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Department of Biochemistry and Molecular Genetics, College of Medicine, University of Illinois at Chicago, Chicago, Illinois 60607
Correspondence: Address reprint requests to Xiubei Liao, Tel.: 312-996-7672; Fax: 312-413-0364; E-mail: xiubei{at}uic.edu.
| ABSTRACT |
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| INTRODUCTION |
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Previous structural determinations have shown that the winged helix motif is constructed from a tightly packed core, constituted from three helices and a three-strand ß-sheet and two dynamic wings (Clark et al., 1993
; Jin et al., 1999
; Lai et al., 1993
; van Dongen et al., 2000
; Weigelt et al., 2001
). The DNA recognition of winged helix proteins is achieved mainly through the contacts made by helix 3 and wing 2. The structure and dynamics of a conserved HNF-3 homolog, Genesis, in complex with a strong DNA binding site indicate that even though both wings contact DNA, wing 1 still shows large amplitude of motions in the complex (Jin et al, 1998
; Jin and Liao, 1999
). Thus, it is not clear what is the role of this wing in the DNA recognitions. Furthermore, the amino acid sequence of wing 1 is one of the divergent sequences in the HNF-3 homologous proteins and these divergent sequences may play important roles for the functions of the HNF-3 family members. In a recent study, the DNA binding domain of HNF-3ß alone was shown to interact with the cut-homeo DNA binding domains of transcription factor HNF-6 (Rausa et al., 2003
). This interaction stimulates the HNF-3ß activity on a promoter, while blocking HNF-6 binding to DNA. In another study, the DNA binding domain of Genesis was recognized by the transcription factor Oct4, which represses the activity of Genesis on a promoter (Guo et al., 2002
). These interactions are highly specific. For example, even though the sequences of HNF-3ß and HNF-3
are almost identical, HNF-6 recognizes HNF-3ß as well as Genesis, but not HNF-3
(Rausa et al., 2003
). Apparently, the relatively divergent sequences such as wing 1, in the winged helix proteins have to function as recognition markers for the recognition of other cofactors in the transcriptional regulation. To understand potential roles of wing 1 in protein-protein, protein-DNA, and DNA-binding dependent protein-protein interactions, a systematic study of wing 1 is necessary.
As the first step in understanding the roles of these divergent sequences, two wing 1 mutants were constructed, and the biophysical and biochemical properties of the mutants and the wild-type Genesis were compared. In this report, we demonstrate that the amino acid substitutions (70NG73KG and 70NP73KP) in the eight-residue wing 1 sequence influence thermodynamic and internal dynamic properties of the winged helix protein Genesis and its DNA complex. Thus, our data demonstrate important roles for this long, divergent, and flexible sequence in the winged helix DNA binding motif.
| MATERIALS AND METHODS |
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1 mM determined with BioRad protein assay (BioRad, Hercules, CA). The concentration of the wild-type Genesis was
0.2 mM. The proteins used for circular dichroism (CD) and fluorescent measurements were grown in LB-rich media.
Thermodynamic stability measurements
CD measurements were performed on a Jasco J-710 spectropolarimeter (Jasco, Victoria, BC, Canada) in 1-mm cells using temperature-scanning mode. The denaturation temperatures of these proteins were calculated using the standard analysis program supplied by the manufacturer.
Fluorescence spectra were obtained in a double spectrometer using 1-cm cells at a protein concentration of 1 µM. The excitation wavelength was set to 284 nm and the bandwidth of excitation and emission was 4 nm. Urea-dependent fluorescence spectra were recorded to follow the unfolding progress and to calculate the Gibbs free energy difference of the proteins unfolding at 0 M urea (
Gu(H2O)). The fluorescence originated mainly from two Trp residues W47 and W77. Their emission maximum shifts from 330 nm to 360 nm during the unfolding process. The ratio of the fluorescence intensity of these two wavelengths (F) is normalized and is a measure of the unfolding progress.
Since F = kn/ku
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Gu(H2O) can be calculated from extrapolation of the unfolding curve to 0 M urea.
NMR experiments
The HSQC and 15N-NOESY-HSQC (mixing time = 180 ms), 15R1, 15N R2, and {1H}-15N NOE spectra were recorded on a Bruker DRX 600 MHz spectrometer. The measurements were performed at 17°C for the DNA-free mutant proteins and at 27°C for the complexes, since the DNA-free proteins are much less stable than the complexes, and at 17°C the signal-to-noise ratios of the spectra of the complexes are not sufficient for accurate determinations of relaxation parameters under the current experimental condition. Standard pulse sequences were used in these measurements (Kay, 1997
; Farrow et al., 1995
). The intensities of peaks in the two-dimensional spectra were determined by a peak-picking macro in the commercial software SYBYL (Tripos Inc., St. Louis, MO). The relaxation rate constants were determined by fitting the measured peak heights to two-parameter single exponential functions by using the linear least-square method as described previously (Press et al., 1989
).
