisapium Bb 2-3T KX447147 100
ASV10 430 Lactobacillus panisapium Bb 2-3T KX447147 99.8
ASV15 428 Lactobacillus panisapium Bb 2-3T KX447147 99.5
ASV24 429 Lactobacillus melliventris Hma8NT JX099551 99.5
ASV90 429 Lactobacillus panisapium Bb 2-3T KX447147 98.4
ASV135 427 Lactobacillus panisapium Bb 2-3T KX447147 99.5
ASV164 428 Lactobacillus panisapium Bb 2-3T KX447147 95.6
ASV129 430 Lactobacillus huangpiensis F306-1T LC597580 99.8
ASV267 429 Lactobacillus panisapium Bb 2-3T KX447147 99.3
ASV271 427 Lactobacillus panisapium Bb 2-3T KX447147 96.7
ASV292 428 Lactobacillus panisapium Bb 2-3T KX447147 93.7
ASV185 428 Lactobacillus panisapium Bb 2-3T KX447147 97.9
Gilliamella ASV2 428 Gilliamella apicola wkB11 JFON01000004 97.4
ASV3 428 Gilliamella apis NO3T NASD01000045 100
ASV4 428 Gilliamella apicola wkB7 CM004509 98.6
ASV5 428 Gilliamella apis NO3T NASD01000045 96.7
ASV8 428 Gilliamella apicola wkB11 JFON01000004 97.7
ASV13 430 Gilliamella apis NO3T NASD01000045 99.8
ASV14 428 Gilliamella apicola wkB7 CM004509 98.4
ASV22 429 Gilliamella apicola wkB7 CM004509 98.4
ASV28 429 Gilliamella apicola wkB7 CM004509 98.4
ASV30 431 Gilliamella apicola wkB11 JFON01000004 97.5
ASV39 429 Gilliamella apicola wkB11 JFON01000004 97.4
ASV41 427 Gilliamella apicola wkB7 CM004509 98.4
ASV58 427 Gilliamella apicola App2-1 LZGR01000055 99.5
ASV71 428 Gilliamella apicola wkB7 CM004509 98.4
ASV73 429 Gilliamella apicola wkB11 JFON01000004 95.3
ASV96 428 Gilliamella apicola wkB11 JFON01000004 94.0
ASV100 432 Gilliamella bombi LMG 29879T FMWS01000047 95.4
ASV102 431 Gilliamella apicola wkB7 CM004509 96.5
ASV104 432 Gilliamella apis NO3T NASD01000045 97.7
ASV109 428 Gilliamella apicola wkB11 JFON01000004 96.5
ASV138 428 Gilliamella apicola wkB7 CM004509 96.0
ASV149 428 Gilliamella apicola wkB7 CM004509 96.0
ASV162 427 Gilliamella apicola wkB7 CM004509 98.1
ASV170 432 Gilliamella apicola wkB11 JFON01000004 95.4
ASV177 429 Gilliamella apicola wkB11 JFON01000004 97.2
ASV190 428 Gilliamella apicola wkB11 JFON01000004 93.7
ASV207 428 Gilliamella apicola wkB7 CM004509 96.3
ASV231 428 Gilliamella apicola wkB7 CM004509 96.3
ASV275 427 Gilliamella apicola wkB7 CM004509 97.7
ASV298 427 Gilliamella apicola wkB7 CM004509 96.5
Snodgrassella ASV7 428 Snodgrassella alvi wkB298 MEIK01000026 100
ASV17 428 Snodgrassella alvi wkB298 MEIK01000026 99.8
ASV18 428 Snodgrassella alvi wkB298 MEIK01000026 98.6
ASV21 429 Snodgrassella alvi wkB298 MEIK01000026 99.0
ASV25 429 Snodgrassella alvi wkB298 MEIK01000026 98.8
ASV27 430 Snodgrassella alvi WF3-3 MEIO01000062 98.6
ASV31 428 Snodgrassella alvi wkB298 MEIK01000026 98.8
ASV35 428 Snodgrassella alvi wkB298 MEIK01000026 98.4
ASV40 428 Snodgrassella gandavensis LMG 30236T OU943324 98.6
ASV45 428 Snodgrassella gandavensis LMG 30236T OU943324 98.8
ASV60 428 Snodgrassella alvi wkB298 MEIK01000026 98.6
ASV66 430 Snodgrassella alvi WF3-3 MEIO01000026 98.8
ASV111 431 Snodgrassella alvi wkB298 MEIK01000026 98.4
ASV143 429 Snodgrassella alvi wkB298 MEIK01000026 96.5
ASV234 431 Snodgrassella alvi wkB298 MEIK01000026 98.1
ASV235 429 Snodgrassella alvi wkB298 MEIK01000026 96.3
ASV276 433 Snodgrassella alvi wkB298 MEIK01000026 93.5
ASV278 430 Snodgrassella alvi wkB298 MEIK01000026 95.6
ASV307 432 Snodgrassella alvi wkB2T CP007446 93.1
ASV310 431 Snodgrassella alvi wkB298 MEIK01000026 93.7
DOI: 10.7717/peerj.20050/table-2

