1 SISFA (Società Italiana degli Storici della Fisica e dell'astronomia) F. Bònoli[*], M. Calisi[**], P. Ranfagni[***] CLASSIFICATION CRITERIA FOR HISTORICAL ASTRONOMICAL INSTRUMENTATION 1. Introduction The interest towards inventorying scientific instruments has largely grown in the last half century and different national inventories have been carried out, most of them under the patronage of the Scientific Instrument Commission of the International Union of the History and Philosophy of Science (the former Commission pour l'inventaire Mondial des Appareils Scientifiques d'intérêt Historique de l'union Internationale d'histoire et de Philosophie des Sciences). The last inventory, which was undertaken in 1967 and finished in 1992, was performed by the British National Committee for the History of Science, Technology and Medicine. 1 An early inventory of instruments in Italy was made by the Museo Nazionale della Scienza e della Tecnica Leonardo da Vinci in , following the suggestions made by Henry Michel in and A few years ago the Italian Consiglio Nazionale delle Ricerche (CNR) supported a project proposed by the Commissione per la Storia dell'astronomia of the Società Astronomica Italiana (SAIt) in order to catalogue the historical astronomical instruments belonging to the Italian astronomical institutions. All these inventories are in paper form, but the development of computers and international networks suggests a fast growing of computerized databases. In fact, today is already possible to have a virtual look at objects from a large number of Museums, collections and exhibits. The on-line availability of a vast number of inventories gives great importance to the possibility, for scholars aiming to search for particular objects or groups of objects, to obtain undoubted, complete and, above all, without losing any item, answers to their queries to the databases. Hence the opportunity to use the same names for the same objects, i.e. the well known, but not completely resolved, problem of "vocabulary control". Here we intend to present the approach used towards this problem - with regard to historical astronomical instrumentation - and the criteria that guided us in defining a proposal for a scheme of classification, derived from previous experiences gained in different instruments cataloguing. Having in mind those experiences we agree that a precise classification of the objects to be catalogued is needed for two main purposes: * to give the the possibility of working interactively with the catalogue; * to have an efficient data retrieval system both for the curator in charge of inserting data in the database, and for the scientist interested in obtaining data from the database 2. The classification criteria Let us start with a few examples of the above mentioned problems. Figure 1 shows five different instruments which can be found in astronomical collections. Objects of the same kind of those shown are classified in different inventories using names which can vary from horizontal plate to horizontal circle, miner's dial, miner's compass, len's dial, Holland circle, surveying circle, graphometer, circumferentor, theodolite and even astrolabe. For instance, the name "astrolabe" for objects like the upper-left one is clearly wrong: the object is a circumferentor and the suggestion it could be an astrolabe merely derives from its shape. The term "theodolite" for some of the objects is not wrong, but it could not be always correct. Scholars who would like to authomatically search for astrolabes or for theodolites will obtain, from their query, objects which do not belong to the requested category. In the contrary, the search for circumferentors will lose the object shown and classified as "astrolabe". Many different examples of this kind could be presented, just in order to emphasize the problem of the "subject classification" or, as we called it before, of the "vocabulary control". More confusion, of course, can derive working with inventories written in different languages. These difficulties could be resolved by the definition of an "authority list" for historical objects in astronomical collections, but: who defines the authority list? In the course of time a lot of people engaged themselves in this hard work. Leaving out the XVIII-century Encyclopédie by Diderot and d'alembert, one can obtain some aids by more modern dictionaries, subject headings, thesauri and so on, as, e.g..: * Art and Architecture Thesaurus * Library of Congress Subject Headings * Subject Headings for Graphic Materials * The Revised Nomenclature for Museum Cataloging 1
2 * Social History and Industrial Classification * McGraw-Hill Dictionary of Scientific and Technical Terms as well as more specifical nomenclatures, most of which are quoted in the References. Nevertheless, in this respect, David Bearman, editor of Archives and Museum Informatics, remembers that: "In a critique of controlled vocabularies for subject retrieval, which I wrote several years ago (American Archivist, vol. 52, no. 3, 1989), I presumed that appropriate terminology existed in a controlled list somewhere.... What I did not consider was what to do when no vocabularies accurately describe the concept we want to represent.... It is obvious that if we have to adopt terms that distort the meaning of the objects we are describing, any benefits with respect to information retrieval, such as improved precision, that could accrue from control of terminology are a hardly an advantage.... At least I'll never again assume that a vocabulary for a given domain of description actually has the terms required to describe that domain." 