Determination of the stability of the Genesis-DNA complexes by gel-shift assay
Binding reaction mixture contained 20 mM Hepes (pH 7.9), 40 mM KCl, 2 mM MgCl2, 0.05 mM DTT, 0.01% NP-40, 5 µg (
5 µM) BSA, 1.5 µg (
0.7 µM) poly(dI-dC), 0.5 ng (
5 nM) Genesis probe HFH-2#12, and either 5 ng (
5 nM) of Genesis or 70NG73KG or 70NP73KP mutant. Total volume was set to 19 µl, and reaction mixtures were incubated for 20 min at room temperature before adding 100-fold of the unlabeled probe. After the incubation for an indicated length for a reaction at room temperature, 4 µl of 20% Ficoll was added and 8 µl of the reaction mixture was immediately analyzed on a 9% nondenaturing acrylamide gel, which was constantly running. The radioactivity of each gel shift band was determined with a PhophorImager (Molecular Dynamics, Sunnyvale, CA) for quantitative analysis.
| RESULTS |
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-helix was monitored at 222 nm. Tm values of wild-type Genesis, and two wing 1 mutants, 70NG73KG and 70NP73KP, were determined at 45.2°C, 42.2°C, and 39.6°C ± 0.2°C, respectively. Even though the reverse curves of the thermal denaturation could not be determined reliably due to the fast precipitation of protein at temperatures above Tm, the result still indicates that the wild-type Genesis is slightly more stable than both the mutants, and that the Gly substituted Genesis is more stable than the Pro substituted Genesis.
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Gu(H2O), were extracted (Fig. 2 B) (Pace et al., 1992
Gu(H2O) (18) of 18.5 kJ mol-1, 17.0 kJ mol-1, and 19.5 kJ mol-1 ± 0.5 kJ mol-1 for the 70NG73KG and 70NP73KP mutants and the wild-type Genesis, respectively. This shows that substitution of residues in a surface-exposed and flexible loop sequence influences the thermodynamic stability of Genesis. The data also show that the Pro mutant decreases the Gibbs free energy of unfolding slightly more than the Gly mutant.
The amino acid substitutions modify the internal dynamics of Genesis
The amino acid substitutions introduced into a long flexible loop reduce the thermodynamic stability of the protein. Whether the substitutions are influencing the stability of the protein by having local or global effects is not clear. To address this question, the relaxation data were acquired on the two DNA-free wing 1 mutants and the wild-type Genesis protein. Due to the resonance overlap, relaxation data were collected only for 54, 56, and 58 residues in the 70NG73KG, the 70NP73KP and the wild-type DNA-free Genesis proteins respectively (Fig. 3). Judged on the data, the wild-type protein and its loop mutants show similar patterns of relaxation parameters. The residues in wing 1 and wing 2 show weaker than average NOE, and the residues between H1 and H2 show longer than average R2 values. In general the relaxation parameters obtained outside of these three regions (wing 1, wing 2, and between H1 and H2) are close to the average value. Therefore, the relaxation data indicate that individual secondary structural elements are not severely perturbed by the loop mutations.
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0.25 mM) of DNA-free Genesis was used in the data collection, since the
m value of the DNA-free Genesis is protein concentration-dependent. A possible cause for this is protein-protein interaction at high concentrations used in the NMR studies. Although, the relaxation parameters for each individual residue are influenced by the protein concentration, the trends of the parameters obtained from various protein concentrations are the same. Therefore, the conclusion drawn from the previous study of Genesis is still valid (Jin et al., 1999
To determine whether the destabilizing effects of the wing 1 amino acid substitution are passed onto the entire sequences, the multiple R1R2 values are used to analyze the internal motions of the proteins and the complexes (Kneller et al., 2001
), which are likely to have complicated and severe anisotropic motions. This criterion requires
n
m >> 1 (
n is the Lamor frequency of 15N,
m is the rotational correlation time of protein DNA complex). In this study the data were acquired at the magnetic field strength of 14.0 T. At this strength, the upper limit of R1R2 (represented as R1R2max) for a residue is 20 as illustrated in the previous study, when a residue is restricted in motions characterized by S2 = 1 and does not have chemical exchange (Kneller et al., 2001
). (0
S2
1 is the order parameter of a residue. S2 describes the degree of spatial restriction of the internal motions of an intranuclear 15N-1H vector). Due to the relatively large
m values (Table 1) estimated from R1/R2 ratios, this limit is approached for the DNA-free proteins. As suggested (Kneller et al., 2001
), a smaller S2 value reduces the R1R2 value of a residue, while a nonzero Rex value increases the R1R2 value of a residue. Therefore, in this study, any residue with a R1R2 value higher than R1R2max contains chemical exchange, while without the effect of anisotropy a residue with a small R1R2 value should have a small S2 value (Fig. 3 D). Due to the large
m values, the average
S2
can also be estimated from
R1R2
(
S2
= (
R1R2
/R1R2max)
), where R1R2max is the calculated maximum value) (Kneller et al., 2001
). In this study, the
S2
of 70NP73KP is 0.72 and is obviously lower than the
S2
values of 0.85 for the wild-type Genesis and 0.80 for 70NG73KG. Thus, the data indicate that the modification of the wing 1 sequence of Genesis increases the overall motional freedom of the folded sequences, probably by destabilizing the hydrophobic core packing, as suggested by the thermodynamic measurement. The data also indicate that the destabilizing effects are passed on to the entire sequence of Genesis.
