Difference between revisions of "2012 AMBER Tutorial with Biotin and Streptavidin"

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===Preparation in Chimera===
 
===Preparation in Chimera===
====Structure Files Preparation====
 
 
In this AMBER tutorial, we will use the same system with previous DOCK part. Chimera can directly get the structure by its PDB ID <b>1DF8</b>. To begin with, we need three files under directory <b>001.CHIMERA.MOL.PREP</b>.
 
In this AMBER tutorial, we will use the same system with previous DOCK part. Chimera can directly get the structure by its PDB ID <b>1DF8</b>. To begin with, we need three files under directory <b>001.CHIMERA.MOL.PREP</b>.
  

Revision as of 13:10, 1 March 2012

For additional Rizzo Lab tutorials see AMBER Tutorials.

In this tutorial, we will learn how to run a molecular dynamics simulation of a protein-ligand complex. We will then post-process that simulation by calculating structural fluctuations (with RMSD) and free energies of binding (MM-GBSA).

I. Introduction

AMBER

Amber - Assisted Model Building with Energy Refinement - is a suite of about multiple programs for perform macromolecular simulations. Amber11, the current version of Amber, includes newly released functionality such as PMEMD, particle mesh Ewald MD and soft-core Thermodynamics Integration MD. For the tutorial, we are using an older version which is AMBER10.

The Amber 10 Manual is the primary resource to get started with Amber10. (Tip: Using Adobe Acrobat to view the file, you can simply search the document for keywords such as the name of a simulation parameter, which saves much time.) In addition, Amber Tools User's Manual serves as another reference while using Amber tools. You can also read the manual for Amber11 on Amber11 and AmberTools Users' Manuals

Here are some programs in Amber

  1. LEaP: an preparing program for constructing new or modified systems in Amber. It consists of the functions of prep, link, edit, and parm for earlier version of Amber.
  2. ANTECHAMBER: in additional to LEap, this main Antechamber suite program is for preparing input files other than standard nucleic acids and proteins.
  3. SANDER: according to the Amber 10 manual, it is 'a basic energy minimizer and molecular dynamics program' that can be used to minimize, equilibrate and sample molecular conformations. And this is the program we mainly use in this tutorial to generate trajectory files of the molecular system.
  4. PMEMD: version of SANDER that has improved parallel scaling property and optimized speed.
  5. PTRAJ: an analysis program for processing trajectory files. One can use ptraj to rotate, translate the structures, evaluate geometrical features and so on.

There is a mailing list you could sign-up for, as an additional resource.

Biotin and Streptavidin

For information of the Biotin and Streptavidin system, see 2012 DOCK tutorial with Streptavidin.

Organizing Directories

While performing MD simulations, it is convenient to adopt a standard directory structure / naming scheme, so that files are easy to find / identify. For this tutorial, we will use something similar to the following:

~username/AMS536/AMBER-Tutorial/001.CHIMERA.MOL.PREP/  
                                002.ANTE.TLEAP/ 
                                003.SANDER/       
                                004.PTRAJ/
                                005.MMGBSA/

II. Structural Preparation

Preparation in Chimera

In this AMBER tutorial, we will use the same system with previous DOCK part. Chimera can directly get the structure by its PDB ID 1DF8. To begin with, we need three files under directory 001.CHIMERA.MOL.PREP.

1DF8.rec.lig.pdb:
1. To lower computational cost and make the system clear, we remove chain B of the dimer. Select - chain - B, Action - Atoms/Bonds - delete
2. Remove the water molecules. Select - residue - HOH, Action - Atoms/Bonds - delete

Then we separate the receiver and its ligand.

1DF8.rec.noH.pdb:
Select the ligand and delete it. Select - Residue - BTN, Action - Atoms/Bonds - delete

1DF8.lig.chimera.mol2:
1. Select the protein and delete it. Select - Residue - BTN, Select - Invert, Action - Atoms/Bonds - delete
2. Use Dock Prep to add hydrogens and charges(AM1-BCC) to the ligand. Tools - Structure Editing - Dock Prep

Antechamber Input Files Preparation

A antechamber input file requires all the atom names to be unique and it only uses the first 3 characters as the name. So if we use 1DF8.lig.chimera.mol2 as the input file, it will cause errors("H102" and "H103" will have the same name "H10").

