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Characterization of atpD of the Fe-Reducing Thermophilic Bacterium Caloramator celere. - Santosh Pudasaini Saint Peter’s College, Jersey City, NJ. Dr. Mack Ivey Center for Space and Planetary Sciences, University of Arkansas, Fayetteville, AR. Iron Reduction.
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Characterization of atpD of the Fe-Reducing Thermophilic Bacterium Caloramator celere - Santosh Pudasaini Saint Peter’s College, Jersey City, NJ. Dr. Mack Ivey Center for Space and Planetary Sciences, University of Arkansas, Fayetteville, AR.
Iron Reduction • Anaerobic, primitive mode of metabolism • Chemolithoautotrophic growth • Evolved very early, thrive under extreme conditions
Scope… • Abundance of Iron and CO2 in Mars. • A potential metabolic pathway in Martian condition
Bacterial Iron Reduction • ATP generated by ATP Synthase • ATP Synthase: - transmembrane multiprotein complex - sits on bacterial plasma membrane - utilizes proton gradient created by the ETC - Fe (III) as electron acceptor
Our Project • Caloramator celere, a novel Fe (III) reducing thermophile • atpD, a β-sub unit gene in the atp operon on C. celere • The most highly conserved of the atp operon genes • Most likely to share sequence similarity with previously sequenced orthologs • Will serve as a probe for isolation of the entire atp operon
Objectives • Prepare C. celere cultures • Design primers using MSA • Extract DNA from the cultures • Perform PCR to amplify, clone and sequence atpD
Culture Preparation • C. celere cultures grown in an anaerobic media. • Electron acceptor: • 90mM amorphous Fe(III) oxide • 20mM 9,10-anthraquinone 2,6 disulfonic acid (AQDS medium)
Reduction of Fe (III) Before reduction After reduction
Reduction of AQDS Before reduction After reduction
Multiple Sequence Alignment • 38 ‘bacterial and Bacillales atpDs’ – gene bank of NCBI • Multiple alignment - vector NTI® AlinX tool • Highly conserved regions- ideal for primer design
Criteria for Primers • The oligonucleotides were, in average, about 20-25 base pairs. • The GC content was about 50-60 percent. • The thermodynamic Tm was about 55-60 oC. • There were no dimers or hairpin loops. • If present, choose ones with a positive or a fairly large dimer dG and loop dG.
Oligonucleotide (DNA): Length: 20 5’-TTCGGTGGTGCCGGTGTAGG-3’ CONDITIONS: - Molecular Weight: 6298.1 - %GC: 65.0 - Thermodynamic Tm: 60.2 - Hairpin Loops: 1 total TTCGGTG ||| G GGATGTGGCCGT Stem Length = 3 Loop Length = 5 Loop dG = -2.3 kcal/mol Dimers: 3 total TTCGGTGGTGCCGGTGTAGG +++ ||| GGATGTGGCCGTGGTGGCTT Stem Length = 3 Dimer dG = -1.7 kcal/mol TTCGGTGGTGCCGGTGTAGG |||| GGATGTGGCCGTGGTGGCTT Stem Length = 4 Dimer dG = -4.7 kcal/mol TTCGGTGGTGCCGGTGTAGG ||| +++ GGATGTGGCCGTGGTGGCTT Stem Length = 3 Dimer dG = -1.7 kcal/mol atpD_476_F
Primers Design • 6 Primers designed from MSA • atpD_476_F 5’-TTCGGTGGTGCCGGTGTAGG-3’ • atpD_542_F 5’-CACGGTGGTATTTCTGTATTCGC-3’ • atpD_935_F 5’-GCCGATGACTATACTGACCCAGC-3’ • atpD_957_R 5’-GCTGGGTCAGTATAGTCATCGGC-3’ • atpD_1272_R 5’-ACCGTAAATTGTTCCGCTACGTGG-3’ • atpD_1377_R 5’-CCAACTAAACGGAATGCATCTTC-3’
DNA Extraction • DNA extracted from the cultures grown following the protocol - ‘Protocols in Molecular Biology’-fourth edition. • Extracted DNA stored in TE buffer overnight. • Agarose gel electrophoresis performed to check for DNA. Marker DNA Lanes ↓ ↓ ↓
DNA Extraction • Agarose gel electrophoresis of DNA sample stored in isopropanol. • Gel ran after extracting DNA sample precipitated in isopropanol. Marker DNA Lanes ↓ ↓ ↓ ↓
DNA Extraction • Agarose gel electrophoresis of DNA sample freshly extracted from culture. • Agarose gel electrophoresis of cells taken directly from culture. Marker DNA Lanes ↓ ↓ ↓
Polymerase Chain Reaction (PCR) • Primers designed from MSA, B. cohnii DNA • DNA sample extracted from C.celere culture
Challenges for successful PCR • Insufficient cell density • Inefficient cell lysis • Rapid degradation of the DNA in extracts.
Future Directions • Extract DNA samples from cultures, keep them from degradation. • Perform PCR with the Primers designed from MSA. • Clone the amplified DNA into a plasmid vector and perform sequencing.
Acknowledgements • Center for Space and Planetary Sciences, University of Arkansas, Fayetteville, AR. • Dr. Mack Ivey • Jackie Denson • NASA Thank You