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October 01, 2009
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Date:08SundayMay 2011Lecture
Journal club - A discussion on selected articles
More information Time 12:30 - 14:00Location Dannie N. Heineman LaboratoryLecturer Dr. Nir Sapir Organizer Nella and Leon Benoziyo Center for AstrophysicsContact -
Date:08SundayMay 2011Lecture
To be announced
More information Time 13:00 - 13:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Efrat Dvash
Menachem Rubinstein's group Dept. of Molecular Genetics, WISOrganizer Department of Molecular GeneticsContact -
Date:08SundayMay 2011Lecture
Sphingosine-1-phosphate: frpom insipid lipid to a regulator of cancer and inflammation
More information Time 14:00 - 14:00Location Max and Lillian Candiotty BuildingLecturer Prof. Sarah Spiegel
Dept. Biochemistry and Molecular Biology Virginia Commonwealth University School of Medicine Richmond, VA. USAOrganizer Department of Immunology and Regenerative BiologyContact -
Date:09MondayMay 2011Cultural Events
Ceremony marking Remembrance Day for Israel's Fallen Soldiers and Victims of Terrorism
More information Time 11:00 - 12:45Location Helen and Milton A. Kimmelman BuildingContact -
Date:11WednesdayMay 2011Lecture
Lumen formation in the Drosophila heart
More information Time 10:00 - 10:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Prof. Talila Volk
Dept. of Molecular Genetics, WISContact -
Date:11WednesdayMay 2011Colloquia
Faculty of Chemistry Colloquium- Prof. Harold Kroto
More information Time 11:00 - 12:30Title CARBON IN NANO AND OUTER SPACELocation Gerhard M.J. Schmidt Lecture HallLecturer Prof. Harold Kroto
Nobel Laureate for the discovery of the C60 Dept. of Chemistry & Biochemistry The Florida State UniversityOrganizer Faculty of ChemistryContact Abstract Show full text abstract about The age-old awe that man has had for the heavens has driven ...» The age-old awe that man has had for the heavens has driven almost all aspects of human culture and knowledge and resulted in technologies with generally positive, though occasionally negative effect. Arguably the most positive have taken place since Galileo recognized that the phases of Venus provided the evidence that confirmed the Copernican heliocentric system and cemented his position firmly as the “Father of Science”. From this moment on we had, at long last, a straightforward philosophical construct and language which enabled mankind to determine what is and is not “True”. Particularly important truths have resulted from the curiosity that humans have had for a detailed understanding of the way Universe works. This led to the development of astrophysics and the associated technologies that have been spun-off. Not least of these has been the telescope – from Galileo’s beautiful original design to the fantastic satellite-born devices put up by NASA. These have not only enabled us to observe the planets and stars more clearly but we have been able to see to the very edge of the Universe and make a plethora of discoveries about all aspects of the Universe from the occupants of the space between stars to the processes occurring deep inside stars. Perhaps the most fundamental advance based on space observations led to the development of Classical Mechanics in order to understand the motions of the planets and comets and concommitantly the development Calculus, one of the greatest of Mathematical achievements. As Quantum Mechanics developed along with Spectroscopy it was inevitable that we should start to study the atomic and molecular composition of heavenly bodies - first hot stars as well as cool comets. With the development of radiotelescopes, the very cold interstellar medium was found to be a veritable Pandora's Box, full to the brim with fascinating and exotic molecules, dust particles and also some highly puzzling material responsible for some as yet unidentified spectroscopic features. These latter are known as the Diffuse Interstellar Bands (DIBs) first observed in the 1920s.
