Open Access Article
Meifeng Lia,
Xiaoning Zhang
*b,
Sining Lic,
Xiaoqing Shaob,
Huixian Chenb,
Lei Lv*b and
Xiaowen Huang*d
aSchool of Public Health, Chengdu University of Traditional Chinese Medicine, Chengdu 610075, China
bSchool of Food Science & Engineering, Qilu University of Technology (Shandong Academy of Sciences), Jinan 250353, China. E-mail: xiaoningzhang@126.com; lvlei831005@163.com
cCollege of Food Science and Technology, Southwest Minzu University, Chengdu 610041, China
dSchool of Bioengineering, Qilu University of Technology (Shandong Academy of Sciences), Jinan 250353, China. E-mail: huangxiaowen2013@gmail.com
First published on 19th May 2021
Gold nanoparticles (AuNPs) provide a novel approach for protein enrichment and analysis due to their protein adsorption properties, forming a so called protein corona. This corona can significantly influence the protein's structure and characteristics, hindering their identification in situ. Dissociation is an important solution to analyze and identify the composition of protein coronas. However, a comprehensive picture of adsorbed protein dissociation is lacking. In this study, the protein dissociation from the protein corona and influencing factors were investigated on the basis of the formation mechanism and time evolution. Temperature and cysteine are the key factors influencing protein dissociation by altering the protein's binding ability. The results showed that half Au–S formation time is an important time point for thio-protein dissociation by the method of high speed centrifugation. When incubated for longer than that time, the thio-protein located in the hard corona could only be separated by β-mercaptoethanol replacement under analytical ultracentrifugation. However, Fourier-transform infrared spectroscopy (FTIR) revealed significant changes that occurred in βlg's secondary structure after ultracentrifugation. The Au–S bond formation time offers the potential to define the protein enrichment time of AuNPs.
Protein corona formation is a complex process and is kinetically divided into two phases.17,18 In phase one, proteins are absorbed on the NP surface in seconds or minutes by fast electrostatic or hydrophobic forces. For example, more than 300 plasma protein species rapidly adsorb onto AuNPs within 0.5 min.19 In phase two, thio-protein sulfhydryl groups, accessible to Au+, form Au–thiol covalent bonds (Au–S bonds) on the order of hours.13 The protein corona contains a two-component system that the proteins direct/indirect interact with NPs. Au–S bonds form a tightly bound layer, called the “hard” corona. Other layers are then surrounded by a “protein cloud,” referred to as the “soft” corona. In general, the hard corona is an irreversible process after the formation of Au–S bonds,20 which is a critical factor for understanding the protein dissociation mechanism.
Thio-proteins and non-thio-proteins exhibit distinct binding mechanisms to AuNPs. The binding mechanism, including the formation of Au–S bond and formation time, is crucial for understanding the adsorbed protein dissociation from the AuNP surface. In practical applications, protein enrichment occurs in the order of minutes to hours, depending on the protein sample and specific application.21,22 The main strategies for improving the enrichment process are decreasing the enrichment time, enhancing the detection efficiency, or lengthening the Au–S formation time. Numerous studies demonstrate that one can decrease the enrichment time or increase the detection efficiency by modifying the AuNPs with probes or combining the technology with a resonance energy transfer technique.4,23 while, the system research for lengthening the Au–S formation time and temperature influences remain elusive.
Here, we characterized the protein adsorption to AuNPs using two model proteins, β-lactoglobulin (βlg, thio-protein) and myoglobin (MB, non-thio-protein), which have similar molecular weights and global conformation.24,25 The binding parameters, including the binding affinities (Ka), binding numbers, and Au–S bond formation time as a function of temperature (4 °C to 44 °C), were detected to assess the centrifugation efficiency method for dissociating adsorbed proteins from the AuNP surface. Fourier transform infrared spectroscopy (FTIR) was used to examine the secondary structure changes before and after dissociation. Our results provide a guideline for the design of AuNPs as a protein enrichment material. Fig. 1 shows the adsorbed protein binding mechanism on AuNPs for the thio- and non-thio-proteins.
