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Issue
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Ann. Phys. Fr.
Volume 27, Number 4, 2002
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1 - 106 |
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10.1051/anphys:2002004 |
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Ann. Phys. Fr., Vol. 27, N°4 2002, pp. 1-106
DOI: 10.1051/anphys:2002004
La physique des bulles de champagne.
Une première approche des processus physico-chimiques liés à l'effervescence des vins de Champagne
G. Liger-Belair
Laboratoire d'oenonologie, Faculté des sciences, B.P. 1039, 51687 Reims Cedex 2, France.
Abstract - Physicochemical approach to the effervescence in Champagne wines.
People have long been fascinated by bubbles and foams dynamics, and since the
pioneering work of Leonardo da Vinci in the early 16th century, this subject has generated a
huge bibliography. However, only very recently, much interest was devoted to bubbles in
Champagne wines. Small bubbles rising through the liquid, as well as a bubble ring (the so-called collar) at the periphery of a flute poured with champagne are the hallmark of this
traditionally festive wine, and even there is no scientific evidence yet to connect the quality of
a champagne with its effervescence, people nevertheless often make a connection between
them. Therefore, since the last few years, a better understanding of the numerous parameters
involved in the bubbling process has become an important stake in the champagne research
area. Otherwise, in addition to these strictly enological reasons, we also feel that the area of
bubble dynamics could benefit from the simple but close observation of a glass poured with
champagne. In this study, our first results concerning the close observation of the three main
steps of a champagne bubble's life are presented, that is, the bubble nucleation on tiny
particles stuck on the glass wall (Chap. 2), the bubble ascent through the liquid (Chap. 3),
and the bursting of bubbles at the free surface, which constitutes the most intriguing and
visually appealing step (Chap. 4). Our results were obtained in real consuming conditions,
that is, in a classical crystal flute poured with a standard commercial champagne wine.
Champagne bubble nucleation proved to be a fantastic everyday example to illustrate
the non-classical heterogeneous bubble nucleation process in a weakly supersaturated liquid.
Contrary to a generally accepted idea, nucleation sites are not located on irregularities of the
glass itself. Most of nucleation sites are located on tiny hollow and roughly cylindrical
exogenous fibres coming from the surrounding air or remaining from the wiping process.
Because of their geometry and hydrophobic properties, such particles are able to entrap gas
pockets during the filling of a flute and to start up the bubble production process. Such
particles are responsible for the clockwork and repetitive production of bubbles that rise in-line into the form of elegant bubble trains. This cycle of bubble production at a given
nucleation site is characterised by its bubbling frequency. The time needed to reach the
moment of bubble detachment depends on the kinetics of the CO
2 molecules transfer from the
champagne to the gas pocket, but also on the geometrical properties of the given nucleation
site. Now, since a collection of particle shapes and sizes exists on the glass wall, the bubbling
frequency may also vary from one site to another. Three minutes after pouring, we measured
bubbling frequencies ranging from less than 1 Hz up to almost 30 Hz, which means that the
most active nucleation sites emit up to 30 bubbles per second.
After their detachment from nucleation sites, champagne bubbles rise in-line through
the liquid into the form of elegant bubble trains. Since they collect dissolved carbon dioxide
molecules, champagne bubbles expand during ascent and therefore constitute an original tool
to investigate the dynamics of rising and expanding bubbles. Hydrodynamically speaking,
champagne bubbles were found to reach a quasi-stationary stage intermediate between that of
a rigid and that a fluid sphere (but nevertheless closer to that of a fluid sphere). This result
drastically differs from the result classically observed with bubbles of fixed radii rising in
surfactant solutions. Since surfactants progressively adsorb at the bubble surface during the
rise, the drag coefficient of a rising bubble of fixed radius progressively increases, and finally
reaches the rigid sphere limit when the bubble interface gets completely contaminated. In the
case of champagne, since a bubble expands during its rise through the supersaturated liquid,
the bubble interface continuously increases and therefore continuously offers newly created
surface to the adsorbed surface-active materials (around 5 mg/l, mostly composed of proteins
and glycoproteins). Champagne bubbles experience an interesting competition between two
opposing effects. Our results suggest that the bubble growth during ascent approximately
balance the adsorption rate of surface-active compounds on the rising bubble. We also
compared the behaviour of champagne bubbles with that of beer bubbles. It was found that
beer bubbles showed a behaviour, very close to that of rigid spheres. This is not a surprising
result, since beer contains much higher amounts of surface-active molecules (of order of
several hundreds mg/l) likely to be adsorbed at a bubble interface. Furthermore, since the gas
content is lower in beer, growth rates of beer bubbles are lower than those of champagne. As a
result, the dilution effect due to the rate of dilatation of the bubble area may be too weak to
avoid the rigidification of the beer bubble interface.
In a third set of experiments, we used instantaneous high-speed photography techniques
to freeze the dynamics of bubbles collapsing at the free surface of a glass poured with
champagne. The process following bubble collapse and leading to the projection of a high-speed liquid jet above the free surface was captured. A structural analogy between the liquid
jet following a bubble collapse and the liquid jet following a drop impact was presented. By
drawing a parallel between the fizz in champagne wines and the "fizz of the ocean", we also
suggested that droplets issued from champagne bursting bubbles contain much higher
amounts of surface-active and potentially aromatic materials than the liquid bulk. The
bursting of champagne bubbles is thus expected to play a major role in flavour release.
