Physical Methods in Biochemistry Fall 2011 Optical Spectroscopy (I): Absorption Peter Qin LJS-251, UPC Tel. (213) 821-2461 e-mail: pzq@usc.edu Summary of previous lecture Interaction between EM radiation and molecules leads to: • Absorption: A transition from a lower level to a higher level with transfer of energy from the radiation field to an absorber, atom, molecule, or solid. • Emission: A transition from a higher level to a lower level with transfer of energy from the emitter to the radiation field. If no radiation is emitted, the transition from higher to lower energy levels is called nonradiative decay. • Scattering: Redirection of light due to its interaction with matter. Might or might not occur with a transfer of energy. Summary of previous lecture Description of an EM wave wave number angular frequency amplitude phase constant E E0 cos(k z t ) phase complex notation E E0 e i ( k z t ) Optical spectroscopy relates to electronic excitation and molecular vibration. Applications of Optical Spectroscopy in Biology • Detection DNA sequencing; Genetic analysis by fluorescence in situ hybridization (FISH); Fluorescence microscopy for cellular localization; Flow cytometry for cell identification & sorting ... • Quantification Absorption measurements for quantifying protein or nucleic acids,.. • Monitoring interaction and conformational phenomena of biological molecules. Monitoring protein folding, protein/DNA binding, ... Advantages: • High sensitivity – Single Photon/Molecule Detection . • Wide range of time resolutions. • In vivo detection. • Simple instrumentation. Limitation: • Spatial Resolution (being improved). UV-Vis absorption spctroscopy • The ultraviolet region falls between 190-380 nm The visible region fall between 380-750 nm • UV and visible radiation causes electronic transitions: promotion of electrons from the ground state to a high energy state. • only pi to pi* and n to pi* transitions occur in the UV-vis region are observed. Possible electronic transitions Observed electronic transitions in functional groups Compound l (nm) Intensity (e) CH4 122 intense s-s* (C-H) CH3CH3 130 intense s-s* (C-C) CH2=CH2 165 16,000 s-s* (C-C) 187 950 p-p* (C=O) 273 14 n-p* (C=O) CH3COCH3 model compound for the peptide bond transition with lowest energy UV-Vis Absorption Spectroscopy • The wavelength (or frequency) of the absorption is determined by DE = h n. • The intensity of absorption: Beer-Lambert Law Beer-Lambert Law (continued) 1. Transmittance vs. Absorbance Transmittance: T = I/I0 Absorbance: A = log(I0/I) and A = -log(T) 2. Determination of concentration A = log(I0/I) = -log(I/I0) = (k/ln10) [C] l = e [C] l and [C] = A / (e l) A: absorbance; e : extinction coefficient, unit in L mol-1 cm-1 3. Linear addition for non-interacting species. A = e1[C1] l + e2[C2] l + ... Extinction coefficient e(l) • Relates to the strength of the transition dipole. • Wavelength dependent – characteristics of individual molecules. • Environmental sensitive. UV-Vis absorption spectra of proteins • Peptide group dominate far UV absorption (<210 nm). poly-lysin in aqueous solution • Aromatic side-chains dominate near UV absorption. Absorption spectra of major nucleic acid bases rATP extinction coefficient (e) rCTP rGTP rUTP dTTP 200 220 240 260 280 300 wavelength (nm) 320 340 Environmental effects due to solvent • Solution spectra are broad due to molecular collisions. • Solvent polarity and H-bonding ability might affect the transition dipole moment, and therefore could affect the intensity, band shape, or wavelength of absorption. Absorption spectra of anisole in gas, perfluorooctane (F), cyclohexane (C), dioxane (D) and water (W) Environmental effects due to chromophore interaction: Hypochromicity • When chromophores are close in space, they could interact electronically. This perturbs their electronic states, and could affect the UV-Vis absorption spectra. • A parallel stack of dipoles are mutually repelling, making it more difficult to create a transition dipole (red) on the absorbing chromophore. The results in a smaller dipole moment, which means less absorption - hypochromism. • Stacking of DNA and RNA gives large hypochromicity – up to 30% less absorption is observed in stacked DNA. UV-Vis Absorption Spectrometer Schematic of a single beam UV-Vis spectrometer UV region (190 – 380 nm): deuterium discharge lamp visible and NIR (380 – 800 nm): tungsten-halogen lamp photodiode, phototube, or photomultiplier tube (PMT) Double beam Absorption Spectrometers Diffraction grating • A surface covered by a regular pattern of parallel lines • Simplest form – a photographic slide with a fine pattern of black lines • For practical applications, most gratings have grooves or rulings on their surface rather than dark lines. • Such gratings can be either transparent or reflective. • The distance between the lines is comparable to the wavelength of light • Light rays that pass through such a surface are bent as a result of diffraction. This diffraction angle depends on the wavelength of the light. Incident white light dsin nl d = slit width Incident