ISG: The Limitations of K/Ar in Gemstone Treatment Testing
|
|
- Derek Rose
- 6 years ago
- Views:
Transcription
1 Like Share this Page: a publication of the International School of Gemology...28 April ISG: The Limitations of K/Ar in Gemstone Treatment Testing Over the past couple of years the jewelry industry has been razzle-dazzled by some rock star famous PhD scientists regarding the claimed use of potassium/argon testing (K/Ar) to identify gemstone treatment. The sheer weight of credentials and initials after these folk s names has invoked shock and awe in the hearts of consumer and professional alike. There is, of course, just one problem..k/ar cannot disprove that a gemstone has been treated. What K/Ar does do is simply show a presence of argon gas inside a crystal as a result of deterioration of potassium to argon over millions of years. High heating will allow this gas to escape leaving the void to demonstrate the result of the heating. While this test can use the absence of argon gas to show that a stone has been subjected to high heating treatment, it cannot prove or disprove that a gemstone has been treated by a variety of other methods. Mainly because there are myriads of treatments out there that do not require high temperatures. In fact, with the latest reports from Ted Themelis, low temperature diffusion of gemstones is a reality. This creates a one way street for K/Ar dating: The absence of argon gas can prove heating, but the presence of argon gas does not disprove other possible treatments. This gives K/Ar testing only a single value purpose in gemology: to identify gemstones that have been subjected to high heating. K/Ar cannot be used to show that a gemstone has not been treated. But a recent report by Dr. Philip Ganz, expert witness in defense of Direct Shopping Network in the DSN v- Robert James legal action, recently issued a report that attempted to use K/Ar to prove a negative in the matter of andesine treatment. The concept put forth by Ganz was that a green andesine supplied by Andegem and sold by DSN was all natural based solely on the positive reaction of argon to K/Ar testing. The problem is that Ganz made erroneous conclusions based on simple math. We can demonstrate this by using the simply math equation: If A=C and B=C then A=B. In the case of this green andesine. A=C but B C therefore A B. This situation can be demonstrated by the copper bearing feldspar that has become quite famous. In this case A = red feldspar color source B = green feldspar color source and C = copper. And since copper has distinct and verifiable absorption spectra in feldspar, we are able to verify the equation by use of the VIS-NIR Spectrometer. For our purposes we used our GL Gem Spectrometer from the CIG, the Challenger Vis-NIR, and our own OPL optical diffraction grating spectroscope. You can see the copper absorption spectra in the visible range below. This is a specimen that obtained direct from the miners of the Outback Sunstone Mine from Oregon while at the Tucson Pueblo Show last February. The absorption band is where the red and green meet. Notice that the absorption area in the 577nm green/red meeting section is an actual digital image taken through our OPL diffraction grating spectroscope of this specimen. This clearly shows the copper absorption area in this stone. This becomes the control spectrum for our testing. The Math of Oregon Sunstone In the case of Oregon sunstone A= Red Sunstone B = Green Sunstone and C=Copper. Notice the rough crystal of Plush Oregon Sunstone from the Double Eagle #16 mine shown at left. We have a distinct red color and green color within this crystal. This is a first test specimen.
2 We also used the specimen you see below that was designed and cut by the world famous John Dyer. Note that this Plush Oregon Sunstone from the Dust Devil Mine demonstrates a pronounced green color, although in our Dixie Cup immersion cell it is clear to see that this stone is of a red and green coloration from the copper. Based on our spectroscopic evaluation of this feldspar dating back to 2008, we know that the red and green areas of Oregon Sunstone result in the diagnostic absorption lines that are known to show copper as the source. This is repeatable and predictable for Oregon Sunstone. As a result of the above we find that our equation works quite well: A=C B=C therefore A=B. The red color is due to copper. The green is due to copper. Therefore the red and green are both due to copper. The spectral analysis positively supports this equation as true. Then.we have Tibet andesine supplied by Andegem, sold by Direct Shopping Network, and tested by Dr. Ganz. The Math of claimed "Tibet Andesine" from Andegem and Direct Shopping Netork As you can see above, we have known that we had a problem with the math on this claimed Tibet andesine since the very early stages of testing. Why? The spectra does not match for the red and green. The math does not work. Jewelry Television also had Andegem as their supplier. JTV now discloses all of their andesine as diffusion treated. The spectral images above are direct digital images taken through our OPL diffraction grating spectroscope of JTV stones from Andegem in Note that while the red has the distinct copper absorption band, the green does not. The green Andegem stone shows no copper absorption spectra. That is the
3 problem with the math of the Andegem andesine sold by JTV: A=C B C therefore A B. Which (we would find out), the green color is not due to copper but instead due to a reported radiation pre-treatment that is done on the stone to prepare it for the copper diffusion, to make the diffusion work better. That radiation treatment has been reported as the cause of the green color in this claimed "Tibet" andesine. The JTV stones had a preliminary treatment that K/Ar simply cannot identify or dispute. Below are three stones sold by DSN and tested by the ISG in 2008 and The dark red stone below right has an extremely strong absorption line in the 577nm region that is known for the copper absorption. But the stone cut in half with light pink color is weak in the absorption. Most important.the green stone shows no copper absorption at all! Once again, this stone shows the results of pre-treatment but very little of the copper diffusion treatment. You can see that results in the image below right. The red coloring is only barely penetrating the stone. And yet the green color is dominant throughout the stone. A(red color source)=c(copper) B(green color source) C(copper) therefore.a(red color source) B(green color source). These stones have different sources for their color. And yet, based solely on his findings that K/Ar testing showed no heating to 1100 C of the green stone above right, Dr. Ganz and DSN reported the stone to be all natural and without treatment. In truth, the above explains a lot of what we have been seeing in this Andegem supplied Tibet andesine for years. The green is not due to copper, and not due to diffusion. The specimens support the reports that a radiation pre-treatment is done on the stones before the high heat diffusion process is performed. The result is that the stones are green first from pre-treatment, and then red after diffusion. Below are a few images to demonstrate this. Consider these images along with the question about why the Andegem andesine was green inside and red outside, while the natural Oregon Sunstone is just the opposite. The Oregon Sunstone is due to copper green and red. The Andegem / DSN andesine color is due to reported radiation treatment induced green, followed by the copper diffusion treated red. A=C B C therefore A B. Check out the images below and consider this equation. The rough specimen below right was tested by OPL Spectroscope specifically in the red and green areas and the above equation was demonstrated in this rough along with many others. The faceted Andegem stone below left shows the green interior color with the red diffused color that was done later.
