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1.
Cell ; 159(5): 1096-1109, 2014 Nov 20.
Artigo em Inglês | MEDLINE | ID: mdl-25416948

RESUMO

The HIV-1 Gag protein orchestrates all steps of virion genesis, including membrane targeting and RNA recruitment into virions. Using crosslinking-immunoprecipitation (CLIP) sequencing, we uncover several dramatic changes in the RNA-binding properties of Gag that occur during virion genesis, coincident with membrane binding, multimerization, and proteolytic maturation. Prior to assembly, and after virion assembly and maturation, the nucleocapsid domain of Gag preferentially binds to psi and Rev Response elements in the viral genome, and GU-rich mRNA sequences. However, during virion genesis, this specificity transiently changes in a manner that facilitates genome packaging; nucleocapsid binds to many sites on the HIV-1 genome and to mRNA sequences with a HIV-1-like, A-rich nucleotide composition. Additionally, we find that the matrix domain of Gag binds almost exclusively to specific tRNAs in the cytosol, and this association regulates Gag binding to cellular membranes.


Assuntos
HIV-1/fisiologia , RNA Viral/metabolismo , Produtos do Gene gag do Vírus da Imunodeficiência Humana/metabolismo , Sequência de Bases , Linhagem Celular , Imunoprecipitação da Cromatina , Genes env , Humanos , Dados de Sequência Molecular , Estrutura Terciária de Proteína , RNA de Transferência/metabolismo , Montagem de Vírus , Produtos do Gene gag do Vírus da Imunodeficiência Humana/química
2.
Nature ; 611(7937): 677-681, 2022 11.
Artigo em Inglês | MEDLINE | ID: mdl-36418451

RESUMO

Most of the light from blazars, active galactic nuclei with jets of magnetized plasma that point nearly along the line of sight, is produced by high-energy particles, up to around 1 TeV. Although the jets are known to be ultimately powered by a supermassive black hole, how the particles are accelerated to such high energies has been an unanswered question. The process must be related to the magnetic field, which can be probed by observations of the polarization of light from the jets. Measurements of the radio to optical polarization-the only range available until now-probe extended regions of the jet containing particles that left the acceleration site days to years earlier1-3, and hence do not directly explore the acceleration mechanism, as could X-ray measurements. Here we report the detection of X-ray polarization from the blazar Markarian 501 (Mrk 501). We measure an X-ray linear polarization degree ΠX of around 10%, which is a factor of around 2 higher than the value at optical wavelengths, with a polarization angle parallel to the radio jet. This points to a shock front as the source of particle acceleration and also implies that the plasma becomes increasingly turbulent with distance from the shock.

3.
J Virol ; 91(17)2017 09 01.
Artigo em Inglês | MEDLINE | ID: mdl-28615207

RESUMO

Recent evidence indicates that inhibition of HIV-1 integrase (IN) binding to the viral RNA genome by allosteric integrase inhibitors (ALLINIs) or through mutations within IN yields aberrant particles in which the viral ribonucleoprotein complexes (vRNPs) are eccentrically localized outside the capsid lattice. These particles are noninfectious and are blocked at an early reverse transcription stage in target cells. However, the basis of this reverse transcription defect is unknown. Here, we show that the viral RNA genome and IN from ALLINI-treated virions are prematurely degraded in target cells, whereas reverse transcriptase remains active and stably associated with the capsid lattice. The aberrantly shaped cores in ALLINI-treated particles can efficiently saturate and be degraded by a restricting TRIM5 protein, indicating that they are still composed of capsid proteins arranged in a hexagonal lattice. Notably, the fates of viral core components follow a similar pattern in cells infected with eccentric particles generated by mutations within IN that inhibit its binding to the viral RNA genome. We propose that IN-RNA interactions allow packaging of both the viral RNA genome and IN within the protective capsid lattice to ensure subsequent reverse transcription and productive infection in target cells. Conversely, disruption of these interactions by ALLINIs or mutations in IN leads to premature degradation of both the viral RNA genome and IN, as well as the spatial separation of reverse transcriptase from the viral genome during early steps of infection.IMPORTANCE Recent evidence indicates that HIV-1 integrase (IN) plays a key role during particle maturation by binding to the viral RNA genome. Inhibition of IN-RNA interactions yields aberrant particles with the viral ribonucleoprotein complexes (vRNPs) eccentrically localized outside the conical capsid lattice. Although these particles contain all of the components necessary for reverse transcription, they are blocked at an early reverse transcription stage in target cells. To explain the basis of this defect, we tracked the fates of multiple viral components in infected cells. Here, we show that the viral RNA genome and IN in eccentric particles are prematurely degraded, whereas reverse transcriptase remains active and stably associated within the capsid lattice. We propose that IN-RNA interactions ensure the packaging of both vRNPs and IN within the protective capsid cores to facilitate subsequent reverse transcription and productive infection in target cells.