Otherwise, since the first photographic investigation were published about fifty years
ago, numerous experiments have been conducted with single bubbles collapsing at a free
surface. But, to the best of our knowledge, and surprising as it may seem, no results
concerning the collateral effects on adjoining bubbles of bubbles collapsing in a bubble
monolayer have been reported up to now. Actually, effervescence in a glass of champagne
ideally lends to a preliminary work with bubbles collapsing in a bubble monolayer. For a few
seconds after pouring, the free surface is completely covered with a monolayer composed of
quite monodisperse millimetric bubbles collapsing close to each others. We took high-speed photographs of the situation which immediately follows the rupture of a bubble cap in a
bubble monolayer. Adjoining bubbles were found to be literally sucked and strongly stretched
toward the lowest part of the cavity left by the bursting bubble, leading to unexpected and
short-lived flower-shaped structures. Stresses in distorted bubbles (petals of the flower-shaped
structure) were evaluated and found to be, at least, one order of magnitude higher than
stresses numerically calculated in the boundary layer around an isolated single millimetric
collapsing bubble. This is a brand-new and slightly counter-intuitive result. While absorbing
the energy released during collapse, as an air-bag would do, adjoining bubble caps store this
energy into their thin liquid film, leading finally to stresses much higher than those observed
in the boundary layer around single millimetric collapsing bubbles. Further investigation
should be conducted now, and especially numerically, in order to better understand the
relative influence of each pertinent parameters (bubble size, liquid density and viscosity,
effect of surfactant...) on bubble deformation.
Résumé
L'objectif général de cet ouvrage consacré à l'étude des processus physico- chimiques de
l'effervescence des vins de Champagne était de décortiquer les différentes étapes de la vie
d'une bulle de champagne en conditions réelles de consommation, dans une flûte. Nous
résumons ci-après les principaux résultats obtenus pour chacune des étapes de la vie de la
bulle, depuis sa naissance sur les parois d'une flûte, jusqu'à son éclatement en surface.
Naissance de la bulle
À l'aide d'une caméra munie d'un objectif de microscope, nous avons pu mettre en
évidence les particules qui jouent le rôle de sites de nucléation des bulles sur les parois
d'une flûte à champagne. Dans la très
grande majorité des cas, ce sont des fibres creuses et
allongées, de quelques dizaines à quelques centaines de microns, qui assurent la production
répétitive de bulles par nucléation hétérogène non classique (de type IV). Cette production
répétitive de bulles au niveau des sites de nucléation est caractérisée par une gamme de
fréquences de bullage assez large. Au sein d'une même flûte, immédiatement après le
versement, nous avons mesuré des fréquences qui varient de moins de 1 Hz à presque 30 Hz. C'est donc jusqu'à 30 bulles qui sont émises chaque seconde par les sites de nucléation
les plus actifs.
Vitesse ascensionnelle d'une bulle
Pour mesurer la vitesse d'une bulle tout au long de son trajet vers la surface libre du
champagne, nous avons tiré profit de la production répétitive de bulles au niveau des sites
de nucléation. Par la mise en place d'un dispositif expérimental simple qui associe une
lumière stroboscopique et un appareil photographique muni de bagues macros, nous avons
pu accéder à l'observation fine des trains de bulles ainsi qu'à la détermination de la vitesse
ascensionnelle des bulles. Les mesures expérimentales du rayon et de la vitesse d'une bulle
nous ont permis de déterminer le coefficient de traînée d'une bulle montante qui constitue
une mesure indirecte de son état de surface en terme de mobilité interfaciale. Ces mesures
nous ont montré que l'interface d'une bulle de champagne conserve une grande mobilité
pendant sa phase ascensionnelle. C'est la faible dilution du champagne en
macromolécules tensioactives et le grossissement continu des bulles pendant l'ascension
qui assurent aux bulles une faible contamination de leur interface en molécules
tensioactives. Pour comparaison, nous avons réalisé le même type de mesures sur des
bulles de bière. Le contenu en macromolécules tensioactives étant beaucoup plus important
dans une bière, l'effet de dilution du matériel tensioactif à la surface des bulles lié à l'accroissement de la surface des bulles ne compense plus l'adsorption massive des
tensioactifs à la surface des bulles. Contrairement aux bulles du champagne, les bulles de
bière adoptent vite un comportement de type sphère rigide.
Éclatement d'une bulle en surface
Nous avons obtenu des images de la situation qui suit immédiatement la rupture du
mince film liquide qui constitue la partie émergée d'une bulle en surface. Nous avons ainsi
pu mettre en évidence l'existence des jets de liquide engendrés par les éclatements de
bulle. En faisant un parallèle légitime entre le pétillement des bulles à la surface du
champagne et le "pétillement de l'océan", nous avons émis l'idée
que les gouttelettes de jet étaient beaucoup plus concentrées en matériel tensioactif (et potentiellement aromatique)
que le coeur de phase du liquide. Il semble donc que les éclatements de bulles jouent un
rôle essentiel dans l'effet exhausteur d'arôme au cours de la dégustation d'un champagne.
Pendant les quelques secondes qui suivent le versement du champagne dans la flûte,
nous avons également réalisé des clichés d'éclatement de bulles en monocouche. Les
premiers résultats de ces observations font apparaître des déformations spectaculaires dans
le film liquide des bulles premières voisines. Ces premières images suggèrent des
contraintes, dans le mince film des bulles déformées, très supérieures à celles qui existent
dans le sillage d'une bulle isolée qui éclate.
© EDP Sciences 2002
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