2.1. Copper
Copper (Cu) is an essential mineral for all living organisms [
80], participating in various biological processes. In bacteria it is found as a cofactor in proteins and enzymes due to its redox potential, acting as an electron donor/acceptor by alternating between the reduced cuprous form [Cu(I) or Cu+] and the oxidized cupric form [Cu(II) or Cu2+], critical for a wide range of cellular metabolic and regulatory functions [
81,
82,
83] (e.g., electron transport, oxidative respiration, denitrification, etc.) [
84,
85]. However, in certain forms and concentrations, it can be toxic and inhibit or kill bacteria [
86,
87].
The antimicrobial properties of copper are well described [
87] and its use dates back to ancient Egypt for the preservation of water and food, as well as for medical applications [
88]. In the agri-food sector, copper-based compounds have been used as antimicrobial since the end of the 19th century, when its activity as fungicide was first described, being used as the “Bordeaux mixture” in vineyards [
89]. Since then, it has been widely used in pesticides and fertilizers [
90,
91]. Although the role of copper as an antimicrobial agent was widely recognized in the past, it lost significance with the advent of antibiotics [
92]. However, the biocidal properties of copper against a wide range of pathogens have made it regain importance as a promising alternative in the fight against the spread of MDR bacteria [
92]. Among the currently authorized copper applications in the EU are several copper-based biocidal products not intended for direct application to humans or animals [
93]. In recent years, the use of copper plating of surfaces, including in the food and medical sectors [
94,
95,
96,
97], has been proposed as a more effective measure to limit bacterial adhesion than stainless steel [
87], being the first solid antimicrobial material registered with the U.S Environmental Protection Agency [
92]. Other antimicrobial applications of copper have been made, most in clinical settings (e.g., medical devices such as copper-impregnated fabrics) [
98,
99,
100,
101].
Although copper is commonly known for its antimicrobial properties, it also plays a crucial role in human and veterinary medicine in the treatment of nutritional deficiencies [
58]. In food-producing animals, feed is routinely supplemented with copper not only to meet the animals’ nutritional needs but also to improve their growth performance by modulating the gastrointestinal tract microbiota, leading to improved nutrient absorption [
102]. Varying concentrations of copper are used, depending on the species, age group and feed composition, as copper can interact with other nutrients, including other metals (e.g., zinc, iron, calcium, molybdenum) and phytates [
103]. As an example, the maximum concentration allowed in poultry feed is 25 mg Cu/kg, while in piglets up to 4 weeks after weaning it is 150 mg Cu/kg and from the 5th to the 8th week after weaning it is 100 mg Cu/kg [
66]. Traditionally, feed supplementation with inorganic trace mineral (ITM) copper has been used as a cost-effective solution ([
104,
105], but the use of other forms, mainly organic species (organic trace mineral, OTM) and copper nanoparticles, has been increasing, as they present higher bioavailability, improving animals’ growth performance, with a less environmental impact [
105,
106,
107]. The application of copper nanoparticles has also been exploited in the food industry and agriculture sectors, mainly to prevent microorganism spoilage (e.g., in food packaging) [
108] and as agro-nanochemicals (e.g., fertilizers and pesticides) with a larger specific surface area than conventional forms [
109]. However, the widespread use of copper-based compounds in many anthropogenic activities has led to its accumulation in different ecosystems, making it a pollutant and potentially toxic to many organisms, including bacteria.
Copper poses a unique challenge to bacteria due to its dual nature – it is an essential trace mineral, but it can also be cytotoxic when present in excess. This ambivalence highlights the importance of strict regulation of cellular copper levels [
110]. Maintaining copper homeostasis requires a delicate balance between providing the required dose of the micronutrient while avoiding toxic excess [
56,
111]. Although the mechanisms of how copper ions affect bacteria are still not fully understood, it seems that the cycling between the cupric [Cu(II)] and the cuprous [Cu(I)] states can disturb the intracellular redox potential, being the main cause of cytotoxicity. In particular, the intracellular soluble fraction of copper [Cu(I)], via a Fenton-like reaction, catalyzes the formation of superoxide (O
2-) and other reactive oxygen species [hydroxyl radicals (OH⋅) and hydrogen peroxide (H
2O
2)], which are responsible for lipid peroxidation, protein oxidation and DNA damage [
112]. Under low oxygen conditions, the reduced ionic species Cu(I) is prevalent and is highly toxic, showing great affinity for thiolates and other sulfur-containing compounds, disrupting the binding of iron-sulfur (Fe-S) clusters, leading to poor protein metallation, protein inactivation and ultimately to dysfunctional cell metabolism [
112,
113,
114]. In human macrophages, copper is pumped to their phagosomes after engulfing pathogenic bacteria to induce bacteria death by oxidative stress [
115].
Copper can often enter the bacterial cells in an unspecific manner by using other metal uptake systems, making it difficult for bacteria to limit the amount of copper entering the cytoplasm [
56]. Bacteria have evolved a number of mechanisms implicated in the uptake, internal traffic, storage and efflux of copper from the cell, including the extracellular sequestration of copper ions, the relative impermeability of outer and inner bacterial membranes to copper ions, the presence of metallothionein-like copper-scavenging proteins in the cytoplasm and periplasm, and the active extrusion of copper from the cell [
92].