4 Below are two specimens from the ISG study collection. Below left is a radiation treated green andesine that shows very little diffusion of red copper color, while below right this stone also shows the radiation induced green color with a greater degree of red diffusion coloration. This also explains the very unusual piece of rough andesine claimed to be from Tibet and supplied to us by Chinese supplier Litto Gems (below left). Notice the green coloring with the red being diffused from the outside in. And the round faceted stone purchased direct from Andegem at the GJX show in It should be noted that AGTA member Andegem sold this stone to us without any disclosure, a violation of AGTA published directives for this stone. Perhaps most profound on this issue is the image below from the ISG archives. This image clearly demonstrates that the green color is a body color of the andesine. The red color shows the diffusion process that occurred at some later time. Again in this image A=C B C therefore A B. The green color does not equal a copper source. It was not due to diffusion. Not identifiable by K/Ar testing.
5 Let s take this whole thing one step further and look at the actual gemstone tested by Dr. Ganz on behalf of Direct Shopping Network. When the DSN lawyers asked for specimens for destructive testing, my recommendation was to not agree to the request on its face. A destructive test precludes any ability to evaluate and/or verify Dr. Ganz test results. My recommendation was to cut the stone in half, allowing for half to be preserved for verification of any findings by Ganz. Therefore the stone you see at left is one half of the original stone belonging to the class action member in the Class v- DSN litigation. We originally tested this stone in Dr. George Rossman of Caltech did the cutting of this stone in half and forwarded a half to us and half to DSN representative. The gemstone in its original condition is seen below. At left is the original ISG image of Ms. Johnson s DSN andesine taken in the ISG office in This is the entire stone seen in 2008 that was cut by Dr. Rossman and seen above in its cut state currently. Dr. Ganz and DSN has declared this stone to be all natural based on K/Ar testing showing argon. But we now know that the green color of this stone is not due to natural copper in fact not to copper at all. And the pre-treatment that imparts this color does not require heating. A point that Ganz s K/Ar testing could not address. Remember the images above showing the green half stone that showed no copper absorption line.that is this very stone. To review, below is the red DSN andesine sold to Ms. Johnson in our Challenger VIS-NIR spectrometer, below right is the green DSN stone sold to Ms. Johnson and cut in half by Dr. Rossman. Both at 577nm where the copper absorption should be located. The green.shows none. No copper. A=C but B C. Let s go back to our Dixie cup immersion cell and see if our original findings support this conclusion. Remember the images with the triangle cut andesine showing different levels of diffusion of the red copper diffusion into the green radiation treated andesine. Here they are again:
6 Now, look at the DSN andesine sold to Ms. Johnson and now cut in half. Clearly this stone shows the green color that we have seen shows no copper absorption, and the very partial red color due to failed or stopped diffusion treatment. The failed or stopped diffusion treatment means that the stone was not subjected to high temperature. Result: K/Ar testing would indicate no heating due to the presence of argon gas. Ganz and DSN therefore said: No heat...no treatment. This was an incorrect conclusion since K/Ar cannot deny all possible treatments. The depth of the red copper diffusion material into the stone can easily be seen in the 90x microphotograph seen at left. Here is our question for DSN and Dr. Ganz,. Of all of the DSN red andesine in question, including all (100%) of the DSN 2008 Beijing Olympic Andesine that are red.why did you pick a green stone to test using K/Ar? With the overwhelming majority of the Tibet andesine colored red, including the DSN 2008 Beijing Olympic Andesine, why pick a green stone to test for the court? Was Dr. Ganz and DSN aware that the green stone would give them the results they needed for this litigation purposes? We don t know. But.. The two stones below were both part of the litigation group sold by DSN and supplied to them by Andegem. Why not pick the stone below right? This stone was also sold by DSN to Ms. Johnson and photographed as you see below right in Both have green centers but one has only very slight red diffusion. That is the stone that DSN and Ganz picked for K/Ar testing. Why?
