Thirty Years of Astronomy at Sussex
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Arthur S. Eddington the Nature of the Physical World
Arthur S. Eddington The Nature of the Physical World Arthur S. Eddington The Nature of the Physical World Gifford Lectures of 1927: An Annotated Edition Annotated and Introduced By H. G. Callaway Arthur S. Eddington, The Nature of the Physical World: Gifford Lectures of 1927: An Annotated Edition, by H. G. Callaway This book first published 2014 Cambridge Scholars Publishing 12 Back Chapman Street, Newcastle upon Tyne, NE6 2XX, UK British Library Cataloguing in Publication Data A catalogue record for this book is available from the British Library Copyright © 2014 by H. G. Callaway All rights for this book reserved. No part of this book may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior permission of the copyright owner. ISBN (10): 1-4438-6386-6, ISBN (13): 978-1-4438-6386-5 CONTENTS Note to the Text ............................................................................... vii Eddington’s Preface ......................................................................... ix A. S. Eddington, Physics and Philosophy .......................................xiii Eddington’s Introduction ................................................................... 1 Chapter I .......................................................................................... 11 The Downfall of Classical Physics Chapter II ......................................................................................... 31 Relativity Chapter III -
Graham Pointer Phd Thesis
THE MAGNETIC FIELD OF AB DORADÛS Graham Richard Pointer A Thesis Submitted for the Degree of PhD at the University of St Andrews 2001 Full metadata for this item is available in St Andrews Research Repository at: http://research-repository.st-andrews.ac.uk/ Please use this identifier to cite or link to this item: http://hdl.handle.net/10023/12940 This item is protected by original copyright THE UNIVERSITY OF ST. ANDREWS The Magnetic Field of AB Doradûs Graham Richard Pointer Submitted for the degree of Ph.D. May 2001 ProQuest Number: 10171062 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a com plete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. uest ProQuest 10171062 Published by ProQuest LLO (2017). Copyright of the Dissertation is held by the Author. All rights reserved. This work is protected against unauthorized copying under Title 17, United States C ode Microform Edition © ProQuest LLO. ProQuest LLO. 789 East Eisenhower Parkway P.Q. Box 1346 Ann Arbor, Ml 48106- 1346 DECLARATION I, Graham Richard Pointer, hereby declare that this thesis, which is approximately 50000 words in length, has been written by me, that it is the record of work carried out by me and that it has not been submitted in any previous application for a higher degree. I was admitted as a research student in September 1997 and as a candidate for the degree of Ph.D . -
Arxiv:1809.10688V2 [Astro-Ph.EP] 26 Jun 2019 Ing Nearby Bright Stars (Howell Et Al
Preprint typeset using LATEX style emulateapj v. 12/16/11 A DISCRETE SET OF POSSIBLE TRANSIT EPHEMERIDES FOR TWO LONG PERIOD GAS GIANTS ORBITING HIP 41378 Juliette C. Becker1, Andrew Vanderburg2;?, Joseph E. Rodriguez3, Mark Omohundro4, Fred C. Adams1;5, Keivan G. Stassun6;7, Xinyu Yao8, Joel Hartman9, Joshua Pepper8, Gaspar Bakos9, Geert Barentsen10, Thomas G. Beatty11, Waqas Bhatti8, Ashley Chontos12, Andrew Collier Cameron13, Coel Hellier14, Daniel Huber12, David James3, Rudolf B. Kuhn15, Michael B. Lund6, Don Pollacco16, Robert J. Siverd6, Daniel J. Stevens11;17;18, Jose´ Vin´ıcius de Miranda Cardoso19, Richard West16, 1Astronomy Department, University of Michigan, 1085 S University Avenue, Ann Arbor, MI 48109, USA 2Department of Astronomy, The University of Texas at Austin, Austin, TX 78712, USA 3Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138, USA 4Citizen Scientist 5Physics Department, University of Michigan, Ann Arbor, MI 48109, USA 6Department of Physics and Astronomy, Vanderbilt University, 6301 Stevenson Center, Nashville, TN:37235, USA 7Department of Physics, Fisk University, 1000 17th Avenue North, Nashville, TN:37208, USA 8Department of Physics, Lehigh University, 16 Memorial Drive East, Bethlehem, PA 18015, USA 9Department of Astrophysical Sciences, 4 Ivy Lane, Princeton University, Princeton, NJ 08544 10NASA Ames Research Center, Moffett Blvd, Mountain View, CA 94035, USA 11Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802 -