The extrusion of excess cytoplasmic copper by homeostatic mechanisms appears to be the main defense mechanism in bacteria, a process that has been extensively studied in both Gram-positive and Gram-negative bacteria [
92]. Specifically, copper efflux occurs through transporters, members of the P
1B-1-ATPase subfamily [Cu(I) transporters] of P
1B-ATPases [
116]. The first copper-transporting ATPases were described in
Enterococcus hirae [
117,
118], represented by the cop operon (
copYZAB), which formed by four genes coding for the following proteins: CopA and CopB, responsible for the uptake and removal of excess Cu(I) from the cytoplasm, respectively [
119]; CopZ, a chaperone responsible for intracellular copper transport; and CopY, a promoter regulator [
120,
121]. Unlike to Gram-positive bacteria which lack a periplasmic space and an outer membrane, Gram-negative bacteria require additional mechanisms to deal with the presence of copper in the periplasm. In the most studied Gram-negative bacterium,
E. coli, in addition to the presence of the Cu(I)-translocating P-type ATPase CopA in the cytoplasmic membrane, responsible for pumping excess Cu(I) from the cytoplasm to the periplasm [
122], there is also the CusCBA multicomponent copper efflux system and the CueO multicopper oxidase. These two systems are chromosomally encoded and play important roles in controlling copper level and redox state, respectively [
56]. Since CueO acts only in the presence of oxygen, presumably oxidizing Cu(I) into the less toxic Cu(II) [
56], the CusCBA transport complex is important to copper detoxification from the periplasm in the absence of CueO [
123]. In
Salmonella, copper defense determinants are quite similar to those of wild-type
E. coli, also containing CopA and CueO. However, most
Salmonella strains do not contain the CusCBA system, instead having the periplasmic copper-binding protein CueP [
112].
In environments with high copper concentrations, which would overwhelm chromosomally encoded copper metabolic systems, some bacteria have acquired copper tolerance mechanisms, regulated mainly by extrachromosomal loci [
124]. The first mechanism described in Gram-negative bacteria was identified in the pRJ1004 plasmid of an Australian pig
E. coli isolate [
125], linked to the presence of the
pco (plasmid-borne copper resistance) system. This system includes different structural proteins, including PcoA, a periplasmic multicopper oxidase, PcoB and PcoD, outer and inner membrane proteins, respectively, and PcoC and PcoE, two periplasmic proteins [
125,
126,
127,
128]. While PcoE is responsible for temporarily sequestering excess copper [
128], PcoC is also capable of transferring it to the membrane-bound PcoD [
56]. In turn, PcoD catalyzes the uptake of Cu(I) into the cell, which is incorporated into PcoA and exported to the periplasm, where it will be detoxified either by sequestration or oxidation and removed via PcoB (
Figure 3) [
129]. A two-component regulatory system, PcoRS, seems to be responsible for the transcription of PcoABCD proteins [
126], while the chromosomally encoded CusRS system regulates the transcription of PcoE protein [
128]. Two additional proteins, PcoF and PcoG, corresponding to a putative copper-binding protein and a putative metallopeptidase, respectively, may be present, but their role has yet to be determined [
130]. The
pco gene cluster encodes proteins responsible for periplasmic copper management, being dependent on the supply of copper by the cytoplasmic CopA protein to confer copper tolerance to bacteria [
110]. Contiguous to the
pco system in pRJ1004 is the
sil gene, first described in the
S. Typhimurium plasmid pMG101, and initially linked to silver tolerance [
131]. The Sil system includes a SilCBA efflux complex responsible for exporting Cu(I) and Cu(II) from the periplasm, three periplasmic proteins, SilE [homolog to PcoE, presumably to bind Cu(I) and Cu(II)], SilF and SilG, the first two acting as chaperones of the SilCBA complex and the last one with unknown function, as well as a P-type ATPase SilP that transports copper and silver ions from the cytoplasm to the periplasm [
132]. The two-component membrane sensor and transcriptional responder SilRS appear to be involved in silCFBAGP expression [
130]. The occurrence of
sil efflux systems is associated with a CuSO
4 tolerance phenotype in several
Enterobacteriaceae under anaerobic conditions, where the more toxic form Cu(I) is predominant, a distinct feature of isolates carrying
sil±
pco genes in comparison with those without it [
44,
133,
134,
135]. A minimum inhibitory concentration (MIC) for CuSO
4 between 16-36 mM has been described in isolates with
sil±
pco, contrasting with a MIC
CuSO4 between 2-12 mM in isolates without these genes [
44,
133,
134], being proposed a CuSO
4 tolerance cut-off ≥ 16 mM to differentiate isolates with and without
sil±
pco gene clusters, under anaerobioses [
44,
134].
Since the entire
sil determinant confers copper tolerance, the contiguous 20-gene clusters of
pco+
sil have been referred to as copper-pathogenicity island [
130]. Although the
pco+
sil determinants were initially identified in plasmids, it is worth noting that this gene cluster may also be located on chromosome [
133,
134], due to the bacteria genetic plasticity, which is often facilitated by the presence of Tn7-like transposons [
134,
136,
137]. Several studies have been describing the wide occurrence and distribution of
sil-
pco clusters in diverse species and multiple environments, including food and food-producing animals [
134,
138], hospitals and urban wastewaters [
139], freshwaters [
140], veterinary clinical settings [
141] and human clinic [
134].