7 We believe we know the answer: They knew that the green stone had not been subjected to high heat, and that K/Ar testing would allow them to claim: No Heat = No Treatment. Unfortunately, that equation did not work, and does not work today. There are a myriad of treatments out there that do not require high heat, which makes K/Ar testing for gemstone treatments to be invalid for anything other than high heat. All of the other treatments can and are missed if only the K/Ar testing is used. Want to test this theory? Ask Dr. Ganz and DSN to run that same K/Ar test on the Johnson stone seen above right, or this DSN 2008 Beijing Olympic Andesine at left. Of course, Dr. George Rossman and his team at Caltech have already done this and found the red stones from Andegem to all have been subjected to high heating. This supports our equation that the red and green colors in the Andegem claimed Tibet andesine are due to treatments, but does not dispute our equation that the colors are due to separate treatments. However, this does leave us with one more equation that is critical based on Art Garabedian's own declaration that Andegem is the supplier of andesine to DSN: A represents andesine supplied by Andegem. B represents andesine sold by DSN. C represents treated andesine as verified by Dr. Rossman and the ISG above. The equation: If A=B and A=C then B=C True! There is nothing in the Ganz report that can dispute this equation. There are serious limitations to K/Ar testing. It cannot be used to disprove a gemstone treatment. In the case of the Oregon Sunstone v- the claimed Tibet Andesine where A is red color source, B is green color source and C is copper. Oregon Sunstone: A=C B=C therefore A=B Tibet Andesine: A=C B C therefore A B There is no K/Ar testing that can refute this. DSN cannot claim that the green andesine sold to Ms. Johnson is natural and without treatment based on K/Ar testing. K/Ar testing cannot prove that a gemstone has not been treated. Robert James President, International School of Gemology To obtain this report in PDF format please click here: The Limitations of K/Ar Testing Contact the ISG by clicking on this icon:
Andesine: The Final, Final Chapter..
Andesine: The Final, Final Chapter.. From the International School of Gemology The complete story of the ISG investigation into the diffusion treatment of andesine, the people who were involved, and the
More informationInterim Report 14-Sep The Red Feldspar Project. George R. Rossman California Institute of Technology
Interim Report 14-Sep-2009 The Red Feldspar Project George R. Rossman California Institute of Technology 1 Chemical Analyses Electron microprobe analyses are an accurate way of determining the composition
More informationNEWS FROM RESEARCH. Observations of Surface Residue Features Found on Andesine from China
NEWS FROM RESEARCH Observations of Surface Residue Features Found on Andesine from China Shane F. McClure Abstract Unusual glassy materials filling crevasses and low areas in rough samples of andesine
More informationNEWS FROM RESEARCH. Argon Isotope Studies of Andesine Collected During the 2010 Expedition to Tibet
NEWS FROM RESEARCH Argon Isotope Studies of Andesine Collected During the 2010 Expedition to Tibet George R. Rossman Abstract Argon isotope studies of samples returned from the 2010 expedition to Tibet
More informationThe Spectroscopy of Stars
The Spectroscopy of Stars In this activity you will use a hand held spectroscope to investigate a number of known and unknown light sources. A spectroscope is an instrument that helps to observe the spectrum
More informationIntroducing Proof 1. hsn.uk.net. Contents
Contents 1 1 Introduction 1 What is proof? 1 Statements, Definitions and Euler Diagrams 1 Statements 1 Definitions Our first proof Euler diagrams 4 3 Logical Connectives 5 Negation 6 Conjunction 7 Disjunction
More informationA Pleochroic Variety of Gem Labradorite From the Rabbit Hills Area, Lake County, Oregon*
A Pleochroic Variety of Gem Labradorite From the Rabbit Hills Area, Lake County, Oregon* By ERNEST H. CARLSON Associate Professor of Geology Kent State University and MICHAEL A. KIRCHER Geologist and Gemologist
More informationAstronomy 101 Exam 3 Form C
Astronomy 101 Exam 3 Form C Name: Lab section number: (In the format M0**. See back page; if you get this wrong you may not get your exam back!) Exam time: one hour and twenty minutes Please put bags under
More informationSpectrometers. Materials: Easy Spectrometer. Old CD Razor Index card Cardboard tube at least 10 inches long
Spectrometers Overview: Spectrometers (spectroscopes) are used in chemistry and astronomy to measure light. In astronomy, we can find out about distant stars without ever traveling to them, because we
More informationSaltwater cultured pearls from Pinctada maxima
NOTES & NEW TECHNIQUES SPECTRAL CHARACTERISTICS OF NATURAL-COLOR SALTWATER CULTURED PEARLS FROM PINCTADA MAXIMA Stefanos Karampelas Natural-color saltwater cultured pearls (SWCPs) from Pinctada maxima
More informationGems And Crystals: From The American Museum Of Natural History (Rocks, Minerals And Gemstones) By George E. Harlow, Anna S.
