ASTRONOMY AND ASTROPHYSICS LIBRARY SeriesEditors: I.Appenzeller,Heidelberg,Germany G.Bo¨rner,Garching,Germany A.Burkert,Mu¨nchen,Germany M.A.Dopita,Canberra,Australia A.Eckart,Köln,Germany T.Encrenaz,Meudon,France M.Harwit,Washington,DC,USA R.Kippenhahn,Go¨ttingen,Germany J.Lequeux,Paris,France A.Maeder,Sauverny,Switzerland V.Trimble,CollegePark,MD,andIrvine,CA,USA Gerhard Beutler Methods of Celestial Mechanics Volume II: Application to Planetary System, Geodynamics and Satellite Geodesy In Cooperation with Prof. Leos Mervart and Dr. Andreas Verdun With266FiguresIncluding14ColorFigures, 28TablesandaCD-ROM 123 ProfessorDr.GerhardBeutler Universita¨tBern AstronomischesInstitut Sidlerstrasse5 3012Bern,Switzerland e-mail:[email protected] Coverpicture: OppolzermotionoftheEarth’srotationpole,generatedbyprogramsystem"CelestialMechanics" LibraryofCongressControlNumber:2004105868 ISSN0941-7834 ISBN3-540-40750-2SpringerBerlinHeidelbergNewYork Thisworkissubjecttocopyright.Allrightsarereserved,whetherthewholeorpartofthematerialisconcerned, specificallytherightsoftranslation,reprinting,reuseofillustrations,recitation,broadcasting,reproductiononmi- crofilmorinanyotherway,andstorageindatabanks.Duplicationofthispublicationorpartsthereofispermitted onlyundertheprovisionsoftheGermanCopyrightLawofSeptember9,1965,initscurrentversion,andpermission forusemustalwaysbeobtainedfromSpringer.ViolationsareliabletoprosecutionundertheGermanCopyrightLaw. 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It consists of Part II: Applications and Part III: ProgramSystem. PartIIfocusesonapplicationsofastrodynamics.Thedevelopmentsarebased on lecture notes about Celestial Mechanics of the planetary system and of artificial satellites, and about the rotation of Earth and Moon. The lectures were intended for diploma students of astronomy,physics,mathematics,and geography at the University of Bern in their first three academic years. In view of the broad and inhomogeneous audience, the lectures had to be self- consistent and based on simple, generally known physical and mathematical facts and concepts. Earthrotation(Chapter2),satellitemotion(Chapter3)andthedevelopment oftheplanetarysystem(Chapter4)aretheconstituentsofPartII.Thethree chapters should be viewed as applications of the theoreticaldevelopments in Chapter I-3. It is recommended to briefly review the corresponding sections ofthisintroductorychapterbeforestudyingoneofthethreeapplicationchap- ters. Volume I also should be consulted whenever subtleties of the equations of motion are in the focus of interest. The mathematical foundations of the developments in this second Volume are (of course) those of Volume I. It should be nevertheless possible to get a good overview of the three applica- tionsofastrodynamicswithoutconsultingVolumeItoooften–providedone is ready to accept the underlying equations of motion and the mathematical tools used as known (“black boxes”). Part III gives an overview of the program system accompanying and illus- trating this work. The algorithms are those developed in Chapter I-7. The programsystemismeanttoillustratethemathematicalconcepts,butalsoto introduce the three central topics rotation of Earth and Moon, satellite mo- tion, and evolution of the planetary system. The three programs ERDROT, SATORB and PLASYS are, from the design point of view, key elements for a thorough understanding of the three topics. They are in particular helpful to develop a proper understanding of the order of magnitude of the effects considered. VIII Preface of VolumeII This Volume is accompanied by a Compact Disk (CD) containing the com- puter programs as executable modules for Personal Computers (PC). The program system is easy to install and to use on PCs with a Windows oper- ating system. Prof.LeoˇsMervartofthe TechnicalUniversityofPraguedesignedandwrote the menu system accompanying the computer programs. It is in essence his merit that the computer-programsare easy to understand and to use. My colleague and co-workerDr. Andreas Verdun was the design expert con- cerningthestructureandtheformalappearanceofthiswork.Inaddition,his collaboration was paramount in all aspects related to his specialization, the history of astronomy, in particular of Celestial Mechanics. He screened and proof-read the entire manuscript. His expertise and never ending encourage- ment was of greatest importance for the realization and completion of this work. Thisworknevercouldhavebeencompletedwithouttheassistanceofthetwo young colleagues. Their contribution is acknowledged with deep gratitude. Prof. Paul Wild, my predecessoras director of the AstronomicalInstitute of the University of Bern (AIUB), contributed in many respects to this book. PaulWildadaptedhisfabulousskilltoscreenSchmidt-platesfornewobjects (minor planets, comets, supernovae, etc.) to the manuscript of this book by performing an amazingly thorough proof-reading of major parts of the manuscript. The final result is undoubtedly very much improved thanks to his effort. Chapter 2 (rotation of Earth and Moon) was proof-read by Claudia Urschl, Chapter 3 (satellite motion) by Michael Meindl. The two young colleagues arePh.D.-candidatesatourinstitute.Dr.ThomasSchildknechtreviewedthe chapter 4 (planetary system). Dr. Urs Hugentobler received his diploma in theoretical physics, then joined the CCD group and wrote a Ph.D. thesis in the field of astrometry and Celestial Mechanics. After a longer research stay at ESOC in Darmstadt, he joined the AIUB team as head of AIUB GPS researchgroup. With his broad backgroundand his sharp mind he was perfectly suited to proof-readthe entire Part II of this work. Profs. Robert Weber from the Technical University of Vienna, Markus Rothacherfromthe TechnicalUniversityofMunich, andProf.WernerGurt- ner,directoroftheZimmerwaldObservatory,alsoreadandcommentedmajor partsofthemanuscript.Dr.JanKoubafromtheNationalGeodeticSurveyof CanadathoroughlyreadthemajorpartofPartII.Thecommentsbythefour distinguished colleagues are very much appreciated. A final proof-reading of the entire manuscriptwas performed by Ms Edith St¨ovekenand Ms Claudia Urschl. The editing and reviewing process of a treatise of this extent is a crucial aspect, at times even a nightmare. The reviewing work was a considerable Preface of VolumeII IX addition to the normalprofessionalduties of the colleaguesmentioned above and to those of the author. It is my sincere desire to thank my friends and colleagues for their assistance. I can only promise to assist them in a similar way, should they decide to achieve something similar. I cannot recommend this to anybody, onthe other hand: My sabbaticalleave from the University of Bern in spring and summer 2001 and the following two years were in essence sacrificed to the purpose of writing and completing this two volume work. The author hopes that the two volumes will be helpful to and stimulating for students and researchers – which in turn would help him to forget the “(blood), sweat and tears” accompanying the creative act. Bern, February 2004 Gerhard Beutler
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