陳金榜 (chinpan chen) room #: n133 tel.: 2652-3035 (i) nmr theory and experiments
TRANSCRIPT
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陳金榜 (Chinpan Chen)
Room #: N133
Tel.: 2652-3035
(I) NMR theory and experiments
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(II) Structure determination: Protein
(III) Structure determination: Nucleic acid
Dr. Yuan-Chau Lou IBMS, Academia Sinica
Dr. Iren Wang IBMS, Academia Sinica
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outline 3 NMR experiments
4
Conclusion5
NMR parameters2
NMR principles 1
NMR resonance assignment
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NMR principles
Nuclear spin (I) : A = Z + N
The number of neutrons
The number of protons(atomic number)
Nominal atomic mass
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NMR can’t be detected when nuclei with I = 0 .
NMR can be detected when nuclei with I≠0
Different isotopes of the same element have different nuclear spins, some of which are detectable by NMR, others of which are not.
A nucleus with an even mass A and even charge Z, and therefore also an even N, will have a nuclear spin I of zero. (12C, 16O and 18O).
A nucleus with an even mass and odd charge (both Z and N odd) will exhibit an integer value of I. [2H(I=1), 14N(I=1) and 10B(I=3)].
A nucleus with odd mass (Z odd and N even, or Z even and N odd) will have nuclear spin with an I value that can be expressed as n/2, where n is an odd integer. [1H(I=1/2), 13C(I=1/2) and 17O(I=5/2)].
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NMR principles
Number of spin states (2I+1) :
0 △E
E
B0
m=-1/2
m=+1/2
E=-mB0(γh/2π)
B0: magnetic field strength h : Planck’s constant m: spin quantum number γ: magnetogyric ratio
A nucleus with spin I can have 2I+1 spin states. Each of
these states has its own spin quantum number m(m=-I, -
I+1, ‧‧‧, I-1, I). For nuclei with I=1/2, only two states are
possible: m=+1/2 and m=-1/2.
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Properties of nuclei in NMR studies
Isotope
1H
2H
3H
12C
13C
14N
15N
16O
17O
19F
31P
Spin
1/2
1
1/2
0
1/2
1
1/2
0
5/2
1/2
1/2
Frequency (MHz) at 11.74T
500.0
76.7
533.3
-------
125.7
36.1
50.7
------
67.8
470.4
202.4
Nature abundance ( % )
99.98
1.5×10-2
0
98.89
1.108
99.63
0.37
~ 100
3.7×10-2
100
100
Relativesensitivity
1.0
9.65×10-3
1.21
------
1.59×10-2
1.01×10-3
1.04×10-3
-------
2.91×10-2
0.83
6.63×10-2
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X-RAY ULTRAVIOLET INFRAREDMICRO-WAVE
RADIOFREQU-ENCY
Energylowhigh Frequency (ν)
ULTRAVIOLET VISIBLEVIBRATIONAL
INTRARED
NUCLEARMAGNETIC
RESONANCE
5 m1 m15μ2.5μ
200 nm 400 nm 800 nm
Wavelength (λ)short long
A Portion of the Electromagnetic Spectrum Showing the Relationship of the Vibrational Infrared to Other Types of Radiation.
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Region of Spectrum
X-rays
Ultraviolet/Visible
Infrared
Microwave
Radiofrequencies
Energy Transitions
Bond Breaking
Electronic
Vibrational
Rotational
Nuclear Spin ( Nuclear Magnetic Resonance ) Electron Spin ( Electron Spin Resonance )
Types of Energy Transitions in Each Region of the Electromagnetic Spectrum
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Conceptual block diagram of the pulsed fourier transform NMR experiment
Sample
Magnetization
Response
Data (FID)
Spectrum
Storage
Magnet
Perturbation
Detection
Fourier transformation
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The normal detection pulse sequence
FID
Data acquisition ( detection )
pulse
delay
Z
M
Y
XB1
(|| B0) Z
M1
Y
X
M2
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1. Chemical shift (δ) defines the location of a nmr line along the rf axis. It is measured relative to a reference compound. In frequency units the chemical shift is proportional to the applied static magnetic field, and therefore chemical shifts are customarily quoted in parts per million (ppm) units.