Gems And Crystals: From The American Museum Of Natural History (Rocks, Minerals And Gemstones) By George E. Harlow, Anna S. Sofianides Gemstones of the World - Page 100 - Google Books Result - Deposits
More informationAstronomy 101 Exam 3 Form A
Astronomy 101 Exam 3 Form A Name: Lab section number: (In the format M0**. See back page; if you get this wrong you may not get your exam back!) Exam time: one hour and twenty minutes Please put bags under
More informationThe X-ray spectra and the structure of the atoms
M A N N E S I E G B A H N The X-ray spectra and the structure of the atoms Nobel Lecture, December 11, 1925 We all know that the discovery of X-rays provided the medical sciences with a new and invaluable
More informationIdentification of Natural and Treated Red Feldspar
Research article Identification of Natural and Treated Red Feldspar Namrawee Susawee 1 * and Chakkaphan Sutthirat 1, 2 1 Department of Geology, Faculty of Science, Chulalongkorn University, Bangkok 10330
More informationAstronomy 101 Exam 3 Form D
Astronomy 101 Exam 3 Form D Name: Lab section number: (In the format M0**. See back page; if you get this wrong you may not get your exam back!) Exam time: one hour and twenty minutes Please put bags under
More informationMath 414, Fall 2016, Test I
Math 414, Fall 2016, Test I Dr. Holmes September 23, 2016 The test begins at 10:30 am and ends officially at 11:45 am: what will actually happen at 11:45 is that I will give a five minute warning. The
More informationEarlier we learned that hot, opaque objects produce continuous spectra of radiation of different wavelengths.
Section7: The Bohr Atom Earlier we learned that hot, opaque objects produce continuous spectra of radiation of different wavelengths. Continuous Spectrum Everyone has seen the spectrum produced when white
More informationEXPERIMENT 09 OBSERVATION OF SPECTRA
EXPERIMENT 09 OBSERVATION OF SPECTRA INTRODUCTION: In physics, as in very other area of study, one of the most valuable questions a student can learn to ask is, How do they know that? Thus, when you read
More informationThe Hydrogen Atom Student Guide
Name: The Hydrogen Atom Student Guide Background Material Carefully read the background pages entitled Energy Levels, Light, and Transitions and answer the following questions to check your understanding.
More informationASTRO Fall 2012 LAB #7: The Electromagnetic Spectrum
ASTRO 1050 - Fall 2012 LAB #7: The Electromagnetic Spectrum ABSTRACT Astronomers rely on light to convey almost all of the information we have on distant astronomical objects. In addition to measuring
More informationAtomic Theory C &03
Atomic Theory Part One: Flame Tests Part Two: Atomic Spectra Part Three: Applications of Spectra (optional) C12-2-02 &03 This activity will focus on the visible portion of the electromagnetic spectrum.
More informationHomework on Properties of Galaxies in the Hubble Deep Field Name: Due: Friday, April 8 30 points Prof. Rieke & TA Melissa Halford
Homework on Properties of Galaxies in the Hubble Deep Field Name: Due: Friday, April 8 30 points Prof. Rieke & TA Melissa Halford You are going to work with some famous astronomical data in this homework.
More informationWhat is proof? Lesson 1
What is proof? Lesson The topic for this Math Explorer Club is mathematical proof. In this post we will go over what was covered in the first session. The word proof is a normal English word that you might
More information21CLD Learning Activity Description
Learning Activity Example: Olympics Site Selection 1 21CLD Learning Activity Description 1. Title of Learning Activity & Average Age of Students Title: Olympics Site Selection Average Age of Students:
More informationPhysics Lab #4: Citizen Science - The Milky Way Project
Physics 10263 Lab #4: Citizen Science - The Milky Way Project Introduction This lab is the first of several Citizen Science labs we will do together this semester as part of the zooniverse.org project
More informationMath 3361-Modern Algebra Lecture 08 9/26/ Cardinality
Math 336-Modern Algebra Lecture 08 9/26/4. Cardinality I started talking about cardinality last time, and you did some stuff with it in the Homework, so let s continue. I said that two sets have the same
More informationProducing and Harnessing Light
Chemical Dominoes Activity 5 Producing and Harnessing Light GOALS In this activity you will: Describe the relationship between energy, frequency, and wavelength of electromagnetic radiation. Explain how
More informationHow to Make Photometric & Colorimetric Measurements of Light Sources using an Ocean Optics Spectrometer and SpectraSuite Software
How to Make Photometric & Colorimetric Measurements of Light Sources using an Ocean Optics Spectrometer and SpectraSuite Software This is a concise guide to setting up and calibrating your Ocean Optics
More informationThis article presents the results of the author s THE CHINESE RED FELDSPAR CONTROVERSY: CHRONOLOGY OF RESEARCH THROUGH JULY George R.