5 Being these preliminary remarks and warnings, the solution of the "authority list" problem must derive from a different approach and the following example, in our opinion, can explain Figure 1 - The instruments shown are from: M. Holbrook, Science Preserved. A directory of scientific instruments in collections in the United Kingdom and Eire, HMSO (London, 1992). the approach we used. Figure 2 shows a splendid instrument made by Arnoldus Scherpenselensis in 1595 for Giovanni Antonio Magini, teacher of Astronomy at Bologna University. It could be classified as "quadrant", "astronomical quadrant", "astrolabe quadrant", "surveyor's quadrant", "Magini's quadrant" - following the use, sometimes misleading, of classifying objects with the name of the craftsman, of the owner or of the user - or, which is clearly uncorrect, merely "astrolabe". In any way, asking the database for "quadrant", one can obtain all the objects of this kind, leaving out the last uncorrect classification. Having in mind the many activities made by the former owner, this example can help us. Magini, as we said, was teacher of Astronomy, but he was also envolved in geography, topography, sailing problems and calculus. His instrument can be used to solve problems in all these fields, both as an "angle measuring instrument" and as a "computing instrument". Hence the suggestion not to use the "supposed object name" in classifying objects, but to subdivide them according to their "type of use". As a consequence, all the instruments shown in figure 1 - anyhow the curator could have been named them: horizontal plates, miner's or len's dials or compasses, Holland's or surveying or horizontal circles, graphometers, circumferentors, theodolites, astrolabes and so on - can easily be recognized in every database by scholars querying simply for: "angle measuring instruments". Moreover, "angle measuring instruments" are used in different fields of science, as the Magini's quadrant example suggests. As a consequence, a different approach in classifying scientific artifacts is to distinguish between the different applications the same instrument could have had inside each section of science, instead of try to identify a name which could be recognized by every researcher all around the world, without any mistake. 3. The classification The previously discussed points, i.e. the "type of use" and the "kind of specialization" of historical instruments - together with the presence, for astronomical objects, of few entries, with very few horizontal associated relations, the vast majority of which are hierarchical - suggested us the use of an "indexed hierarchical classification". Organizing the classification we followed in principle the criteria defined by the above mentioned Commission pour l'inventaire Mondial des Appareils Scientifiques d'intérêt Historique, with the later suggestions by M. Calisi 6. We defined a hierarchical classification of each instrument divided in three main levels: "section", "type" and "object". Starting from the division of science into the 27 categories defined by the Commission, we selected the first 15 categories and added the section Geology and Geophysics, not previously defined, thus obtaining 16 "sections" in which the instruments could be classified according to the main field of science for which the instrument was designed and realized by the maker, i.e. Mathematics, Navigation, Astronomy, Optics and so on. Table 1 shows the 16 sections. 2
3 After that, we divided the instruments in "types", according to the particular application and specialization of use inside every section of science. As a consequence we have, for instance, in the section Mathematics the types "drawing instruments", "analog measuring instruments and computing machines", "digital computers" and "models". In the section Astronomy we have the types "astrometric instruments", "refracting telescopes", "reflecting telescopes", "solar telescopes", "eyepieces", "micrometers", "focal plane photographic instruments" and so on. Table 2 shows the sections and the lower level subdivions in types. Figure 2 - Quadrant made "Per Arnoldum Scherpenselensem, Anno 1595, Bononiae" for "Io: Antonius Maginus, in Exm. Gymnasio Mathematicarum Professor". Giovanni Antonio Magini ( ) held the chair of Astronomy in Bologna University from 1588 to Among the candidates for the chair vacated by Ignatio Danti was the 23 year-old Galilei. The Bolognese Senate, however, went for the older and better known Giovanni Antonio Magini from Padua. (Courtesy of Gunnar Pipping, National Museum of Science and Technology, Stockholm) Finally, at the third level of classification there are "objects". First of all it is important to define the so called "catalographic unit", bearing in mind that the instrument to be classified must be an autonomous unit worth of being catalogued. A telescope supplied with a given lens, a given eyepiece and a given mounting is an object to be classified, for instance, as a "refracting telescope with achromatic object glass, galilean optical system, in equatorial German mounting", whereas a micrometer built to be used at various telescopes must be catalogued independently like, for instance, a "heliometer". The choice between cataloguing different single objects as part of a "complex object" or as different "simple objects" depends on the knowledge of the history of the instrument itself and of its use and applications. In particular, in experimental physics and chemistry many examples of experiments made using a lot of instruments can be found. Usually objects and not experiments are catalogued, unless the historical importance of the overall apparatus is wider than that of its single parts. At this level of classification the curator in charge of cataloguing instruments could be completely free of inserting the "supposed name" of the object. Anyway, we tried to identify most of the historical instruments one can usually find in the astronomical institutions, without claiming any level of completeness, but bearing in mind to suggest a preliminary list of objects and preferred nomenclature just as a cataloguing help. In a preliminary presentation of our proposal 7,8 we reported the whole suggested list of ~ 400 objects we identified as autonomous units to be catalogued inside the subdivision in types and sections, following our experience and referring to international catalogues and inventories We do not report here the suggested list of "objects" with the index relative to the various types and sections in which the object could be classified with regard to the main type and/or section for which the instrument was intended or in which the instrument was used. This is made both for space reasons and, above all, for stressing the main criteria which guided us in the definition of the "indexed hierarchical classification". Table 3 reports, exempli gratia, the subdivision in sections, types and objects only for a few types of section 6 "Astronomy". Table 4 lists the same objects from table 3 alphabetically. Together