Thermostability of a protein is a property which cannot be attributed to th
e presence of a particular amino acid or to a post synthetic modification.
Thermostability seems to be a property acquired by a protein through many s
mall structural modifications obtained with the exchange of some amino acid
s and the modulation of the canonical forces found in all proteins such as
electrostatic (hydrogen bonds and ion-pairs) and hydrophobic interactions.
Proteins produced by thermo and hyperthermophilic microorganisms, growing b
etween 45 and 110 degrees C are in general more resistant to thermal and ch
emical denaturation than their mesophilic counterparts. The observed struct
ural resistance may reflect a restriction on the flexibility of these prote
ins, which, while allowing them to be functionally competent at elevated te
mperatures, renders them unusually rigid at mesophilic temperatures (10-45
degrees C). The increased rigidity at mesophilic temperatures may find a st
ructural determinant in increased compactness. In thermophilic proteins a n
umber of amino acids are often exchanged. These exchanges with some strateg
ic placement of proline in beta-turns give rise to a stabilization of the p
rotein. Mutagenesis experiments have confirmed this statement. From the com
parative analysis of the X-ray structures available for several families of
proteins, including at least one thermophilic structure in each case, it a
ppears that thermal stabilization is accompanied by an increase in hydrogen
bonds and salt bridges. Thermostability appears also related to a better p
acking within buried regions. Despite these generalisations, no universal r
ules can be found in these proteins to achieve thermostability. (C) Societe
francaise de biochimie et biologie moleculaire / Elsevier, Paris.