Gram-positive bacteria with high acquired tolerance to copper have also been described, namely in several species of
Enterococcus genus. The most characterized gene is the plasmid encoded
tcrB (transferable copper resistance gene B) initially identified in an
E. faecium isolate from pigs in Denmark [
142]. The
tcrB gene codes for an efflux pump, presumably belonging to the P
1B-3-ATPase subfamily of copper transporters P
1B-ATPases, which is activated mainly by Cu(II) and to a lesser extent by Cu(I) [
129,
143]. This gene is part of the
tcrYAZB operon (homologous to the
copYZAB copper-homeostasis gene cluster of
E. hirae) [
144], together with the
tcrA gene, an additional P
1B-ATPase of the P
1B-1-ATPase subfamily and responsible for Cu(I) export, the
tcrZ gene, which encodes a cytoplasmic copper chaperone (TcrZ) responsible for Cu(I) transport, and the
tcrY gene, a copper-dependent regulator (TcrY) involved in controlling operon expression (
Figure 4) [
142,
144]. These copper tolerant determinants are often flanked by insertion sequences, allowing their transferability [
145,
146,
147].
As the
sil efflux systems, the acquisition of the
tcrYAZB operon represents a clear advantage for bacteria in anaerobic environments, allowing them to survive in higher Cu concentrations [
148].
Enterococcus spp. carrying
tcrYAZB operon have shown a MIC
CuSO4 between 16-36 mM, while in isolates without these genes the MIC
CuSO4 ranged between 4-12 mM [
148,
149,
150]. Thus, a CuSO
4 tolerance cut-off ≥ 16 mM was proposed to differentiate isolates with and without
tcrB gene, under anaerobic conditions [
148]. In the vicinity of the
tcrYAZB operon is often a multicopper oxidase (CueO), potentially involved in the oxidation of Cu(I) to Cu(II) [
145].
As in Gram-negative bacteria, the
tcrYAZB operon genes are located mainly in plasmids [
142,
146,
149], unlike chromosomal genes related to copper homeostasis [
151]. Since the first description of the
tcrYAZB operon in the pA17sv1 plasmid of an
E. faecium from a healthy pig [
144], the presence of the
tcrB gene has been mainly associated with
Enterococcus genus isolates from food-animal production environments [
145,
146] and foodstuffs [
145,
149,
152], with few studies describing its occurrence in humans (clinical and community isolates) and aquatic environments [
145,
148].
A major issue is that copper tolerance has been strongly associated with antibiotic- resistant bacteria in different environments (e.g., aquatic, animal-food production, agri-food, clinical settings) [
153,
154,
155], including those without antimicrobial pressure (e.g., pristine environments) [
75]. Co-selection of copper tolerance genes and ARGs often occurs because they all share the same genetic elements [
146,
150,
156]. Shortly after the first description of the
tcrB gene, a link to macrolide and glycopeptide resistance was established by the co-occurrence of such resistance determinants on the same conjugative plasmid of porcine
E. faecium [
142,
156]. More recently, other ARGs (e.g.,
vanA- vancomycin;
tet(M) or
tet(L)-tetracycline;
aadE-streptomycin;
aac(6’)-Ie-aph(2’’)-Ia-gentamycin) have also been described in the same
Enterococcus plasmids as the
tcrYAZB operon and other metals in
Enterococcus spp. of the food-chain and other niches [
149,
150]. A single description of
tcrYAZB on the chromosome is available for
E. faecalis from poultry meat alongside mercury (
merA) tolerance genes [
149]. Plasmids carrying
sil±
pco genes (and other metal tolerance genes, including to mercury –
mer genes) and ARGs for beta-lactams (
blaTEM-1,
blaCTX-M), aminoglycosides [
aac(3),
aadA], sulfonamides (
sul), trimethoprim (
dfrA), chloramphenicol (
cmlA) and tetracyclines (
tet) have also been described in
E. coli,
Klebsiella pneumoniae and
S. enterica isolates from food-producing environments and human sources [
133,
134,
157,
158]. In addition, chromosomal co-localization of copper (
pco+
sil) with other metal tolerance genes (e.g.,
mer) and ARGs for beta-lactams (
blaTEM-1), aminoglycosides (
aadA,
str) sulfonamides (
sul), trimethoprim (
dfrA) and tetracyclines (
tet) was described in
S. enterica isolates from various sources (animal-food production; food; human) [
133,
134]. Cross-resistance and co-regulation mechanisms have been poorly described, with some studies suggesting the role of efflux systems (e.g., membrane transporters belonging to the RND family) in the extrusion of both copper and antibiotics (e.g., cefotaxime) in some Gammaproteobacteria [
159,
160], and overexpression of some binding proteins (e.g., Rob encoded by
robA gene) associated with increased resistance to metals (including copper) and multiple antibiotics (e.g., tetracycline, chloramphenicol) in
E. coli [
161].
