Fecal Components Modulate Human Astrovirus Infectivity in Cells and Reconstituted Intestinal Tissues.

Human astroviruses (HAstV) are among the most common causative agents of viral gastroenteritis, especially in children, and extraintestinal manifestations have also been described. These viruses are transmitted by the fecal-oral route, implying that stool composition and the gut microbiota may impact their ability to remain infectious. For some enteric viruses, individual bacterial envelope components and other polysaccharide-containing molecules, which are abundant in stools, have been shown to enhance capsid stability. However, the role of the complex stool environment and, most importantly, the role of interindividual differences have been poorly studied. We used HAstV as a model to investigate how the stool environment in itself, its interindividual variability, and some specific stool components could affect HAstV stability and infectivity. Using two different HAstV genotypes, we found that stools as a whole modulate astrovirus infectivity not only in an individual-dependent manner but also in a manner that depends on the viral genotype. A virus-protective effect was observed after incubation with various Gram-positive and Gram-negative bacteria as well as with bacterial components, such as lipopolysaccharide and peptidoglycan. These results were further confirmed in human intestinal tissues, a more physiologically relevant system. Astrovirus infectivity was also preserved by mucin, a major component of intestinal mucus. We further confirmed that these components stabilize the viral capsid. These results show that although HAstV benefits from the stabilizing effect of fecal components, the complexity and variability of the stool composition and the multiple potential interactions may explain the interindividual differences in viral transmission observed in real life.IMPORTANCE To ensure transmission, enteric viruses must maintain their infectivity during the various environmental challenges that they face in transit within and between hosts. Increased knowledge of the factors affecting enteric virus survival may help to control their transmission. This study reveals that specific fecal bacterial components preserve classic human astrovirus infectivity by stabilizing viral particles. However, the outcomes of stool-virus interactions are very variable, ranging from protection to a reduction of viral infectivity, depending on the viral genotype and the individual from whom the stool has been collected. We show that the transmissibility of enteric viruses is dependent on the intestinal contents of the infected individual and highlight the complex multiple interactions that could explain the stochastic nature of enteric virus transmission in humans.

Development of a novel DNA based reverse genetics system for classic human astroviruses.

Human astroviruses (HAstVs) are a frequent cause of gastroenteritis in young children and immunocompromised patients. The current report describes a new approach to recover genetically defined HAstVs through the use of a reverse genetics system based on a single DNA plasmid. This plasmid, carrying the full-length virus genome under a T7 promoter, is directly transfected into cells expressing T7 RNA polymerase, resulting in the rapid and robust recovery of infectious HAstV. The efficiency of the system was tested with the generation of a chimeric astrovirus having the HAstV serotype 1 replication machinery and the capsid derived from a HAstV serotype 8 virus. This new system provides an efficient and reproducible method to deepen our knowledge of astrovirus biology.

Human Astrovirus MLB Replication In Vitro: Persistence in Extraintestinal Cell Lines.

MLB astroviruses were identified 10 years ago in feces from children with gastroenteritis of unknown etiology and have been unexpectedly detected in severe cases of meningitis/encephalitis, febrile illness of unknown etiology, and respiratory syndromes. The aim of this study was to establish a cell culture system supporting MLB astrovirus replication. We used two clinical strains to infect several cell lines, an MLB1 strain from a gastroenteritis case, and an MLB2 strain associated with a neurologic infection. Efforts to propagate the viruses in the Caco-2 cell line were unsuccessful. In contrast, we identified two human nonintestinal cell lines, Huh-7 and A549, permissive for both genotypes. After serial passages in the Huh-7.5 cell line, the adapted strains were able to establish persistent infections in the Huh-7.5, Huh-7AI, and A549 cell lines, with high viral loads (up to 10 log10 genome copies/ml) detected by quantitative reverse transcription-PCR (RT-qPCR) in the culture supernatant. Immunofluorescence assays demonstrated infection in about 10% of cells in persistently infected cultures. Electron microscopy revealed particles of 32 to 33 nm in diameter after negative staining of cell supernatants and capsid arrays in ultrathin sections with a particularly high production in Huh-7.5 cells. Interferon (IFN) expression by infected cells and effect of exogenous IFN varied depending on the type of infection and the cell line. The availability of a cell culture system to propagate MLB astroviruses represents a key step to better understand their replicative cycle, as well as a source of viruses to conduct a wide variety of basic virologic studies.IMPORTANCE MLB astroviruses are emerging viruses infecting humans. More studies are required to determine their exact epidemiology, but several reports have already identified them as the cause of unexpected clinical diseases, including severe neurologic diseases. Our study provides the first description of a cell culture system for the propagation of MLB astroviruses, enabling the study of their replicative cycle. Moreover, we demonstrated the unknown capacity of MLB astrovirus to establish persistent infections in cell culture. Whether these persistent infections are also established in vivo remains unknown, but the clinical consequences would be of high interest if persistence was confirmed in vivo Finally, our analysis of IFN expression provides some trails to understand the mechanism by which MLB astroviruses can cause persistent infections in the assayed cultures.