Notes:

The ASVs showing <98.7% homology against the top-hit taxon are bold.
The superscript T means type strains of the bacteria species.

The result of the NMDS plot of β-diversity of the hindgut microbiota at the ASVs level based on Bray-Curtis dissimilarity is shown in Fig. 2. Pairwise comparisons among the three sampling periods revealed a significant difference in hindgut microbiota composition only between the BO and OW groups (F = 3.037, R2 = 0.121, p = 0.029; Table S7).

Nonmetric multidimensional scaling (NMDS) ordination plots of hindgut microbiota of the Japanese honey bees (Apis cerana japonica) at three sampling periods.

Figure 2: Nonmetric multidimensional scaling (NMDS) ordination plots of hindgut microbiota of the Japanese honey bees (Apis cerana japonica) at three sampling periods.

The plot was generated with the Bray–Curtis dissimilarity index based on the ASVs obtained from each sample. BO, before overwintering; OW, during overwintering; and AO, after overwintering.

Comparison of the core genera among the three periods

The GLMM analysis revealed that the OW group had a significant positive effect on the read counts of Bifidobacterium, Bombilactobacillus, and Lactobacillus (coefficients: 0.977, 1.036, and 0.320; 95% CI [0.237–1.716], [0.138–1.933], and [0.131–0.509]; p = 0.009, 0.024, and 0.001, respectively; Table S8).

Data availability

The raw amplicon sequence datasets generated in this study are available in the DDBJ Sequence Read Archive (accession numbers: DRR685263DRR685298 for DRA Run and PRJDB20791 for BioProject). All scripts and datasets are deposited to figshare under DOI: 10.6084/m9.figshare.29396408.

Discussion

This study revealed that the hindgut microbiota of Apis cerana japonica was dominated by four phyla: Actinobacteriota, Bacteroidota, Firmicutes, and Proteobacteria, and six core bacterial genera: Apibacter, Bifidobacterium, Bombilactobacillus, Gilliamella, Lactobacillus, and Snodgrassella. This finding is consistent with previous studies on the gut microbiota of honey bees (Kwong et al., 2017; Dong et al., 2020). In contrast, compared with the core gut microbiota of A. mellifera, Apibacter is more abundant in Asian honey bee species, such as A. cerana, A. dorsata, and A. andreniformis (Kwong & Moran, 2016; Kwong et al., 2017; Duong et al., 2020; Ellegaard et al., 2020; Khan et al., 2023). The hindgut microbiota of Apis cerana japonica showed a similar trend at the genus level, suggesting that host phylogeny influenced microbial community structure. However, the identification of ASVs with similarities lower than the threshold for distinguishing closely related species suggests the presence of many potentially novel bacterial species, despite their genus-level similarity. Further studies involving bacterial isolation, biochemical characterization, and genome analysis are warranted to elucidate the taxonomy and function of these candidate novel bacteria.

The hindgut microbiota composition of A. c. japonica in the OW group differed significantly from that of the BO group. Notably, the mean relative abundance of Bifidobacterium, Bombilactobacillus, and Lactobacillus in OW group was higher than that in BO group. These three core bacterial genera are known to produce SCFAs from pollen-derived polysaccharides and nectar-derived glucose (Zheng et al., 2017, 2019). Among the SCFAs derived from honey bee gut bacteria, butyrate is absorbed into the hemolymph via the ileum or rectum and is therefore considered an important energy source for thermogenesis to maintain hive temperature during the overwintering period (Den Besten et al., 2013; Zheng et al., 2017). Moreover, genera Bifidobacterium and Lactobacillus contribute substantially to infection control and immune regulation in honey bees through mechanisms such as antimicrobial activity against pathogens (Wu et al., 2013) and upregulating antimicrobial peptide expression (Daisley et al., 2020). Therefore, the genus-level increase in Bifidobacterium, Bombilactobacillus, and Lactobacillus in the OW group may play a beneficial role in the overwintering of honey bees in terms of thermogenesis and immune activation. This study has limitations, as it did not experimentally evaluate the SCFAs-producing capacities or the immunomodulatory effects of Bifidobacterium, Bombilactobacillus, and Lactobacillus. Further studies quantifying SCFA levels in the gut and analyzing the expression of immune-related genes during OW are necessary to clarify the functional roles of these gut bacteria in successful overwintering.