2.2. Arsenic
Arsenic (As) is a metalloid naturally present in the earth’s crust and widely distributed in soil, sediments, water, air and living organisms [
162,
163]. Unlike other elements (e.g., copper, zinc), arsenic is not required for biological functions in most bacteria, exerting a toxic effect on the cell [
164,
165]. The toxicity of arsenic greatly depends on its oxidation state, and it can occur in four valence states: As
3- (arsine gas, AsH
3), As
0 (elemental arsenic), As
3+ (trivalent arsenic or arsenite) and As
5+ (pentavalent arsenic or arsenate) [
166]. Arsenite and arsenate are the predominant species under reduced and oxygenated conditions, respectively, the former being 100 times more toxic than the pentavalent form [
166].
Regardless of its ubiquitous distribution and the contribution of natural processes to increasing environmental arsenic contamination (e.g., mineralized and mined areas, volcanogenic activity, thermal springs and Holocene alluvial sediments) [
167], it is human activity that has greatly contributed to increase arsenic concentrations in different environments [
163]. Arsenic or arsenic-based compounds have historically been used in a range of applications, including pharmaceuticals, wood preservatives, agricultural chemicals (e.g., pesticides, cotton desiccants, defoliants and soil sterilant) and in industry (e.g., mining, and metallurgy) [
162]. Inorganic arsenic compounds have been used in medicine since 2000 BC, when arsenic trioxide (As
2O
3, commonly referred to as ATO) was used as both a drug and a poison [
168]. Over time, the use and development of arsenicals in medicine has evolved, with important milestones including its use by Hippocrates to treat skin cancers (using orpiment – As
2S
3, and realgar – As
4S
4) and its recommendation by Paracelsus for use in medicine [
168]. After the 17th century, ATO became widely used as a drug to cure headaches and specifically to treat trypanosomiasis, syphilis and leukemia [
168]. Currently, ATO is still used as an anticancer chemotherapeutic agent for hematological diseases, listed as one of the essential medicines by the World Health Organizations [
169]. Although arsenic has this history of use in medicine, it is the agricultural and industrial sectors that have contributed the most to environmental pollution by arsenic. In agriculture and animal-farming, arsenic-based compounds have been extensively in pesticides [e.g., sodium arsenite or sodium arsenate, Na
2HAsO
3/Na
2HAsO
4; calcium arsenite or calcium arsenate, Ca(AsO
2)
2/Ca
3(AsO
4)
2], as coccidiostats and as a feed additive, mainly in the poultry and swine industries [
57,
168,
170]. Roxarsone, a pentavalent nitroaromatic arsenical, has been used exclusively for animal husbandry, particularly poultry, to promote growth, treat coccidiosis and prevent gastrointestinal infections [
57]. Despite possible accumulation in animals’ meat [
57], most of the roxarsone ingested by animals is excreted in feces and urine, which might contribute to its accumulation in and around the animal production environment (e.g., manure, waste lagoons, amended soils) [
171,
172]. For this reason, roxarsone is now banned in several countries around the world (e.g., EU countries, USA and China) [
173,
174].
Although many arsenic compounds are no longer used, their residues persist from past activities. A recent study showed that arsenic concentrations in more than half of European agricultural soils exceeded the threshold of 5 mg/kg [
175], posing a threat to the environment, food safety and human health. Moreover, concentrations found in animal-production environments (e.g., total arsenic in manure: ~0.016-2.5 mM; sludge: ~0.15 mM; feed: ~0.0003-0.174 mM) [
176,
177,
178,
179], suggest that arsenic may create a selective pressure on bacteria in these environments, favoring the selection of those with tolerance to arsenic (and other metals), with particular concern for MDR zoonotic bacteria [
180].
Throughout Earth’s evolutionary history, bacteria have always been exposed to arsenic in different environments and have evolved numerous mechanisms to deal with it, either through detoxification or metabolic pathways [
181,
182]. Several arsenic biotransformation systems have been identified in bacteria, most of which are associated with detoxification processes. These include the arsenic resistance efflux system (
ars), arsenic methylation and associated pathways (e.g.,
arsM), as well as metabolic processes such as arsenite oxidation (aio/arx) and reduction (arr) systems (
Figure 5) [
181].
Arsenic metabolic pathways involving biotransformation between As
3+ and As
5+ (aio/arx and arr systems), represent an important energy-generating process in the respiratory process of some bacteria [
182,
184]. However, for most bacteria, arsenic is not essential, which explains the absence of specific arsenic uptake systems [
165]. In fact, the analogy of some arsenic species with other molecules allows arsenic entrance into bacterial cell via non-specific intrinsic transporters [
185]. For example, arsenate is a phosphate analogue, entering to cell through phosphate transporters (Pit or Pst) (
Figure 5) and inhibiting phosphorylation reactions (such as glycolysis and ATP production) [
186]. However, it is unstable and can rapidly dissociate into the more toxic trivalent arsenite (As
3+) [
187]. Arsenite has a structural similarity to glycerol and enters the cell via aqua-glycerolporins (GlpF), the glycerol transport system (
Figure 5) [
165,
181]. The greater toxicity of arsenite is related to its ability to bind strongly with sulfhydryl groups in proteins, impairing the function of many proteins important for biochemical processes, and to bind weakly to other small thiol molecules (glutathione, lipoic acid, and cysteine), affecting respiration [
184,
186].