60 10/
ppm
referencesignal
8 6 4 2 0 -2
CH3
H
H
H
CH3 CH4
(CH3)4Si
CH3Li
Chemical shift δ(ppm)downfield high
frequencyupfield low frequency
Increased shielding
Increased deshielding
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Diamagnetic Anisotropy in Benzene
Anisotropy Caused by the Presence of π Electrons in Some Common
Multiple Bond Systems
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COMPOUND CH3X CH3F CH3OH CH3Cl CH3Br CH3I CH4 (CH3)4Si
ELEMENT X F O Cl Br I H Si
ELECTRONEGATIVITY OF X 4.0 3.5 3.1 2.8 2.5 2.1 1.8
CHEMICAL δ 4.26 3.40 3.05 2.68 2.16 0.23 0
SHIFT τ 5.74 6.60 6.95 7.32 7.84 9.77 10
The Dependence of the Chemical Shift of CH3X on the Element X
N129
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Backbone NH
Aromatic protons
Indo NH of Trp
H2O
H H
Other side-chain protons
Methyl protons
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Groups of Hydrogen Atoms in the Common Amino Acid Residues with similar Random Coil 1H Chemical Shiftsa.
10 5 1 δ(ppm)
2H(H) Ring α,β(S.T) CH3
β(a)β(b)NH(W)* NH(bb)* NH(sc)*
CodeCH3
β(a)β(b)
α,β(S.T)Ring2H(H)
NH(sc)*NH(bb)*NH(W)*
δ(ppm)0.9-1.41.6-2.32.7-3.31.2-3.33.9-4.86.5-7.77.7-8.6
6.6-7.68.1-8.810.2
Comments
βH of V, I, L, E, Q, M, P, R, KβH of C, D, N, F, Y, H, WOther aliphatic CHAll αH, βH of S and TAromatic CH of F, Y, W; 4H of H2H of h in the pH range 1-11
Side chain NH of N, Q, K, RBackbone NHIndole NH of W
a In model peptides the labile protons (identified by *) are only observed in H2O solution. The singlet resonance of εCH3 in met is at 2.13 ppm
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2. Spin-spin coupling constant (J) characterize scalar interactions (through-bond) between nuclei linked via a small number of covalent bonds in a chemical structure. J is field independent and is customarily quoted in hertz (Hz ).
J J J J J
(Quartet) δCH2
(Triplet) δCH3
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Singlet
Doublet
Triplet
Quartet
Quintet
Sextet
Septet
1
1 1
1 2 1
1 3 3 1
1 4 6 4 1
1 5 10 10 5 1
1 6 15 20 15 6 1
pascal’s Triangle
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ψ Ψ
Cα
Cβ
Cγ
ω
O
N
χ1
χ2
C’
N
Dihedral Angles: ψ, Ψ, ω, χ1, χ2
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Parameters for regular polypeptide conformations
ββpα-helix310-helix
π-helixPolyproline IPolyproline II
Polyglycine II
ψ-139-119-57-49-57-83-78-80
Ψ+135+113-47-26-70+158+149+150
ω-1781801801801800180180
Residuesper turn
2.02.03.63.04.43.333.03.0
Translationper residue
3.43.21.502.001.151.93.123.1
Bond Angle (deg)
Adapted from G. N. Ramachandran and V. Sasisekharan, Adv. Protein Chem. 23, 283-437(1968); IUPAC-IUB Commission on biochemical Nomemclature, Biochemistry 9, 3471-3479 (1970).
