Inventing Temperature General Editor: Paul Hnmnhrf'vs
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Cavendish Weighs the Earth, 1797
CAVENDISH WEIGHS THE EARTH Newton's law of gravitation tells us that any two bodies attract each other{not just the Earth and an apple, or the Earth and the Moon, but also two apples! We don't feel the attraction between two apples if we hold one in each hand, as we do the attraction of two magnets, but according to Newton's law, the two apples should attract each other. If that is really true, it might perhaps be possible to directly observe the force of attraction between two objects in a laboratory. The \great moment" when that was done came on August 5, 1797, in a garden shed in suburban London. The experimenter was Lord Henry Cavendish. Cavendish had inherited a fortune, and was therefore free to follow his inclinations, which turned out to be scientific. In addition to the famous experiment described here, he was also the discoverer of “inflammable air", now known as hydrogen. In those days, science in England was often pursued by private citizens of means, who communicated through the Royal Society. Although Cavendish studied at Cambridge for three years, the universities were not yet centers of scientific research. Let us turn now to a calculation. How much should the force of gravity between two apples actually amount to? Since the attraction between two objects is proportional to the product of their masses, the attraction between the apples should be the weight of an apple times the ratio of the mass of an apple to the mass of the Earth. The weight of an apple is, according to Newton, the force of attraction between the apple and the Earth: GMm W = R2 where G is the \gravitational constant", M the mass of the Earth, m the mass of an apple, and R the radius of the Earth. -
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Cronfa - Swansea University Open Access Repository _____________________________________________________________ This is an author produced version of a paper published in: Transactions of the Honourable Society of Cymmrodorion Cronfa URL for this paper: http://cronfa.swan.ac.uk/Record/cronfa40899 _____________________________________________________________ Paper: Tucker, J. Richard Price and the History of Science. Transactions of the Honourable Society of Cymmrodorion, 23, 69- 86. _____________________________________________________________ This item is brought to you by Swansea University. Any person downloading material is agreeing to abide by the terms of the repository licence. Copies of full text items may be used or reproduced in any format or medium, without prior permission for personal research or study, educational or non-commercial purposes only. The copyright for any work remains with the original author unless otherwise specified. The full-text must not be sold in any format or medium without the formal permission of the copyright holder. Permission for multiple reproductions should be obtained from the original author. Authors are personally responsible for adhering to copyright and publisher restrictions when uploading content to the repository. http://www.swansea.ac.uk/library/researchsupport/ris-support/ 69 RICHARD PRICE AND THE HISTORY OF SCIENCE John V. Tucker Abstract Richard Price (1723–1791) was born in south Wales and practised as a minister of religion in London. He was also a keen scientist who wrote extensively about mathematics, astronomy, and electricity, and was elected a Fellow of the Royal Society. Written in support of a national history of science for Wales, this article explores the legacy of Richard Price and his considerable contribution to science and the intellectual history of Wales. -
Cavendish the Experimental Life
Cavendish The Experimental Life Revised Second Edition Max Planck Research Library for the History and Development of Knowledge Series Editors Ian T. Baldwin, Gerd Graßhoff, Jürgen Renn, Dagmar Schäfer, Robert Schlögl, Bernard F. Schutz Edition Open Access Development Team Lindy Divarci, Georg Pflanz, Klaus Thoden, Dirk Wintergrün. The Edition Open Access (EOA) platform was founded to bring together publi- cation initiatives seeking to disseminate the results of scholarly work in a format that combines traditional publications with the digital medium. It currently hosts the open-access publications of the “Max Planck Research Library for the History and Development of Knowledge” (MPRL) and “Edition Open Sources” (EOS). EOA is open to host other open access initiatives similar in conception and spirit, in accordance with the Berlin Declaration on Open Access to Knowledge in the sciences and humanities, which was launched by the Max Planck Society in 2003. By combining the advantages of traditional publications and the digital medium, the platform offers a new way of publishing research and of studying historical topics or current issues in relation to primary materials that are otherwise not easily available. The volumes are available both as printed books and as online open access publications. They are directed at scholars and students of various disciplines, and at a broader public interested in how science shapes our world. Cavendish The Experimental Life Revised Second Edition Christa Jungnickel and Russell McCormmach Studies 7 Studies 7 Communicated by Jed Z. Buchwald Editorial Team: Lindy Divarci, Georg Pflanz, Bendix Düker, Caroline Frank, Beatrice Hermann, Beatrice Hilke Image Processing: Digitization Group of the Max Planck Institute for the History of Science Cover Image: Chemical Laboratory. -