To cope with continued exposure to arsenic toxicity, most bacteria have evolved and acquired genes for arsenic detoxification, mostly encoded by
ars operons (
Figure 5), often found among prokaryotic genomes, either on chromosomes or on plasmids of Gram-positive and Gram-negative bacteria [
165,
181,
184,
188], which reflects its ubiquitous presence in nature. The first description of arsenic tolerance genes occurred more than 50 years ago, when a clinical strain of
S. aureus was identified as carrying a plasmid (pI258) conferring tolerance to arsenate, arsenite and other metals and resistance to antibiotics [
189]. Shortly thereafter, another plasmid (R773) identified in a clinical strain of
E. coli also revealed the occurrence of arsenic tolerance genes [
190]. In both cases,
ars operons involved in the arsenic tolerance phenotype were identified, encoding homologous proteins, but with different configurations: the three-gene
arsRBC operon in the
Staphylococcus pI258 plasmid and the extended five-gene
arsRDABC operon in the
E. coli R773 plasmid [
184]. In fact, several genomic configurations of
ars operons have been described and suggested to be strain-specific [
165,
184]. Most of
ars operons are involved in inorganic arsenic detoxification, although coupling with other
ars-related genes also allows for organoarsenicals detoxification (
Figure 5) [
181]. In both types of
ars operons, the core genes include a trans-acting transcriptional repressor protein (ArsR) that binds to the promoter region of the
ars operons, an arsenite efflux pump (ArsB) and an arsenate reductase (ArsC) (
Figure 5) [
184]. ArsR interacts with arsenite, dissociating the repressor protein from DNA, thereby downregulating transcription of other
ars operon genes [
184,
191]. ArsB is an integral membrane protein responsible for the extrusion of arsenite [As(OH)
3/H
+ antiporter) from the cell cytoplasm, representing the basic mechanism of arsenite detoxification by decreasing its accumulation [
192]. ArsB activity can involve two types of energy sources: acting independently on the arsenite transport channel, using the membrane potential to catalyze the extrusion of As
3+ from the cell; or acting in conjugation with ArsA (in the case of operons
arsRDABC), to potentiate arsenic tolerance to a higher degree [
181]. Specifically, the ArsA ATPase protein catalyzes the hydrolysis of ATP, which energizes the arsenite efflux pump, forming the ArsA-ArsB membrane-bound complex (
Figure 5). The ArsC protein is an arsenate reductase enzyme, capable of reducing intracellular arsenate to arsenite, which will then be extruded out of the cell through the ArsB pump [
193]. Finally, the ArsD protein, which occurs in the extended
ars operons (
arsRDABC), is a metallochaperone responsible for sequestering cytosolic arsenite and transferring it to the ArsA subunit of the efflux pump, increasing the efficiency of arsenic extrusion (
Figure 5) [
192].
Genomic analysis has been contributed to identify the existence of atypical
ars clusters [
194,
195] or the occurrence of additional genes associated with these clusters and involved in arsenic tolerance genes, including the
acr3 gene [
196,
197]. Acr3 (also known as ACR3 or ArsY) is a member of the BART (bile/arsenite/riboflavin transporter) superfamily, first reported in the
arsRBC operon of
B. subtilis as a typical ArsB membrane protein (
Figure 5) [
184]. In fact, the literature often describes members of the Acr3 family as ArsB-type, even though they do not exhibit significant sequence similarity to ArsB [
198]. While the ArsB-type is mostly restricted to bacteria, including Bacillota (formerly Firmicutes) and Pseudomonadota (formerly Proteobacteria) [
180,
199,
200], the Acr3-type family has a wide distribution, also being found in archaea and eukaryotes (mainly fungi and some plants) [
187,
201,
202]. Interestingly, a predominance of
acr3 over
arsB genes was found in arsenic tolerant bacterial isolates from arsenic-contaminated soils, and in some cases, concurrently with the
arsB gene [
203]. However, no evidence of the coexistence of the two transporters encoded in the same operon has been reported so far [
202]. As with the ArsB-type, Acr3 can also couple with ArsA to form a more efficient arsenite efflux system [
201]. A phenotype of increased arsenate (sodium arsenate Na
2AsO
4) tolerance was observed in Gram-positive (
Enterococcus spp.) and Gram-negative (
Salmonella enterica) bacteria with arsenic tolerance genes (
arsA,
arsB or
acr3) compared to those without these genes, with MICs ranging between 8 and ≥ 128 mM and between 0.5 and 4 mM, respectively, regardless of the atmosphere used (aerobic or anaerobic) [
150,
180].