white light Detectors Photo Multiplier Tube (PMT) The initial detector in a PMT is a photo-emissive cathode surface, made from alkali metal compounds, which ejects a single electron in response to a photon absorption. A series of other "secondary electron emissive" surfaces (the "dynode chain") amplifies this into a burst of ~106-7 electrons. Array-Detector Spectrophotometer These spectrometers use photodiode arrays (PDAs) or charge-coupled devices (CCDs) as the detector. All wavelengths pass through the sample. The light is dispersed by a diffraction grating after the sample and the separated wavelengths fall on different pixels of the array detector. UV-Vis absorption for proteins and nucleic acids UV and visible radiation causes electronic transitions: Promotion of electrons from the ground state to a high energy state. p -> p * and n -> p * transitions occur in the UV-Vis region The occupied and unoccupied orbitals of the amide chromophore showing possible transitions from the filled orbitals to unoccupied orbitals. Three classes of chromophores in protein 1. Peptide bond 2. Amino acid side chains 3. Prosthetic groups 1. Peptide bond (amide group) The peptide n -> p* absorption band is typically observed at 210-220 nm with a very weak intensity (emax 100) Much stronger p -> p* transition (emax 7000) is observed at far UV region around 190 nm Absorption is influenced by secondary structures • helix, sheet, or random coil give sufficiently distinctive absorption spectra • This can be used for diagnostic purposes for the native protein (pH 10.8, 52oC) (pH 6.0, 25oC) (pH 10.8, 25oC) UV absorption spectrum of poly-L- lysine in aqueous solution (K. R.and P.D. PNAS 47:1775 (1961)) Amino Acid Side Chains • A number of amino acid side chains have electronic transitions overlapping with in the strong amide transition (190-220 nm). Absorption of these side chains are difficult to detect Asparagine (Asn); Aspartic acid (Asp); Glutamine (Gln); Glutamic acid (Glu); Arginine (Arg); and Histidine (His) • The following aromatic amino acids have p -> p* absorption bands between 230 - 300 nm. e Tryptophan (Trp) Tyrosine (Tyr) Phenylalanine Cysteine (Phe) (Cys) Distinctive absorption maximum is observed around 280 nm in the aromatic amino acids Extinction coefficients at 280 nm Residue e280 L Moles-1 cm-1 Trp 5,690 Tyr 1,280 Cystine (s-s bond) 300 If a protein contained 3 Tyrosines and one Tryptophan its extinction coefficient would be: e =3 x 1,280 + 1 x 5,690 at 280 nm Protein concentration estimated from UV absorbance Monitors the absorbance of aromatic amino acids, tyrosine and tryptophan Advantages •Quick •Sample can be recovered •Useful for estimation of protein before using a more accurate method •Well suited for identifying protein in column fractions Disadvantages • Highly susceptible to contamination by buffers, biological materials and salts • Some extinction coefficients are influenced by pH and ionic strength of the solution. • Light scattering due to aggregates can cause overestimation of material Example Annexin B12 0.45 Absorbance 0.40 A280 = 0.21 0.35 0.30 e = 12287.8 0.25 0.20 l = 0.1 cm 0.15 0.10 0.05 0.00 -0.05 240 260 280 300 320 340 360 Wavelength (nm) More accurate colorimetric assays are available: • Lowry • Biuret • Bradford assay • Bicinchoninic Acid (BCA) assay. Quantitation of protein in HPLC/FPLC Prosthetic Groups (co-factors) • A number of prosthetic groups have intense absorption bands in the UV-Vis region. • The absorption is generally sensitive to to the local environment and the state of oxidation and/or coordination. heme heme-CO free and w/ peptide heme-CO bind to full length & truncated PrP from: Pato et.al., “Heme as an optical probe of a conformational transition of ovine recPrP”. Protein Sci, 2004, 13:1100-1107 UV absorption by nucleic acids • All nucleic acids (DNA and RNA) have strong near-UV absorption (260 nm) due to the aromatic nitrogenous bases. • The sugar phosphate backbone has an insignificant contribution to absorption at l > 200 nm Estimation of DNA purity • The major absorption band for purified DNA occurs at about 260 nm • Protein material, the primary contaminant of DNA, has a maximum absorption at 280 nm • The ratio A260/A280 is often used as a relative measure of the nucleic acid/protein content of a DNA sample • The typical A260/A280 for pure isolated DNA is 1.8 • A smaller ratio indicates increased contamination with protein. Extinction coefficients at 260 nm for nucleic acids (*) Individual base (*) In an oligonucleotide, e is determined by both base composition and base order (sequence). This is due to stacking interaction between bases (Hypochromicity). (*) For large DNA and RNA, an average of e = 10,000 M-1cm-1 per nucleotide is used. Thermal denaturation of DNA and RNA The transition from one conformation (double strand) to another (single strand) leads to reduce stacking. This reduces hypochromicity and goes along with an increase in absorption. The Tm-value (blue line) corresponds to the temperature at which half of the molecules is single and the other half double stranded.