The observed compositional changes in the hindgut microbiota of Apis cerana japonica in the overwintering period are intriguing. A possible contributing factor is the difference in pollen and nectar sources consumed by honey bees before and during overwintering period. Honey bees forage across a wide temperature range (10–40 °C) (Abou-Shaara et al., 2017), but during the overwintering period, when temperatures fall below 10 °C, they rarely leave the hive to forage (Joshi & Joshi, 2010). Consequently, honey bees are more likely to consume stored pollen and honey during overwintering period. Furthermore, the consumption of aged or stored pollen and honey can influence gut microbiota composition through changes in physiological parameters (Maes et al., 2016). In our study, although daily maximum temperatures exceeded 10 °C on all sampling days before and after overwintering period, only one-third of the days during the overwintering period reached this threshold (Japan Meteorological Agency, 2025). Another factor that may influence hindgut microbiota is variations in hive temperature. Typically, the hive temperature is maintained at 33–35.5 °C (Abou-Shaara et al., 2017). In A. c. japonica, the average winter hive temperature is 30.7 °C, while the average temperature before and after winter is 34.3 °C (Akimoto, 2000). This temperature fluctuation may affect bacterial growth rates, thereby altering microbiota composition (Ludvigsen et al., 2015; Kešnerová et al., 2017).

It is important to note that slight differences in microbiota composition were observed among colonies. Differences in gut microbiota between colonies have been reported to be influenced by the diet collected from habitat-specific floral sources (Castelli et al., 2022; Ricigliano, Williams & Oliver, 2022) and host genotype (Bridson et al., 2022). Our findings highlight the necessity of considering variation among colonies when evaluating seasonal changes in the hindgut microbiota of honey bees.

Conclusions

This study on the hindgut microbiota of A. c. japonica revealed the influence of phylogeny on microbiota composition, the presence of potentially novel species, and distinctive compositional changes during the overwintering period. The biochemical properties of the genera that increased during overwintering period (i.e., genera Bifidobacterium, Bombilactobacillus, and Lactobacillus) suggest that these changes supply energy for thermogenesis and activate the host immune system. Further surveys in other regions with different dietary environments and studies focusing on elucidating the functional roles of hindgut microbiota during overwintering and their symbiotic relationship with host health are warranted.

Supplemental Information

Supplementary figure and tables.

DOI: 10.7717/peerj.20050/supp-1

Raw forward sequence data of X12-3.

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Raw forward sequence data of X3-1.

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Raw forward sequence data of X12-1.

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Raw reverse sequence data of X12-2.

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Raw forward sequence data of X10-1.

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Raw forward sequence data of X3-3.

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Raw reverse sequence data of X3-1.

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Raw reverse sequence data of X10-1.

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Raw reverse sequence data of X12-1.

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Raw forward sequence data of X3-2.

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Raw forward sequence data of X10-3.

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Raw reverse sequence data of X10-3.

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Raw reverse sequence data of X10-2.

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Raw reverse sequence data of X3-2.

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Raw reverse sequence data of X3-3.

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Raw forward sequence data of X12-2.

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Raw forward sequence data of X10-2.

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Raw reverse sequence data of X12-3.

DOI: 10.7717/peerj.20050/supp-19

Raw reverse sequence data of T10-2.

DOI: 10.7717/peerj.20050/supp-20

Raw reverse sequence data of T3-2.

DOI: 10.7717/peerj.20050/supp-21

Raw reverse sequence data of T12-1.

DOI: 10.7717/peerj.20050/supp-22

Raw reverse sequence data of T3-1.

DOI: 10.7717/peerj.20050/supp-23

Raw reverse sequence data of T3-3.

DOI: 10.7717/peerj.20050/supp-24

Raw reverse sequence data of T10-1.

DOI: 10.7717/peerj.20050/supp-25

Raw forward sequence data of T10-1.

DOI: 10.7717/peerj.20050/supp-26

Raw forward sequence data of T10-2.