EPSC2018-1115-2, 2018 European Planetary Science Congress 2018 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2018
EPSC Abstracts Vol. 12, EPSC2018-1115-2, 2018 European Planetary Science Congress 2018 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2018 Ultra-short Period Rocky Super-Earths Luca Malavolta (1,2) , Andrew W. Mayo (3,4) , Tom Louden (5) , Vinesh M. Rajpaul (6) , Aldo S. Bonomo (7) , Lars A. Buchhave (4) , Laura Kreidberg (3,8) , Martti H. Kristiansen (9,10), Mercedes Lopez-Morales (3) , Annelies Mortier (11) , Andrew Vanderburg (3,12) , Adrien Coffinet (13), David Ehrenreich (13) , Christophe Lovis (13), Francois Bouchy (13), David Charbonneau (3) , David R. Ciardi (14), Andrew Collier Cameron (11) , Rosario Cosentino (15), Ian J. M. Crossfield (16,17), Mario Damasso (7) , Courtney D. Dressing (18) , Xavier Dumusque(13) , Mark E. Everett (19) , Pedro Figueira (20), Aldo F. M. Fiorenzano (15), Erica J. Gonzales (16,28), Raphaëlle D. Haywood (3,27) , Avet Harutyunyan (15), Lea Hirsch (18) , Steve B. Howell (21) , John Asher Johnson (3) , David W. Latham (3) , Eric Lopez (22), Michel Mayor (13), Giusi Micela (23), Emilio Molinari (15,24) , Valerio Nascimbeni (1,2) , Francesco Pepe (13), David F. Phillips (3) , Giampaolo Piotto (1,2) , Ken Rice (25), Dimitar Sasselov (3) , Damien Ségransan (13) , Alessandro Sozzetti (7) , Stéphane Udry (13), and Chris Watson (26) (1) Dipartimento di Fisica e Astronomia “Galileo Galilei,” Università di Padova, Italy ([email protected]) (2) INAF— Osservatorio Astronomico di Padova, Italy (3) Harvard-Smithsonian Center for Astrophysics, USA (4) Centre for Star and Planet Formation, Denmark (5) Department -
Raphaëlle D. Haywood Phd Thesis
HIDE AND SEEK: RADIAL-VELOCITY SEARCHES FOR PLANETS AROUND ACTIVE STARS Raphaëlle D. Haywood A Thesis Submitted for the Degree of PhD at the University of St Andrews 2015 Full metadata for this item is available in Research@StAndrews:FullText at: http://research-repository.st-andrews.ac.uk/ Please use this identifier to cite or link to this item: http://hdl.handle.net/10023/7798 This item is protected by original copyright This item is licensed under a Creative Commons Licence Hide and seek Radial-Velocity Searches For Planets Around Active Stars by Rapha¨elleD. Haywood Accepted for the degree of Doctor of Philosophy in Astrophysics 3 September 2015 Declaration I, Rapha¨elleD. Haywood, hereby certify that this thesis, which is approximately 33,000 words in length, has been written by me, that it is the record of work carried out by me and that it has not been submitted in any previous application for a higher degree. Date Signature of candidate I was admitted as a research student in September 2011 and as a candidate for the degree of PhD in September 2015; the higher study for which this is a record was carried out in the University of St Andrews between 2011 and 2015. Date Signature of candidate I hereby certify that the candidate has fulfilled the conditions of the Resolution and Regulations appropriate for the degree of PhD in the University of St Andrews and that the candidate is qualified to submit this thesis in application for that degree. Date Signature of supervisor i Copyright Agreement In submitting this thesis to the University of St Andrews we understand that we are giving permission for it to be made available for use in accordance with the regula- tions of the University Library for the time being in force, subject to any copyright vested in the work not being affected thereby. -