    14 O3         26.9770   10.6020   12.2050 O.2       1 BTN201     -0.6531
    15 N2         28.6480   12.1210   11.8210 N.pl3     1 BTN201     -0.4789
    16 C4         28.9670   13.2060   10.9010 C.3       1 BTN201      0.0816
    17 H102       32.0358   17.4077   15.9597 H         1 BTN201      0.0272
    18 H103       30.6885   18.0473   15.0102 H         1 BTN201      0.0219
    19 H92        30.5603   15.6243   15.3130 H         1 BTN201     -0.0094
    20 H93        32.1288   15.4384   14.4982 H         1 BTN201      0.0384
    21 H82        29.6624   16.7125   13.2433 H         1 BTN201      0.0275

We need to manually rename the atoms. One way is to use the first column numbers to be the atom names. If you are using Vim, the visual block mode can help by selecting a rectangular section of text. We rename the atoms and save the file as 1DF8.lig.mol2.

    14 O14       26.9770   10.6020   12.2050 O.2       1 BTN201     -0.6531
    15 N15       28.6480   12.1210   11.8210 N.pl3     1 BTN201     -0.4789
    16 C16       28.9670   13.2060   10.9010 C.3       1 BTN201      0.0816
    17 H17       32.0358   17.4077   15.9597 H         1 BTN201      0.0272
    18 H18       30.6885   18.0473   15.0102 H         1 BTN201      0.0219
    19 H19       30.5603   15.6243   15.3130 H         1 BTN201     -0.0094
    20 H20       32.1288   15.4384   14.4982 H         1 BTN201      0.0384
    21 H21       29.6624   16.7125   13.2433 H         1 BTN201      0.0275

Copy Working Directory to Seawulf

In order to finish further work on a cluster, we copy the whole directory to Seawulf.

scp -r AMBER-Tutorial sw:~/AMBER-Tutorial

antechamber

A antechamber input file requires all the atom names to be unique and it only uses the first 3 characters as the name. So if we use 1DF8.lig.chimera.mol2 as the input file, it will cause errors("H102" and "H103" will have the same name "H10").

    14 O3         26.9770   10.6020   12.2050 O.2       1 BTN201     -0.6531
    15 N2         28.6480   12.1210   11.8210 N.pl3     1 BTN201     -0.4789
    16 C4         28.9670   13.2060   10.9010 C.3       1 BTN201      0.0816
    17 H102       32.0358   17.4077   15.9597 H         1 BTN201      0.0272
    18 H103       30.6885   18.0473   15.0102 H         1 BTN201      0.0219
    19 H92        30.5603   15.6243   15.3130 H         1 BTN201     -0.0094
    20 H93        32.1288   15.4384   14.4982 H         1 BTN201      0.0384
    21 H82        29.6624   16.7125   13.2433 H         1 BTN201      0.0275

We need to manually rename the atoms. One way is to use the first column numbers to be the atom names. If you are using Vim, the visual block mode can help by selecting a rectangular section of text. We rename the atoms and save the file as 1DF8.lig.mol2.

    14 O14       26.9770   10.6020   12.2050 O.2       1 BTN201     -0.6531
    15 N15       28.6480   12.1210   11.8210 N.pl3     1 BTN201     -0.4789
    16 C16       28.9670   13.2060   10.9010 C.3       1 BTN201      0.0816
    17 H17       32.0358   17.4077   15.9597 H         1 BTN201      0.0272
    18 H18       30.6885   18.0473   15.0102 H         1 BTN201      0.0219
    19 H19       30.5603   15.6243   15.3130 H         1 BTN201     -0.0094
    20 H20       32.1288   15.4384   14.4982 H         1 BTN201      0.0384
    21 H21       29.6624   16.7125   13.2433 H         1 BTN201      0.0275

LEaP

Visualization in VMD

III. Simulation using sander

Minimization and equilibration

Production

IV. Simulation Analysis

Ptraj

MMGBSA Energy Calculation

V. Frequently Encountered Problems