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10 min for the wild-type DNA complex to <1 min for the mutant DNA complexes (Fig. 4). Therefore, even though wing 1 is highly dynamic in the wild-type protein Genesis DNA complex, it still contributes to the kinetic stability of the complex. Even though the complex is destabilized due to the wing 1 substitution, the forming of the complex band in the gel shift assay indicates that Genesis still binds to the DNA site. The question that remains unanswered is whether the protein-DNA interaction will increase the stability of the hydrophobic core of the mutants.
The effect of the protein-DNA interaction on the dynamic properties of the 70NP73KP-DNA complex
The relaxation data of the 70NP73KP-DNA complex and the wild-type Genesis DNA complex measured at 27°C are compared (Fig. 5). The protein-DNA interaction reduces the motions of highly flexible wing 2 and the chemical exchanges of the sequence between helix 1 and helix 2, as observed previously with the Genesis-DNA complex at different temperatures (Jin and Liao, 1999
). These two sequences are directly engaged in the DNA recognition, and the interactions therefore reduce the motional amplitudes of these two sequences. However, the increased motional freedom in DNA-free 70NP73KP can still be detected in the 70NP73KP-DNA complex calculated from the R1R2 products (Fig. 5). The mutant shows an
S2
of 0.77 at 27°C, while the wild-type Genesis-DNA complex shows
S2
values of 0.85. The result indicates that the protein-DNA interactions greatly reduce the motional freedoms of the DNA contact residues, which undergo structural transitions in the complex, but have reduced influences on the motional properties of non-DNA contact sequences in the protein.
| DISCUSSION |
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In this study, two wing 1 mutants were constructed and their properties were studied. Our data show that the substitutions in this 8-residue wing sequence influence the DNA binding properties, the thermodynamics, and the internal dynamics of Genesis and one of its DNA complexes. Even though the amino acid substitutions do not disrupt the helix-turn-helix motif, they reduce the stability and increase the internal motions of the protein. Furthermore, the double Pro substitution has a slightly more destabilizing effect on Genesis than the double Gly substitution. This is reasonable since the proline substitution is expected to introduce restraints in wing 1, which likely influence conformational freedom of strand 2 and strand 3 in the hydrophobic core packing and lead to the destabilization of the protein. The resulting destabilization is small, since the hydrophobic core of Genesis is still intact and the mutants only show a slight drop in the Gibbs free energy of unfolding (
Gu(H2O)) and a small reduction in thermodynamic stability (
Tm). The winged helix DNA binding motif is a small motif, and is involved in the packing of three helixes and three ß-strands. Due to the small hydrophobic core, the winged helix proteins only contain several highly conserved hydrophobic core residues. Thus the
Gu(H2O) value of the wild-type Genesis is relatively small compared to that of large and well-folded proteins (Ladbury et al., 1993
). Also due to this small hydrophobic potential, the structure is prone to perturbation. Thus, even the amino acid substitutions in wing 1 can destabilize the protein.
However, this destabilization has a profound effect on the internal dynamics of Genesis. The
S2
values for both mutants are lower than that of the wild-type, and the Pro-substituted Genesis shows a considerably reduced
S2
value. The data indicate that the dynamics of a protein should also be viewed as an entity and can be influenced by a flexible linker sequence outside of the hydrophobic core. Our data also show that the increased internal motions of 70NP73KP cannot be completely reversed by the strong protein-DNA interaction. Our data indicate that amino acid substitutions in this flexible internal wing can influence the dynamic properties of the winged helix domain globally, while protein-DNA interactions may only modify dynamic properties of the domain locally. Furthermore, although, the wing 1 mutations do not disrupt the Genesis-DNA interaction, the altered dynamic properties may influence the protein-protein interactions between Genesis and other transcription factors. This possibility deserves a careful study, especially since our preliminary result implicates the interaction between wing 1 and HNF-6 (Yan and Liao, unpublished).
| ACKNOWLEDGEMENTS |
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This research was supported by a National Institutes of Health grant to X.L. The Bruker DRX600 was purchased with funds from the University of Illinois at Chicago and grants from the National Science Foundation Academic Research Infrastructure Program.
Submitted on December 16, 2002; accepted for publication July 24, 2003.
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