THE CHINESE RED FELDSPAR CONTROVERSY: CHRONOLOGY OF RESEARCH THROUGH JULY 2009 George R. Rossman Red copper-containing plagioclase feldspar from Oregon has been available for over a century. In the early
More informationBellwork: Calculate the atomic mass of potassium and magnesium
Bellwork: Calculate the atomic mass of potassium and magnesium Chapter 5 - electrons in atoms Section 5.1: Revising the atomic model What did Ernest Rutherford think about electrons? In Rutherford s model,
More informationIDS 102: Electromagnetic Radiation and the Nature of Light
IDS 102: Electromagnetic Radiation and the Nature of Light Major concepts we will cover in this module are: electromagnetic spectrum; wave intensity vs. wavelength, and the difference between light reflection,
More informationSpectral Lines. I've done that with sunlight. You see the whole rainbow because the prism breaks the light into all of its separate colors.
Spectral Lines At the end of 19th century, physicists knew there were electrons inside atoms, and that the wiggling of these electrons gave off light and other electromagnetic radiation. But there was
More informationKETCHUM ARTS COMMISSION INTERACTIVE ART CALL FOR ARTISTS Request for Qualifications
KETCHUM ARTS COMMISSION INTERACTIVE ART CALL FOR ARTISTS Request for Qualifications I N T R O D U C T I O N The City of Ketchum, Idaho, invites professional artists, architects or designers to apply for
More informationLight and Matter(LC)
Light and Matter(LC) Every astronomy book that I ve seen has at least one chapter dedicated to the physics of light. Why are astronomers so interested in light? Everything* that we know about Astronomical
More informationAt this point, most readers will
The Limitations of Origin Determination In this second instalment of a series of articles on the origin determination of coloured gemstones, the Gubelin Gem Lab Ltd, in Lucerne, Switzerland, focuses on
More informationELECTRICITY. This chain is similar to the fire fighter's bucket brigades in olden times. But
ELECTRICITY Electricity figures everywhere in our lives. Electricity lights up our homes, cooks our food, powers our computers, television sets, and other electronic devices. Electricity from batteries
More informationFor instance, for a particular star cluster, these data were derived:
Astronomy 100 Name(s): Exercise 5: The H-R diagram and spectroscopy A very basic correlation using the color index By the 1920 s, various astronomers had evidence that the temperature of a star was also
More informationAtomic Structure. Niels Bohr Nature, March 24, 1921
1 of 5 4/26/2013 12:47 AM Atomic Structure Niels Bohr Nature, March 24, 1921 In a letter to NATURE of November 25 last Dr. Norman Campbell discusses the problem of the possible consistency of the assumptions
More informationTeam members (First and Last Names): Fossil lab
Team members (First and Last Names): Period: Group #: Fossil lab Background: Fossils are traces of organisms that lived in the past. When fossils are found, they are carefully excavated and then analyzed.
More informationElectric Current Model-Evidence Link Diagram (MEL)
A C o n t e n t S e c o n d a r y S c i e n c e N e w s l e t t e r f r o m t h e Southo u t h ern r n Nevada e v a d a R egional g i o n a l Professional r o f e s s i o n a l Development e v e l o p
More informationMeteorites Land at KU! In this Issue: Meteorites Land Page 1. Spring 2016 Planetarium Schedule. Page 2. Laser Light Shows. Page 5
Meteorites Land at KU! In this Issue: Meteorites Land at KU! Page 1 Spring 2016 Planetarium Schedule Page 2 Laser Light Shows Page 5 Open House at the Observatory Have you ever wanted to touch something
More information2. Discrete means unique, that other states don t overlap it. 3. Electrons in the outer electron shells have greater potential energy.
30 Light Emission Answers and Solutions for Chapter 30 Reading Check Questions 1. At these high frequencies, ultraviolet light is emitted. 2. Discrete means unique, that other states don t overlap it.
More informationNatural Questions. About 2000 years ago Greek scientists were confused about motion. and developed a theory of motion
Natural Questions First natural question: Next question: What these things made of? Why and how things move? About 2000 years ago Greek scientists were confused about motion. Aristotle --- First to study
More informationLAB 3: SPECTROSCOPY. GEOL104: Exploring the Planets
LAB 3: SPECTROSCOPY OBJECTIVES: I. Review the basics of spectroscopy, including how to identify different materials on the basis of spectra. II. Develop an understanding of general spectroscopic features
More informationThe Main Point. How do light and matter interact? Lecture #7: Radiation and Spectra II. How is light absorbed and emitted?
Lecture #7: Radiation and Spectra II How is light absorbed and emitted? Models of Atomic Structure. Formation of Spectral Lines. Doppler Shift. Applications in Solar System Studies Detecting gaseous phases
More informationA Test For Length Contraction
Rothwell Bronrowan physbron@t-online.de The history of recent physics, by which I refer to the past 120 years give or take ten, has been deeply influenced by a theory separately proposed in the late 1880s
More informationAPAS Laboratory { PAGE } Spectroscopy SPECTROSCOPY
SPECTROSCOPY SYNOPSIS: In this lab you will eplore different types of emission spectra, calibrate a spectrometer using the spectrum of a known element, and use your calibration to identify an unknown element.
