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Review

Human Astroviruses

Albert Bosch, Rosa M. Pintó, Susana Guix
Albert Bosch
Enteric Virus Laboratory, Department of Microbiology and Institute of Nutrition and Food Safety, University of Barcelona, Barcelona, Spain
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  • For correspondence: abosch@ub.edu
Rosa M. Pintó
Enteric Virus Laboratory, Department of Microbiology and Institute of Nutrition and Food Safety, University of Barcelona, Barcelona, Spain
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Susana Guix
Enteric Virus Laboratory, Department of Microbiology and Institute of Nutrition and Food Safety, University of Barcelona, Barcelona, Spain
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DOI: 10.1128/CMR.00013-14
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  • FIG 1
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    FIG 1

    Human astrovirus particles observed by transmission immunoelectron microscopy in feces negatively stained with phosphotungstic acid. Bar, 50 nm.

  • FIG 2
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    FIG 2

    Genome organization and polyprotein products of human astrovirus. (A) Genomic and subgenomic RNA organization, with open reading frames (ORFs) ORF1a, ORF1b, ORF2, and putative ORFX represented as boxes. Nucleotide sequences represent highly conserved sequences located in the ribosomal frameshift (RFS) signal and upstream of the initiation site of subgenomic RNA transcription. Putative RNA secondary structures conserved in the RFS and in the 3′ end of the genome are depicted. (B) Characteristic motifs of the HAstV polyprotein products. HEL, putative helicase domain; TM, transmembrane domain; CC, coiled-coil domain; PRO, protease domain; VPg, coding region for a VPg protein; HVR, hypervariable region; NLS, putative nuclear localization signal; DD, putative death domain; RdRp, RNA dependent-RNA polymerase motif. The ORF2-encoded structural polyprotein (VP90) consists of conserved regions (shell and P1 domains), a variable region containing the P2 domain (capsid spikes), and an acidic C-terminal region which is cleaved by cellular caspases to result in the VP70 precursor. Particles containing VP70 are further cleaved by trypsin to yield the VP34, VP27/29, and VP25/26 proteins.

  • FIG 3
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    FIG 3

    Replication of human astroviruses. After binding to one or more cellular receptors, virus uptake occurs via clathrin-dependent endocytosis. A drop in the pH leads to viral uncoating. Two main nonstructural polyproteins, nsP1a and nsP1a1b, are translated from the VPg-linked genomic RNA and further cleaved by viral and cellular proteases, resulting in mature nonstructural proteins (nsPs), which are required for genome replication. Replication complexes assemble in close association with intracellular membranes. The nsP1a/4 protein or one of its precursors, which would include the VPg domain, may interact with the RdRp protein and contribute to the regulation of the synthesis of negative- and positive-sense RNA strands as well as of subgenomic RNA. The phosphorylation status of the nsP1a/4 protein may contribute to this regulation step. Subgenomic RNAs are produced in large quantities and are used for the expression of capsid proteins. The structural VP90 polyprotein initially assembles into immature virions in association with intracellular membranes. Several cellular caspases further cleave these VP90 polyproteins once they have dissociated from membranes, resulting in VP70 immature viral capsids. Release of VP70 particles into the medium seems to occur without cell lysis, and virions mature extracellularly by the action of trypsin.

  • FIG 4
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    FIG 4

    Putative processing of the astrovirus nonstructural proteins expressed from ORF1a and ORF1b. HEL, putative helicase domain; CC, coiled-coil domain; TM, transmembrane domain; PRO, protease domain; VPg, viral protein genome-linked coding region; HVR, hypervariable region; RdRp, RNA-dependent RNA polymerase motif; P, posttranslational phosphorylation. Triangles depict proteolytic cleavage sites described in the literature (75, 77, 78, 80).

  • FIG 5
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    FIG 5

    HAstV particles are associated with membranes in infected cells. Ultrastructural analysis of CaCo-2 cells infected with HAstV-4 at 48 h postinfection shows aggregates of virions accumulated in the cytoplasm in close association with double-membrane vesicles (V). Nuclei (N) of infected cells show masses of condensed chromatin dispersed at the periphery (c).

  • FIG 6
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    FIG 6

    Phylogenetic relationships within the family Astroviridae. The predicted amino acid sequences of the entire capsid polyprotein were aligned using Clustal Omega (309). The phylogenetic tree was generated using the neighbor-joining algorithm (310) implemented in the MEGA6 program (311). The percentages of replicate trees in which the associated taxa clustered together in the bootstrap test (1,000 replicates) which are higher than 70 are shown next to the branches. The tree is drawn to scale, with branch lengths in the same units as those of the evolutionary distances (p-dist) used to infer the phylogenetic tree. All positions containing alignment gaps and missing data were removed only in pairwise sequence comparisons (pairwise deletion option). Genotype species officially recognized by the ICTV are indicated, with hosts of origin shown in parentheses. Human viruses are colored in red, porcine viruses are colored in dark blue, mink viruses are colored in dark gray, bovine viruses are colored in brown, ovine viruses are colored in light blue, bat viruses are colored in black, murine viruses are colored in purple, turkey viruses are colored in orange, and chicken viruses are colored in green. Arrows indicate strains which have been isolated from neurologic tissues. HAstV, human astrovirus; FAstV, feline astrovirus; PAstV, porcine astrovirus; CaAstV, canine astrovirus; RabAstV, rabbit astrovirus; OAstV, ovine astrovirus; BoAstV, bovine astrovirus; MuAstV, murine astrovirus; WBAstV, wild boar astrovirus; CcAstV, deer astrovirus; TAstV, turkey astrovirus; CAstV, chicken astrovirus; ANV, avian nephritis virus; WPIAstV, wild pigeon astrovirus.