DOI: 10.7717/peerj.20050/supp-27

Raw forward sequence data of T12-1.

DOI: 10.7717/peerj.20050/supp-28

Raw forward sequence data of T12-2.

DOI: 10.7717/peerj.20050/supp-29

Raw forward sequence data of T3-2.

DOI: 10.7717/peerj.20050/supp-30

Raw forward sequence data of T10-3.

DOI: 10.7717/peerj.20050/supp-31

Raw reverse sequence data of T12-2.

DOI: 10.7717/peerj.20050/supp-32

Raw reverse sequence data of T12-3.

DOI: 10.7717/peerj.20050/supp-33

Raw reverse sequence data of T10-3.

DOI: 10.7717/peerj.20050/supp-34

Raw forward sequence data of T12-3.

DOI: 10.7717/peerj.20050/supp-35

Raw forward sequence data of T3-1.

DOI: 10.7717/peerj.20050/supp-36

Raw forward sequence data of T3-3.

DOI: 10.7717/peerj.20050/supp-37

Raw forward sequence data of I3-1.

DOI: 10.7717/peerj.20050/supp-38

Raw reverse sequence data of I12-3.

DOI: 10.7717/peerj.20050/supp-39

Raw forward sequence data of I12-3.

DOI: 10.7717/peerj.20050/supp-40

Raw forward sequence data of I3-2.

DOI: 10.7717/peerj.20050/supp-41

Raw reverse sequence data of I12-1.

DOI: 10.7717/peerj.20050/supp-42

Raw reverse sequence data of I10-3.

DOI: 10.7717/peerj.20050/supp-43

Raw reverse sequence data of I10-1.

DOI: 10.7717/peerj.20050/supp-44

Raw forward sequence data of I3-3.

DOI: 10.7717/peerj.20050/supp-45

Raw reverse sequence data of I3-2.

DOI: 10.7717/peerj.20050/supp-46

Raw forward sequence data of I10-3.

DOI: 10.7717/peerj.20050/supp-47

Raw reverse sequence data of I3-1.

DOI: 10.7717/peerj.20050/supp-48

Raw forward sequence data of I10-1.

DOI: 10.7717/peerj.20050/supp-49

Raw reverse sequence data of I3-3.

DOI: 10.7717/peerj.20050/supp-50

Raw forward sequence data of I12-2.

DOI: 10.7717/peerj.20050/supp-51

Raw reverse sequence data of I12-2.

DOI: 10.7717/peerj.20050/supp-52

Raw forward sequence data of I10-2.

DOI: 10.7717/peerj.20050/supp-53

Raw reverse sequence data of I10-2.

DOI: 10.7717/peerj.20050/supp-54

Raw forward sequence data of I12-1.

DOI: 10.7717/peerj.20050/supp-55

Raw forward sequence data of H10-1.

DOI: 10.7717/peerj.20050/supp-56

Raw forward sequence data of H10-2.

DOI: 10.7717/peerj.20050/supp-57

Raw forward sequence data of H12-2.

DOI: 10.7717/peerj.20050/supp-58

Raw reverse sequence data of H3-2.

DOI: 10.7717/peerj.20050/supp-59

Raw reverse sequence data of H12-1.

DOI: 10.7717/peerj.20050/supp-60

Raw reverse sequence data of H12-3.

DOI: 10.7717/peerj.20050/supp-61

Raw reverse sequence data of H10-2.

DOI: 10.7717/peerj.20050/supp-62

Raw forward sequence data of H3-3.

DOI: 10.7717/peerj.20050/supp-63

Raw forward sequence data of H10-3.

DOI: 10.7717/peerj.20050/supp-64

Raw forward sequence data of H3-1.

DOI: 10.7717/peerj.20050/supp-65

Raw forward sequence data of H12-1.

DOI: 10.7717/peerj.20050/supp-66

Raw reverse sequence data of H10-1.

DOI: 10.7717/peerj.20050/supp-67

Raw reverse sequence data of H10-3.

DOI: 10.7717/peerj.20050/supp-68

Raw reverse sequence data of H3-3.

DOI: 10.7717/peerj.20050/supp-69

Raw reverse sequence data of H12-2.

DOI: 10.7717/peerj.20050/supp-70

Raw forward sequence data of H3-2.

DOI: 10.7717/peerj.20050/supp-71

Raw forward sequence data of H12-3.

DOI: 10.7717/peerj.20050/supp-72

Raw reverse sequence data of H3-1.

DOI: 10.7717/peerj.20050/supp-73