Assuntos
Capsídeo/metabolismo , Proteínas de Transporte/metabolismo , Genoma Viral , Inibidores de Integrase de HIV/farmacologia , Integrase de HIV/metabolismo , Transcriptase Reversa do HIV/metabolismo , Animais , Fatores de Restrição Antivirais , Células CHO , Cricetulus , Células HEK293 , HIV-1/efeitos dos fármacos , HIV-1/genética , Humanos , RNA Viral/genética , Proteínas com Motivo Tripartido , Ubiquitina-Proteína Ligases , Montagem de Vírus/efeitos dos fármacos
4.
PLoS Pathog ; 12(8): e1005833, 2016 08.
Artigo em Inglês | MEDLINE | ID: mdl-27541140

RESUMO

The APOBEC3 (A3) cytidine deaminases are antiretroviral proteins, whose targets include human immunodeficiency virus type-1 (HIV-1). Their incorporation into viral particles is critical for antiviral activity and is driven by interactions with the RNA molecules that are packaged into virions. However, it is unclear whether A3 proteins preferentially target RNA molecules that are destined to be packaged and if so, how. Using cross-linking immunoprecipitation sequencing (CLIP-seq), we determined the RNA binding preferences of the A3F, A3G and A3H proteins. We found that A3 proteins bind preferentially to RNA segments with particular properties, both in cells and in virions. Specifically, A3 proteins target RNA sequences that are G-rich and/or A-rich and are not scanned by ribosomes during translation. Comparative analyses of HIV-1 Gag, nucleocapsid (NC) and A3 RNA binding to HIV-1 RNA in cells and virions revealed the striking finding that A3 proteins partially mimic the RNA binding specificity of the HIV-1 NC protein. These findings suggest a model for A3 incorporation into HIV-1 virions in which an NC-like RNA binding specificity is determined by nucleotide composition rather than sequence. This model reconciles the promiscuity of A3 RNA binding that has been observed in previous studies with a presumed advantage that would accompany selective binding to RNAs that are destined to be packaged into virions.


Assuntos
Citosina Desaminase/metabolismo , HIV-1/metabolismo , Nucleocapsídeo/metabolismo , RNA Viral/metabolismo , Produtos do Gene gag do Vírus da Imunodeficiência Humana/metabolismo , Desaminases APOBEC , Citidina Desaminase , Citosina Desaminase/genética , Células HEK293 , HIV-1/genética , Humanos , Nucleocapsídeo/genética , RNA Viral/genética , Produtos do Gene gag do Vírus da Imunodeficiência Humana/genética
5.
Science ; 378(6620): 646-650, 2022 11 11.
Artigo em Inglês | MEDLINE | ID: mdl-36356124

RESUMO

Magnetars are neutron stars with ultrastrong magnetic fields, which can be observed in x-rays. Polarization measurements could provide information on their magnetic fields and surface properties. We observed polarized x-rays from the magnetar 4U 0142+61 using the Imaging X-ray Polarimetry Explorer and found a linear polarization degree of 13.5 ± 0.8% averaged over the 2- to 8-kilo-electron volt band. The polarization changes with energy: The degree is 15.0 ± 1.0% at 2 to 4 kilo-electron volts, drops below the instrumental sensitivity ~4 to 5 kilo-electron volts, and rises to 35.2 ± 7.1% at 5.5 to 8 kilo-electron volts. The polarization angle also changes by 90° at ~4 to 5 kilo-electron volts. These results are consistent with a model in which thermal radiation from the magnetar surface is reprocessed by scattering off charged particles in the magnetosphere.

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