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    FIG 7

    Flowchart of potential routes of environmental transmission of human astroviruses (see the text for details).

Tables

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  • TABLE 1

    Main characteristics of the Astroviridae family

    Characteristic
    Virion structure
        Icosahedral particles, 28–41 nm in diam
        Nonenveloped
        Distinctive five- or six-pointed star-like shape under the electron microscope in about 10% of the virions
    Genome
        A single molecule of infectious, positive-sense ssRNA, 6.4–7.7 kb, with a poly(A) tail
        Three ORFs: ORF1a and ORF1b at the 5′ end encoding the nonstructural proteins and ORF2 at the 3′ end encoding the structural proteins
        VPg protein linked to the 5′ end
        A ribosomal frameshifting signal present between ORF1a and ORF1b
        Lack of a helicase domain
    Replicative cycle
        Structural proteins are expressed from an ∼2.8-kb subgenomic RNA
  • TABLE 2

    Studies of human astrovirus prevalence in stool

    Region and country (setting, period of study)Age (yr) of study populationAstrovirus prevalence (%)Detection methodReference
    North Africa
        Egypt (rural, 1995–1998)<226.7EIA 237
        Tunisia (urban and rural 2003–2005)<56.0EIA 306
    Sub-Saharan Africa
        Botswana (urban, 2001–2002)<52.7EIA 245
        Kenya (urban and rural 1999–2005)<55.3EIA 246
        Ghana (urban, 2005–2006)<124.8RT-PCR 247
    Asia
        Thailand (urban, 1985–1987)<58.6EIA 239
        Japan (urban and rural 1982–1992)Children of all age groups, mostly <1018EIA 249
        China (urban and rural, 1998–2005)<55.5EIA plus RT-PCR 307
        Vietnam (urban, 2005–2006)<313.9RT-PCR 241
        India (urban, 2004–2008)<8 years, adults3.1RT-PCR 308
        Japan (urban 2008–2009)Children of all age groups1.7RT-PCR 250
    North America
        Mexico (rural, 1992–1995)<361EIA and RT-PCR 94
        USA (urban, 1993–1994)<320EIA 266
        USA (urban, 1996–1997)Children of all age groups, mostly <36.9EIA 230
    Central America
        Guatemala (rural, 1987–1989)<338.6EIA 33
    South America
        Chile (urban, 1985–1987; 1993–1995)<323.5EIA 240
        Brazil (urban, 1990–1992)<25.8EIA plus RT-PCR 265
        Argentina (urban, 1995–1998)<33.7EIA plus RT-PCR 267
        Colombia and Venezuela (urban, 1997–1999)<55.0EIA 167
    Europe
        France (urban, 1995–1998)<36.0EIA 242
        Spain (urban, 1997–2000)Children of all age groups, Mostly <54.9RT-PCR 164
        Italy (urban, 1999–2000)<23.1EIA 264
        Germany (urban, 2000)All ages1.2EIA 276
        France (urban, 2007)<51.8EIA 248
    Oceania
        Australia (urban, 1995)<54.2Northern (RNA) dot blot 35
  • TABLE 3

    Prevalence of serotypes (genotypes) of classic human astrovirus

    Region and country (setting, period of study)Prevalence (%) of serotype: Reference
    12345678
    North Africa
        Egypt (rural, 1995–1998)43.33.612.04.815.77.2012.0 237
    Asia
        Vietnam (urban, 2005–2006)100.00000000 241
        India (urban, 2004–2008)67079.7006.5 a 0016.0 308
        Japan (urban 2008–2009)91.009.000000 250
    North America
        USA (urban, 1993–1994)55.017.0— b ————— 266
    South America
        Brazil (urban, 1990–1992)45.527.312.112.103.000 265
        Argentina (urban, 1995–1998)41.013.013.025.08.0000 267
    Europe
        Spain (urban, 1997–2000)38.06.019.026.000011.0 164
    Oceania
        Australia (urban, 1995)85.00015.00000 35
    • ↵a ORF1a/ORF2 recombinant strains.

    • ↵b —, there were no data on this genotype in the study.

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Human Astroviruses
Albert Bosch, Rosa M. Pintó, Susana Guix
Clinical Microbiology Reviews Oct 2014, 27 (4) 1048-1074; DOI: 10.1128/CMR.00013-14

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Human Astroviruses
Albert Bosch, Rosa M. Pintó, Susana Guix
Clinical Microbiology Reviews Oct 2014, 27 (4) 1048-1074; DOI: 10.1128/CMR.00013-14
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  • Top
  • Article
    • SUMMARY
    • INTRODUCTION
    • BASIC VIROLOGY
    • PATHOLOGY, PATHOGENESIS, AND HOST RESPONSE
    • TAXONOMY, EVOLUTION, AND EMERGENCE
    • EPIDEMIOLOGY
    • LABORATORY DIAGNOSTICS
    • PREVENTION AND TREATMENT
    • CONCLUSIONS
    • ACKNOWLEDGMENTS
    • REFERENCES
    • Author Bios
  • Figures & Data
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