The wide distribution of arsenic tolerance genes in bacteria from diverse sources (environment, food, clinical) reflects not only the ubiquitous nature of this metal, but also bacteria adaptive characteristics. In particular, arsenic tolerance genes (
arsA/
arsB/
acr3) have been predominantly found in bacteria from natural environmental sites, regardless of whether they had a history of arsenic contamination, including soils (from forests or close to gold mining activities or geothermal effluents), creek water and sewage [
200,
203,
204,
205]. Additionally, other contexts have been associated with the occurrence of arsenic tolerance genes, such as clinical (e.g., human samples, clinical settings) [
141,
206] and food-associated environments (e.g., food-producing animals, processing plants, food products) [
206,
207]. In animal-food production environments, arsenic can accumulate and persist in sublethal concentrations, leading to long-term selective pressure on bacteria, which favors those with reduced susceptibility to arsenic and other antimicrobials (metals and antibiotics) [
154]. In fact, there is growing evidence of the wide dispersion of arsenic tolerance genes in these environments, ranging from animals to other variable stages in food production, including raw, processed, and ready-to-eat animal products (e.g., swine, poultry, cattle), associated or not with foodborne pathogens [
207,
208,
209].
The co-localization of arsenic and other metal tolerance operons (e.g., mercury and copper) in the same genetic context have been described, either in plasmids or in chromosomal regions. These genetic regions have been pointed as potential hotspots for the accretion of metal tolerance genes, either in bacteria with an environmental lifestyle (e.g.,
Alteromonas sp.) or food-chain associated bacteria (e.g.,
Listeria sp.,
Salmonella sp.) [
206,
210]. Furthermore, arsenic tolerance genes have been described as being on the same mobile genetic elements as other metal tolerance genes or ARGs, including in plasmids (e.g.,
E. coli,
Klebsiella,
Listeria monocytogenes,
E. faecalis) [
44,
188,
211], or ICEs (Integrative Conjugative Elements) (e.g.,
S. Typhimurium) [
212]. The variability of mobile genetic elements carrying arsenic tolerance genes may favor their horizontal transfer between bacterial hosts. Also, when integrated and fixed in the chromosome, arsenic tolerance genes can confer a lower fitness cost to bacteria and be spread by vertical transmission. In all cases, there is a selective advantage for bacterial survival, particularly in food-animal production or other metal polluted environments. In fact, arsenic-polluted environments (e.g., water reservoirs, urban soils) have been described as contributing to the co-selection of ARGs [e.g., for aminoglycosides –
aadA/
aacC, beta-lactams –
blaCMY/
ampC, MLSB –
erm(F) tetracyclines –
tet(B)] and mobile genetic elements (e.g., integron –
intI-1, transposon – Tn
21/Tn
22/Tn
24/Tn
614) [
213,
214]. The occurrence of arsenic and other metals (e.g., copper, zinc, cadmium, lead) in a Chinese poultry production environment has also recently been found to have a greater impact on MeT and ARGs gene composition than some antibiotics, showing a positive correlation between arsenic concentrations and resistance genes to aminoglycosides [aac(6’)-Ia], macrolides (
erm35), bacitracin (
bacA) and, in particular, with resistance genes to tetracycline (
tet genes), probably promoted by co-selection events [
154].
2.3. Mercury
Mercury (Hg) is a highly toxic heavy metal widely dispersed in nature [
215]. Like arsenic and other heavy metals, mercury is a non-essential element for living organisms, with no known beneficial function for cells [
216]. The toxicological properties of mercury depend on the different chemical forms in which it can occur [
217]. In the environment and in biological systems, mercury can be present in three oxidation states, namely, elemental mercury (Hg
0) (known as metallic mercury, a highly volatile liquid, at room temperature), and the mercuric [Hg
2+ /Hg(II)] and mercurous [Hg
+/Hg(I)] forms [
218]. It can also occur as organic (or organomercuric) forms, such as the methylmercury (MeHg) ion (HgCH
3+) and its compounds methylmercury chloride (CH
3HgCl), methylmercury hydroxide (CH
3HgOH), dimethylmercury and phenylmercury, identified as the most toxic forms of Hg [
219,
220]. The occurrence of these different chemical species depends on the environmental physicochemical features and how they are metabolized by different biological processes that occur in the local microbiota [
217]. While Hg
0 occurs mainly in the atmosphere, mercuric species [Hg(II)] are dominant in water, soil and sediments and methylmercury (MeHg) in biota [
221].
Mercury is a natural component of the Earth’s crust, often found as salts such as mercury sulfide (HgS, known as cinnabar) and other sulfate minerals (e.g., HgSO
4), mercury oxide (HgO), mercury chloride (HgCl
2) or as elemental mercury [
222]. It can be released into atmosphere through natural events such as volcanic activity, geothermal sources, biomass burning, and soil-water-air exchanges [
223]. Both biotic (including bacteria) and abiotic (e.g., meteorological conditions, human activity) processes are involved in the transformation of mercury (geochemistry mercury cycle) into different inorganic and organic forms, as well as the gaseous element that returns to the atmosphere and contributes to its wide dispersion [
224]. Nonetheless, 75% of the global mercury input and distribution to the environment is caused by extensive anthropogenic use [
225], making it one of the most prevalent and persistent environmental pollutants [
215].
