Structural Insights into the Human Astrovirus Capsid.

Astroviruses (AstVs) are non-enveloped, positive single-stranded RNA viruses that cause a wide range of inflammatory diseases in mammalian and avian hosts. The T = 3 viral capsid is unique in its ability to infect host cells in a process driven by host proteases. Intercellular protease cleavages allow for viral egress from a cell, while extracellular cleavages allow for the virus to enter a new host cell to initiate infection. High-resolution models of the capsid core indicate a large, exposed region enriched with protease cleavage sites. The virus spike protein allows for binding to target cells and is the major target for naturally occurring and engineered neutralizing antibodies. During maturation, the capsid goes through significant structural changes including the loss of many surface spikes. The capsid interacts with host membranes during the virus life cycle at multiple stages such as assembly, host cell entry and exit. This review will cover recent findings and insights related to the structure of the capsid and its function. Further understanding of the viral capsid structure and maturation process can contribute to new vaccines, gastric therapeutics, and viral engineering applications.

Minimal capsid composition of infectious human astrovirus.

Human astrovirus is an important etiological agent of acute gastroenteritis in young children. Despite advances in the characterization of the structure of the virion by cryo-electron microscopy and of capsid proteins by x-ray crystallography, the definition of the minimal polypeptide composition of infectious virus particles has been elusive. In this work we show that mature infectious particles are composed by only two proteins; VP34 that forms the core domain of the virus, and VP27 that constitutes the 30 dimeric spikes present on the virus surface. Our results also indicate that during the transition of immature (90 spikes) to mature (30 spikes) virus particles, that occur during trypsin activation, the viral protein VP25, that most likely forms the 60 spikes that are lost during maturation, detaches from the virus particle. This information is relevant to better understand the biology of virus entry and also for the efficient development of subunit vaccines.

Structural Basis for Escape of Human Astrovirus from Antibody Neutralization: Broad Implications for Rational Vaccine Design.

Human astroviruses are recognized as a leading cause of viral diarrhea worldwide in children, immunocompromised patients, and the elderly. There are currently no vaccines available to prevent astrovirus infection; however, antibodies developed by healthy individuals during previous infection correlate with protection from reinfection, suggesting that an effective vaccine could be developed. In this study, we investigated the molecular mechanism by which several strains of human astrovirus serotype 2 (HAstV-2) are resistant to the potent HAstV-2-neutralizing monoclonal antibody PL-2 (MAb PL-2). Sequencing of the HAstV-2 capsid genes reveals mutations in the PL-2 epitope within the capsid's spike domain. To understand the molecular basis for resistance from MAb PL-2 neutralization, we determined the 1.35-Å-resolution crystal structure of the capsid spike from one of these HAstV-2 strains. Our structure reveals a dramatic conformational change in a loop within the PL-2 epitope due to a serine-to-proline mutation, locking the loop in a conformation that sterically blocks binding and neutralization by MAb PL-2. We show that mutation to serine permits loop flexibility and recovers MAb PL-2 binding. Importantly, we find that HAstV-2 capsid spike containing a serine in this loop is immunogenic and elicits antibodies that neutralize all HAstV-2 strains. Taken together, our results have broad implications for rational selection of vaccine strains that do not contain prolines in antigenic loops, so as to elicit antibodies against diverse loop conformations.IMPORTANCE Human astroviruses (HAstVs) infect nearly every person in the world during childhood and cause diarrhea, vomiting, and fever. In this study, we investigated how several strains of HAstV are resistant to a virus-neutralizing monoclonal antibody. We determined the crystal structure of the capsid protein spike domain from one of these HAstV strains and found that a single amino acid mutation induces a structural change in a loop that is responsible for antibody binding. Our findings reveal how viruses can escape antibody neutralization and provide insight for the rational design of vaccines to elicit diverse antibodies that provide broader protection from infection.

Crystal Structure of the Human Astrovirus Capsid Protein.

