The Role of Clays in Shielding DNA against X-Ray Radiation: Possible Implications on the origin of life Angela Ciaravella F. Scappini (2), M. Franchi (3),

Slides:



Advertisements
Similar presentations
TWO STEP EQUATIONS 1. SOLVE FOR X 2. DO THE ADDITION STEP FIRST
Advertisements

1 Yell / The Law and Special Education, Second Edition Copyright © 2006 by Pearson Education, Inc. All rights reserved.
Matter takes up space and has mass Everything composed of matter Any biological process, function or structure can be broken down to its chemical level.
Advanced Piloting Cruise Plot.
1
THE EFFECT OF 12 C(α,γ) 16 O ON WHITE DWARF EVOLUTION Pier Giorgio Prada Moroni Dipartimento di Fisica - Università di Pisa Osservatorio Astronomico di.
1_Panel Production. 380 pannelli 45 giorni di produzione = 8.4 pannelli/day.
Cirrone G. A. P. , Cuttone G. , Raffaele L. , Sabini M. G
Feichter_DPG-SYKL03_Bild-01. Feichter_DPG-SYKL03_Bild-02.
1 Copyright © 2013 Elsevier Inc. All rights reserved. Chapter 116.
1 Copyright © 2013 Elsevier Inc. All rights reserved. Appendix 01.
1 Copyright © 2013 Elsevier Inc. All rights reserved. Chapter 28.
1 Copyright © 2013 Elsevier Inc. All rights reserved. Chapter 38.
By D. Fisher Geometric Transformations. Reflection, Rotation, or Translation 1.
Chapter 1 Image Slides Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
CIPS SEWG FR, JET 2008C. Hopf O 2 /He glow discharge cleaning: Experience at IPP Christian Hopf, Volker Rohde, Wolfgang Jacob Max-Planck-Institut für Plasmaphysik.
David Burdett May 11, 2004 Package Binding for WS CDL.
0 - 0.
What gas makes up 78% of our atmosphere?
FACTORING ax2 + bx + c Think “unfoil” Work down, Show all steps.
Addition Facts
Who Wants To Be A Millionaire? Decimal Edition Question 1.
Irradiation of 300 m phi detectors from MICRON and HAMAMATSU cont. Second independent estimate: 6h 2 cycles, 12h 1 cycle, 14h no beam, 5.5h 1cycle estimated.
ZMQS ZMQS
ACTIVE GALACTIC NUCLEI X-ray broad--band study A. De Rosa, L. Piro Ginga/ROSAT/ASCA IASF-Roma Universita' di Roma La Sapienza Institute of.
Università di Parma Pisa, Nov. 29, 2005 A. Bononi, 2nd Korea-Italy S&T Forum 1/30 Research at Parma University in Optical Communications and Networks Alberto.
Module IV - Dose terms and units
Photo Slideshow Instructions (delete before presenting or this page will show when slideshow loops) 1.Set PowerPoint to work in Outline. View/Normal click.
SPHINX DATA ANALYSIS Magdalena Gryciuk Astronomical Institute, University of Wroclaw Space Research Centre, Polish Academy of Sciences I SOLARNET SPRING.
Richmond House, Liverpool (1) 26 th January 2004.
Break Time Remaining 10:00.
S. N. HOM Impedance in Vacuum … 1 of 40 Sasha Novokhatski SLAC, Stanford University Machine-Detector Interface Joint Session April 22, 2005 HOM Impedance.
4/2003 Rev 2 I.3.6 – slide 1 of 23 Session I.3.6 Part I Review of Fundamentals Module 3Interaction of Radiation with Matter Session 6Buildup and Shielding.
PP Test Review Sections 6-1 to 6-6
1 10 pt 15 pt 20 pt 25 pt 5 pt 10 pt 15 pt 20 pt 25 pt 5 pt 10 pt 15 pt 20 pt 25 pt 5 pt 10 pt 15 pt 20 pt 25 pt 5 pt 10 pt 15 pt 20 pt 25 pt 5 pt Vocabulary.
Oil & Gas Final Sample Analysis April 27, Background Information TXU ED provided a list of ESI IDs with SIC codes indicating Oil & Gas (8,583)
Power Systems Design -II
15. Oktober Oktober Oktober 2012.
Copyright © 2012, Elsevier Inc. All rights Reserved. 1 Chapter 7 Modeling Structure with Blocks.
Basel-ICU-Journal Challenge18/20/ Basel-ICU-Journal Challenge8/20/2014.
1..
2)Do children’s adjustment problems transact over time with parent-teacher communication? Yes. When children showed more externalizing and internalizing.
Introduction to Feedback Systems / Önder YÜKSEL Bode plots 1 Frequency response:
SuperNEMO Thoughts about next generation NEMO experiment Ruben Saakyan UCL.
1 TSD-160 Introduction to Network Analyzers and Error Correction Doug Rytting 4804 Westminster Place Santa Rosa, CA
Chapter Six Study Guide.
Addition 1’s to 20.
: 3 00.
5 minutes.
Analyzing Genes and Genomes
©Brooks/Cole, 2001 Chapter 12 Derived Types-- Enumerated, Structure and Union.
Figure Essential Cell Biology (© Garland Science 2010)
Essential Cell Biology
Clock will move after 1 minute
Intracellular Compartments and Transport
PSSA Preparation.
Essential Cell Biology
8 th RD50 Workshop Prague June Università degli Studi Università degli Studi di Perugia di Perugia 1 Annealing effects on p + n junction 4H-SiC.
1 Chapter 13 Nuclear Magnetic Resonance Spectroscopy.
Energy Generation in Mitochondria and Chlorplasts
Select a time to count down from the clock above
Murach’s OS/390 and z/OS JCLChapter 16, Slide 1 © 2002, Mike Murach & Associates, Inc.
EXAMPLE 3 Use synthetic division
EPIC Meeting, Palermo Ottobre 2003 Short and Medium term Variability study of NGC2516 late type stars with EPIC-XMM Outline: NGC 2516 characteristics.
Angela Ciaravella Study the effects of X-ray radiation on biological molecules: DNA free and clay adsorbed in water solution Amino Acids in water solution.
ESA/ESTEC Feb Effects of X-ray and UV Radiation from Very Young Sun on Biomolecules Angela Ciaravella INAF – Osservatorio Astronomico di Palermo.
Water in Laboratory J.R. Brucato INAF-Arcetri Astrophysical Observatory, Firenze Italy Water in Asteroids and Meteorites Paris.
Mg Films Grown by Pulsed Laser Deposition as Photocathodes: QE and surface adsorbates L. Cultrera INFN – National Laboratories of Frascati.
Presentation transcript:

The Role of Clays in Shielding DNA against X-Ray Radiation: Possible Implications on the origin of life Angela Ciaravella F. Scappini (2), M. Franchi (3), E. Gallori (3), C. Cecchi-Pestellini (4), M. Barbera (1), R. Candia (1), G. Micela (1) (1)INAF – Osservatorio Astronomico di Palermo, Italy (2)ISMN –CNR, Bologna, Italy (3)Dipartimento di Biologia Animale e Genetica, Univ. di Firenze, Italy (4)Dipartimento di Fisica, Univ di Lecce, Italy Firenze 28/02 – 1/03/05

First evidence of life on the Earth 3.8 × 10 9 yr Earth Atmosphere : a big unknow, very little screening from Sun radiation Conditions on the Early Earth Early X-ray Sun: more active, hard and bright 3 × (0.1 keV) = erg/sec 5 × (0.2 keV) Yohkoh-SXT 3-40 Å band 1-10 keV band: the photon flux today is ~10 -3 the flux at the age of Pleiades min max How and under which conditions life was created?

DNA Irradiation Free DNA type B Clay Adsorbed DNA type A 34 Å per turn B Å per turn A Why DNA? DNA is already life An easy and well tested method to estimate damage We irradiate free and clay absorbed DNA from Bacillus Subtilis CLAYS: Montmorillonite Na 0.2 Ca 0.1 Al 2 Si 4 O 10 (OH) 2 (H 2 O) 10 Kaolinite Al 2 Si 2 O 5 (OH) 4

Vacuum tight container X-ray, UV, Vis eV ( A). 17 m stainless-steel vacum beam line class 1000 clean_room (Barbera et al 1999). The XACT Facility: Al Ti Cu Flux (erg sec -1 cm -2 ) Line (keV ) DNA X-Ray Irradiation Irradiation Dose : × 10 4 erg Exposure Time : 2 m - 16 h minimum 3 × maximum large flares The Sun today (1.5 –12.4 keV): DNA Samples: Free 10μg DNA l of H 2 O Clay Adsorbed 10μg DNA + 2mg Clay l of H 2 O

DNA Damage Evaluation The integrity of DNA molecules is estimated by transformation experiments : efficiency of irradiated DNA to transform competent cell in a bacterial culture Comparing Ftf with Ftf 0 the damage is evaluated Typical errors on Ftf are 20 % The transformation frequence is: Transformation frequence for non irradiated DNA

Results and Conclusions I *** Free DNA is severely damaged by X-rays and the damage depends on the energy dose rather than the hardness of radiation Clay Adsorbed DNA is resistent to the X-ray irradiation Can clays shield DNA against X-rays? Diluted clay is much more transparent than H 2 O to X-rays The more compact configuration (A) of clay adsorbed DNA binding to the substrate by electrostatic and/or hydrogen bonds can play protective role

Results and Conclusions II Are X-rays directly responsible for DNA damage? Num X photons (Cu 5 × 10 4 erg) 4 × Num H 2 O molecules 5 × Num DNA molecules 4 × Secondary UV UV irradiation of free and clay adsorbed DNA give similar results (Scappini et al 2004) 2.5 mm 1 mm 0.2 mm 0.01 mm Are clays essential in protecting the basic building blocks of life as well ? DNA adsorbed on clays do survive X-rays and UV photodegradation