Wine Protein Haze: Mechanisms of Formation and Advances in


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Wine Protein Haze: Mechanisms of Formation and Advances in Prevention Steven C Van Sluyter, Jacqui M. McRae, Robert John Falconer, Paul A. Smith, Antony Bacic, Elizabeth J. Waters, and Matteo Marangon J. Agric. Food Chem., Just Accepted Manuscript • Publication Date (Web): 07 Apr 2015 Downloaded from http://pubs.acs.org on April 7, 2015

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Journal of Agricultural and Food Chemistry is published by the American Chemical Society. 1155 Sixteenth Street N.W., Washington, DC 20036 Published by American Chemical Society. Copyright © American Chemical Society. However, no copyright claim is made to original U.S. Government works, or works produced by employees of any Commonwealth realm Crown government in the course of their duties.

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Journal of Agricultural and Food Chemistry

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Wine Protein Haze: Mechanisms of Formation and Advances in Prevention

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Steven C. Van Sluytera,b,c*, Jacqui M. McRaea, Robert J. Falconerd, Paul A. Smitha, Antony

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Bacicb, Elizabeth J. Watersa,e, Matteo Marangon a,f*

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a

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Australia

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b

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University of Melbourne, Victoria 3010, Australia

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c

Department of Biological Sciences, Macquarie University, New South Wales 2109, Australia

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d

Department of Chemical & Biological Engineering, ChELSI Institute, University of Sheffield,

The Australian Wine Research Institute, P.O Box 197, Glen Osmond, South Australia 5064,

School of BioSciences and the Bio21 Molecular Sciences & Biotechnology Institute,

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Sheffield, S1 3JD, England

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e

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Australia

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f

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*Corresponding authors: E-mail: [email protected]. Phone: +61 (0)2 9850 6316.

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Fax: +61 (0)2 9850 8245. E-mail: [email protected]. Phone: +44 (0)1273

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890454. Fax: +44 (0) 1273 890071

Australian Grape and Wine Authority, P.O. Box 2733, Adelaide, South Australia 5000,

Plumpton College, Ditchling Road, Nr Lewes, BN7 3AE, England

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Abstract

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Protein haze is an aesthetic problem in white wines that can be prevented by removing

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grape proteins that have survived the winemaking process. The haze forming proteins are

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grape pathogenesis-related proteins that are highly stable during winemaking, but some of

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them precipitate over time and with elevated temperatures. Protein removal is currently

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achieved by bentonite addition, an inefficient process that can lead to higher costs and

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quality losses in winemaking. The development of more efficient processes for protein

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removal and haze prevention requires understanding mechanisms such as the main drivers

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of protein instability and the impacts of various wine matrix components on haze formation.

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This review covers recent developments in wine protein instability and removal and

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proposes a revised mechanism of protein haze formation.

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Keywords

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bentonite alternatives, chitinases, pathogenesis-related proteins, protease, protein

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aggregation, thaumatin-like protein, wine haze, wine heat instability, wine protein

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Introduction

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In 2012 there were 7.528 million hectares of cultivated grape vines among 92 countries,

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making grapes the largest fruit crop by land area in the world.1,2 Furthermore, much value is

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added in the form of winemaking to over half the world’s grapes, with the production of 252

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millions of hectolitres of wine in 2012.2 The contribution of the wine sector to the world

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economy in 2013 reached a value of $277.5 billion3 with a large proportion of the wine

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exported. Thus a substantial volume of wine is subject to potentially damaging conditions

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during transportation and storage, such as inappropriate temperature or humidity, that can

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cause deleterious modifications of the organoleptic features of the wine.4

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Wine clarity, especially that of white wines (Figure 1), is important to most consumers and is

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also one of the characteristics that is most easily affected by inappropriate shipping and

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storage conditions. For this reason, securing wine stability prior to bottling is an essential

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step of the winemaking process and presents a significant challenge for winemakers. A

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stable white wine is one that is clear and free from precipitates at the time of bottling,

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through transport and storage to the time of consumption. Hazy wine and the presence of

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precipitates are most commonly caused by three factors: microbial instability, tartrate

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instability, and protein heat instability.5 Microbial stability is achieved prior to bottling by

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sulfur dioxide addition and filtration;6 tartrate stability is achieved by either cold

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stabilization, ion exchange resins or electrodialysis.7

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Protein stability in commercial winemaking is almost always achieved by the addition of

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bentonite, a clay cation exchanger that binds proteins and removes them from wine

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through precipitation. Protein-bound bentonite settles loosely to the bottom of wine tanks

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as lees, which account for around 3-10% of the original wine volume.8 Wine is recovered

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from bentonite lees through processing using rotary drum vacuum filtration, specialized lees 3 ACS Paragon Plus Environment

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filtration equipment, or centrifugation - processes that are considered laborious and that

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can potentially degrade wine quality.8–10 Quality degradation and loss of wine through

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bentonite usage has been estimated to cost the global wine industry around US$ 1 billion

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per year.11 Other issues and costs related to bentonite use include tank downtime for

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bentonite treatment, occupational health risks associated with inhalation of bentonite dust

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and slip hazards induced by bentonite slurry spills, the disposal of hazardous bentonite

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waste, and bentonite interference with increasingly common membrane-based winemaking

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technologies.12 Consequently, winemakers aim to use the minimum amount of bentonite

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required for protein stability and would welcome the introduction of alternatives with fewer

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drawbacks than the current practice.

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Since the last extensive review on the topic a decade ago8, research efforts have been

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equally divided into the elucidation of protein haze-forming mechanisms, in particular the

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effects of different wine components, as well as improving bentonite efficiency and finding

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alternative stabilization strategies. Significant attention has also been paid to developing

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methods for protein purification, quantification and identification, as well as predicting wine

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haze potential (Figure 2).

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This review summarizes recent advances in the knowledge of how protein haze forms in

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wine, as well as the latest alternatives to bentonite wine protein stabilization. The findings

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of recent research and the newly-proposed mechanisms for haze will be discussed in Part I.

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New alternatives to bentonite will be discussed in Part II.

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Part I. Mechanisms of protein haze formation in white wines

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Current model of haze formation. The mechanisms associated with haze formation in wines

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are not well understood and yet is commonly cited as a two-stage process. In the first stage,

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wine proteins unfold in response to stimuli such as elevated storage temperatures. Once 4 ACS Paragon Plus Environment

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unfolded, the proteins aggregate and flocculate to form a visible haze.13 Recent

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investigations of the proteins associated with haze formation, as well as the roles of other

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wine components, have enabled the proposed model to be revised into three separate

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stages described below. The steps include protein unfolding, protein self-aggregation and

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aggregate cross-linking.

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Haze-forming proteins. The isolation and characterization of proteins from white wines has

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traditionally been a difficult task due to the presence of grape and yeast proteins as well as

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their modified versions and degradation products caused by winemaking, which produces a

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complex protein mixture.14,15 However recent advances in techniques for wine protein

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purification,16,17 as well as applications of newly-developed proteomic techniques16,18–25,

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and the release of the grape genome,26 have significantly improved research capabilities in

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the identification and quantification of grape and wine proteins.

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The most abundant classes of haze-forming proteins that occur in grape (Vitis vinifera) juice

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and white wines are chitinases and thaumatin-like proteins (TLPs).14,27–29 These proteins are

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small (