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Interaction of quinolines and artemisinin based antimalarials drugs with ferriprotoporphyrin IX

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par Bienvenu MAVAKALA KIAZOLUA
Tsinghua University - Master en chimie physique 2003
  

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Chapter 2 Literature Survey

2.1 Biology of the malaria parasite

2.1.1 Life cycle of malaria parasite

In humans, malaria is caused by four species of the genus Plasmodium, namely Plasmonium falciparum, Plasmodium vivax, Plasmodium ovale and Plasmodium malariae (Wernsdorfer and McGregor, 1988).

Of these, P. falciparum is the most important as it causes almost all malaria-associated deaths. There is, however, significant morbidity associated with P. vivax (Trigg and Kondrachine, 1998). The biology of P. falciparum is fortunately the best understood of the four species. The life cycle of P. falciparum is complex and divided into three overall stages: mosquito, liver and blood stages.

Sexual reproduction of gametocytes occurs in the gut of the female vector mosquito (Anophele genus) and leads to the formation of zygotes that bury themselves in the gut lining of the mosquito. These then develop into oocysts and after some time form sporozoites that migrate to the salivary glands of the mosquito. When an infected mosquito bites a human host, these sporozoites enter the blood stream and rapidly make their way to the liver, invading hepatocytes. During a period of development in the liver of about a week as tissue schizonts, the parasites multiply asexually, finally simultaneously rupturing the host cells and entering the blood stream as merozoites. These merozoites invade red blood cells, entering into the blood cycle consisting of ring, trophozoite and blood schizont stages as shown in Figure 1-1.

Asexual reproduction in the blood cell leads to further merozoites and hence to ever increasing parasitaemia. Some of the merozoites develop into gametocytes. Upon entering the red cell the gametocytes may be taken up by mosquitoes to complete the life cycle. Symptoms of the disease (high fever, headache, malaise, muscle aches...) are entirely associated with the blood stage and so any curative drug must be specifically active against this part of the life cycle (Wernsdorfer and McGregor, 1988).

By knowing what is happening in the blood stage of parasite life cycle, we can understand why, generally speaking, individuals with abnormal hemoglobin S are resistant to malaria? Normally, about 2% of the erythrocytes of individuals with sickle -cell anemia are observed to sickle under low-oxygen concentration conditions found in the capillaries. However, the lower pH of infected erythrocytes increases the proportion of sickling in the capillaries up to 40%. Thus during the early stages of malarial infection, parasite-enhanced sickling probably causes the preferential removal of infected erythrocytes from the circulation. In the latter stages of infection, when the parasitized erythrocytes are attached to the capillary walls, the sickling induced by the low oxygen environment may mechanically and /or metabolically disrupt the parasite. Consequently, bearers of the sickle cell trait in a malarial region have an adaptive advantage (Voet and Voet, 1995).

Figure 1-1 A representation of the life cycle of Plasmodium falciparum. Ring forms, trophozoites and blood schizonts are collectively referred to as the blood stages of the cycle and are the specific targets of chloroquine and related antimalarial drugs. After invading red cells, most merozoites form ring stages and then trophozoites, but a small fraction instead develop into sexual forms called gametocytes which then reproduce in the gut of a mosquito when the insect feeds on the infected host. (Egan et al., 1999).

2.1.2 Hemozoin formation by malaria parasite

During its blood stage, P. falciparum utilises host's hemoglobin as a food source. This stage occurs in an acidic compartment within the parasite called a food vacuole that has a pH in the range 5.0-5.6 (Spiller et al., 2002). Plasmodia degrade hemoglobin and use the amino acids derived from proteolytic digestion for their biosynthetic requirements. Hemoglobin degradation is a highly ordered process involving several proteases (Eggleson, 1999; Banerjee, 2002; Rosenthal et al., 2002). Denatured globin formed by the action of plasmepsins is further degraded into small peptides by other proteases. A cysteine protease, falcipain, has been characterized from P. falciparum, which degrades denatured globin (Eggleson, 1999).

