senior thesis poster
TRANSCRIPT
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Background: Astroviruses are a major cause of diarrhea in c h i l d r e n a n d immuno comp rom i s e d popula5ons. Infec5ons are seasonal in nature, following the rainy season in tropical areas and the winter season in temperate areas. The different serotypes have varying clinical presenta5ons, with diarrhea, fever, and vomi5ng being common symptoms.
Human astroviruses (HAstV) are non-‐enveloped, single-‐stranded, posi5ve sense RNA viruses. The HAstV capsid protein contains 5 dis5nct structural domains. One of these (known as the acidic domain), is thought to be involved in virus matura5on and assembly.
Methods: • Cloning was performed to produce a pET52b expression plasmid containing the acidic domain nucleo5de sequence
• Protein was expressed in the BL21 E. coli cell line
• Purifica9on was performed by affinity and size exclusion chromatography
• Computa5onal tools were used to predict secondary and ter5ary structure
• Nuclear magne5c resonance (NMR) and circular dichroism (CD) were performed to corroborate predicted secondary structural characteris5cs
• A trypsin digest was performed to isolate the puta5ve helical bundle
• Screening trays were set up to find ideal crystalliza9on condi5ons
Acknowledgments: !
! ! Thank you to Professor DuBois for acting as my senior thesis advisor, and to Crown College !! ! for project funding.
Results: Cloning, expression, and purifica5on produced an ample supply of stable acidic domain protein.
Conclusions: While the ter5ary structure of the acidic domain is s5ll unknown, protocols for successfully producing and purifying it have been demonstrated here.
Several lines of evidence (including tryp5c digest paWern, circular dichroism, and sizing behavior) have helped confirm the predicted secondary structure of approximately 40% helix and 60% unstructured.
AWempts to crystallize both the en5re domain and the puta5ve helices isolated by tryp5c digest were ul5mately unsuccessful.
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Elizabeth A. LagesseDuBois Lab, University of California, Santa Cruz
Structural Studies of the Human Astrovirus 1 Capsid Acidic Domain
SDS PAGE aHer size exclusion chromatography showing the acidic domain protein as a bright band just below 25 kDa
Computa5onal tools predicted an N-‐terminal disordered region and a C-‐terminal region consis5ng of four helices. Several ter5ary structure predic5ons were also produced.
RobeLa secondary structure predic9on, showing predicted helices as red “H”s
NMR and CD studies were consistent with a secondary structure of approximately 40% helices and 60% unstructured regions.
2 of 5 RoseLa ter9ary structural predic9ons
To isolate the helices, limited proteolysis was performed with trypsin. The result was a stable band present at all protease concentra5ons. This band was separated using a size exclusion column.
Full length protein and trypsinized fragment were concentrated and used to prepare crystalliza5on condi5on screening trays. Unfortunately, degrada5on of the fragment had already occurred due to residual trypsin in the sample.
No crystals were observed in full length protein or intact fragment. A variety of condi5ons produced crystals in the degraded fragment, but even these were bundles of crystals, unsuitable for diffrac5on.
Trypsin digest concentra9on test ranging from 10:1 to 2500:1 acidic domain:trypsin ra9o (by mass). The red arrow corresponds to the full length construct, and the blue arrow corresponds to the stable band
Crystal bundles formed from degraded protein sample
Domain diagram for the human astrovirus capsid protein
Future Direc9ons: !
• Cloning was performed to produce an expression plasmid with only the helical regions of the acidic domain. (avoiding t ryps in d iges5on) Express ion and purifica5on tests will be performed using this new construct.
!• Func5onal assays are currently in development, which aim to localize the protein within the cell and determine what effect (if any) this domain has on mammalian cells without the presence of the full virus. !• If crystalliza5on proves difficult, a structure for one or both constructs may be pursued via NMR.
Electron micrographs of a single immature astrovirus (leH) and a group of mature astroviruses (right). (Dreyden et. al. 2012, Crea9ve Commons 2.0, respec9vely)