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Karplus Equations:
8.1cos6.1cos5.9
8.1)120cos(6.1)120(cos5.9
9.1)60cos(4.1)60(cos4.6
112
23
112
13
23
J
J
JNH
Dihedral Angles: , ψ, ω, χ1, χ2
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3. Nuclear Overhauser enhancement or Nuclear Overhauser effect (NOE) is the fractional change in intensity of one NMR line when another resonance is irradiated in a double irradiation experiment. Nuclear Overhauser effects are due to dipolar interactions (through-space) between different nuclei and are correlated with the inverse sixth power of the internuclear disran.
obs
irr
r
r
2
1
Example: the maximum NOE signal enhancement of a13C{1H} signal.
988.11026.67
105.267
2
1
2
16
6
obs
irr
r
r
NOEαR-6 (R: interproton distance)
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ii+1
i+2
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ParameterdαN(i,i)
dαN(i,i+1)
dαN(i,i+2)
dαN(i,i+3)
dαN(i,i+4)
dNN(i,i+1)
dNN(i,i+2)
dβN(i,i+1)
dαβ (i,i+3)
dαα (i,j)
dαN (i,j)
dNN (i,j)
3JHNα(HZ)NH exchange rate
α-helix2.63.54.43.44.22.84.22.5-4.12.5-4.1
( 4)≦slow
310-helix2.63.43.83.3(>4.5)2.64.12.9-4.43.1-5.1
( 4)≦slow
β2.82.2
4.3
3.2-4.5
2.33.23.3( 9)≧slow
βP
2.82.2
4.2
3.7-4.7
4.83.04.0( 9)≧slow
Short sequential and medium-range 1H-1H distances, vicinalcoupling constants, and amide hydrogen exchange rates.
dαα(i,j), dαN (i,j) and dNN (i,j) refer to interstrand distances.
The first four residues in the α-helix and the first three residues in the 310-helix will have fast amide proton exchange rates.
Every second residue in the flanking strand will have slow amide proton exchange rates
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dNN(i,i+1)
dαN(i,i+1)
dαN(i,i+3)
dαβ (i,i+3)
dαN(i,i+2)
dNN(i,i+2)
dαN(i,i+4)
3JHNα(HZ)
The characteristic patterns of short-range NOEs involving amide, alpha, beta protons observed for ideal α-helices, 310-helices and β-strand.
α-helix
1234567
310-helix
1234567
β-strand
1234567
4444444 4444444 9999999
The thickness of the lines is an indication of the intensity of the NOEs
The values of J coupling are approximate.
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4. Longitudinal relaxation time or spin-lattice relaxation time (T1) describes the rate at which the
magnetization returns to the thermodynamic equilibrium orientation along the static magnetic field after a rf pulse.
5. Transverse relaxation time or spin-spin relaxation time (T2) describes the decay rate of the effective magnetization observed in the x,y plane after a rf pulse.
Half height
2
1
Tlinewidth
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NMR parameters
Labile protons:
- NH ; - OH ; - SH Most of time, NMR signals of these labile protons can not be seen, due to their fast exchange with H2O.
However,
C N C C
O H H O
R
+ D2O C N C C
O D H O
RExchange rate study of amide proton can be used to identify the amide protons that form H-bond or are shielded from the solvent.
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Structural information
Interproton distances :
NOE α R-6
Dihedral angles:
J-coupling and Karplus equations
Chemical Shift Index (CSI):
Chemical shift of 1Hα, 13Cα, 13Cβ, 13C’
Hydrogen bonding:
Amide proton exchange rates
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Recommended atom identifiers for the twenty common amino acids follow the 1969 IUPAC-IUB guidelines.
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Backbone NH
Aromatic protons
Indo NH of Trp
H2O
H H
Other side-chain protons
Methyl protons
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Resonance assignment strategiesfor small proteins
Spin system identification :
DQF-COSY and TOCSY experiments
Sequence-specific assignment:
NOESY experiment
For protein < 10 kDa, 2D homonuclear experiments may be sufficient for resolvingoverlapping NMR resonances.
