Biosignatures and structures in the geological record indicate that microbial life has inhabited Earth for the past 3.5 billion years or so. Research in the physical sciences has been able to generate statements about the ancient environment that hosted this life. These include the chemical compositions and temperatures of the early ocean and atmosphere. Only recently have the natural sciences been able to provide experimental results describing the environments of ancient life. Our previous work with resurrected proteins indicated that ancient life lived in a hot environment. Here we expand the timescale of resurrected proteins to provide a palaeotemperature trend of the environments that hosted life from 3.5 to 0.5 billion years ago. The thermostability of more than 25 phylogenetically dispersed ancestral elongation factors suggest that the environment supporting ancient life cooled progressively by 30 degrees C during that period. Here we show that our results are robust to potential statistical bias associated with the posterior distribution of inferred character states, phylogenetic ambiguity, and uncertainties in the amino-acid equilibrium frequencies used by evolutionary models. Our results are further supported by a nearly identical cooling trend for the ancient ocean as inferred from the deposition of oxygen isotopes. The convergence of results from natural and physical sciences suggest that ancient life has continually adapted to changes in environmental temperatures throughout its evolutionary history.

The 68 residue peptide IA 3 is an intrinsically unstructured protein that serves as an endogenous inhibitor of the yeast aspartic proteinase A (YPrA). Although unstructured in free solution, IA 3 forms an N-terminal alpha helix as it binds to YPrA, leading to subnanomolar inhibition of the protease. Equilibrium structural and inhibition studies provide little insight into the mechanism and kinetics of the coupled folding and binding interaction. We have used laser temperature jump spectroscopy to study the kinetics of folding of free IA 3 and of the interaction between IA 3 and YPrA. Inducing folding with trifluoroethanol cosolvent allows us to determine the folding rate (kf approximately 0.3 (micros)(-1)) and the unfolding rate (ku approximately 3 (micros)(-1)) for free IA 3 in water at 25 degrees C. A substantially faster relaxation process is observed in the presence of the proteinase; this process appears to be the kinetic signature of an intermediate binding step in the coupled folding and binding interaction of IA 3 and YPrA.

IA(3) is a highly specific and potent 68-amino acid endogenous inhibitor of yeast proteinase A (YprA), and X-ray crystallographic studies have shown that IA(3) binds to YprA as an alpha-helix [Li, M., Phylip, L. H., Lees, W. E., Winther, J. R., Dunn, B. M., Wlodawer, A., Kay, J., and Gustchina, A. (2000) Nat. Struct. Biol. 7, 113-117]. Surprisingly, only residues 2-32 of IA(3) are seen in the X-ray structure, and the remaining residues are believed to be disordered in the complex. We have used circular dichroism (CD) and nuclear magnetic resonance (NMR) spectroscopy to show that IA(3) is unstructured in the absence of YprA. Specifically, IA(3) produced a CD spectrum characteristic of an unstructured peptide, and the (15)N HSQC NMR spectra of IA(3) were characteristic of a polypeptide lacking intrinsic structure. We characterized the unstructured state of IA(3) by using singular-value decomposition (SVD) to analyze the CD data in the presence of TFE, by fully assigning the unbound IA(3) protein by NMR and comparing the chemical shifts to published random-coil values, and by measuring (1)H-(15)N heteronuclear NOEs, which are all consistent with an unfolded protein. The IA(3) samples used for NMR analyses were active and inhibited YprA with an inhibition constant (K(i)) of 1.7 nM, and the addition of YprA led to a large spectral transition in IA(3). Calorimetric (ITC) data also show that the overall enthalpy of the interaction between IA(3) and YprA is exothermic.