UNLABELLED: Human astrovirus (HAstV) is a leading cause of viral diarrhea in infants and young children worldwide. HAstV is a nonenveloped virus with a T=3 capsid and a positive-sense RNA genome. The capsid protein (CP) of HAstV is synthesized as a 90-kDa precursor (VP90) that can be divided into three linear domains: a conserved N-terminal domain, a hypervariable domain, and an acidic C-terminal domain. Maturation of HAstV requires proteolytic processing of the astrovirus CP both inside and outside the host cell, resulting in the removal of the C-terminal domain and the breakdown of the rest of the CP into three predominant protein species with molecular masses of ∼34, 27/29, and 25/26 kDa, respectively. We have now solved the crystal structure of VP90(71-415) (amino acids [aa] 71 to 415 of VP90) of human astrovirus serotype 8 at a 2.15-Å resolution. VP90(71-415) encompasses the conserved N-terminal domain of VP90 but lacks the hypervariable domain, which forms the capsid surface spikes. The structure of VP90(71-415) is comprised of two domains: an S domain, which adopts the typical jelly-roll ß-barrel fold, and a P1 domain, which forms a squashed ß-barrel consisting of six antiparallel ß-strands similar to what was observed in the hepatitis E virus (HEV) capsid structure. Fitting of the VP90(71-415) structure into the cryo-electron microscopy (EM) maps of HAstV produced an atomic model for a continuous, T=3 icosahedral capsid shell. Our pseudoatomic model of the human HAstV capsid shell provides valuable insights into intermolecular interactions required for capsid assembly and trypsin-mediated proteolytic maturation needed for virus infectivity. Such information has potential applications in the development of a virus-like particle (VLP) vaccine as well as small-molecule drugs targeting astrovirus assembly/maturation. IMPORTANCE: Human astrovirus (HAstV) is a leading cause of viral diarrhea in infants and young children worldwide. As a nonenveloped virus, HAstV exhibits an intriguing feature in that its maturation requires extensive proteolytic processing of the astrovirus capsid protein (CP) both inside and outside the host cell. Mature HAstV contains three predominant protein species, but the mechanism for acquired infectivity upon maturation is unclear. We have solved the crystal structure of VP90(71-415) of human astrovirus serotype 8. VP90(71-415) encompasses the conserved N-terminal domain of the viral CP. Fitting of the VP90(71-415) structure into the cryo-EM maps of HAstV produced an atomic model for the T=3 icosahedral capsid. Our model of the HAstV capsid provides valuable insights into intermolecular interactions required for capsid assembly and trypsin-mediated proteolytic maturation. Such information has potential applications in the development of a VLP vaccine as well as small-molecule drugs targeting astrovirus assembly/maturation.

The C-terminal end of the capsid protein of Avian Nephritis Virus is antigenic and induces broadly cross-reactive antibodies.

Avian nephritis virus (ANV) has been isolated frequently from commercial broilers in many countries. The prevalence and economic impact of ANV however has been difficult to ascertain due to the lack of convenient serological techniques. In this study the full-length and fragments of the ANV capsid protein were expressed in Baculovirus and affinity purified recombinant proteins used for the detection of ANV antibodies in ELISA. The crystal structure of Human Astrovirus (HAstV) was used as a model to determine potential homologous C-terminal antigenic regions in ANV. The rp37 fragment from three ANV strains NSW_3, ANV-1 and ANV-2, and a shorter NSW_3 fragment (rp33) were compared for their ability to detect ANV antibodies in seven reference chicken sera. The ANV-1 rp37 antigen was the most strain specific whereas the NSW_3 rp37 and rp33 antigens detected antibodies in all heterologous sera, including ANV-1 serum. Irrespective of the strain used, the two NSW_3 protein fragments rp37 and rp33 were found to be superior as antigens for ELISA when compared to the full-length capsid protein rp75. An ELISA designed using the NSW_3 rp33 could reliably differentiate between uninfected and infected commercial broiler flocks, as demonstrated by statistically significant differences between the OD values. This study identified an ANV immunogenic region and successfully used recombinant protein expression of this region to detect cross-reactive ANV antibodies. The results of this study facilitate future studies into the epidemiology and importance of ANV infections in commercial poultry.

Potent inhibition of the classical pathway of complement by a novel C1q-binding peptide derived from the human astrovirus coat protein.