Construction of a reverse genetic system for porcine astrovirus.

In order to construct a full-length infectious cDNA clone of porcine astrovirus, three fragments covering the complete genome of PAstV1-GX1 strain were amplified by RT-PCR. All three PCR-amplified fragments were cloned into T-Vector pMD19 (Simple), and subsequently assembled into a full-length cDNA clone by subcloning. A silent nucleotide change creating a PstI site was engineered into the full-length cDNA clone to distinguish the rescued virus from the parental virus. Upon transfection of BHK-21 cells with the in vitro transcripts of both the original and constructed cDNAs, typical cytopathic effects were observed on PK-15 cells after serial passaging of the cell supernatant. The construction and recovery of the infectious cDNA clone of porcine astrovirus will provide a valuable experimental system to study the genome function and pathogenesis of astroviruses.

Enteric viruses in HIV-1 seropositive and HIV-1 seronegative children with diarrheal diseases in Brazil.

Diarrheal diseases (DD) have distinct etiological profiles in immune-deficient and immune-competent patients. This study compares detection rates, genotype distribution and viral loads of different enteric viral agents in HIV-1 seropositive (n = 200) and HIV-1 seronegative (n = 125) children hospitalized with DD in Rio de Janeiro, Brazil. Except for group A rotavirus (RVA), which were detected through enzyme immunoassay, the other enteric viruses (norovirus [NoV], astrovirus [HAstV], adenovirus [HAdV] and bocavirus [HBoV]) were detected through PCR or RT-PCR. A quantitative PCR was performed for RVA, NoV, HAstV, HAdV and HBoV. Infections with NoV (19% vs. 9.6%; p<0.001), HBoV (14% vs. 7.2%; p = 0.042) and HAdV (30.5% vs. 14.4%; p<0.001) were significantly more frequent among HIV-1 seropositive children. RVA was significantly less frequent among HIV-1 seropositive patients (6.5% vs. 20%; p<0.001). Similarly, frequency of infection with HAstV was lower among HIV-1 seropositive children (5.5% vs. 12.8%; p = 0.018). Among HIV-1 seropositive children 33 (16.5%) had co-infections, including three enteric viruses, such as NoV, HBoV and HAdV (n = 2) and NoV, HAstV and HAdV (n = 2). The frequency of infection with more than one virus was 17 (13.6%) in the HIV-1 negative group, triple infection (NoV + HAstV + HBoV) being observed in only one patient. The median viral load of HAstV in feces was significantly higher among HIV-1 positive children compared to HIV-1 negative children. Concerning children infected with RVA, NoV, HBoV and HAdV, no statistically significant differences were observed in the medians of viral loads in feces, comparing HIV-1 seropositive and HIV-1 seronegative children. Similar detection rates were observed for RVA, HAstV and HAdV, whilst NoV and HBoV were significantly more prevalent among children with CD4+ T lymphocyte count below 200 cells/mm3. Enteric viruses should be considered an important cause of DD in HIV-1 seropositive children, along with pathogens more classically associated with intestinal infections in immunocompromised hosts.

Epidemiology and genetic diversity of classic human astrovirus among hospitalized children with acute gastroenteritis in Uruguay.