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| Fig. 1 A schematic representation of proteins adsorbed on AuNPs and the consequences for the thio- and non-thio-proteins. | ||
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| Fig. 2 Typical DLS spectrum of AuNPs–protein coronas incubated at different temperature. (A) AuNPs–βlg corona; (B) AuNPs–MB corona. | ||
The results showed that the AuNPs–βlg corona diameters decreased from 60 ± 2.6 nm to 44 ± 3.1 nm with an increase in temperature from 4 °C to 44 °C (Fig. 2A). In contrast, the AuNPs–MB coronas exhibited a smaller decrease in diameter (ΔD = 10 nm) with temperature increasing. The AuNPs–βlg protein corona thickness was several times larger than the βlg protein diameter (2.1 ± 0.5 nm) at all experimental temperatures, indicating that it consisted of both “hard” and “soft” coronas.16 The hard corona proteins form Au–S bonds with the surface of the AuNPs, representing approximately irreversible bound proteins.19 Thereby, the hard corona defined the centrifugation dissociation efficiency. Cysteine residues and temperature played key roles in the protein corona formation. Temperature influences the degree of protein coverage and the composition of adsorbed proteins on AuNPs surface at which the protein corona is formed.28,29 The higher temperature means the smaller proteins were adsorbed by the AuNPs.
| ΔG = −RT ln Ka | (1) |
| ΔG = ΔH − TΔS | (2) |
The raw data for βlg titration into the AuNP solutions at different temperatures are shown in Fig. 3. Each heat exchange curve corresponds to a single injection. The negative signals (ΔH < 0) indicate that the protein binding to the AuNPs is a strongly exothermic process.30 The signal intensities gradually decreased with an increasing number of injections and reached equilibrium at distinct molar ratios at different temperatures. Additionally, the equilibrium molar ratio decreased from ∼7500 to ∼5000 at ∼20 min when the temperature increased from 4 °C to 44 °C, which indicated that the decrease of the binding number and the fast electrostatic forces, including van der Waals interactions, electrostatics and hydrogen bond dominated the formation of protein corona during the ITC detection. The MB titration into AuNPs exhibited a smaller heat exchange, albeit with the similar behaviour (Fig. S1†).
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| Fig. 3 The Raw ITC data for βlg (30 μM) titrated into the AuNP solution (4 × 10−4 μM) with continuous stirring at 1000 rpm at different temperatures. (A) 4 °C; (B) 24 °C; (C) 44 °C. | ||
The stoichiometry thermodynamic parameters, Ka, ΔH, ΔS, and ΔG for proteins titrated into the AuNP solutions were derived using a nonlinear least-squares model and are summarized in Table 1. The results indicate that protein association with AuNPs is exothermic and therefore enthalpically favoured. Ka is important for describing the interaction between proteins and NPs, and it can give a general idea of the binding force and strength. A higher incubation temperature resulted in a lower binding affinity and stoichiometry of the protein adsorbed to AuNPs. The βlg's Ka decreased from 34 ± 10 × 105 M−1 to 25 ± 6 × 105 M−1, and the stoichiometry decreased from 3900 to 2600 when the temperature increased from 4 °C to 44 °C. Likewise, the MB's Ka decreased from 2.6 ± 0.4 × 105 M−1 to 2.1 ± 0.5 × 105 M−1, and the stoichiometry decreased from 3600 to 2600. Based on these decrease of stoichiometry data, inconsistent with the DLS, temperature exerts a greater influence on the adsorption of thio-proteins than non-thio-proteins in thermodynamics.