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PREPARATION EVOLUTION MIXING DETECTION
t1
t1
t1t2
t2
t2
τM
(A)
(B)
(C)
(D)
(A) The elements of a generalized two- dimensional NMR experiment
(B) DQFCOSY experiment
(C) NOESY experiment
(D) TOCSY experiment
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Cα
Hα3
Gly
NC
OH
3.97
8.39COSY
Hα2
NH
H (p
pm)
H (ppm)
TOCSY
Hα
NH
H (p
pm)
45.0
H (ppm)
173.6
Hα2
Hα3
Hα3
108.9
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Cα
HαCβ
Hβ
Ala
N C
OH
1.39
4.35
8.25
COSY
Hα
Hβ
NH
H (p
pm)
H (ppm)
TOCSY
Hα
Hβ
NH
H (p
pm)
52.5
H (ppm)
19.0
177.1
Hβ
Hβ
122.5
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Cα
Hα
Cβ
Hβ
Val
N C
OH
0.97
4.18
8.44
COSY
Hα
Hβ
NH
H (p
pm)
H (ppm)63.0 177.1
Cγ2 Cγ1
Hγ2
Hγ2 Hγ2
Hγ1
Hγ1Hγ1
2.13
0.94
31.7
Hγ1Hγ2
TOCSY
Hα
Hβ
NH
H (p
pm)
H (ppm)
Hγ1Hγ2
121.1
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Cα
Hα
Cβ
Hβ3
Ser
NC
OH 8.38
COSY
Hα
NH
H (p
pm)
H (ppm)
4.50
173.7
3.88
3.88
58.3
Hβ2
62.7
Hβ2
Hβ3
Oγ
Hγ
TOCSY
Hα
NH
H (p
pm)
H (ppm)
Hβ2
Hβ3
116.7
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C C
OH
R1
NH3 N
H
C C
OH
R2
N
H
C C
OH
R3
N
H
C C
OH
R4
N
H
C C
OH
R5
N
H
C C
OH
R6
F V Q A T A’
+
α-helical NOEs dαN(i,i+3), dNN(i,i+1)
Val
Gln
Ala
Ala’
Thr
Fingerprint region
Amide protons (ppm)
Hα (
ppm
)
NOESY
Phe
Hα
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2D 1H NMR Resonance Assignments
(1) Identify spin-system (amino acid type) using 2D COSY & TOCSY a. Unique residues: Gly, Ala, Val, Ser, Thr b. Long-chain residues: Arg, Ile, Leu, Lys c. Containing CH2 residues: Gln, Glu, Met d. AMX residues: Asn, Asp, His, Phe, Trp, Tyr, Cys e. No amide proton residue: Pro
(2) Distinguish aromatic residues
(3) Using residues possessing unique side-chain chemical shifts
(4) Sequential assignments based on NOEs
(5) Assign Cis or Trans conformer of Pro residue
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Methods for resolving overlappingNMR resonances
2D/3D homonuclear NMR experiments
such as 2D-DQFCOSY, 2D-TOCSY, 2D-
NOESY, 3D-NOESY-TOCSY.
2D/3D heteronuclear NMR experiments
such as 2D-15N-HSQC, 3D-15N-NOESY-
HSQC and triple-resonance experiments (
1H, 13C, 15N).