Classic Human Astrovirus (Classic HAstV) are one of the most important causes of pediatric acute gastroenteritis (AGE), after rotaviruses and arguably caliciviruses. The aim of this study was to determine the molecular epidemiology of Classic HAstV from 175 clinical samples, being 153 stools and 22 vomits, collected from pediatric hospitalized patients with AGE in Salto city, Uruguay, from January 2011 to December 2012. Classic HAstV were detected and genotyped by using a qualitative Retro Transcription-Polimerase Chain Reaction (RT-PCR) directed to the Open Reading Frame-2 (ORF2) region C. Amplicons were sequenced and phylogenetic analyses were carried out in order to determine genotypes and lineages. Classic HAstV were detected in 18 out of 175 analyzed samples (10.3%) and 14 of them (78.0%) were successfully sequenced being 6 (42.8%) classified as HAstV-1 (1a lineage), 4 (28.6%) as HAstV-2 (2c lineage), and 4 (28.6%) as HAstV-3 (3c lineage). A higher detection of Classic HAstV infections was observed in autumn for both years of surveillance, and the majority of the positive cases were observed in 2011. The group of children between 2 and 5 years old presented the higher percentage of infections. To our knowledge, the present study represents the first report of astrovirus from acute gastroenteritis cases in Uruguay, evidencing its role as a relevant etiologic agent in severe cases of this disease.

Alternative cell lines to improve the rescue of infectious human astrovirus from a cDNA clone.

A reverse genetics system for human astrovirus (HAstV) was established previously; however, it has not been exploited mainly because cells used for virus packaging are not permissive, requiring several rounds of replication to obtain acceptable infectious virus. In this work, in the search for alternative permissive cell lines to be used as packaging cells, Hek-293 and Huh7.5.1 were tested. Given that HAstV infection in Hek-293 showed differences with that in Caco-2, the gold standard for HAstV growth but scarcely transfectable, and it was more similar to that observed in the hepatoma Huh7.5.1 cell line, these last cells were further used to transfect viral RNA. Virus titers near to 10(8) infectious particles per ml (ffu/ml) were obtained at 16-20 h after transfection with RNA from infected cells. However, virus titers close to 10(6) ffu/ml were obtained by using in vitro transcribed RNA from a cDNA HAstV-1 clone. In contrast, virus recovery in BHK-21, reported previously as the packaging cells, from this RNA was of about 10(4) ffu/ml, two logarithms less than in Huh7.5.1. Apparently, the 5'-end modification of the viral RNA determined its specific infectivity, since virus recovery was abolished when the total RNA was treated with proteinase-K, probably by removing a protein-linked genome protein, but it increased when capping of the in vitro transcribed RNA was more efficient. Thus, an alternative and more efficient reverse genetics system for HAstV was established by using Huh7.5.1 cells.

Association of the astrovirus structural protein VP90 with membranes plays a role in virus morphogenesis.

VP90, the capsid polyprotein precursor of human astrovirus Yuc8, is assembled into viral particles, and its processing at the carboxy terminus by cellular caspases, to yield VP70, has been correlated with the cell release of the virus. Here, we characterized the effect of the VP90-VP70 processing on the properties of these proteins, as well as on their intracellular distribution. VP90 was found in membrane-enriched fractions (mVP90), as well as in fractions enriched in cytosolic proteins (cVP90), while VP70 was found exclusively in the latter fractions. Upon trypsin activation, infectivity was detected in all VP90-containing fractions, confirming that both mVP90 and cVP90 are able to assemble into particles; however, the two forms of VP90 showed differential sensitivities to trypsin, especially at their carboxy termini, which in the case of mVP90 was shown to remain membrane associated after protease digestion. Structural protein oligomers were detected in purified VP70-containing viruses, as well as in membrane-enriched fractions, but they were less evident in cytosolic fractions. Ultrastructural studies of infected cells revealed different types of viral particles, some of which appeared to be associated with membranes. By immunoelectron microscopy, structural proteins were shown to form virus particles in clusters and to associate with the edges of vesicles induced during infection, which also appear to contain subviral particles inside. Nonstructural proteins and viral RNA colocalized with mVP90, but not with cVP90, suggesting that mVP90 might represent the form of the protein that is initially assembled into particles, at the sites where the virus genome is being replicated.

Quantitation of human astrovirus by real-time reverse-transcription-polymerase chain reaction to examine correlation with clinical illness.