More informationCauses of Color in Minerals and Gemstones
,..4 Causes of Color in Minerals and Gemstones ;3 h Paul F. Hlava >&%/=J,F* %ndia National Laboratories < f $/42 Department 1822 $[pu. LO Mail Stop 1405 y z~o~ Albuquerque, NM 87185-1405 0 8~ P The colors
More informationBuild and Use a Simple Spectroscope
Build and Use a Simple Spectroscope Subject Area: Physical Sciences Grade Level: 9 12 Overview In this activity students will build a spectroscope to analyze the composition of light. Our scope is inexpensive,
More informationTelescopes (Chapter 6)
Telescopes (Chapter 6) Based on Chapter 6 This material will be useful for understanding Chapters 7 and 10 on Our planetary system and Jovian planet systems Chapter 5 on Light will be useful for understanding
More informationHomework #7: Properties of Galaxies in the Hubble Deep Field Name: Due: Friday, October points Profs. Rieke
Homework #7: Properties of Galaxies in the Hubble Deep Field Name: Due: Friday, October 31 30 points Profs. Rieke You are going to work with some famous astronomical data in this homework. The image data
More informationRemote Sensing/Reflectance Spectrometer
Remote Sensing/Reflectance Spectrometer REMOTE SENSING / REFLECTANCE SPECTROMETER TEACHER NOTES The remote sensing experiment is designed to take a full hour to complete, and can be undertaken using just
More informationBig Bang, Black Holes, No Math
ASTR/PHYS 109 Dr. David Toback Lecture 5 1 Prep For Today (is now due) L5 Reading: No new reading Unit 2 reading assigned at the end of class Pre-Lecture Reading Questions: Unit 1: Grades have been posted
More informationGALAXIES. Hello Mission Team members. Today our mission is to learn about galaxies.
GALAXIES Discussion Hello Mission Team members. Today our mission is to learn about galaxies. (Intro slide- 1) Galaxies span a vast range of properties, from dwarf galaxies with a few million stars barely
More informationLaboratory Atomic Emission Spectrum
Laboratory Atomic Emission Spectrum Pre-Lab Questions: Answer the following questions in complete sentences by reading through the Overview and Background sections below. 1. What is the purpose of the
More informationActive Gem Mining at the Cryo Genie Pegmatite Mine, southern California; Report #1, August 26, 2002 Jim Clanin, JC Mining
Active Gem Mining at the Cryo Genie Pegmatite Mine, southern California; Report #1, August 26, 2002 Jim Clanin, JC Mining Editor s note The following report from Jim Clanin (JC Mining, El Cajon, California)
More informationExperiment 7: Spectrum of the Hydrogen Atom
Experiment 7: Spectrum of the Hydrogen Nate Saffold nas2173@columbia.edu Office Hour: Mondays, 5:30-6:30PM INTRO TO EXPERIMENTAL PHYS-LAB 1493/1494/2699 Introduction The physics behind: The spectrum of
More informationNo Math. ASTR/PHYS 109 at. Texas A&M University November Big Bang, Black Holes, No Math ASTR/PHYS 109 at Texas A&M 1
Big Bang, Black Holes, No Math ASTR/PHYS 109 at Texas A&M David Toback Texas A&M University November 2009 ASTR/PHYS 109 at Texas A&M 1 Talk Outline Motivation, Intended Audience and Class Goals Course
More informationIntroduction to Archaeology: Notes 9 Chronology, part 2 Copyright Bruce Owen 2009 Trapped-charge dating methods Several different kinds, one basic
Introduction to Archaeology: Notes 9 Chronology, part 2 Copyright Bruce Owen 2009 Trapped-charge dating methods Several different kinds, one basic principle All measure the accumulated damage (displaced
More informationACCESS TO SCIENCE, ENGINEERING AND AGRICULTURE: MATHEMATICS 1 MATH00030 SEMESTER / Lines and Their Equations
ACCESS TO SCIENCE, ENGINEERING AND AGRICULTURE: MATHEMATICS 1 MATH00030 SEMESTER 1 017/018 DR. ANTHONY BROWN. Lines and Their Equations.1. Slope of a Line and its y-intercept. In Euclidean geometry (where
More informationMONTHLY OBSERVER S CHALLENGE
Introduction MONTHLY OBSERVER S CHALLENGE Compiled by: Roger Ivester, Boiling Springs, North Carolina & Fred Rayworth, Las Vegas, Nevada April 2009 The Virgo Cluster (Markharian s Chain) The purpose of
More informationGemstones, in particular rubies, Gemstones: Origin Determination
The Roots of Origin Determination The Gübelin Gem Lab Ltd, in Lucerne, Switzerland, is largely responsible for developing the science of origin determination in gemstones. Pioneered by the late Dr Eduard
More informationMARS PUBLIC MAPPING PROJECT (MP)2
KWL Prior Knowledge/Engagement Activity In your small group, brainstorm ideas about what you think you know about geologic features that may be found on Mars. Also include what questions you have about
More informationLab 10: Spectroscopy & the Hydrogen Atom Phy208 Fall 2008
Lab 10: Spectroscopy & the Hydrogen Atom Phy208 Fall 2008 Name Section This sheet is the lab document your TA will use to score your lab. It is to be turned in at the end of lab. To receive full credit
More informationPHYSICS 116 SPECTROSCOPY: DETERMINATION OF THE WAVELENGTH OF LIGHT
Name Date Lab Time Lab TA PHYSICS 116 SPECTROSCOPY: DETERMINATION OF THE WAVELENGTH OF LIGHT I. PURPOSE To use a diffraction grating to investigate the spectra produced by several unknown gas discharge
More informationEA Notes (Scen 101), Tillery Chapter 7. Light
EA Notes (Scen 101), Tillery Chapter 7 Light Introduction Light is hard to study because you can't see it, you only see it's effects. Newton tried to explain the energy in a light beam as the KE of a particle
More informationESS103A Igneous Petrology
Welcome to ESS103A Igneous Petrology Please pick up handouts Plan for today: Who are we? What is this class about? What is the structure of this course? How does the scientific method work? Who are we?