Historical records reveal the use of quicksilver (liquid metallic mercury) in ancient Greek, Indian, Persian, Arabic and Chinese medicine and alchemy [
226,
227]. In fact, it has been employed in traditional Chinese medicine for over 3000 years [
226]. Additionally, evidence suggests that this metal was used as a preservative in Egyptian tombs [
226]. Mercury compounds gained significant importance in medical applications during the late 15th century in Europe, particularly in the treatment of syphilis [
228]. Moreover, the use of mercury became common in the 20th century in many applications (e.g., dental amalgam fillings; drug preservative; antiseptics) [
217,
229,
230]. Currently, it is still used in very small amounts as a preservative in some human and animal vaccines and pharmaceuticals, in the form of ethylmercury (known as thiomersal) [
59]. In the agri-food sector, mercury was also used for decades, until the mid/late 20th century, in pesticides, mainly insecticides and fungicides, in the form of mercurous chloride and ethylmercury [
230,
231,
232]. Although mercury contamination from industrial sources has declined globally in recent years due to stricter regulations (mainly as a result of Minamata Convention on Mercury involving several countries worldwide) [
232,
233], anthropogenic processes are still responsible for a significant input of mercury into the environment [
221,
233]. Among the main activities that have been contributing to environmental contamination with mercury are cinnabar mining, coal combustion for energy production (an important source of atmospheric mercury), cement production, metal processing (gold, silver), waste incineration (from urban, medical and industrial sources), chlor-alkali and steel industry and the production of electric equipment, paints and wood [
223,
232,
234].
The extensive use of mercury in different applications has led to severe pollution in aquatic and terrestrial ecosystems. In recent years, a wide range of mercury concentrations have been found in soil (topsoil/agricultural land: 0 – 8 889 mg/kg) water (marine sediments: 0.0023 – 5 330 mg/kg; marine water: 0.5 – 27 060 ng/L; surface freshwater: 1.6 – 28.7 ng/L) [
175,
235,
236,
237], and across food webs, particularly in aquatic ecosystems where predatory fish (e.g., dusky grouper, barracuda, porbeagle) bioaccumulate mercury (sea fish: 0.001-3.1 mg/kg; estuarine/freshwater fish: 0.04 – 1.74 mg/kg) [
238,
239]. Given the wide distribution of mercury in the environment and the abundance of bacteria on Earth, microorganisms are commonly exposed to and affected by toxic levels of mercury [
240]. As a result, there is a widespread prevalence of genetic determinants of mercury tolerance among bacterial populations, which allows their survival and adaptation in the presence of this toxic element in diverse environments. However, the mechanisms underlying mercury toxicity in bacterial cells are still not fully understood and continue to be the subject of study. Mercury exhibits a similar chemical reactivity to other metals (e.g., cadmium, lead, arsenic) within cells, where it binds to sulfhydryl groups of enzymes and proteins [
241], causing changes in protein structure and often loss of function [
242]. Recently, the affinity of mercury for the low molecular weight thiol molecules cysteine and glutathione (the most prevalent) and for proteins was described as involved in the replacement of essential zinc cofactors in DNA-binding proteins, which are involved in the transcription of tRNA genes and DNA repair, vital for many cellular functions [
240].
Bacterial tolerance to mercury has been described in various Gram-positive and Gram-negative species from diverse sources (e.g., natural environments such as water, soil, and glaciers) or in human commensal/pathogenic bacteria [
243,
244,
245,
246], but mainly associated with environments contaminated by mercury [
247]. In fact, the first description of bacterial mercury tolerance (phenotypic feature) occurred at a time when mercurial compounds were widely used as topical disinfectants and antiseptics in hospitals, community and food-producing animals [
248,
249], and it was observed in a clinical isolate of
S. aureus also resistant to penicillin [
250]. At the same time the role of some anaerobic bacteria in the geochemistry of mercury, participating in the production of the most toxic form, methylmercury, was recognized in aquatic bottom sediments and fish [
251]. To cope with mercury toxicity, bacteria have evolved the ability to convert toxic forms of mercury into nontoxic or relatively less harmful species, including the reduction of the highly reactive Hg
2+ to metallic Hg
0 (relatively inert, water insoluble, and volatile) [
252,
253], or the degradation of organomercury compounds to inorganic mercury [
248]. The
mer operon is the most extensively studied cluster of genes that lead to mercury tolerance. It is highly variable among bacteria [
248,
254] and allows them to resist both inorganic and organic forms of mercury, known as narrow- or broad-spectrum mercury tolerance operons, respectively [
215]. They typically consist of a combination of operators, regulators, promoter genes, and functional genes (e.g.,
merT,
merP,
merE,
merC,
merA,
merG,
merB and
merD), all or part of which are present, which contribute to the proper functioning of the operon system [
247] (
Figure 6).
The central enzyme in the mercury detoxification system is the mercuric reductase – MerA (encoded by the
merA gene) [
252], a cytosolic flavin disulfide oxidoreductase, which uses NAD(P)H as a reducing agent [
248]. This protein is responsible for the volatilization of mercury, catalyzing the conversion of Hg
2+ to Hg
0 [
255], and it is present both in narrow- and broad-spectrum
mer operons [
215]. While exhibiting a similar function role, variations in MerA amino acid sequences have been observed among Gram-positive and Gram-negative bacteria [
255], suggesting a distinct ancestral origin of the
mer operon for these two bacterial groups during the course of evolution [
255]. In addition to MerA, a cytoplasmatic organomercury lyase – MerB (encoded by the
merB gene) might also occur, allowing bacteria to resist organomercurials [
215], catalyzing the demethylation of organic mercury compounds by lysing the carbon-Hg bond, transforming it into relatively less toxic Hg
2+, which is then reduced by MerA to form Hg
0 [
215]. Therefore, the
merB gene is associated only with the broad-spectrum
mer operon [
215]. The presence of
merB gene is more common in Gram-negative
mer than in Gram-positive operons [
248].