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NMR parameters
α
β
13C 15N OH
α
β
β
140 Hz
30 to 40 Hz
55 Hz
90 to 100 Hz
15 Hz11 Hz
用於多維異核核磁共振的單鍵異核偶合常數之概要圖
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130.0
125.0
120.0
115.0
110.0
105.0
ppm
10.0 9.0 8.0 7.0 6.0 ppm
HSQC
1H Chemical Shifts
15N
Ch
em
ical
Sh
ifts
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Triple (1H, 13C, and 15N) Resonance Experiments
Through-bond experiments:
(a) HNCA and HN(CO)CA(b) HNCACB and CBCA(CO)NH(c) HNCO and HNCACO (d) C(CO)NH and HCC(CO)NH(e) HCCH-TOCSY
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NMR experiment
二項常用的三核共振實驗之脈衝圖譜
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24 25 26F3
F1
sequence
Data reduction for 3D NMR. Once the 15N and 1H frequencies Of each amide group have been tabulated, strips running parallel to F1 can be extracted by software in order to build a 2 spectrum. The strips are order arbitrarily before assignment and according the sequence after assignment (D. Marion).
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NMR Resonance Assignments Using Triple Resonance Experiments
(1) Carry out HNCACB, CBCA(CO)NH, HNCO, and HNCACO. HNCA and HN(CO)CA may also be needed.
(2) Sequential backbone assignments: a. Identify those residues that have unique chemical shifts. For example, C of Thr, Ile, Val, and Pro (> 60 ppm); C of Thr, and Ser (> 60 ppm) b. C of Ala (~ 50 ppm), C of Gly (~ 45ppm), and C of Pro (~ 50 ppm) c. C of Leu, Asp, Asn, Ile, Phe, and Tyr (36~ 43ppm); C of Pro and Val (30 ~ 35 ppm) d. Others
(3) Using C(CO)NH or HCC(CO)NH etc to distinguish AMX residues from the long-chain residues.
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F6
122.24122.24
Q7
116.61116.61
K8
117.55117.55
K9
115.36115.36
H10
106.93106.93
L11
120.05120.05
T12
113.80113.80
D13
124.43124.43
T14
113.80113.80
K15
124.43124.43
70.00
60.00
50.00
40.00
30.00
20.00
10.00
CBCACONH HNCACB
8.81 8.13 7.46 8.27 7.83 8.32 8.25 8.28 8.12 8.24
70.00
60.00
50.00
40.00
30.00
20.00
10.00F6 Q7 K8 K9 H10 L11 T12 D13 T14 K15
122.24122.24 116.61116.61 117.55117.55 115.36115.36 106.93106.93 120.05120.05 113.80113.80 124.43124.43 113.80113.80 124.43124.43 D2 /ppmD2 /ppm
8.81 8.13 7.46 8.27 7.83 8.32 8.25 8.28 8.12 8.24
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180.000
177.500
175.000
172.500
170.000
180.000
177.500
175.000
172.500
170.000
F6 Q7 K8 K9 H10 L11 T12 D13 T14 K15 F6 Q7 K8 K9 H10 L11 T12 D13 T14 K15
122.24 116.61 117.55 115.36 106.93 120.05 113.80 124.43 113.80 124.43 122.24 116.61 117.55 115.36 106.93 120.05 113.80 124.43 113.80 124.43D1 /ppm
HNCO HNCACOD1 /ppm
8.81 8.13 7.46 8.27 7.83 8.32 8.25 8.28 8.12 8.24 8.81 8.13 7.46 8.27 7.83 8.32 8.25 8.28 8.12 8.24
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70.00
60.00
50.00
40.00
30.00
20.00
10.00
5.00
4.00
3.00
2.00
1.00
0.00
F6 Q7 K8 K9 H10 L11 T12 D13 T14 K15
122.24 116.61 117.55 115.36 106.93 120.05 113.80 124.43 113.80 124.43
F6 Q7 K8 K9 H10 L11 T12 D13 T14 K15
122.24 116.61 117.55 115.36 106.93 120.05 113.80 124.43 113.80 124.43D1 /ppm D1 /ppm
HCCONH CCONH
8.81 8.13 7.46 8.27 7.83 8.32 8.25 8.28 8.12 8.24 8.81 8.13 7.46 8.27 7.83 8.32 8.25 8.28 8.12 8.24