More informationThe Interstellar Medium (ch. 18)
The Interstellar Medium (ch. 18) The interstellar medium (ISM) is all the gas (and about 1% dust) that fills our Galaxy and others. It is the raw material from which stars form, and into which stars eject
More informationBeyond the Book. FOCUS Book
FOCUS Book A diamond is a kind of crystal that forms deep underground. Use simple materials to model how crystals form. Add sugar to a cup of water, a little bit at a time. Stir it each time you add sugar.
More informationPhysics Lab #2: Spectroscopy
Physics 10263 Lab #2: Spectroscopy Introduction This lab is meant to serve as an introduction to the science of spectroscopy. In this lab, we ll learn about how emission and absorption works, and we ll
More informationPhotographs of a Star Cluster. Spectra of a Star Cluster. What can we learn directly by analyzing the spectrum of a star? 4/1/09
Photographs of a Star Cluster Spectra of a Star Cluster What can we learn directly by analyzing the spectrum of a star? A star s chemical composition dips in the spectral curve of lines in the absorption
More informationOrbit: Nasa Astronauts Photograph The Earth By Michael & Wilkinson, Justin, Jay & HELFERT, APT READ ONLINE
Orbit: Nasa Astronauts Photograph The Earth By Michael & Wilkinson, Justin, Jay & HELFERT, APT READ ONLINE Orbit: NASA Astronauts Photograph the Earth Paperback October 1, 2003. Jay Apt (Author), Michael
More informationLight Quantum Hypothesis
50 My God, He Plays Dice! Light Quantum Hypothesis Light Quantum Hypothesis 51 Light Quantum Hypothesis In his miracle year of 1905, Einstein wrote four extraordinary papers, one of which won him the 1921
More informationNIST: Promoting U.S. Innovation and Industrial Competitiveness. George W. Arnold, Eng. Sc.D. Deputy Director, Technology Services
NIST: Promoting U.S. Innovation and Industrial Competitiveness George W. Arnold, Eng. Sc.D. Deputy Director, Technology Services NIST Today: Mission To promote U.S. innovation and industrial competitiveness
More informationPhysics 1CL OPTICAL SPECTROSCOPY Spring 2009
Introduction In this lab, you will use a diffraction grating to split up light into the various colors which make up the different wavelengths of the visible electromagnetic spectrum. You will assemble
More informationALTA Reflectance Spectrometer Activity: Mars Mystery Rocks
ALTA Reflectance Spectrometer Activity: Mars Mystery Rocks What is this activity about? Students learn to use the ALTA reflectance spectrometer to take reflectance measurements of Mars rocks at different
More informationLecture 2. In this lecture we will go through the chronological development of the Atomic physics.
Lecture 2 TITLE: A brief history of the development of structure of atom Page 1 Objectives In this lecture we will go through the chronological development of the Atomic physics. We will find out the thoughts
More informationMITOCW watch?v=byeau9ilhmw
MITOCW watch?v=byeau9ilhmw PROFESSOR: Last time, we spoke about photons in the context of an interferometer. The Mach-Zehnder interferometer. And we saw the very unusual properties of photons and interference,
More informationC. Incorrect! The velocity of electromagnetic waves in a vacuum is the same, 3.14 x 10 8 m/s.
AP Physics - Problem Drill 21: Physical Optics 1. Which of these statements is incorrect? Question 01 (A) Visible light is a small part of the electromagnetic spectrum. (B) An electromagnetic wave is a
More informationSpectroscopy - is the study of the interaction between matter and radiated energy.
Spectroscopy www.oakland.edu/?id=171 www.d.umn.edu/~mharvey/co www.spinoff.nasa.gov/spinoff201 www.aerodata-surveys.com/data_processin www.loke.as.arizona.edu/~ckulesa/camp/spectroscop www.rgbstock.com/photo/milvggk/color+model+%28
More informationDAY LABORATORY EXERCISE: SPECTROSCOPY
AS101 - Day Laboratory: Spectroscopy Page 1 DAY LABORATORY EXERCISE: SPECTROSCOPY Goals: To see light dispersed into its constituent colors To study how temperature, light intensity, and light color are
More informationSpectroscopy. Materials Diffraction grating Grating tube Spectrometer Incandescent light source
Name: Date: Spectroscopy Hazards: The power supply used to run the lights is HIGH VOLTAGE. You should not need to change any tubes, but if you do please call the instructor over for assistance, and turn
More informationMineralogy By John Sinkankas READ ONLINE
Mineralogy By John Sinkankas READ ONLINE If searched for a book Mineralogy by John Sinkankas in pdf format, in that case you come on to the loyal website. We furnish full variant of this book in txt, PDF,
More informationImage 1: Earth from space
Image 1: Earth from space Credit: NASA Spacecraft: Apollo 17 Sensor: camera using visible light Image date: December 7, 1972 This image is a photograph of Earth taken by Harrison "Jack" Schmitt, an astronaut
More informationExperiment 9. Emission Spectra. measure the emission spectrum of a source of light using the digital spectrometer.
