The original aim was to understand molecular vibrational dynamics In a carbon plasma simulating a stellar atmosphere we discovered C 60 Thus a totally.

Slides:



Advertisements
Similar presentations
Multi-wavelength Observations of Galaxies at z>~2 Mauro Giavalisco (UMass) + The GOODS Team + The COSMOS Team.
Advertisements

BuckyBalls By Jordan May. How Buckyballs were discovered? Buckyballs were discovered by accident in space by R.E Smalley, H.F Kroto and graduate students.
Improving mass and age estimates of unresolved stellar clusters Margaret Hanson & Bogdan Popescu Department of Physics.
Chemistry in the Atmosphere Chapter 17 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
English 9 Mr. Rinka - Lesson #35
STELLAR EVOLUTION. SINGLE CLUSTER – TURNOFF MASS – AGE OF CLUSTER.
F.6 Chemistry Internet Searching Activity 2 Discovery and Application of Fullerenes By Chor Tak Lam (1) F.6B.
Discovery of Bucky Or at least how I remember it!!
Chapter 12: Stellar Evolution Stars more massive than the Sun The evolution of all stars is basically the same in the beginning. Hydrogen burning leads.
Conjugated Polymers and Carbon Nanotubes for Optoelectronic Applications Liming Dai Department of Polymer Engineering College of Polymer Science and Polymer.
Globules in Planetary Nebulae Review of some recent advances on the nature and origin of globules P. J. Huggins (NYU)
Quasars and Other Active Galaxies
Spectral Line Survey with SKA Satoshi Yamamoto and Nami Sakai Department of Physics, The Univ. of Tokyo Tomoya Hirota National Astronomical Observatory.
An Intoduction to Carbon Nanotubes
Unit 3 Nanomaterials.
1 Buckminsterfullerene synthesis Maryam Ebrahimi Chem 7530 Feb. 7 th, 2006.
Magnetic Pulsed Valve 1.The valve opens and shuts Rotating Disk He Pulsed Valve Lens to focus the laser beam.
Molecular Nanostuctures 1. Introduction. Carbon hybridization and allotropes Alexey A. Popov, IFW Dresden
INTRODUCTION TO NANOTECHNOLOGY Prashant Sharma MCA 3 rd Semester.
The Chemistry of Comet Hale-Bopp Wendy Hawley Journal Club April 6, 2006.
1 Chemistry in the Atmosphere Chapter 17 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
In fact all our atoms were formed in a star long ago.
The hot core that is not a “Hot Core”: Orion KL
What's in our galaxy?.
Graphite rod surface coated with C60
HWK Nature, 329, 529 (1987) Polaroid image of the first molecular model of C 28 C 28.
Nano-Technology Lee Zi Jing 3i3 (13).
NH 3 Orion RA Chiu ea 1967 HC 5 N synth Alexander ea HC 7 N in TMC1 HC 7 N Red Giant Star C 60 Kroto et al C 28 Kroto C 60 Ph 5 Cl Taylor ac1976 C 240.
Light … is an electromagnetic wave: … is a wave pattern of electric and magnetic fields … propagates in vacuum … has wavelength (blue: 400 nm, red: 700.
Interstellar Chemical Models with Molecular Anions Eric Herbst, OSU T. Millar, M. Cordiner, C. Walsh Queen’s Univ. Belfast R. Ni Chiumin, U. Manchester.
Lecture 20…The Formation of Stars: where and how Nature provides a hint: young star clusters The proto- typical object.
Quasars and Other Active Galaxies
Bob Curl had invited me to Rice after the conference.
Chemistry Level 2 Giant covalent structures and nanomaterials.
DIBs McKellar1936 C 33 Hinten- berger ea l1960 Supersonic Nozzle Smalley Levy Wharton NH 3 Orion RA Chiu ea 1967 C 3 comets Douglas 1936 RC 32 R Walton.
Globular Clusters. A globular cluster is an almost spherical conglomeration of 100,000 to 1,000,000 stars of different masses that have practically.
Between 1985 and 1990 more than half a dozen publications claimed we were wrong.
Rick Smalley Rice University Metal Clusters Fe10 Si6 Al20 etc lens
The rod translated and rotated by stepper motor laser pulse vaporises rod Helium pulse C 60 reacts with C, C 2 exits and undergo supersonic expansion.
2002/02/01 p.1 奈米碳管的性質與應用 Dr. Rational You IEK/ITRI 2002/02/01 Source:
C 28 ”superatom” analogue of sp 3 carbon atom Suggests T d C 28 H 4 Nature (1987) Support C 28 U tetravalent (Smalley and coworkers) C 28 H.
Stars, galaxies and planets Dept. of Physics, Bangalore University Bangalore B. A. Kagali.
Amit Sarkar’s 3 rd year undergraduate project supervised by grad student Jonathan Hare.
FIRST LIGHT A selection of future facilities relevant to the formation and evolution of galaxies Wavelength Sensitivity Spatial resolution.
Jim got me some money yet again to come to the Austin conference in Easter 1984.
Searching for Vibronic Progressions in the Diffuse Interstellar Bands via Agglomerative Clustering Jane Huang Astro 193 Final Project Spring 2015.
ISM & Astrochemistry Lecture 1. Interstellar Matter Comprises Gas and Dust Dust absorbs and scatters (extinguishes) starlight Top row – optical images.
Rick Smalley Magnetic Pulsed Valve Hole for the laser pulse.
“Globular” Clusters: M15: A globular cluster containing about 1 million (old) stars. distance = 10,000 pc radius  25 pc “turn-off age”  12 billion years.
Lecture 1 Stories of Fullerenes and Carbon nanotubes.
Astronomy: Stars & Light
The Faith needs Patience
Rhyme Schemes.
Only three lines observed R(0) R(1) P(1)
TA06 International Symposium on Molecular Spectroscopy TA. Astronomy
Chemistry in the Atmosphere
Graphite, Graphene (= single sheet) 2D
IMF inferred based on field stars (red) and based on a variety of clusters (blue, green, and black) (Kroupa 2002)
The first giant fullerene C240
General thermolytic routes to new unstable species - thiocarbonyls
Drift -Tube Ion Mobility Measurements
We use hexagonal carbon network to make all sorts of curved structures
Bob Curl had invited me to Rice after the conference
Fusion Reactions in Stars
FSU Harry Kroto 2004.
The Discovery of C60 ACS Philadelphia 2016.
Chemistry in the Atmosphere
Image-potential States in Carbon Nanotubes
Harry Kroto 2004.
Sussex NNC.
Presentation transcript:

The original aim was to understand molecular vibrational dynamics In a carbon plasma simulating a stellar atmosphere we discovered C 60 Thus a totally new field of Chemistry was born We discovered carbon chains in space It is found that fullerenes improve plastic solar cell efficiency …then our carbon chains were discovered in stars Structure clues came from architecture and models …then by radioastronomy

All that is gold does not glitter Not all those who wander are lost The old that is strong does not whither Deep roots are not reached by the frost

From the ashes a fire shall be woken A light from the shadows shall spring Renewed shall be the blade that is broken The crownless again shall be king

All that is gold does not glitter Not all those who wander are lost The old that is strong does not whither Deep roots are not reached by the frost

NH 3 Orion RA Chiu ea 1967 HC 5 N synth Alexander ea HC 7 N in TMC1 HC 7 N Red Giant Star C 60 Kroto et al C 28 Kroto C 60 Ph 5 Cl Taylor ac1976 C 240 C 540 McKay ea Cluster Beam Smalley ec NH 3 HC 5 N HC 7 N HC 9 N HC 7 N Sussex research Solar Cells Heeger et al

DIBs McKellar1936 C 33 Hinten- berger ea l1960 Supersonic Nozzle Smalley Levy Wharton NH 3 Orion RA Chiu ea 1967 C 3 comets Douglas 1936 RC 32 R Walton ea HC 3 N SgrB2 Turner Cluster Beam Duncan..Smalley SiC 2 Smalley HC 5 N synth Alexander HC 5 N SgrB2 Avery ea HC 7 N in TMC1 Kroto HC 9 N in TMC1 Kroto HC 7 N Red Giant Star C 60 Kroto et al Cluster Beam HC 7 N 60 Heath ea C 28 Kroto Carbon Huffman C 60 IR Theory C 60 IR Krätschmer ea C 60 extraction Krätschmer ea Nanotube Endo ac1976 Nanotubes Iijima 1990 C 60 formation Heath 1992 CNT formation Endo Kroto nm UV Hump UV Hump Krätschmer Huffman Graphene 1990 C 60 extraction Hare Taylor nmr C 70 derivative in printed solar cells…Heeger ac 1992 C 60 Ph 5 Cl Taylor ac1976 Fullerene formation Dunk ea gateway Dunk ea 2012 C 60 in space? Kroto Jura 1992 C 60 in space Cami 2010