MODULE 11: GLOSSARY and CONVERSIONS Cell Engines
Hydrogen Fuel MODULE 11: GLOSSARY AND CONVERSIONS Cell Engines CONTENTS 11.1 GLOSSARY.......................................................................................................... 11-1 11.2 MEASUREMENT SYSTEMS .................................................................................. 11-31 11.3 CONVERSION TABLE .......................................................................................... 11-33 Hydrogen Fuel Cell Engines and Related Technologies: Rev 0, December 2001 Hydrogen Fuel MODULE 11: GLOSSARY AND CONVERSIONS Cell Engines OBJECTIVES This module is for reference only. Hydrogen Fuel Cell Engines and Related Technologies: Rev 0, December 2001 PAGE 11-1 Hydrogen Fuel Cell Engines MODULE 11: GLOSSARY AND CONVERSIONS 11.1 Glossary This glossary covers words, phrases, and acronyms that are used with fuel cell engines and hydrogen fueled vehicles. Some words may have different meanings when used in other contexts. There are variations in the use of periods and capitalization for abbrevia- tions, acronyms and standard measures. The terms in this glossary are pre- sented without periods. ABNORMAL COMBUSTION – Combustion in which knock, pre-ignition, run- on or surface ignition occurs; combustion that does not proceed in the nor- mal way (where the flame front is initiated by the spark and proceeds throughout the combustion chamber smoothly and without detonation). ABSOLUTE PRESSURE – Pressure shown on the pressure gauge plus at- mospheric pressure (psia). At sea level atmospheric pressure is 14.7 psia. Use absolute pressure in compressor calculations and when using the ideal gas law. See also psi and psig. ABSOLUTE TEMPERATURE – Temperature scale with absolute zero as the zero of the scale. In standard, the absolute temperature is the temperature in ºF plus 460, or in metric it is the temperature in ºC plus 273. Absolute zero is referred to as Rankine or r, and in metric as Kelvin or K. -
The Kelvin and Temperature Measurements
Volume 106, Number 1, January–February 2001 Journal of Research of the National Institute of Standards and Technology [J. Res. Natl. Inst. Stand. Technol. 106, 105–149 (2001)] The Kelvin and Temperature Measurements Volume 106 Number 1 January–February 2001 B. W. Mangum, G. T. Furukawa, The International Temperature Scale of are available to the thermometry commu- K. G. Kreider, C. W. Meyer, D. C. 1990 (ITS-90) is defined from 0.65 K nity are described. Part II of the paper Ripple, G. F. Strouse, W. L. Tew, upwards to the highest temperature measur- describes the realization of temperature able by spectral radiation thermometry, above 1234.93 K for which the ITS-90 is M. R. Moldover, B. Carol Johnson, the radiation thermometry being based on defined in terms of the calibration of spec- H. W. Yoon, C. E. Gibson, and the Planck radiation law. When it was troradiometers using reference blackbody R. D. Saunders developed, the ITS-90 represented thermo- sources that are at the temperature of the dynamic temperatures as closely as pos- equilibrium liquid-solid phase transition National Institute of Standards and sible. Part I of this paper describes the real- of pure silver, gold, or copper. The realiza- Technology, ization of contact thermometry up to tion of temperature from absolute spec- 1234.93 K, the temperature range in which tral or total radiometry over the tempera- Gaithersburg, MD 20899-0001 the ITS-90 is defined in terms of calibra- ture range from about 60 K to 3000 K is [email protected] tion of thermometers at 15 fixed points and also described. -
Henry Cavendish Outline
Ann Karimbabai Massihi Sveti Patel Sandy Saekoh Thomas Choe Chemistry 480 Dr. Harold Goldwhite Henry Cavendish I. Childhood A. Henry Cavendish was born in Nice, France, on 10 October1731, and died alone on 24 February 1810. B. His parental grandfather was Duke of Devonshire and his maternal grandfather was Duke of Kent 1 C. His parents were English aristocrats. D. His father was Lord Charles Cavendish, a member of Royal Society in London and an experimental scientist. E. His father made his own scientific equipment for him. II. Education A. At age of 11, he attended Dr. Newcome’s Academy in Hackney, London from 1749-1753. B. In 1749, he went to Peterhouse College. C. He left the college at 1753 without a degree. D. His father encouraged his scientific interest and introduced him to the Royal Society and he became a member in 1760. III. Papers A. Since he did his scientific investigation for his pleasure, he was careless in publishing the results. B. In 1776, he published his 1st paper about the existence of hydrogen as a substance. 1. He received the Copley Medal of the Royal Society for this achievement. C. In 1771, a theoretical study of electricity. D. In 1784, the synthesis of water. E. In 1798, the determination of the gravitational constant. IV. Experiments A. Fixed air (CO2) produced by mixing acids and bases. B. “Inflammable air” (hydrogen) generated by the action of acid on metals. 2 Figure 1. Cavendish's apparatus for making and collecting hydrogen Gas bladder used by Henry Cavendish 3 C. -
