# Metabolic Characterization of Two Flor Yeasts During Second Fermentation in the Bottle for Sparkling Wine Production

**Authors:** Juan Carlos García-García, María Trinidad Alcalá-Jiménez, Juan Carlos Mauricio, Cristina Campos-Vázquez, Inés M. Santos-Dueñas, Juan Moreno, Teresa García-Martínez

PMC · DOI: 10.3390/ijms262110457 · 2025-10-28

## TL;DR

This study compares two flor yeast strains during sparkling wine fermentation, showing they produce distinct flavors and could improve wine diversity.

## Contribution

The study provides new insights into the metabolic profiles of two flor yeast strains in sparkling wine production.

## Key findings

- Strain N62 fermented faster and reached 3 bar pressure in 27 days, while G1 took 52 days.
- G1 produced higher levels of 3-methyl-1-butanol and acetaldehyde, while N62 generated more glycerol and amino acids.
- Both strains produced distinct volatile and nitrogen compound profiles, suggesting unique sensory impacts.

## Abstract

The global sparkling wine market continues to grow steadily, reaching approximately 24 million hectoliters in 2023, with an annual increase of around 4% despite a general decline in overall alcoholic beverage consumption. This growth highlights the importance of employing diverse yeast strains to improve product variety and quality. Flor yeasts are specialized strains of Saccharomyces cerevisiae that develop a biofilm on the surface of certain wines during biological ageing. They possess unique physiological properties, including high ethanol tolerance and the capacity to adhere, which supports wine clarification. They also have the ability to contribute unique volatile compounds and aroma profiles, making them promising candidates for sparkling wine production. This study evaluated two flor yeast strains (G1 and N62), which were isolated from the Pérez Barquero winery during the second fermentation process using the traditional method. Sparkling wines were produced by inoculating base wine (BW) with each strain, and the wines were monitored at 3 bar CO2 pressure and after 9 months of ageing on lees. Comprehensive metabolomic analysis was performed using GC-MS for volatile compounds and HPLC for nitrogen compounds, with statistical analysis including PCA, ANOVA, Fisher’s LSD, and correction FDR tests. Strain N62 demonstrated faster fermentation kinetics and higher cellular concentration, reaching 3 bar pressure in 27 days compared to 52 days for strain G1. Both strains achieved similar final pressures, 5.1–5.4 bars. Metabolomic profiling revealed significant differences in the profiles of volatile and nitrogen compounds between the two strains. G1 produced higher concentrations of 3-methyl-1-butanol, 2-methyl-1-butanol, and acetaldehyde, while N62 generated elevated levels of glycerol, ethyl esters, and amino acids, including glutamic acid, aspartic acid, and alanine. These findings demonstrate that both flor yeast strains successfully complete sparkling wine fermentation while producing distinct metabolic signatures that could contribute to unique sensory characteristics. This supports their potential as alternatives to conventional sparkling wine yeasts for enhanced product diversification.

## Linked entities

- **Chemicals:** 3-methyl-1-butanol (PubChem CID 31260), 2-methyl-1-butanol (PubChem CID 8723), acetaldehyde (PubChem CID 177), glycerol (PubChem CID 753), glutamic acid (PubChem CID 611), aspartic acid (PubChem CID 424), alanine (PubChem CID 239)
- **Species:** Saccharomyces cerevisiae (taxon 4932)

## Full-text entities

- **Chemicals:** nitrogen (MESH:D009584), glycerol (MESH:D005990), ethanol (MESH:D000431), CO2 (MESH:D002245), 2-methyl-1-butanol (-), 3-methyl-1-butanol (MESH:C029683), alanine (MESH:D000409), aspartic acid (MESH:D001224), acetaldehyde (MESH:D000079), glutamic acid (MESH:D018698), ethyl esters (MESH:C465446), amino acids (MESH:D000596)
- **Species:** Saccharomyces cerevisiae (baker's yeast, species) [taxon 4932]

## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/PMC12609295/full.md

---
Source: https://tomesphere.com/paper/PMC12609295