AJ Mesko Ian Wagner Stefanie Milam Susanna Widicus Weaver

Slides:



Advertisements
Similar presentations
Photodesorption of Ices Karin Öberg, Ruud Visser Ewine van Dishoeck, Harold Linnartz.
Advertisements

School of Chemistry, University of Nottingham,UK 1 Why Does Star Formation Need Surface Science? Using Laboratory Surface Science to Understand the Astronomical.
School of Chemistry University of Nottingham Probing the Morphology of Interstellar Ice Analogues In Memory of Rui Chen. Mark Collings School of Chemistry,
Nuria Marcelino (NRAO-CV) Molecular Line Surveys of Dark Clouds Discovery of CH 3 O.
METO 637 Lesson 22. Jupiter Jupiter and Saturn are known as the gas planets They do not have solid surfaces, their gaseous materials get denser with.
Millimeter/Submillimeter Spectroscopy of Prebiotic Molecules Formed from the O( 1 D) Insertion Into Methylamine Brian Hays, Althea Roy, and Susanna Widicus.
Near-Infrared Spectroscopy of Interstellar and Planetary Ice Analogs
Laboratory Chemistry of the Outer Solar System Marla Moore NASA/Goddard Space Flight Center January 28, 2008 Cosmic Ice Lab Polar Gateways Arctic Circle.
Laboratory Submillimeter Spectroscopy as a Probe of Methanol Photodissociation Jacob C. Laas & Susanna L. Widicus Weaver Department of Chemistry, Emory.
L'Equipe Astro-OP est composée de plusieurs groupes de recherche sur le site "Observatoire de Paris", qui travaillent sur cinq grands thèmes : le Milieu.
The chemistry and physics of interstellar ices Klaus Pontoppidan Leiden Observatory Kees Dullemond (MPIA, Heidelberg) Helen Fraser (Leiden) Ewine van Dishoeck.
Development of a Near-IR Cavity Enhanced Absorption Spectrometer for the detection of atmospheric oxidation products and amines Nathan C. Eddingsaas Breanna.
Hot molecules in helium nanodroplets: a new route to optical spectra Benjamin Shepperson, Adrian Boatwright, Cheng Feng, Daniel Spence, Shengfu.
Methanol Photodissociation Studies using Millimeter and Submillimeter Spectroscopy Jacob C. Laas & Susanna L. Widicus Weaver Department of Chemistry, Emory.
Nanonics CryoView 2000™ CryoView 2000™ Product Presentation.
Detection, Identification, and Correlation of Complex Organic Molecules in 32 Interstellar Clouds Using Submm Survey Observations Nadine Wehres, Shiya.
G. Lopes, A. Ferreira, A.P. Gonçalves and J.B. Branco Instituto Tecnológico e Nuclear, Estrada Nacional 10, Sacavém, Portugal Unidade de Ciências.
G. Lopes, A. Ferreira, A. P. Gonçalves and J. B. Branco Instituto Tecnológico e Nuclear, Estrada Nacional 10, Sacavém, Portugal Unidade de Ciências.
Testing grain-surface chemistry in massive hot-core regions and the laboratory (A&A, 465, 913 and A&A submitted) Suzanne Bisschop Jes Jørgensen, Ewine.
Laser Photolysis at the Australian Synchrotron, THz Beamline.
METHOD DEVELOPMENT FOR GAS-PHASE STUDY OF INTERSTELLAR ICE ANALOGUES AJ Mesko, Ian Wagner, Houston Smith, Stefanie Milam, Susanna Widicus Weaver.
Millimeter and Submillimeter Studies of O( 1 D) Insertion Reactions to Form Molecules of Astrophysical Interest Brian Hays, Nadine Wehres, Bridget Alligood.
Fast Sweeping Double Resonance Microwave - (sub)Millimeter Spectrometer Based on Chirped Pulse Technology Brian Hays 1, Susanna Widicus Weaver 1, Steve.
The coating thermal noise R&D for the 3rd generation: a multitechnique investigation E. Cesarini 1,2), M.Prato 3), M. Lorenzini 2) 1)Università di Urbino.
Complex Organic Molecules formation on Interstellar Grains Qiang Chang Xinjiang Astronomical Observatory Chinese Academy of Sciences April 22, 2014.
Kinetics measurements of HO 2 and RO 2 self and cross reactions using infrared kinetic spectroscopy (IRKS) A.C. Noell, L. S. Alconcel, D.J. Robichaud,
The Design of a Novel Ultra High Vacuum Surface Machine to Determine the Formation of Glycolaldehyde in the Interstellar Medium By Chris Bennett.
UV/VIS SPECTROSCOPY.
Detection and classification of snow/ice using infrared imaging
Analytical Chemistry II ChEm 321
The Liberation of CO from Photoprocessed Methanol Ice
Searching for Aminomethanol Amongst the Reaction Products of O(1D) Insertion into Methylamine Morgan McCabe, Brian Hays, Carson powers, Sam Zinga, and.
Су- әмбабап табиғи еріткіш / Water – the universal solvent
Light is the only information we get from most astronomical objects
SRI 2000 Berlin, August 21-25, 2000 High-Pressure Low-Energy X-Ray Absorption Spectroscopy: A Tool to investigate heterogeneous catalytic Processes under.
Chapter 2: Matter and Change
Chapter 17 Thermochemistry 17.3 Heat in Changes of State
On the Formation of Molecules on Interstellar Grains
Goddard Space Flight Center
R. M. E. Mastrapa, M. Bernstein, S. Sandford NASA Ames Research Center
Section 2 Changes of State.
Outline RAIRS of Methanol on clean Cu(110)
Section 1.1 – 1.2 What is Chemistry Classification of Matter
Carson Powers, Morgan N. McCabe, Susanna L. Widicus Weaver
Adsorption and Desorption of Mixed Ices
Matter and Change Unit Review
Physical Change A process by which no change in composition occurs
8TH GRADE SCIENCE Chapter 1 Lesson 1
Interstellar Ice Formation on Dust Grains
Using IR Spectroscopy to Probe the Temperature Dependence of the H + N2O Reaction in Parahydrogen Crystals Fredrick Mutunga and David T. Anderson Department.
Phase Change – depends on heat energy
انواع المخاليط (التدريس الابداعي )
Phase Diagrams: Solid, Liquid & Gas Roadmaps
Physical and Chemical Change
formation of H2CO and CH3OH
Chemistry and Contrails
Energy (2-4).
States of Matter Vocabulary Week 7.
Chemistry II Honors Chapters 1-5
Chemistry Matter and Change.
Solutions.
K.Nagasawa1), H.Nakatsugawa1) and Y.Okamoto2)
Water = 2 Hydrogen atoms + 1 Oxygen atom “H2O”
Matter And Energy SAVE PAPER AND INK!!! When you print out the notes on PowerPoint, print "Handouts" instead of "Slides" in the print setup. Also, turn.
Phases of Matter, and Melting/Freezing Point
Food is matter-A pure substance or mixture
Chemical Properties February
Vocabulary Week 3.
Latent Heat of Phase Changes
Chemistry I Honors: Chapter 2
Presentation transcript:

AJ Mesko Ian Wagner Stefanie Milam Susanna Widicus Weaver PROBING GAS PHASE CHEMISTRY ABOVE ICE SURFACES WITH MILLIMETER/ SUBMILLIMETER SPECTROSCOPY The Trifid Nebula, NASA AJ Mesko Ian Wagner Stefanie Milam Susanna Widicus Weaver http://apod.nasa.gov/apod/ap130128.html The Trifid Nebula

Why is Ice Important Icy Grain Chemistry Our Experiment The Spectrometer Proof of Concept Future Experimentation

Icy Grain Chemistry

http://chemistry.emory.edu/faculty/widicusweaver/prebiotic.html

What we do Analyzing the gas phase products of Icy Grain Reactions by mm/sub-mm Spectroscopy UV Lamp Photolyzing Radiation CH3OH mm/sub-mm source .OH H2O Detector .CH3O H2O CH3OH CH3OH H2O CH3OH H2O Gold Substrate Heating

http://chemistry.emory.edu/faculty/widicusweaver/prebiotic.html

Why We Do It Gain information on chemical mechanisms by which COMs can form by icy grain chemistry. Analyze the effects that different ice compositions and physical properties have on the formation of COMs

The Budget Spectrometer Built mostly of borrowed parts and on a strict budget Cryopad Setup 1 Liquid Helium Cryostat Sapphire windows Gold substrate on cold head Say it was the Leiden group who developed instead of butchering the name 1. van Broekhuizen, F. 2005, Ph.D. Thesis, Leiden University

Temperature Controller Microwave Synthisizer Multiplier Chain Cryostat To pump UV Lamp Sample Line Detector Lock In Amplifier Temperature Controller Microwave Synthisizer CPU

Temperature Programmed Desorption of Pure Water Ices Proof of Concept Temperature Programmed Desorption of Pure Water Ices

Comperable as to what was seen by Fraiser et al 2001

Proof of Concept Continued: Temperature Programmed Desorption of Pure Methanol Ice

Conclusions A working mm/sub-mm spectrometer capable of detecting desorption products has been built Results from other Temperature programmed desorption experiments of pure water2 are in agreement with those produced by this instrument 2. Fraser et. Al 2001

The Future Photolysis and photodesorption testing The Addition of RAIRS for solid phase analysis A Dirty Chamber Water/organic mixture studies Effect of Ice thickness and crystallinity Gas phase photolysis and thermal product studies Reflection Absorption InfraRed Spec

Acknowledgements Danna Qasim The Widicus Weaver Research Group Emory University NASA GSFC SIF Program