Section 1 – Oxygen: the Gas That Changed Everything
MYSTERY OF MATTER: SEARCH FOR THE ELEMENTS 1. Oxygen: The Gas that Changed Everything CHAPTER 1: What is the World Made Of? Alignment with the NRC’s National Science Education Standards B: Physical Science Structure and Properties of Matter: An element is composed of a single type of atom. G: History and Nature of Science Nature of Scientific Knowledge Because all scientific ideas depend on experimental and observational confirmation, all scientific knowledge is, in principle, subject to change as new evidence becomes available. … In situations where information is still fragmentary, it is normal for scientific ideas to be incomplete, but this is also where the opportunity for making advances may be greatest. Alignment with the Next Generation Science Standards Science and Engineering Practices 1. Asking Questions and Defining Problems Ask questions that arise from examining models or a theory, to clarify and/or seek additional information and relationships. Re-enactment: In a dank alchemist's laboratory, a white-bearded man works amidst a clutter of Notes from the Field: vessels, bellows and furnaces. I used this section of the program to introduce my students to the concept of atoms. It’s a NARR: One night in 1669, a German alchemist named Hennig Brandt was searching, as he did more concrete way to get into the atomic every night, for a way to make gold. theory. Brandt lifts a flask of yellow liquid and inspects it. Notes from the Field: Humor is a great way to engage my students. NARR: For some time, Brandt had focused his research on urine. He was certain the Even though they might find a scientist "golden stream" held the key. -
The Conservatives in British Government and the Search for a Social Policy 1918-1923
71-22,488 HOGAN, Neil William, 1936- THE CONSERVATIVES IN BRITISH GOVERNMENT AND THE SEARCH FOR A SOCIAL POLICY 1918-1923. The Ohio State University, Ph.D., 1971 History, modern University Microfilms, A XEROX Company, Ann Arbor, Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED THE CONSERVATIVES IN BRITISH GOVERNMENT AND THE SEARCH FOR A SOCIAL POLICY 1918-1923 DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of the Ohio State University By Neil William Hogan, B.S.S., M.A. ***** The Ohio State University 1971 Approved by I AdvAdviser iser Department of History PREFACE I would like to acknowledge my thanks to Mr. Geoffrey D.M. Block, M.B.E. and Mrs. Critch of the Conservative Research Centre for the use of Conservative Party material; A.J.P. Taylor of the Beaverbrook Library for his encouragement and helpful suggestions and his efficient and courteous librarian, Mr. Iago. In addition, I wish to thank the staffs of the British Museum, Public Record Office, West Sussex Record Office, and the University of Birmingham Library for their aid. To my adviser, Professor Phillip P. Poirier, a special acknowledgement#for his suggestions and criticisms were always useful and wise. I also want to thank my mother who helped in the typing and most of all my wife, Janet, who typed and proofread the paper and gave so much encouragement in the whole project. VITA July 27, 1936 . Bom, Cleveland, Ohio 1958 .......... B.S.S., John Carroll University Cleveland, Ohio 1959 - 1965 .... U. -
Modern Outlook on the Concept of Temperature Edward Bormashenko Chemical Engineering Department, Engineering Faculty, Ariel University, P.O.B
What Is the Temperature? Modern Outlook on the Concept of Temperature Edward Bormashenko Chemical Engineering Department, Engineering Faculty, Ariel University, P.O.B. 3, 407000 Ariel, Israel ORCID id 0000-0003-1356-2486 Abstract The meaning and evolution of the notion of “temperature” (which is a key concept for the condensed and gaseous matter theories) is addressed from the different points of view. The concept of temperature turns out to be much more fundamental than it is conventionally thought. In particular, the temperature may be introduced for the systems built of “small” number of particles and particles in rest. The Kelvin temperature scale may be introduced into the quantum and relativistic physics due to the fact, that the efficiency of the quantum and relativistic Carnot cycles coincides with that of the classical one. The relation of the temperature to the metrics of the configurational space describing the behavior of system built from non-interacting particles is demonstrated. The Landauer principle asserts that the temperature of the system is the only physical value defining the energy cost of isothermal erasing of the single bit of information. The role of the temperature the cosmic microwave background in the modern cosmology is discussed. Keywords: temperature; quantum Carnot engine; relativistic Carnot cycle; metrics of the configurational space; Landauer principle. 1. Introduction What is the temperature? Intuitively the notions of “cold” and “hot” precede the scientific terms “heat” and “temperature”. Titus Lucretius Carus noted in De rerum natura that “warmth” and “cold” are invisible and this makes these concepts difficult for understanding [1]. The scientific study of heat started with the invention of thermometer [2]. -