Particularly fascinating, curious and crucial has been the role that the element carbon has played in almost every aspect of the development of our understanding of both the physical and natural sciences. The fact that the element is at all abundant is due to a curious set of coincidences involving its nucleosynthesis from helium in stars. If one furthermore adds into the overall carbon equation its uniquely profuse chemistry, ie Organic Chemistry, it is hard to conceive that life could be based on any other element. The most recent big surprise that the element had up its sleeve was the existence of C60, Buckminsterfullerene, the third well-defined form of carbon. The discovery was made serendipitously in 1985 during laboratory experiments which attempted to explain the chemical synthesis of some unusually long linear carbon chain molecules detected in the interstellar medium in the 1970’s. A second aim of these experiments involved curiosity as to whether the carriers of the DIBs might be long linear carbon chains. Interestingly the extraction of C60 in 1990 by Kraetschmer and Huffman resulted from experiments aimed at understanding another mysterious feature known as the 217nm hump and conjectured to also involve carbon – perhaps carbonaceous dust particles. The fact that this third, well-defined, form of carbon had been hiding in the shadows since time immemorial brings to mind the mysterious character lurking in the dark streets of Vienna, made famous by Orson Welles in the classic movie “The Third Man”. In fact we now know that the molecule forms fleetingly within sooting flames but is immediately destroyed as it passes through the flame barrier into an oxygen atmosphere. On the basis of such revelations the suggestion that C60 might exist in space and be responsible for the DIBs (Kroto & Jura) seemed an as good, if not a better, possibility than most other ideas that had heretofore been proposed. Especially compelling support for the idea that C60 existed in space lay in the fact that the original discovery was made serendipitously during laboratory experiments designed to simulate the atmospheric conditions in cool red giant carbon stars. This conjecture has just been confirmed by Cami et al who have found infra red bands in the spectra obtained by NASA’s Spitzer satellite telescope. The discovery also makes some recent work here at FSU on endohedral fullerenes, in which atoms are trapped inside the carbon cage, extremely relevant to certain anomalous isotope ratios observed in meteorites, in particular carbonaceous chondrites. This is yet another example of the remarkably synergistic relationship between terrestrial and space science. In these difficult times it lends useful support for the fundamental value of "Blue Skies" or perhaps more accurately “Black Skies” cross-disciplinary research. All these results taken together suggest that the 90 year-old mystery of the carrier of the DIBs might be close to being resolved at long last.
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Date:11WednesdayMay 2011Lecture
"Proteomics analysis of lipid bodies and endomembranes of the marine haptophyte Emiliania huxleyi: clues to biosynthesis of potential biofuels"
More information Time 14:00 - 15:00Location Ullmann Building of Life SciencesLecturer Prof. Gordon Wolfe
Biological Sciences Dept., California State Univ. Chico, USAOrganizer Department of Plant and Environmental SciencesContact -
Date:12ThursdayMay 2011Conference
Students Probability Day III
More information Time All dayLocation Jacob Ziskind BuildingOrganizer The Y. Leon Benoziyo Institute for Molecular MedicineHomepage Contact -
Date:12ThursdayMay 2011Lecture
Magnetic Resonance Seminar
More information Time 09:00 - 10:00Title Solid State NMR Investigations of Lipid Bilayers and Biomembrane Binding Molecules: Dendrimers and AmylinLocation Gerhard M.J. Schmidt Lecture HallLecturer Dr. Pieter Smith
Chemical Physics Dept Post Doc WISOrganizer Department of Chemical and Biological PhysicsContact -
Date:12ThursdayMay 2011Lecture
"New Strategies for the Commercialization of Precision Polyolefins"
More information Time 11:00 - 11:00Title Department of Organic Chemistry - Special seminarLocation Helen and Milton A. Kimmelman BuildingLecturer Prof. Lawrence R. Sita
Department of Chemistry and Biochemistry University of Maryland, College ParkOrganizer Department of Molecular Chemistry and Materials ScienceContact -
Date:12ThursdayMay 2011Lecture
TBA
More information Time 11:15 - 12:30Location Edna and K.B. Weissman Building of Physical SciencesLecturer Eliezer Rabinovici
Hebrew UniversityOrganizer Faculty of PhysicsContact -
Date:12ThursdayMay 2011Colloquia
"Sesame- from a parallel universe to reality?"