Other functional genes are primarily related to mercury transport and may include:
merT, encoding an inner cytoplasmic membrane (MerT) protein responsible for accepting organic and inorganic mercury from MerP and transporting it to the cytoplasmic side of the membrane [
248];
merP, which encodes a periplasmic scavenger protein that aids in the exchange of Hg
2+ in the early transmembrane domain of MerP to MerT [
215,
248];
merE, which encodes a transport protein (MerE) that helps transport both inorganic and organic mercury compounds across the bacterial cell membrane into the cytoplasm [
215,
248]; and
merC, which encodes an inner membrane-spanning transporter protein (MerC), which helps transport inorganic (Hg
2+) and organic (C
6H
5Hg) mercury from the periplasm to the cytosol [
215]. Additionally,
merG is responsible for decreasing cell membrane permeability to phenylmercury (since it and other organomercurials can potentially undergo simple diffusion [
248]), contributing along with
merB to broad-spectrum resistance against mercurial compounds [
256]. The
merR gene is associated with mercury tolerance expression, as it encodes an Hg
2+-dependent transacting activator-repressor protein (MerR), which activates the
mer genes in the presence of Hg
2+ or represses it when a deficiency in Hg
2+ occurs [
257]. Other genes are also involved in the regulation of the
mer operon, including the
merD gene, which encodes a regulatory protein (MerD), responsible for downregulation of the mercury tolerance system [
215] and the
merO gene, which is the operator region linked to the
merR gene, responsible to upregulating and downregulating the expression of the
mer operon genes [
215]. A mercury tolerance phenotype associated with the presence of only the
merR and
merA genes was recently described in
Enterococcus spp., with MICs to HgCl
2 ranging between 16 and 64 μM, contrasting with those of 4-8 μM among isolates without such genes [
150].
Mercury tolerance determinants are often located on the chromosome or plasmids of Gram-positive and Gram-negative bacteria, usually as components of transposable elements, in a striking diversity of arrangements [
248]. The
mer operon was first described in Gram-negative bacteria associated with Tn
501 and related transposons [
246] and since then several associations with plasmids and transposons have been identified in bacteria from natural environments [
258] or with clinical relevance, including pathogenic strains of
E. coli (e.g., genomic island GI-3) [
259], and
S. Typhimurium (e.g, GI-DT12 containing a Tn
21-like transposon) [
260]. In Gram-positive bacteria,
mer operons have been found in diverse MGEs, including in
S. aureus [e.g., plasmid pTW20_1 borne SCCmec (beta-lactamase) cassette] [
261] and in
E. faecalis and
E. faecium (e.g., chromosomal Tn
5385-like, pPPM1000) isolated from human (clinical) and animal samples, respectively [
253,
262]. The same mercury tolerance-associated transposons or plasmids often carry ARGs genes, which makes them potential vectors of multiple genes involved in co-resistance and co-selection events. Shortly after the first description of mercury tolerance in
S. aureus resistant to penicillin, a plasmid (pI285) carrying both mercury tolerance and penicillin resistance genes was identified [
189,
263], along with other metal tolerance genes (arsenic/antimony, lead/zinc, cadmium) [
189]. In recent years, several reports have been published on the co-occurrence of mercury tolerance, ARGs and biocide tolerance genes in the same MGEs, including in conjugative plasmids [
253,
264,
265,
266]. Specific associations of mercury tolerance genes with aminoglycosides [e.g.,
aac(3)-IV,
aadA], sulfonamides (e.g.,
sul) or tetracycline [e.g.,
tet(A)] were described in plasmids of
Klebsiella,
Escherichia,
Salmonella, and
Enterobacter isolated from diverse sources (human, animal, wastewater and sludge) [
133,
134,
267]. Additionally, co-location of
mer operon genes with β-lactams genes (
blaCTX-M,
blaOXA, or
blaTEM) has also been described in plasmids of
K. pneumoniae,
E. coli and
Salmonella from clinical, surveillance, food and environmental samples [
133,
134,
268,
269,
270]. In Gram-positive bacteria, particularly
Enterococcus spp. from different sources (e.g., animal, healthy human, clinical, hospital sewage), mercury tolerance genes have been co-localized on plasmids with ARGs, mainly for erythromycin [
erm(B)], tetracycline [
tet(M),
tet(L)], aminoglycosides [
aadE,
aadK,
aac(6’)-aph(2’)] and vancomycin (
vanA) [
150,
253]. The distribution of mercury tolerance genes in MGEs along with ARGs genes highlights the potential impact of mercury on the co-transfer and dissemination of such determinants among bacteria of different sources.