| Protein | Temperature (°C) | Stoichiometry (103) | Kaa (105 M−1) | ΔH (105 J M−1) | ΔSb (103 J M−1 deg.) | ΔGb (104 J) |
|---|---|---|---|---|---|---|
| a Derived from one site binding model.b Calculated according to the eqn (1) and (2). | ||||||
| βlg | 4 | 3.9 | 34 ± 10 | −39 ± 12 | −13.9 | −3.5 |
| 24 | 3.1 | 29 ± 7 | −32 ± 9 | −10.6 | −3.7 | |
| 44 | 2.6 | 25 ± 6 | −29 ± 7 | −9.0 | −3.9 | |
| MB | 4 | 3.6 | 2.6 ± 0.7 | −4.9 ± 0.7 | −1.6 | −2.9 |
| 24 | 3.0 | 2.3 ± 0.4 | −4.6 ± 0.8 | −1.4 | −3.0 | |
| 44 | 2.6 | 2.1 ± 0.5 | −4.3 ± 0.5 | −1.2 | −3.2 | |
To investigate how temperature influences the protein adsorption speed to AuNPs, we examined the changes in the AuNPs–βlg corona SERS intensity prepared at different temperatures as a function of incubation time; these results are shown in Fig. 4. The intensity increased as time went on until reaching a plateau, indicating the formation time of Au–S bond. The Au–S bond formation for AuNPs–βlg coronas took ∼12 h at 4 °C, whereas it decreased to ∼9 h and ∼6 h at 24 °C and 44 °C, respectively. Notably, this result (about 9 h at 24 °C) was approximate to our previous results that detected at 20 °C because of the experimental error.16 In contrast, there was no Raman shift in the AuNPs–MB corona spectroscopy (Fig. S2†). No Au–S bonds were formed in AuNPs–MB corona, indicating weak forces, such as electrostatic or hydrophobic forces, were the main binding force for MB adsorbed on AuNPs. Higher temperatures promoted a faster AuNP–protein interaction and a shorter Au–S formation time. Au–S bonds are the main force involved in attaching thio-proteins to the surface of AuNPs, resulting in these proteins secondary structure and characteristics changes.
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| Fig. 4 AuNPs–βlg corona SERS intensity change, prepared at different temperatures as a function of incubation time. Insert: the Au–S formation time at different temperatures. | ||
The AuNPs–protein corona fluorescence emission intensities prepared at 4 °C as the function of time after centrifugation are shown in Fig. 5. Centrifugation resulted in different dissociation efficiencies for thio-proteins and non-thio-proteins. The MB amount dissociated was temperature-independent, as most of the adsorbed MB in both “hard” and “soft” coronas were separated by high-speed centrifugation at 15
000 rpm for 15 min, for all incubation times (Fig. 5A). Whereas, the βlg amount dissociated was strongly related to the incubation time. The longer incubation time shows the higher emission intensities, which indicated that βlg was weakly dissociated. In general, most of the adsorbed βlg could be separated from the corona by high-speed centrifugation when incubated shorter than 4 h (half the Au–S bond formation time). However, there were no significant changes after incubated longer than 9 h (the Au–S bond formation time), maintaining a high level of fluorescence intensity due to the residual βlg located in the “hard” corona (Fig. 5B). The fluorescence intensities of protein corona prepared at 24 °C and 44 °C showed similar phenomenon (data not show).
In order to separate those remaining βlg in hard corona, β-mercaptoethanol added in AuNPs–βlg corona solution and analytical ultracentrifugation at 80
000 rpm for 20 min were performed. The result shows that most of these remaining βlg in “hard” corona can be separated by this synergistic action (Fig. 5C). While this action, especially of the presence of β-mercaptoethanol may bring new challenges for the proteins, such as altering the structure and functional properties. The bind force, in terms of Au–S bonds or weak force, and incubation time are the key criteria for choosing the dissociation methods.
