 | Starting with version
6, YASARA can derive (Y)AMBER force field parameters for unknown molecules fully automatically,
allowing to simulate 98% of the structures in the PDB at the touch of a button. Manual intervention is only needed in case of exotic metal ions. The approach behind the
AutoSMILES algorithm can be summarized as follows:
- Assignment of pH dependent fractional bond orders and protonation patterns, typing of ring systems by a graph-theoretic approach.
- Identification of known molecules (from the force field definition file or the AMBER Parameter Database using SMILES strings. If no hit is found, proceed to step 3).
- Calculation of semi-empirical AM1 Mulliken point charges[3]. This step involves a geometry optimization with the COSMO solvation model[4] and avoids fatal rearrangements sometimes found when optimizing highly charged molecules like ATP4- in vacuo.
- Assignment of AM1BCC atom- and bond types.
- Application of the 'AM1 Bond Charge Correction' to improve the AM1 charges and make them better represent the electrostatic potential around the molecule - just like RESP charges.
- Further improvement of the AM1BCC charges using the known ideal RESP charges of similar molecule fragments, identified via SMILES strings.
- Assignment of GAFF (General AMBER Force Field) atom types and remaining force field parameters.
- In the end, the newly created parameters are cached for instantaneous availability next time.
Since all this is done automatically, only one step is required in practice: Press
<F12> to run the simulation. YASARA also produces a detailed force field parameter assignment report in the console,
which you can examine in detail to see what happened.
| | Figure: The steps of the AutoSMILES force field parameter assignment procedure. |
If a residue contains more atoms than YASARA's QM module can handle
, YASARA will try to split it up into smaller pieces that can easily be parameterized independently. While this works well for lipids,
where each hydrophobic tail is usually parameterized separately, you may have to give YASARA a hint for other large molecules by following these steps:
- Identify an aliphatic carbon that is as far away as possible from polar atoms, and
- if removed - would split your residue in two parts in the soup (i.e. all atoms with
lower numbers precede the carbon, all atoms with higher numbers follow it in the soup).
- Mark the carbon, then right-click to activate the context menu and click Split > Atom.
- In the bottom sequence selector, your residue should now have been split in exactly
two parts. Now you can run the simulation.
If you nevertheless want to define force field parameters manually
, this implies adding at least a residue topology in AMBER PREP format to one of the force field definition files
(*.fof) in the yasara/fof subdirectory. The best location is probably gafftopo.fof,
since this file is included in all force fields. Try to follow these steps for AMBER-style force fields:
- Look at the repository of AMBER force field parameters at http://pharmacy.man.ac.uk/amber/.
Maybe your molecule has already been parameterized. Also try to Google it.
Note that most of the AMBER Parameter Database is already included in YASARA
by default.
- Read the introduction to parameter fitting on page 287 of the AMBER 7 manual.
(Downloadable from http://amber.scripps.edu).
- Exit YASARA and open the force field definition file in a text editor.
You can find the force fields at yasara/fof/ForceFieldName.fof, e.g.
yasara/fof/yamber2.fof for the YamberII force field.
- Go to the end of the file and add a topology entry for your residue. The format
of these topology entries is also described on the AMBER website. YASARA does not
use the bond length, angle and dihedral data, so these columns can be set to zero.
The information needed for every atom is the sequential number
(column 1), the atom name in the PDB file (column 2), the force field atom type
(column 3) and the point charge on the atom (last column). Just keep the header
(including the three DUMMy atoms), and replace the name of the compound (line 1) and the three letter code of your residue
(line 3, 'AGS' in the example below). The second line must stay empty. If your ligand contains planar groups (around resonance or double bonds),
you must also add improper dihedral entries (see IMPROPER statements below).
The LOOP statement used by AMBER is not needed and ignored.
N-Acetyl-D-glucosamine-6-sulfate ( 1' O and no 4' OH-group, Gaussian98, RESP)
AGS INT 1
CORR OMIT DU BEG
0.000000
1 DUMM DU M 0 -1 -2 0.0000 0.0000 0.0000 0.000
2 DUMM DU M 1 0 -1 1.0000 0.0000 0.0000 0.000
3 DUMM DU M 2 1 0 1.0000 90.0000 0.0000 0.000
4 C1 AC M 0 0 0 0.0000 0.0000 0.0000 0.124693
5 C2 CT M 0 0 0 0.0000 0.0000 0.0000 0.032432
6 C3 CT M 0 0 0 0.0000 0.0000 0.0000 0.107401
7 C4 CT M 0 0 0 0.0000 0.0000 0.0000 0.044439
8 C5 CT M 0 0 0 0.0000 0.0000 0.0000 0.098935
9 C6 CT M 0 0 0 0.0000 0.0000 0.0000 0.031706
10 N N M 0 0 0 0.0000 0.0000 0.0000 -0.466264
11 O1 OG M 0 0 0 0.0000 0.0000 0.0000 -0.430845
12 O3 OH M 0 0 0 0.0000 0.0000 0.0000 -0.658535
13 O5 OS M 0 0 0 0.0000 0.0000 0.0000 -0.386715
14 O6 OS M 0 0 0 0.0000 0.0000 0.0000 -0.399527