More information Time 11:15 - 12:30Location Edna and K.B. Weissman Building of Physical SciencesLecturer Eliezer Rabinovici
HUJIOrganizer Faculty of PhysicsContact -
Date:12ThursdayMay 2011Lecture
Internal Statistics of a Single Natural Image
More information Time 12:00 - 12:00Location Ziskind Bldg.Lecturer Maria Zontak
Organizer Faculty of Mathematics and Computer Science -
Date:12ThursdayMay 2011Lecture
Some like it hot – Biomolecule Analytics using Microscale Thermophoresis
More information Time 12:30 - 12:30Location Ullmann Building of Life SciencesLecturer Dr. Moran Jerabek-Willemsen
NanoTemper Technologies GmbH, MunichOrganizer Department of Biomolecular SciencesContact Abstract Show full text abstract about This presentation gives an overview on a new technology for ...» This presentation gives an overview on a new technology for the measurement of biomolecule interaction that is termed Microscale Thermophoresis (MST).
The term Microscale Thermophoresis refers to the directed movement of molecules in optically generated microscopic temperature gradients. This thermophoretic movement is determined by the entropy of the hydration shell around the molecules. Almost all interactions between molecules and virtually any biochemical process related to a change in size, stability and conformation of molecules alters this hydration shell and can be quantified. Such changes allow quantification of binding affinities of proteins, nucleic acids and small molecules as well as measurement of enzymatic activities with MST. In addition also functional studies of small molecule inhibitors are possible. The microscopic temperature gradient is generated by an IR-Laser, which is strongly absorbed by water. The readout method of the interaction analysis is based on fluorescence: fluorescently labeled proteins/peptides/nucleic acids can be used as well as proteins expressed with GFP/YFP/RFP. In this presentation we will describe the technical details and the benefits of the Microscale Thermophoresis technology platform. We will show examples for interaction measurements ranging from protein – ribosome, protein – protein, small molecule – receptor binding studies to experiments where the interactions between a receptor incorporated in a vesicle and soluble proteins are analyzed.
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Date:13FridayMay 2011Cultural Events
Free Exchange Fair
More information Time 10:30 - 13:00Location Ruthie & Samy Cohn Building for Magnetic Resonance Studies in Structural BiologyHomepage Contact -
Date:15SundayMay 2011Lecture
Spectral Sparsification of Graphs and Approximations of Matrices
More information Time 11:00 - 11:00Location Ziskind Bldg.Lecturer Daniel Spielman
Yale UniversityOrganizer Faculty of Mathematics and Computer Science -
Date:15SundayMay 2011Lecture
SOLAR-DRIVEN CO2 REDUCTION USING CONJUGATED PHOTO-THERMAL-ELECTRO-CHEMICAL (PTEC) PROCESS
More information Time 11:00 - 11:00Lecturer Gidon Fridman
Environmental Sciences and Energy Research Dept. Weizmann Institute of ScienceOrganizer Department of Earth and Planetary SciencesContact -
Date:15SundayMay 2011Lecture
Journal club - A discussion on selected articles
More information Time 12:30 - 14:00Location Dannie N. Heineman LaboratoryLecturer Dr. Dong Xu, Prof. Eli Waxman Organizer Nella and Leon Benoziyo Center for AstrophysicsContact -
Date:15SundayMay 2011Lecture
The effect of musculature contraction on skeletal morphogenesis
More information Time 13:00 - 13:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Yulia Shwartz
Elazar Zelzer's group Dept. of Molecular Genetics, WISOrganizer Department of Molecular GeneticsContact -
Date:15SundayMay 2011Lecture
"The use of metabolic modeling in the post-genomics era: studying interactions in multi-species systems"
More information Time 13:00 - 14:00Location Ullmann Building of Life SciencesLecturer Dr. Shiri Freilich
School of Computer Sciences & Medicine, Tel Aviv UniversityOrganizer Department of Plant and Environmental SciencesContact