Large amounts of free nontoxic heme is released as a product of hemoglobin degradation (Mavakala and Gushimana, 1991). Released heme from hemoglobin is autoxidized into ferric form (hematin, hemin or aquaferriprotoporphyrin IX or H2O-Fe(III)PPIX) that is highly toxic, inhibiting vacuolar proteases and damaging parasite membranes [Berman and Adams, 1997]. Detoxification of heme is therefore necessary for the survival and growth of malaria parasite (Meshnick, 2002).

In the host, detoxification of heme is achieved by an enzyme called heme oxygenase, which breaks heme to form biliverdin. Another enzyme, biliverdin reductase, converts biliverdin into bilirubin, which is converted into a water-soluble conjugate and excreted through urine. Malaria parasite does not seem to use this pathway for the heme catabolism. Inside the food vacuole of malaria parasite, heme is converted into hemozoin, popularly known as malaria pigment. This hemozoin pigment is a dimer of heme units linked through an iron-carboxylate bond (Pagola et al., 2000).

Pagola et al. have revealed that hemozoin is a hemin dimer with hydrogen bonding between the dimer units in the crystal as shown in Figure1-2. In the light of this, the continued use of the word polymer to describe malaria pigment or -hematin, or the word polymerization to describe its formation is inappropriate and inaccurate (Pagola et al., 2000; Egan, 2002).

Figure 1-2 Chemical structures are shown for (a) hematin (aqua or hydroxyferriprotoporphyrin IX), (b) heme. The dimeric structure for beta-hematin is also indicated (c). The OH-, H2O group is represented by X in (a) and the histidine is represented by Y in (b) (Egan, 2002).

In the dimer, a bond is formed by the linking of central ferric iron of one heme unit with the propionate side chain of another heme. This pigment is inert in parasite and released into the host blood supply after infected erythrocytes burst open at the end of parasite life cycle (Pandey and Tekwani, 1996). Hemozoin is insoluble in organic solvents (methanol, ethanol, and acetone) and mildly soluble in alkaline bicarbonate buffer (100 mM, pH 9.0), whereas free heme is soluble in these solvents.

2.2 Some proposed mechanisms of action of antimalarial drugs

Numerous conflicting theories have been put forward over the past five decades to describe the mechanism of action of antimalarial drugs. Hypothesis for the mode of action of chloroquine essentially fall into two broad categories: those in which the drug exerts its action outside the food vacuole of the parasite and those in which the activity is located inside the food vacuole.

2.2.1 Mechanism of action of chloroquine and related antimalarials

2.2.1.1 Extravacuolar mechanisms: DNA binding

Chloroquine and related drugs exhibit antibacterial activity, blocking both DNA and RNA synthesis but the required chloroquine concentration is about one thousand times as much as that needed in curative treatment of malaria. No binding of mefloquine to DNA has been observed (Slater, 1993; Egan and Marques, 1999).

2.2.1.2 Intravacuolar mechanisms

Intravacuolar mechanisms seem more plausible because of substantial accumulation of the drugs in the vacuole. Most workers in the field currently favour a hypothesis in which quinoline antimalarial drugs inhibit formation of hemozoin. There is, however disagreement over how this occurs and there are essentially three variations of the hypothesis:

1. Slater and Cerami (1992) originally suggested that these drugs inhibit the putative heme polymerase enzyme.

2. Fitch and Chou (1996) have extended this hypothesis by suggesting that these drugs are potential regulators of the putative heme polymerase enzyme.

3. Egan and coworkers (Egan et al., 1994) have shown that chloroquine, amodiaquine and quinine can directly inhibit formation of synthetic -hematin and suggested that activity of these drugs in vivo involves inhibition of hemozoin formation by direct interaction with Fe(III)PPIX. This hypothesis has also been supported by Dorn and co-workers (Dorn et al., 1995; Dorn et al., 1998) and further support for this type of mechanism has been presented by several other laboratories (Sullivan et al., 1996; Basilico et al., 1997; Hawley et al., 1998) although there are some differences in detail.