O stretch vibrations in the peptide linkages (∼80%).39 The fitted inverted second-derivative amide I curves of βlg, AuNPs–βlg coronas, and dissociated βlg by centrifugation and ultracentrifugation with β-mercaptoethanol were shown in Fig. 6. The resulting secondary structural components were summarized in Table 2. The β-sheet (1628 and 1637 cm−1) is the most common secondary structure component in native βlg and in separated βlg by high-speed centrifugation (approximately 80%, Fig. 6A and C). The β-sheet and 310-helix (1663 cm−1) decreased after being adsorbed on AuNPs, thereby, the bands assigned to the α-helix (1658 cm−1), β-turn (1667 and 1675 cm−1), and random coil (1648 cm−1) increased (Fig. 6B). Most cysteine residues located in β-sheet conformation according to the three-dimensional model,23 which would form Au–S bond with AuNPs, resulting in destroying the β-sheet conformation.40 Although most of the adsorbed βlg can be separated by analytical ultracentrifugation, the secondary structure occurs significantly changes due to the presence of β-mercaptoethanol that β-sheet decreased, while other structure components increased (Fig. 6D).
| 310-Helixa | α-Helixb | β-Sheetc | β-Turnd | Random coilse | |
|---|---|---|---|---|---|
| a 310-Helix is 1663 cm−1.b α-Helix is 1658 cm−1.c β-Sheet is 1628 and 1637 cm−1.d β-Turn is 1667 and 1675 cm−1.e Random coils is 1648 cm−1 in the FTIR spectrum. | |||||
| Native | 15% | 0 | 81% | 0 | 4% |
| Corona | 0 | 26% | 31% | 24% | 19% |
| Centrifugation | 19% | 0 | 76% | 0 | 5% |
| Ultra-centrifugation | 0 | 15% | 56% | 18% | 11% |
MB exhibited an α-helix content above 70%, representing the most common secondary structure in the protein (Fig. S3†). Table S1† shows no changes in secondary structure components after MB was adsorbed on and dissociated from AuNPs. MB likely adsorbed to the AuNP surface because of a weak force that did not destroy the forces stabilizing the protein spatial structure.
Cysteine residues and Au–S bonds are the key factors influencing the proteins' dissociation efficiency from protein corona. Half the Au–S formation time has significant meanings to the AuNPs bioapplications. When the enrichment time is shorter than that time, most of the adsorbed proteins can be separated by high speed centrifugation without structure changes, conversely, when the enrichment is longer than that time, the dissociation is more difficult and complex, even changing the secondary structures after separation.
000 rpm for 5 min. 50 μL PBS (10 mM, pH 7.2) was used to re-suspend the sediment. The protein solutions of AuNPs and protein coronas formed at different temperatures, and were filtered through a PTFE 0.45 μm filter. Their hydrometers were measured by DLS (Nicomp 380, PSS, USA) to estimate the protein corona thickness change with increasing temperature. The data collection time was set to 90 s for temperature equilibrium and 5 s during the kinetic series acquisition.
000 rpm for 15 min to separate the adsorbed MB and βlg located on the soft corona. AuNPs–βlg corona solution (0.3 mL) was incubated for 15 h and interacted with 0.5 mL of β-mercaptoethanol for 2 h at 44 °C, then centrifuged at 80
000 rpm for 20 min. All the precipitates were re-suspended in 1 mL of PBS to detect the fluorescence emission intensity (Varian, Sweden). Excitation experiments were performed at 280 nm with a slit width of 5 nm, and the emission signal was collected from 300 to 450 nm. The values were calculated as an average of triplicate measurements.
In summary, temperature plays a key role in the protein adsorption on the AuNP surface, especially for thio-proteins. The binding force decreased with increasing temperatures, resulting in lower Ka and a reduced adsorbed protein number. And the Au–S bond formation speed was faster in the AuNPs–βlg corona. The Au–S bond formation time for AuNPs–βlg corona was ∼12 h at 4 °C. Centrifugation at 16
000 rpm for 15 min separated most of the adsorbed βlg; the incubation time was shorter than half the Au–S bond formation time. However, βlg was only be separated by β-mercaptoethanol replacement and ultracentrifugation. Moreover, FTIR revealed significant changes that occurred in βlg's secondary structure after ultracentrifugation. Contrasting, most of the MB was be separated from the AuNPs in a short time because of the weak binding forces. An enrichment time that is shorter than half the Au–S formation time provides a guide for AuNP bio-application and can help avoid the need for more complex dissociation methods.
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/d1ra02116h |
| This journal is © The Royal Society of Chemistry 2021 |