15 C2N C M 0 0 0 0.0000 0.0000 0.0000 0.749408
16 O2N O M 0 0 0 0.0000 0.0000 0.0000 -0.632137
17 CME CT M 0 0 0 0.0000 0.0000 0.0000 -0.448969
18 HME HC M 0 0 0 0.0000 0.0000 0.0000 0.119617
19 HME HC M 0 0 0 0.0000 0.0000 0.0000 0.119617
20 HME HC M 0 0 0 0.0000 0.0000 0.0000 0.119617
21 S SO M 0 0 0 0.0000 0.0000 0.0000 1.131685
22 O1S O2 M 0 0 0 0.0000 0.0000 0.0000 -0.603269
23 O2S O2 M 0 0 0 0.0000 0.0000 0.0000 -0.603269
24 O3S O2 M 0 0 0 0.0000 0.0000 0.0000 -0.603269
25 H1 HC M 0 0 0 0.0000 0.0000 0.0000 0.160956
26 H2 HC M 0 0 0 0.0000 0.0000 0.0000 0.127396
27 H3 HC M 0 0 0 0.0000 0.0000 0.0000 0.137259
28 H4 HC M 0 0 0 0.0000 0.0000 0.0000 0.139063
29 H5 HC M 0 0 0 0.0000 0.0000 0.0000 0.086498
30 H6 HC M 0 0 0 0.0000 0.0000 0.0000 0.085794
31 H6 HC M 0 0 0 0.0000 0.0000 0.0000 0.085794
32 HN H M 0 0 0 0.0000 0.0000 0.0000 0.296182
33 HO3 HO M 0 0 0 0.0000 0.0000 0.0000 0.434306
LOOP
O5 C1
IMPROPER
C2N C2 N HN
CME N C2N O2N
DONE
- Update the force field by starting YASARA with the command line option -upd:
yasara -upd
YASARA will then recompile all force fields and tell you if something went wrong. If you do not get an error message,
restart YASARA and try to initialize the simulation again. If YASARA still complains,
consider the following points:
- Numbering of chemically equivalent hydrogens. The AMBER force fields do not
follow the PDB convention that hydrogens bound to the same atom are numbered in
the first column. YASARA corrects this problem for standard residues, but cannot
guess the right answer for 'your' new residues.
To avoid problems, do not additionally number hydrogens that are bound
to the same atom. If you look at the example above, atoms 30 and 31 are bound to C6,
and are both named H6, and neither H61/H62 nor 1H6/2H6.
- If you created a topology for an unusual amino acid by copying from a standard
residue, you also have to delete the numbers of chemically equivalent hydrogens
as just described above.
References: [1] Fast,
efficient generation of high-quality atomic charges. AM1-BCC model: II. Parameterization and validation
Jakalian A, Jack DB and Bayly CI (2002) J Comput Chem 23,1623-1641
[2] Development and Testing of a General Amber Force Field
Wang J, Wolf RM, Caldwell JW, Kollman PA and Case DA (2004) submitted.
[3] MOPAC: A semiempirical molecular orbital program Stewart JJP
(2000) J.Comp.Aided Mol.Des. 4,1-103 [4] Conductor-like screening model for real solvents: a new approach to the quantitative calculation of solvation phenomena
Klamt A (1995) J.Phys.Chem. 99, 2224-2235 NOVA uses molecular trees to assign force field parameters. Most of the time,
it is enough to follow this procedure:
- Load a PDB file of the structure with the unknown ligand(s).
If the PDB file does not contain CONECT records (no chemical bonds defined, the ligand
appears as a point cloud in ball&stick display) let YASARA find the bonds
(Edit > Find bonds in). In any case clean the structure (Edit > Clean),
and save it in the yasara/fof directory.
- Edit the file yasara/fof/nova.fof, search for the text 'OTHER MOLECULES' and
insert the name of your PDB file below. If your PDB file also contains a protein,
you should place a question mark '?' in front (this will tell YASARA to look only
at new features in your structure and ignore the rest). This structure will now be
used to learn equilibrium bond lengths and angles, it must therefore have an accurate
covalent geometry.
Example:
;
;SOME OTHER MOLECULES
;====================
?MyStructureWithProtein.pdb
MyLigandAlone.pdb
smallmol.pdb
heparin.pdb
- Update the force field by starting YASARA with the command line option -upd:
yasara -upd
YASARA will then recompile all force fields and tell you if something went wrong.
If you do not get an error message, restart YASARA and try to initialize the simulation
again.
- If you still get the error message 'NOVA force field tree not found' and your
molecule contains fused ring systems, simply use one of the other force fields
which automatically detect and handle planarity.
- You can always check that the bond types were assigned correctly by loading the PDB
file and clicking on the atoms: the bond types are displayed in the lower left HUD.
- If your residue contains unusual chemical groups that do not look like anything
you find in proteins, DNA and sugars, the NOVA force field may not contain point
charge definitions for the group. This will result in polar atoms without
a charge. You can verify that by clicking on the polar atoms after initializing the simulation.
The simulation HUD on the right lists all point charges on this atom. If there is more
than one charge on an atom, you can cycle through them with <Home> and <End>.
If you are really missing a charge and doing more than a quick&dirty modeling task,
you must add an entry to the CHARGE_POSITION_DATA section in yasara/fof/nova.fof
and recompile the force field.
- The same principle holds for planar groups. If a group is not recognized as planar,
a corresponding entry has to be added to the PLANE_CONFORMATION_PLANES section to
avoid an out-of-plane distortion.
As NOVA has been optimized for proteins only, it is generally advised that you use the
(Y)AMBER/YASARA force fields when working with small molecules. |