Previous work from our laboratories has demonstrated that purified, recombinant human astrovirus coat protein (HAstV CP) binds C1q and mannose-binding lectin (MBL) inhibiting activation of the classical and lectin pathways of complement, respectively. Analysis of the 787 amino acid CP molecule revealed that residues 79-139 share limited sequence homology with human neutrophil defensin-1 (HNP-1), a molecule previously demonstrated to bind C1q and MBL, inhibiting activation of the classical and lectin pathways of complement, respectively. A 30 amino acid peptide derived from this region of the CP molecule competitively inhibited the binding of wild-type CP to C1q. The parent peptide and various derivatives were subsequently assayed for C1q binding, inhibition of C1 and C4 activation as well as suppression of complement activation in hemolytic assays. The parent peptide and several derivatives inhibited complement activation in these functional assays to varying degrees. One peptide derivative in particular (E23A) displayed superior inhibition of complement activation in multiple assays of classical complement pathway activation. Further analysis revealed homology to a plant defensin allowing development of a proposed structural model for E23A. Based upon these findings, we hypothesize that further rationale optimization of E23A may result in a promising therapeutic inhibitor for the treatment of inflammatory and autoimmune diseases in which dysregulated activation of the classical and lectin pathways of complement contribute to pathogenesis.

Genome prediction of putative genome-linked viral protein (VPg) of astroviruses.

Positive-sense single-stranded RNA (+ssRNA) viruses replicate by uncoating the RNA genome for translation to provide viral proteins essential for genome replication and the production of new viral particles. The viral proteins are synthesized from a polyprotein precursor, which is cleaved nascently. The synthesized proteins include viral RNA-dependent RNA polymerase (RdRP), viral genome-linked protein (VPg), and a helicase. VPg is covalently attached to the genomic form of +ssRNA viruses. Helicases and NTPase unwind the RNA before replication. VPg and helicases have been identified in +ssRNA families, however, the presence of VPg and helicase in the Astroviridae, another +ssRNA family, has not been fully elucidated. Computational tools were utilized to provide sequence analysis evidence for the presence and genomic location of astrovirus VPg and helicase. HMMER program v2.1.1 was used to build Hidden Markov Model (HMM) profile for calicivirus VPg to search for conserved motifs in the astrovirus genome. We performed phylogenetic analysis of two genomic regions of astroviruses and caliciviruses (encoding the RdRP and VPg). We identified a putative VPg coding region in astrovirus. This region was located in open reading frame 1a (ORF1 a) and included sites with high sequence similarity to the VPg coding regions of Caliciviridae, Piconaviridae, and Potyviridae. A region encoding a putative astrovirus helicase identified conserved motifs only with pestivirus helicase sequences. Sequence analysis and comparison to other +ssRNA viruses supports the presence of VPg in the Astroviridae. Further laboratory analysis will be necessary to confirm these findings.

Profile-profile comparisons by COMPASS predict intricate homologies between protein families.

Recently we proposed a novel method of alignment-alignment comparison, COMPASS (the tool for COmparison of Multiple Protein Alignments with Assessment of Statistical Significance). Here we present several examples of the relations between PFAM protein families that were detected by COMPASS and that lead to the predictions of presently unresolved protein structures. We discuss relatively straightforward COMPASS predictions that are new and interesting to us, and that would require a substantial time and effort to justify even for a skilled PSI-BLAST user. All of the presented COMPASS hits are independently confirmed by other methods, including the ab initio structure-prediction method ROSETTA. The tertiary structure predictions made by ROSETTA proved to be useful for improving sequence-derived alignments, because they are based on a reasonable folding of the polypeptide chain rather than on the information from sequence databases. The ability of COMPASS to predict new relations within the PFAM database indicates the high sensitivity of COMPASS searches and substantiates its potential value for the discovery of previously unknown similarities between protein families.

Astrovirus infection in children.