Human astroviruses (HAstVs) cause gastroenteritis. Real-time, reverse-transcription-polymerase chain reaction (RT2-PCR) was developed to quantitate HAstV RNA. An 88 bp amplicon from the conserved 3' genomic region was detected by binding of SYBR Green. RT2-PCR was reproducible, with a correlation coefficient of 0.998-1.00 and PCR efficiency of 94.4-100% (mean 97%). The coefficient of variation was 0.6-2.5%, dynamic range with RNA standard up to 5 x 10(8) RNA copies (RNACN) and sensitivity 5 RNACN. Of 54 blinded, archived stool samples from children hospitalized because of gastroenteritis tested by RT-PCR, 49 (91%) agreed by RT2-PCR for HAstV-positivity (Cohen kappa=0.81, 95%CI 0.66-0.97). HAstV RNACN in stools ranged from 7.6 x 10(1) to 3.6 x 10(14)copies/0.1g. Children coinfected with rotavirus had lower RNACN (mean log 4.22/standard deviation=2.26) than those without coinfection (7.57/3.06; p=.019). Children taking infant formula also had lower RNACN (5.96/2.98) than breast-fed or weaned children (8.73/2.92; p=.027). Higher RNACN tended to occur with longer duration of diarrhea for the episode (r=0.49, p=.064), but was not associated with change in age, gender, illness day, severity or breast-feeding. RT2-PCR quantitated HAstV RNA and RNACN in stool correlates with features of clinical illness.

Development of an astrovirus RT-PCR detection assay for use with conventional, real-time, and integrated cell culture/RT-PCR.

Astrovirus is a common cause of gastroenteritis in humans that has been determined to be responsible for outbreaks of illness in several countries. Since astrovirus can be waterborne, it is important to be able to identify this virus in environmental water. We have developed and optimized a reverse transcription - polymerase chain reaction (RT-PCR) method that was able to amplify all eight astrovirus serotypes in a single reaction. In addition, a positive control construct was designed so that any inhibitors of this astrovirus assay could be detected. The assay was adapted for use in a real-time PCR assay and the sensitivity of these two methods was compared. The real-time assay was then combined with CaCo2 cell culture to produce an integrated cell culture/RT-PCR (ICC/RT-PCR) assay that was able to detect low levels of astrovirus after an incubation of 7 days or less. Also, the sensitivity of the ICC/RT-PCR assay was compared with RT-PCR alone. The methods were used to detect astrovirus in acute phase illness stool samples as well as in a water sample spiked with astrovirus.

Astrovirus induces diarrhea in the absence of inflammation and cell death.

Astroviruses are a leading cause of infantile viral gastroenteritis worldwide. Very little is known about the mechanisms of astrovirus-induced diarrhea. One reason for this is the lack of a small-animal model. Recently, we isolated a novel strain of astrovirus (TAstV-2) from turkeys with the emerging infectious disease poult enteritis mortality syndrome. In the present studies, we demonstrate that TAstV-2 causes growth depression, decreased thymus size, and enteric infection in infected turkeys. Infectious TAstV-2 can be recovered from multiple tissues, including the blood, suggesting that there is a viremic stage during infection. In spite of the severe diarrhea, histopathologic changes in the intestine were mild and there was a surprising lack of inflammation. This may be due to the increased activation of the potent immunosuppressive cytokine transforming growth factor beta during astrovirus infection. These studies suggest that the turkey will be a useful small-animal model with which to study astrovirus pathogenesis and immunity.

Localization of astrovirus in experimentally infected turkeys as determined by in situ hybridization.

Twenty-one 3-day-old turkey poults from British United Turkeys of America were orally inoculated with a recently characterized astrovirus, TAstV-2, isolated from turkeys with poult enteritis and mortality syndrome. At 1, 2, 3, 4, 5, 7, and 9 days postinfection (dpi), three inoculated birds were euthanatized, and tissues (intestines, spleen, bursa, and thymus) were collected immediately into 10% neutral buffered formalin. Inoculated birds were diarrheic by 3 dpi, and frothy feces persisted throughout the experimental period. Histologically, there was only slight evidence of enteric damage, which was characterized by mild epithelial necrosis, lamina propria infiltrates, minimal villus atrophy, and mild crypt hyperplasia. In situ hybridization, using a negative sense digoxigenin-labeled riboprobe to the capsid gene of TAstV-2, revealed viral RNA in intestinal epithelial cells at the basal margins of the villi, in distal small intestine, and in cecum at 2 dpi, with subsequent extension to epithelium of the large intestine and proximal small intestine (3-5 dpi). Minimal virus remained by 9 dpi.

Potential role of fomites in the vehicular transmission of human astroviruses.