An Additional Non-Transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets
The Astronomical Journal, 154:122 (17pp), 2017 September https://doi.org/10.3847/1538-3881/aa832d © 2017. The American Astronomical Society. All rights reserved. Three’s Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets Jessie L. Christiansen1 , Andrew Vanderburg2 , Jennifer Burt3 , B. J. Fulton4,5 , Konstantin Batygin6, Björn Benneke6, John M. Brewer7 , David Charbonneau2 , David R. Ciardi1, Andrew Collier Cameron8, Jeffrey L. Coughlin9,10 , Ian J. M. Crossfield11,32, Courtney Dressing6,32 , Thomas P. Greene9 , Andrew W. Howard5 , David W. Latham2 , Emilio Molinari12,13 , Annelies Mortier8 , Fergal Mullally10, Francesco Pepe14, Ken Rice15, Evan Sinukoff4,5 , Alessandro Sozzetti16 , Susan E. Thompson9,10 , Stéphane Udry14, Steven S. Vogt17 , Travis S. Barman18 , Natasha E. Batalha19 , François Bouchy14, Lars A. Buchhave20 , R. Paul Butler21 , Rosario Cosentino13, Trent J. Dupuy22 , David Ehrenreich14 , Aldo Fiorenzano13, Brad M. S. Hansen23, Thomas Henning24, Lea Hirsch25 , Bradford P. Holden17 , Howard T. Isaacson25 , John A. Johnson2, Heather A. Knutson6, Molly Kosiarek11 , Mercedes López-Morales2, Christophe Lovis14, Luca Malavolta26,27 , Michel Mayor14, Giuseppina Micela28, Fatemeh Motalebi14, Erik Petigura6 , David F. Phillips2, Giampaolo Piotto26,27 , Leslie A. Rogers29 , Dimitar Sasselov2 , Joshua E. Schlieder33 , Damien Ségransan14, Christopher A. Watson30, and Lauren M. Weiss31,34 1 NASA Exoplanet Science Institute, California Institute of Technology, M/S 100-22, 770 -
Cosmical Magnetism NATO ASI Series Advanced Science Institutes Series
Cosmical Magnetism NATO ASI Series Advanced Science Institutes Series A Series presenting the results of activities sponsored by the NATO Science Committee, which aims at the dissemination of advanced scientific and technological knowledge, with a view to strengthening links between scientific communities. The Series is published by an international board of publishers in conjunction with the NATO Scientific Affairs Division A Life Sciences Plenum Publishing Corporation B Physics London and New York C Mathematical Kluwer Academic Publishers and Physical Sciences Dordrecht, Boston and London D Behavioural and Social Sciences E Applied Sciences F Computer and Systems Sciences Springer-Verlag G Ecological Sciences Berlin, Heidelberg, New York, London, H Cell Biology Paris and Tokyo I Global Environmental Change NATO-PCO-DATA BASE The electronic index to the NATO ASI Series provides full bibliographical references (with keywords and/or abstracts) to more than 30000 contributions from international scientists published in all sections of the NATO ASI Series. Access to the NATO-PCO-DATA BASE is possible in two ways: - via online FILE 128 (NATO-PCO-DATA BASE) hosted by ESRIN, Via Galileo Galilei, 1-00044 Frascati, Italy. - via CD-ROM "NATO-PCO-DATA BASE" with user-friendly retrieval software in English, French and German (© WTV GmbH and DATAWARE Technologies Inc. 1989). The CD-ROM can be ordered through any member of the Board of Publishers or through NATO-PCO, Overijse, Belgium. Series C: Mathematical and Physical Sciences - Vol. 422 Cosmical Magnetism edited by D. Lynden-Bell Institute of Astronomy & Clare College, Cambridge, U.K. Springer Science+Business Media, B.V. Proceedings of the NATO Advanced Research Workshop on Cosmlcal Magnetlsm Cambridge, U.K. -
Augmentation of Uk Space Debris Observing Capabilities Using University Optical Telescopes