PURPOSE OF REVIEW: Public health concerns related to enteric viral agents, such as astroviruses and caliciviruses, include their ability to cause sporadic diarrhea, large outbreaks of gastroenteritis, and hospitalizations or deaths resulting from vomiting, diarrhea, and dehydration. Improved surveillance and application of sensitive molecular assays has increased awareness of these enteric pathogens and reduced the 'diagnostic gap' or unknown causes of non-bacterial gastroenteritis. RECENT FINDINGS: Molecular assays have been applied to further describe the epidemiology of human astroviruses from a variety of geographic areas. The burden of astrovirus infections compared with other enteric viral agents, including rotaviruses, caliciviruses, and enteric adenoviruses have been reported. New methods for detection of astroviruses such as reverse transcription-polymerase chain reaction and molecular typing methods have advanced the understanding of the epidemiology. Additional molecular studies have described the protein processing mechanisms of this single-stranded RNA virus. SUMMARY: Astroviruses are increasingly recognized as significant gastrointestinal pathogens. The understanding of molecular epidemiology and molecular processing of the virus may lead to specific prevention strategies.

Complete genomic sequences of astroviruses from sheep and turkey: comparison with related viruses.

The genomes of astroviruses infecting sheep and turkey were sequenced. Detailed analyses of these sequences were performed, including comparison with the other complete astrovirus sequences available as well as with other RNA virus sequences, with focus on the non-structural proteins and RNA sequences. Earlier postulated functional astrovirus RNA motifs and protein domains could in most cases be recognised in the sheep and turkey astrovirus sequences. In addition, analyses of the available astrovirus sequences revealed: two protein regions with the potential for forming coiled coils, differences in the postulated transmembrane region, a similarity between the putative astrovirus nuclear localisation signal and calicivirus genome-linked proteins, and a stretch of a highly conserved RNA sequence with a possible role in the astrovirus capsid gene expression. The present analyses contribute to the deciphering of pertinent functions of the astrovirus genomes.

Molecular analysis of a serotype 8 human astrovirus genome.

Human astroviruses are an important cause of gastroenteritis. As part of a molecular epidemiological study carried out in Mexico a human astrovirus isolate, Yuc-8, was adapted to grow in CaCo-2 cells, and its entire genome was sequenced. A 15 amino acid deletion in ORF1a, which has been associated with adaptation of astroviruses to grow in cells other than CaCo-2, was present in Yuc-8. Comparative sequence analysis of the Yuc-8 ORF2 with reported human astrovirus sequences revealed that this isolate belongs to genotype (serotype) 8. Two distinct domains in ORF2 were observed: an amino-terminal domain (residues 1 to 415), with identities higher than 81% among the strains analysed, and a carboxy-terminal domain (residues 416 to 782) with identities between 36 and 60%. Two non-superimposable phylogenetic trees were generated by separate analysis of these two domains, suggesting that a differential selective pressure is exerted along the structural polyprotein.

Capsid protein composition of reference strains and wild isolates of human astroviruses.

Astroviruses are small RNA viruses that are frequently associated with gastroenteritis in humans and animals. Despite much work on the genetic analysis of astrovirus strains, little progress has been made in the characterization of the proteins composing mature virions. We have analyzed the capsid protein composition of the reference strains and several wild isolates of human astroviruses using high-resolution polyacrylamide gradient gels. For reference strains of the seven serotypes analyzed, a consistent pattern of three infection-specific proteins--designated P1, P2, and P3 -was generally observed. The strains could be divided into two groups, based upon the reactivity of these proteins in immune precipitation assays that used homologous rabbit serum. One group included reference types 1 4 for which all three proteins were precipitated by homologous rabbit sera; for the other group, types 5 7, only proteins P2 and P3 were precipitated. When wild isolates from around the world were compared to the reference strains, a correlation between genetic type and the pattern of protein sizes and immune reactivity was observed for strains of the common types (1-4). Strains of types 2 and 4 consistently exhibited P3 proteins larger than those of types 1 and 3. Unusual patterns of proteins or immune reactivity were detected in strains of types 5-7, indicating that there may be incomplete processing of the capsid precursor during growth in cell culture.

Prevalence of human astrovirus serotype 4: capsid protein sequence and comparison with other strains.

Astrovirus serotype 4 has increased in relative prevalence in the Oxford, UK area in 1993. The structural gene of human astrovirus serotype 4 has been sequenced and the results indicate that this protein differs substantially from serotypes 1 and 2. In particular, conservation at the C terminus is greatly reduced. However, amino acid substitutions in this region show a strong conservation in character suggesting that structural or functional constraints operate in this region.