The persistence of human astroviruses dried on representative porous (paper) and nonporous (china) surfaces was investigated. Long-term astrovirus survival on fomites was monitored by an integrated cell culture-reverse transcription-PCR procedure. Viruses were applied to inanimate surfaces in the presence and absence of fecal material, and their survival was assayed at 4 and 20 degrees C with high relative humidity. Astroviruses exhibited a notable persistence when dried on porous and nonporous materials, particularly at low temperature. Short-term survival of astroviruses on fomites was compared to that of other enteric viruses significant for health, such as rotavirus, adenovirus, poliovirus, and hepatitis A virus. Overall, astroviruses persisted better than poliovirus and adenovirus, although they exhibited a shorter survival than rotavirus and hepatitis A virus. Astroviruses show a high level of persistence at the desiccation step, which is of major significance in determining the chance of subsequent virus survival dried on fomites. Astroviruses are able to survive on inert surfaces long enough to suggest that fomites may play a relevant role in the secondary transmission of astrovirus diarrhea.

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.

Human astrovirus isolation and propagation in multiple cell lines.

Laboratory adapted human astrovirus serotypes 1 through 7 were tested for growth in 15 human, 7 simian, and 10 other non-primate mammalian cell lines. Propagation of all seven serotypes was successful in the human cell lines Caco-2, T84, HT-29, and in the African green monkey kidney cell line MA-104. Both primary and secondary African green monkey kidney cells were more effective than Rhesus monkey kidney cells for cultivation of astrovirus. Except for human foreskin cells, all of the other human and simian cell lines supported growth of at least one astrovirus serotype. The only non-primate cell line that permitted sustained passage of astroviruses was the BHK-21 (C13) cell line for astrovirus serotype 2. Seventeen human stool specimens that had previously been shown to be astrovirus positive by ELISA were cultured in Caco-2, T84, HT-29, SK-CO-1, PLC/PRF/5, MA-104, and VERO cells. Caco-2 cells (13 isolates), T84 cells (12 isolates) and PLC/PRF/5 cells (12 isolates) were the cell lines most effective for isolation of human astroviruses from clinical stool specimens. By immunofluorescent staining of infected cells, culturing of the same 17 specimens in shell vials for 18 h was positive for astroviruses in all 17 specimens in Caco-2 cells, 12 in T84 cells, and 7 in PLC/PRF/5 cells. Shell vial assay is suitable as a rapid and sensitive culture technique for detection of astroviruses in clinical specimens.

Detection of astroviruses, enteroviruses, and adenovirus types 40 and 41 in surface waters collected and evaluated by the information collection rule and an integrated cell culture-nested PCR procedure.

We evaluated the use of an integrated cell culture-reverse transcription-PCR (ICC-RT-PCR) procedure coupled with nested PCR to detect human astroviruses, enteroviruses, and adenovirus types 40 and 41 in surface water samples that were collected and evaluated by using the Information Collection Rule (ICR) method. The results obtained with the ICC-RT-PCR-nested PCR method were compared to the results obtained with the total culturable virus assay-most-probable-number (TCVA-MPN) method, the method recommended by the U.S. Environmental Protection Agency for monitoring viruses in surface and finished waters. Twenty-nine ICR surface water samples were analyzed. Viruses were concentrated by using filter adsorption-beef extract elution and organic flocculation techniques, and then the preparations were evaluated for viruses by visualizing cytopathic effects in the Buffalo green monkey kidney (BGMK) cell line. In the ICC-RT-PCR-nested PCR technique we used Caco-2 cells to propagate astroviruses and enteroviruses (ICC step), and we used BGMK cells to propagate adenovirus types 40 and 41, as well as enteroviruses. Fifteen of the 29 samples (51.7%) were positive for astrovirus as determined by the ICC-RT-PCR-nested PCR method, and eight of these samples (27.5%) contained infectious astrovirus. Seventeen of the 29 samples (58.6%) were positive for enteroviruses when the BGMK cell line was used, and six (27.6%) of these samples were determined to be infectious. Fourteen of the 29 samples (48.3%) were positive for adenovirus types 40 and 41, and 11 (37.9%) of these samples were determined to be infectious. Twenty-seven of the 29 samples (93.1%) were positive for a virus, and 19 (68.9%) of the samples were positive for an infectious virus. Only 5 of the 29 samples (17.2%) were positive as determined by the TCVA-MPN method. The ICC-RT-PCR-nested PCR method provided increased sensitivity compared to the TCVA-MPN method.

Improved sensitivity of astrovirus-specific RT-PCR following culture of stool samples in CaCo-2 cells.