AUGMENTATION OF UK SPACE DEBRIS OBSERVING CAPABILITIES USING UNIVERSITY OPTICAL TELESCOPES Philip Herridge(1), David Brown(2), Richard Crowther(3) (1) Space Insight Limited, P.O. Box 2993, Eastbourne, East Sussex, BN21 9BD, UK. Email: [email protected] (2) School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife, KY16 9SS, UK. Email: [email protected] (3) UK Space Agency, Polaris House, North Star Avenue, Swindon, Wiltshire, SN2 1SZ, UK. Email: [email protected] ABSTRACT The study of space debris requires a range of different sensors. Debris population monitoring requires survey, follow-on and characterisation capable sensors. In order to fully participate in space debris measurement the range of sensors available to the UK Space Agency needs to be augmented with additional capability. One source of untapped resource resides within the UK university sector. This paper discusses investigation into extending the optical sensor diversity available to the UK for participation in study of the debris environment through a collaboration between Space Insight Limited, a commercial company providing Space Situational Figure 1. Chilbolton Awareness (SSA) services to the UK Space Agency, and Observatory 25 m radar antenna the Astronomy Group at the University of St Andrews. +LJKO\ HOOLSWLFDO RUELW REMHFWV PD\ EHQH¿W IURP D 1 INTRODUCTION fusion of radar observations near perigee and optical observations near apogee, but their orbits may mean that The space resident population of man-made objects perigee or apogee occurs where there is sparse sensor occupies a wide range of differing orbits each coverage. -
Donald Lynden-Bell (1935–2018)
RETROSPECTIVE RETROSPECTIVE Donald Lynden-Bell (1935–2018) Martin J. Reesa,1 Donald Lynden-Bell was lucky in his heredity and his film-maker, Alison Rose, accompanied them and created environment. His great-grandfather knew the famous a movie called Star Men,inwhichtheprotagonists(all astronomer John Herschel. His father, an army Colo- elderly) reminisced about life, the universe, and every- nel, inherited a telescope and introduced Donald to thing. Donald, a keen mountaineer in his youth, enjoyed the wonders of the sky. At his school, Marlborough making this movie and spoke at several special showings. College, Donald was exceedingly well taught. He came But the most important event for Donald in his up to Clare College to read mathematics. In his second postdoctorate years was his marriage to Ruth in 1961. year, he was supervised by the great physicist Abdus She moved to California to finish her chemistry doctor- Salam, who advised him to divert for a year to study ate, but they both returned to Cambridge in 1962. physics, which Donald did before returning to mathe- Donald then became an assistant lecturer in matics for his fourth year. He thereby had a superb mathematics and a Fellow of Clare College. I attended launching-pad for research. his course on statistical mechanics. It was one of his Donald’s doctoral supervisor was Leon Mestel, a favorite subjects and he gave spirited performances. world expert on cosmic magnetism. But Donald found But Donald felt his teaching obligations didn’t leave Leon’sproblems“too intractable,” so instead he began to enough time for research, so he soon moved to the forge his lifetime interest in stel- Royal Observatory at Herstmonceux in Sussex. -
Lecture Notes in Physics
Lecture Notes in Physics Editorial Board R. Beig, Wien, Austria W. Beiglböck, Heidelberg, Germany W. Domcke, Garching, Germany B.-G. Englert, Singapore U. Frisch, Nice, France P. Hänggi, Augsburg, Germany G. Hasinger, Garching, Germany K. Hepp, Zürich, Switzerland W. Hillebrandt, Garching, Germany D. Imboden, Zürich, Switzerland R. L. Jaffe, Cambridge, MA, USA R. Lipowsky, Golm, Germany H. v. Löhneysen, Karlsruhe, Germany I. Ojima, Kyoto, Japan D. Sornette, Nice, France, and Los Angeles, CA, USA S. Theisen, Golm, Germany W. Weise, Garching, Germany J. Wess, München, Germany J. Zittartz, Köln, Germany The Lecture Notes in Physics The series Lecture Notes in Physics (LNP), founded in 1969, reports new developments in physics research and teaching – quickly and informally, but with a high quality and the explicit aim to summarize and communicate current knowledge in an accessible way. Books published in this series are conceived as bridging material between advanced grad- uate textbooks and the forefront of research to serve the following purposes: • to be a compact and modern up-to-date