These findings motivated a number of studies on antimalarial-hematin interactions in both aqueous and non-aqueous solution, as well as on their interactions with other iron-porphyrins. Many of the earlier studies concentrated on obtaining visible, Mössbauer and NMR spectroscopic evidences for hematin-drug interactions and some association constants were determined. For example, Log K values for the bonding of hemin-drug are 5.52 (chloroquine), 5.39 (amodiaquine), 4.10 (quinine), 4.04 (9-epiquinine) and 3.09 (mefloquine), in 40% aqueous DMSO solution, at an apparent pH of 7.5 and 25oC (Egan et al., 1997; Adams et al., 1999). It is clear from the recent investigation of Egan and coworkers that only 2- and 4-aminoquinolines and their derivatives form strong complexes with Fe(III)PPIX. Under the conditions of their studies, quinoline, 3-, 5-, 6-, and 8-aminoquinoline, and 4,7-dichloroquinoline exhibited no evidence of complexation with Fe(III)PPIX. Then, there is a simple correlation between hemin binding and -hematin inhibitory activity because those of compounds, which do not form measurable complexes, fail to inhibit -hematin. Surprisingly, however, not all quinolines, which do form strong complexes with Fe(III)PPIX, inhibit -hematin formation.(Egan, 2000). Perhaps, they are capable of inhibiting -hematin formation at high concentration. Egan et al. proposed a detailed model of the structure-function relationships in chloroquine as follows:

1. The 4-aminoquinoline nucleus alone provides an hemin complexing template but is not sufficient for inhibiting the formation of hemozoin;

2. Introduction of the 7-chloro group is responsible for inhibition of hemozoin formation but probably has little influence on the strength of association with hemin;

3. The aminoalkyl side chain is a requirement for strong antiplasmodial activity. It probably assists in drug accumulation in the food vacuole. It also appears to enhance the strength of association with hemin in some cases, but this effect does not appear to be essential for its activity.

Figure 1-3 Proposed structure-function relationships in chloroquine based on findings of Egan and coworkers (Egan et al., 2000).

2.2.1.3 Increased vacuolar pH mechanism

It has been reported that several enzymes like aspartic proteases, cysteine proteases and metalloproteases (Rosenthal, 1999) are thought to be involved in the degradation of hemoglobin. Many of these enzymes are optimally active at pH 4.5-5.0 and it is argued that the food vacuole would probably need to maintain a similar pH to permit the efficient proteolysis of hemoglobin (Francis et al., 1997). The work of Homewood and coworkers (Homewood et al., 1972) in the early 1970s outlined the potential importance of the pH of the digestive vacuole (pHDV) in the mode of action of chloroquine (CQ) and similar drugs. CQ is a lipophilic weak base that will pass through biological membranes in the uncharged form. Once, inside acidic compartments, CQ is protonated and trapped because the protonated base is relatively impermeable. If we assume that the digestive vacuole (DV) has a pH of ~5.0, then this mechanism would permit concentrative uptake of the drug (Geary et al., 1986). Homewood suggested that CQ might kill parasites by increasing pHDV, so that the acid proteases of the parasite could no longer function effectively (Spiller et al., 2002).

2.2.2 Mechanism of action of artemisinin and its derivatives

2.Artemisinin 3. R= OH Dihydroartemisinin

R= OCH3 Artemether

R= OCH2CH3 Arteether

R= O2CCH2CH2CO2H Artesunate

1.Deoxyartemisinin

Artemisinin was developed from an ancient Chinese herbal remedy. Artemisia annua (sweet wormwood or`qinghao') was used by Chinese herbal medicine practitioners for at least 2000 years. In 1596, Li Shi zhen, a famous herbalist, recommended it to patients with fever. In 1967, Chinese scientists screened a series of traditional remedies for drug activities, and found that extracts of qinghao had potent antimalarial activity. In 1972, the active ingredient was purified and first named qinghaosu (essence of qinghao), and then later renamed artemisinin. Western interest in Artemisinin derivatives (artesunate, artemether, dihydroartemisinin, arteether) began to grow as multidrug resistant Plasmodium falciparum strains began to spread. Hundreds of synthetic second generation artemisinin derivatives and other natural peroxide compounds with good antimalarial activity have been reported like yingzhaosu, arteflene (Lian et al., 1988; Hofneiz et al., 1994) as shown in scheme 2-1. Due to their potent antimalarial activity, fast action, and low toxicity, artemisinin and its derivatives have distinguished themselves as a new generation of antimalarial drugs. Actually, it has been established that the dihydroartemisinin combined to the holotransferrin would be a promising drug against cancer (Singh and Lai, 2001).