BACKGROUND: During an epidemiological study on the incidence of astrovirus infection in children hospitalized with acute gastroenteritis, a Northern hybridization method was used to screen stool samples for astrovirus RNA. Positive results were confirmed using reverse transcriptase-polymerase chain reaction (RT-PCR), which showed surprisingly low sensitivity. The low sensitivity of the RT-PCR method was considered likely to be due to the presence of non-specific inhibitors. OBJECTIVE: To develop and use a simple culture method to improve the sensitivity of diagnosis of astrovirus in clinical stool samples using RT-PCR. STUDY DESIGN: Stool samples from children hospitalized with acute gastroenteritis were screened for astrovirus using Northern hybridization. The presence of astrovirus RNA was then confirmed using an astrovirus-specific RT-PCR. Hybridization positive samples that failed to generate an RT-PCR product were cultured in CaCO-2 cells for 48 h. RNA was isolated from cultures and re-tested using the same RT-PCR method. RESULTS: Using Northern hybridization, human astroviruses were detected in the stools of 31 patients and confirmed by RT-PCR in 16 samples. RNA extracted directly from 15 faecal specimens could not be amplified by RT-PCR. After culture for 48 h in CaCO-2 cells, RNA extracted from these samples could be amplified and confirmed the presence of astrovirus in all 15 specimens. CONCLUSIONS: Development of a simplified culture method for astrovirus positive faecal specimens improved the sensitivity of astrovirus-specific RT-PCR from 52 to 100%. The technique should be of value as a confirmatory test in surveys of human astrovirus infection.

Propagation of human astrovirus in the PLC/PRF/5 hepatoma cell line.

Astroviruses are associated with gastroenteritis in humans and many diseases in animals. Human astroviruses (HAstVs) cannot be propagated readily or isolated in conventional cell cultures. The presence of trypsin supports HAstV growth in selected cell cultures such as the continuous colonic carcinoma cell line (CaCo-2). This study reports on the propagation of cell culture adapted reference strains of HAstV, and the direct isolation of HAstV from stool specimens in the human hepatoma cell line PLC/PRF/5.

Use of the colonic carcinoma cell line CaCo-2 for in vivo amplification and detection of enteric viruses.

The use of the continuous cell line CaCo-2 as an in vivo amplification system for the detection of fastidious human enteric viruses is reported. CaCo-2 cells showed an increased sensitivity to laboratory strains of group A rotavirus 3, reovirus 3, astrovirus 1, poliovirus 1, coxsackievirus A 24, enterovirus 70, and adenovirus 5, 40 and 41, when compared to a routine host cell line for each virus. Nucleic acids from wild-type infectious rotavirus, astrovirus, and adenovirus 40 in stool samples of patients with acute gastroenteritis could be amplified after infection of CaCo-2 cells with trypsin-pre-treated virus inocula. Virus diagnosis was carried out subsequently by dot-blot hybridisation with specific cDNA probes. An amplification factor between 10 and 1,000x was obtained by infection of CaCo-2 cells, thus enabling specific detection of low numbers of a wide range of enteric viruses, and the differentiation between infectious and noninfectious particles.

Temporal synthesis of proteins and RNAs during human astrovirus infection of cultured cells.

Astroviruses are nonenveloped particles with a distinctive star-shaped surface structure that have been detected by electron microscopy in stool samples from humans and animals with gastroenteritis. We examined the patterns of macromolecular synthesis in astrovirus-infected cells with a goal of establishing a molecular basis for taxonomic classification. Trypsin is required for continuous replication of astrovirus in cultured cells; however, during a single cycle of infection, astrovirus antigen was synthesized earlier and at higher levels when serum, rather than trypsin, was included in the growth medium. This enhanced production of antigen, as measured by enzyme immunoassay, was accompanied by the appearance of aggregates of virus particles in the cytoplasm of infected cells. During astrovirus replication in cells cultured in the presence of serum, we detected a single infection-specific protein (90 kDa) beginning at 12 h postinfection. This protein was recognized by antiastrovirus rabbit serum and was sensitive to trypsin digestion in vitro, with the concomitant appearance of three smaller immunoreactive proteins (31, 29, and 20 kDa). We also detected two dactinomycin-resistant RNAs (7.2 and 2.8 kb), both of which were polyadenylated, in the cytoplasm of astrovirus-infected cells. The larger of these two RNAs is presumably the viral genome, whereas the smaller species may be a subgenomic messenger. Comparison of the proteins and RNAs synthesized in astrovirus-infected cells with those of the recognized families of nonenveloped single-stranded RNA animal viruses suggests that astroviruses should not be classified as members of either Caliciviridae or Picornaviridae.