Experiment 9 Emission Spectra 9.1 Objectives By the end of this experiment, you will be able to: measure the emission spectrum of a source of light using the digital spectrometer. find the wavelength of
More informationLight III The Atom & Spectra. February 12, 2012
Light III The Atom & Spectra February 12, 2012 Average: 65 20 Test 1 15 10 5 0 0-50 50-60 60-70 70-80 80-90 90-100 Takeaway Message: YOU NEED TO STUDY MORE you need to come to class EVERY DAY (TPS questions
More informationNaturally occurring means minerals are found and made in nature, not laboratories.
What are Minerals How important are minerals to you? Minerals are very important, actually. Almost everything you own and use was manufacture using as least some minerals. You own or encounter many things
More informationThe Early Church Acts 2:42-47; 4:32-37
Lesson 286 The Early Church Acts 2:42-47; 4:32-37 MEMORY VERSE ACTS 2:42 And they continued steadfastly in the apostles' doctrine and fellowship, in the breaking of bread, and in prayers. WHAT YOU WILL
More informationAdding and Subtracting Rational Expressions Interactive Math Notebook Activities and Scaffolded Notes
Adding and Subtracting Rational Epressions Interactive Math Notebook Activities and Scaffolded Notes Review: Simplifying Fractions What is a common denominator? Steps for Adding Fractions with a Common
More informationChapter 8. Spectroscopy. 8.1 Purpose. 8.2 Introduction
Chapter 8 Spectroscopy 8.1 Purpose In the experiment atomic spectra will be investigated. The spectra of three know materials will be observed. The composition of an unknown material will be determined.
More informationWhat is light? What is Light? Energy. Clearly, Light Can Be Described as a Wave 2/6/2013. The photoelectric effect
What is light? What is Light? The photoelectric effect Is there any evidence that light is a form of energy? Energy Can be carried as a waves (continuous) Can be carries by baseballs (discrete) Which is
More informationGrant Cameron: The Government's UFO Disclosure Plan
There has been a lot of discussion in the UFO community lately about disclosure. There has been so much, in fact, that many people don't want to hear the word anymore. The word disclosure has become almost
More informationMar 22, INSTRUCTIONS: First ll in your name and social security number (both by printing
ASTRONOMY 0089: EXAM 2 Class Meets M,W,F, 1:00 PM Mar 22, 1996 INSTRUCTIONS: First ll in your name and social security number (both by printing and by darkening the correct circles). Sign your answer sheet
More informationPreAP Chemistry. Unit 4 Atomic Structure, the Periodic Table, and Nuclear Radiation
PreAP Chemistry Unit 4 Atomic Structure, the Periodic Table, and Nuclear Radiation Democritus A Greek who lived ~400 BC, was the first to suggest the existence of atoms. He believed atoms to be indivisible
More informationPeople. The Shadow Shadow People. The Shadow People A Reading A Z Level O Leveled Book Word Count: 874 LEVELED BOOK O.
The Shadow People A Reading A Z Level O Leveled Book Word Count: 874 LEVELED BOOK O The Shadow Shadow The People People Written by Ann Weil Illustrated by Stephen Marchesi Visit www.readinga-z.com for
More informationIs evolution the great lie part 4?
Is evolution the great lie part 4? Organic evolution Organic evolution is the origin of life (evolution of non-living material) How did life get started? Here are some texts The history of life on earth
More informationBig Bang, Black Holes, No Math
ASTR/PHYS 109 Dr. David Toback Lectures 16 & 17 1 Was due Today L17 Reading: (BBBHNM Unit 2) Pre-Lecture Reading Questions: Let us know if you were misgraded on any submissions End-of-Chapter Quizzes:
More informationError Correcting Codes Prof. Dr. P. Vijay Kumar Department of Electrical Communication Engineering Indian Institute of Science, Bangalore
(Refer Slide Time: 00:15) Error Correcting Codes Prof. Dr. P. Vijay Kumar Department of Electrical Communication Engineering Indian Institute of Science, Bangalore Lecture No. # 03 Mathematical Preliminaries:
More informationSpectra of a Star Cluster. Photographs of a Star Cluster. What can we learn directly by analyzing the spectrum of a star? 4/1/09
Photographs of a Star Cluster Spectra of a Star Cluster What can we learn directly by analyzing the spectrum of a star? A star s chemical composition dips in the spectral curve of lines in the absorption
More informationPhysics 1CL OPTICAL SPECTROSCOPY Spring 2010
Introduction In this lab, you will use a diffraction grating to split up light into the various colors which make up the different wavelengths of the visible electromagnetic spectrum. You will assemble
More information