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10.00
7.50
5.00
2.50
0.00
F6 Q7 K8 K9 H10 L11 T12 D13 T14 K15
122.24 116.61 117.55 115.36 106.93 120.05 113.80 124.43 113.80 124.43D1 /ppm
TOCSY-HSQC
F6 Q7 K8 K9 H10 L11 T12 D13 T14 K15
122.24 116.61 117.55 115.36 106.93 120.05 113.80 124.43 113.80 124.43D1 /ppm
NOESY-HSQC
8.81 8.13 7.46 8.27 7.83 8.32 8.25 8.28 8.12 8.24 8.81 8.13 7.46 8.27 7.83 8.32 8.25 8.28 8.12 8.24
10.00
7.50
5.00
2.50
0.00
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130.0
125.0
120.0
115.0
110.0
105.0
ppm
10.0 9.0 8.0 7.0 6.0 ppm
HSQC
D2
W3
E4
T5
F6
Q7
K8
K9
H10
L11
T12
D13
T14
K15
K16
V17
K18
C19
D20
V21
E22
M23
A24
K25
A26
L27
K32
T33
N34
T35
N92
I37
Y38A39
L40
G42
R43
V44
K45
A46
L47
C48
K49
N50
I51
R52
D53
N54
T55
D56
V57
L58
S59
R60
D61
A62
F63
S80
S81
T83
N84
T85
I86
C87
I88
T89
C90
V91
A99
G100
V101
G102
C104
C75
H76
Y77
K78
L79
Q93
L94
L64
L65
F28
D29
C30I96
H97
F98
F36R70
Q67L73
K73
I71
W3(N1H)
S103
Q7*
N84*
N92*
N54*N50*
Q93*
N34*
Q67*
R*R*R*
R*C68
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Three-dimensional structure determination by simulated annealing using X-PLOR ( CNS ) program
tornoerepimproperanglebondtotal EEEEEEE +++++=
Keep the correctness of protein geometry
The energy terms of experimental data
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K82K11
K67
K68
K32
K30
D85
D79
D17
E14
E76 K19K77
K63D42
E36E35
D33
D57
K60
K78
180-0.3 0.3
(C)
C-
N-
(A)
β1
β2β3
β4
β5
β6β8
β7 β9
β10
Loop I
Loop II
Loop IV
Loop V
Loop III
(B)
(A) Superimposition of backbone atoms for 20 porcine MSP structures (B) The
ribbon and (C) surface representations of the averaged structure of porcine MSP
(A) (B)
(C)
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The flowchart of the protein structure determination from NMR data.
Structure refinement using Molecular dynamics simulation
Calculation of initial structureusing distance geometry
Extraction of Structuralinformation
Sequence-specificResonance assignment
NMR spectroscopy1D, 2D, 3D, …
Protein in solution~0.5 ml, 2 mM concentration Sample preparation:
protein isolation
purification,
characterization,
cloning,
isotopic labelling.
Sample preparation:
protein isolation
purification,
characterization,
cloning,
isotopic labelling.
Secondary
structure of
protein
Secondary
structure of
protein
Distances between
protons (NOE),
Dihedral angles(J
coupling), Amide-
proton exchange,
Chemical shifts
index
Distances between
protons (NOE),
Dihedral angles(J
coupling), Amide-
proton exchange,
Chemical shifts
index
Final 3DstructuresFinal 3D
structures
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High-throughput NMR structure determinationHigh-throughput NMR structure determination
1. Cloning, protein expression and purification: 15N/13C- and/or 2H/13C/15N-labeled protein; specifically amino acid-labeled protein.
2. NMR hardwares: Using higher-field NMR instrument (800 MHz or 900 MHz) and Cryoprobe.
3. NMR experiments: performing RDC and TROSY exp.
3. Data analysis: Using automatic resonance assignment program (Autoassign, Ansig, etc.)
4. Structure calculation: Aria, Cyana, etc.