source of reference on a well-defined topic; • to serve as an accessible introduction to the field to postgraduate students and nonspe- cialist researchers from related areas; • to be a source of advanced teaching material for specialized seminars, courses and schools. Both monographs and multi-author volumes will be considered for publication. Edited volumes should, however, consist of a very limited number of contributions only. Pro- ceedings will not be considered for LNP. Volumes published in LNP are disseminated both in print and in electronic formats, the electronic archive is available at springerlink.com. -
The Rossiter–Mclaughlin Effect in Exoplanet Research
The Rossiter–McLaughlin effect in Exoplanet Research Amaury H.M.J. Triaud Abstract The Rossiter–McLaughlin effect occurs during a planet’s transit. It pro- vides the main means of measuring the sky-projected spin–orbit angle between a planet’s orbital plane, and its host star’s equatorial plane. Observing the Rossiter– McLaughlin effect is now a near routine procedure. It is an important element in the orbital characterisation of transiting exoplanets. Measurements of the spin–orbit an- gle have revealed a surprising diversity, far from the placid, Kantian and Laplacian ideals, whereby planets form, and remain, on orbital planes coincident with their star’s equator. This chapter will review a short history of the Rossiter–McLaughlin effect, how it is modelled, and will summarise the current state of the field before de- scribing other uses for a spectroscopic transit, and alternative methods of measuring the spin–orbit angle. Introduction The Rossiter–McLaughlin effect is the detection of a planetary transit using spec- troscopy. It appears as an anomalous radial-velocity variation happening over the Doppler reflex motion that an orbiting planet imparts on its rotating host star (Fig.1). The shape of the Rossiter–McLaughlin effect contains information about the ratio of the sizes between the planet and its host star, the rotational speed of the star, the impact parameter and the angle l (historically called b, where b = −l), which is the sky-projected spin–orbit angle. The Rossiter–McLaughlin effect was first reported for an exoplanet, in the case of HD 209458 b, by Queloz et al.(2000). -
Donald Lynden-Bell (1935–2018)
RETROSPECTIVE RETROSPECTIVE Donald Lynden-Bell (1935–2018) Martin J. Reesa,1 Donald Lynden-Bell was lucky in his heredity and his film-maker, Alison Rose, accompanied them and created environment. His great-grandfather knew the famous a movie called Star Men,inwhichtheprotagonists(all astronomer John Herschel. His father, an army Colo- elderly) reminisced about life, the universe, and every- nel, inherited a telescope and introduced Donald to thing. Donald, a keen mountaineer in his youth, enjoyed the wonders of the sky. At his school, Marlborough making this movie and spoke at several special showings. College, Donald was exceedingly well taught. He came But the most important event for Donald in his up to Clare College to read mathematics. In his second postdoctorate years was his marriage to Ruth in 1961. year, he was supervised by the great physicist Abdus She moved to California to finish her chemistry doctor- Salam, who advised him to divert for a year to study ate, but they both returned to Cambridge in 1962. physics, which Donald did before returning to mathe- Donald then became an assistant lecturer in matics for his fourth year. He thereby had a superb mathematics and a Fellow of Clare College. I attended launching-pad for research. his course on statistical mechanics. It was one of his Donald’s doctoral supervisor was Leon Mestel, a favorite subjects and he gave spirited performances. world expert on cosmic magnetism. But Donald found But Donald felt his teaching obligations didn’t leave Leon’sproblems“too intractable,” so instead he began to enough time for research, so he soon moved to the forge his lifetime interest in stel- Royal Observatory at Herstmonceux in Sussex.