4. R=H R1=C6H5 5. .Arteflene 6.Yinzhaosu

R=H R1=CH3

R= OH R1=C6H5

Scheme 2-1 Structures of artemisinin analogous

The unusual structure of artemisinin molecules might be indicative of a different mode of action from those of other antimalarial drugs and hence the high potency against the resistant strains. Although the mechanism of its antimalarial activity is not clear and still under debate, there is general agreement that the endoperoxide bridge is essential for the antimalarial activity of artemisinin since deoxyartemisinin compounds which lack the endoperoxide moiety are inactive (China cooperative group on qinghaosu, 1982).

Meshnick et al. proposed a two-step mechanism for the antimalarial action of endoperoxide:

In the first step, artemisinin is activated by intraparasitic heme or free Fe (II) ion to produce free toxic carbon-centred radicals, confirmed by electron paramagnetic resonance (EPR) studies (Meshnick et al., 1993; Taranto et al., 2002].

In the second step, once formed, the artemisinin-derived free radicals appear to damage specific intracellular targets, possibly via alkylation (Berman and Adams, 1997).

But Pandey et al. proposed three possible ways for the effect of endoperoxide drugs on malaria (Pandey et al., 1999; Kannan et al., 2002):

-Inhibition of hemoglobin degradation

-Inhibition of hemozoin biosynthesis

-Interaction of artemisinin with hemozoin leading to the breakdown of the hemozoin pigment which could then form a complex with the heme unity.

These mechanisms are supported by the characterization of a covalent adduct between artemisinin and heme (Robert and Meunier, 1997) and by protein alkylation (Meshnick et al., 1991; Yang et al., 1994). Artemisinin also forms covalent adducts with protein but not with DNA (Yang et al., 1994). Thus, heme is both an activator and target of the artemisinin derivatives (Posner et al., 1995).

About the free radicals generated by artemisinin, there are some controversial discussions on the mechanism of their production. There is much stronger evidence that carbon-centred free radicals are involved. In fact, monoelectronic transfer from iron (II) to peroxide resulted in the cleavage of endoperoxide bond with primary formation of an unstable oxygen-centred radical, rearrangement and creation of toxic C4-centred free radicals. It has been proposed that heme attacks the endoperoxide linkage of artemisinin either at the O1 [Shukla et al., 1995] or O2 position [Tonmumphean, 2001] as shown in scheme 2-2. In pathway A, heme iron attacks the compound at the O2 position. Later, it rearranges to form C4 free radical. In pathway B, heme iron attacks the compound at the O1 position after that C3-C4 bond is cleaved to give carbon radical at C4 as shown in scheme 2.

Thus the presence of heme is necessary for the activation of artemisinin into an alkylating agent, which preferentially attacks proteins.

The fact that artemisinin becomes cytotoxic in the presence of ferrous, have triggered some researchers to study its effect on the therapy of cancer. Since iron influx is high in cancer cells, artemisinin and its analogous, after incubation with holotransferrin which increase the concentrations of ferrous iron in cancer cells, selectively kill cancer cells (Singh and Lai, 2001). In addition to the more largely accepted mechanisms summarized above, other mechanisms of action have also been proposed. For example, Jefford proposed that peroxides could interrupt the detoxification process of heme by transferring an O atom to heme, creating iron-oxene or oxyheme intermediates, which subsequently disable parasite (Jefford et al., 1995).

Scheme 2-2 Proposed mechanism of action of artemisinin (Tonmumphean , 200)].

Haynes and co-workers (Haynes et al., 1999) pointed out that activity is due to the trioxane unity acting as a source of hydroperoxide, which provides electrophilic oxygenating species, hydroxyl or alkoxyl radicals via reductive cleavage with Fe (II) or other reducing agents. These species would be able to hydroxylate biomolecules.

In summary, a schematic diagram of hemoglobin degradation and related pathways is given in Figure 2-4 (Pandey et al., 1999; Egan, 2002).

Drug effect 1 :

complex formation with heme

Drug effect 3 :

proteases inhibitors (by endoperoxide only)

Drug effect 2 : inhibition of hemin dimerization

Drug effect 4 :

Interaction with hemozoin

Toxic effects of heme accumulation :

1. Membrane damage

2. Inhibition of cysteine proteases

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