Constructive Empiricism in the Social Sciences
Constructive empiricism in the social sciences Abstract ‘What problems face the aspirant empiricist today?’ is the question Bas C. van Fraassen asks in his seminal work The Scientific Image (1980). In this thesis, I interpret this question as a challenge to develop constructive empiricism [CE] in a field of scientific inquiry other than the context of physics in which it was conceived. The first part of the thesis expounds CE with reference to classical empiricism, discloses some of its fundamental assumptions, and spells out in detail its account of science. In the second part of the thesis, CE is extended to social science. Since CE was developed in the context of natural science, I take an articulation of the alleged fundamental differences between natural and social science as indicating challenges a CE-outlook on social science must address. I also provide a brief history of the gap between the sciences. Then, in the bulk of this thesis, I argue that CE’s model view accommodates social science, that description, prediction and explanation in the light of CE are proper fruits of inquiry in social science, and that CE is able to make sense of the differences in the concepts used in natural and social science. In the discussion of the feasibility of CE for social science, I show concurrently that contemporary articulations of the differences between the natural and the social sciences pose no insuperable problems for the constructive empiricist. Bram van Dijk | 3691454 History & Philosophy of Science | Utrecht University Daily supervisors | dr. Guido Bacciagaluppi & dr. Ruud Abma Third examiner | dr. -
1. Temperature and the Ideal Gas Law (Note: This Is a Fairly Long Experiment
Physics 341 Chapter 1 Page 1-1 1. Temperature and the Ideal Gas Law (Note: This is a fairly long experiment. To save time, much of the graphing can be done “at home”. As always, make sure that you have all the data you need before you leave.) 1.1 Introduction The most important concept at the foundation of thermodynamics is that of thermal equilibrium. We take this for granted in our daily experiences. We know, for instance, that an ice cube will melt when taken out of the freezer – no matter what object “at room temperature” it is brought into contact with. This is the essence of the utility of temperature and thermal equilibrium: the direction of heat flow is independent of the substance involved - it depends on only temperature. In fact, this defines temperature. More precise observations of thermal equilibrium are as follows. First of all, as with the equally familiar notion of mechanical equilibrium, we may say that an isolated macroscopic system is in thermal equilibrium, or thermodynamic equilibrium, whenever it attains a state that is not observed to change with time, at least at a macroscopic level. Obviously, for such a situation to occur, it is also necessary that the system in question is in (internal) mechanical and chemical equilibrium. At the foundations of thermodynamics is the experimental fact that two systems in thermal equilibrium with a third system must also be in thermal equilibrium with each other. This is often referred to as the zeroth law of thermodynamics. It is what leads to the empirical notion of a temperature scale. -
Class – 9 Chemistry
Class – 9 Chemistry The common unit of Temperature :- The common unit of measuring temperature is degree Celsius which is written in short form as°C. There is another scale of temperature called Kelvin scale of temperature the SI unit of measuring temperature is Kelvin it is denoted by the symbol K . 0°C = 273 K The relation between Kelvin scale and Celsius scale of temperature can be written as Temperature of Kelvin scale = Temperature of Celsius scale+273 Example 1. convert the temperature of 25 °Cto the Kelvin scale. Solution :- Temperature on Kelvin scale = Temperature on Celsius scale + 273 =25+273 =298K Thus a temperature of 25 degree Celsius on Celsius scale is equal to 298 Kelvin on the Kelvin scale. Example 2 . Convert the temperature of 300 Kelvin to the Celsius scale. Solution. we know that temperature on Kelvin scale =Temperature on Celsius scale + 273 so , 300 = temperature on Celsius scale + 273 and , temperature on Celsius scale = 300 – 273 =27 degree Celsius Thus a temperature of 300 Kelvin on Kelvin scale is equal to 27 degree Celsius on Celsius scale. Note. It is clear from the above discussion that: 1. To convert a temperature on Celsius scale to the Kelvin scale we have to add 273 to the Celsius temperature. 2. and the convert a temperature on Kelvin scale to the Celsius scale we have to subtract 273 from the Kelvin temperature. Temperature is measured in Fahrenheit also. People in USA used the Fahrenheit degree while Indians use the Celsius degree. So we need to find out the exact temperature on means, if he says that he is at 100° F.