with every object we report the index relative to the various types and sections in which the object could be classified with regard to the main type and/or section for which the instrument was intended or in which the instrument was used. A quadrant, for instance, could have been built or used as an "angle measuring instrument" in the section Topography and Geodesy, or as a "celestial body altitude measuring instrument" in the section Navigation, or, finally, as an "astrometric instrument" in Astronomy. It is the cataloguer's responsibility to decide the main section in which the instrument should be classified, based on a good knowledge of the instrument's history. The use of a glossary which defines terms would permit a "free vocabulary", whereas the use of hierarchic descriptors and subject headings suggests a "controlled vocabulary": clearly the difference between the two choices is a basic one and a lot of literature is available. Our aim, many times previously stated, is not to give a contribution to this kind of discussion (even if we prefer, of course, a controlled vocabulary), but a help to classify scientific artifacts. We have not the presumption to solve all problems presented, but we "tried to avoid" them defining a logical tree and subdividing instruments in Types. In fact, the hierarchical scheme "Section, Type, Object" forms the carrier axis of the suggested classification and, in our opinion, foresees the above widely discussed problems: * giving a particular importance to the subdivision in "types", according to the technological and usage purposes of the historical astronomical artifacts in the various disciplines, * leaving the possibility of assigning more classification indexes to the same instrument, classifying it in different types (being different its uses), * suggesting (if requested) an 'object authority file' or leaving the cataloguer free to use what he thinks to be the 'correct name' of the instrument to be classified. We want to stress the importance of the fact that the definition of types has not been induced by a collation of objects, but has 3
4 been deduced from the analysis of the technological and usage purposes in the various disciplines. As a consequence, the cataloguer must classify the object from both a historical and technological point of view, using all the relative knowledge in his possession. In fact, a precise instrument is to be classified and not a generic one: the classifier must (or should) know the main purposes that instrument was used for, or for which was built and, as a consequence, assign it to that particular Section and Type. In this way one has the possibility to "mark the history" of that instrument, assigning it to a defined Section and to a defined Type, and extracting from the data base only the instruments used or realized for that Section or all the instruments having the same usage characteristics classified. It depends on the scientist's purposes. It is our opinion that the cataloguer and the scientist interested in information retrieval could not be completely dark about the "object" they are classifying or they are looking for. For instance, cataloguing or searching for a "compass", one has to know if he is looking for "an instrument for indicating a horizontal reference direction relative to the earth" (e.g. in our classification: section Navigation, type Compasses) or for "an instrument used for describing arcs or circles with pencil or pen" (e.g.: section Mathematics, type Drawing instruments). Being these differences not known to the cataloguer and to the scientist, it is not clear how to help both of them unless giving a descriptive "fiche" and a photo for each "object". Not knowing the "correct name" of the object, one can classify it without assigning a name, just putting it inside a type or even, in the most hopeless case, only inside a section. Not knowing the name nor the kind of use nor the field of science in which the instrument could have been used... there is no hope for a solution. The suggested classification is intended for the historical instruments in the astronomical collections. Bearing in mind all the non-astronomical instruments used in a certain section of discipline, and our poor knowledge of disciplines different from astronomy, our list is naturally incomplete. Paying attentiont to which kind of collection and/or museum we are dealing with, i.e. "general", "semi-specialized", "specialized", our case is, of course, the third one. Nevertheless, the use of hierarchical descriptors leaves this kind of classification extremely flexible and easily expansible to "general" and "semi-specialized" collections. Adding a Section (e.g. Medicine or Chemistry) to our suggested list, and creating a hierarchical classification inside the section itself, based on the same criteria, more indexes can simply be added to those we defined. A hiearchical description can be specialized exploding one Section or one Type. Therefore, our hope is that curators and scholars, analyzing the above defined criteria which guided us in the hierarchical scheme of the classification, will contribute to improve our work by pointing out mistakes, new or revised types, new objects and synonyms, or by applying our criteria to the classification of historical instruments in more fields of science. Acknowledgements The authors would like to thank all those who have helped during the work and all the colleagues partecipating in the CNR project Strumentaria Astronomica, coordinated by E. Proverbio. Special thanks for helpful suggestions go to W.J.H. Andrewes of the Science Center, Harvard University, Cambridge; A. Brachner of the Deutsches Museum, München; Randall C. Brooks of the National Museum of Science and Technology, Ottawa; D.J. Bryden and H.C. McCorry of the Royal Museum of Scotland, Edinburgh; S. Débarbat of the Observatoire de Paris; A. McConnell; Derek A. Robinson of the Science Museum, London; J. Wetton of the Museum of Science & Industry, Manchester; S. Pilloni of the Osservatorio Astronomico, Cagliari; and S. Spinelli and M. Zuccoli respectively of the Dipartimento di Italianistica and Dipartimento di Astronomia of the University of Bologna. Table 1: Sections 1. MATHEMATICS 2. METROLOGY 3. TOPOGRAPHY AND GEODESY 4. GEOGRAPHY 5. NAVIGATION 6. ASTRONOMY 7. METEOROLOGY 8. GNOMONICS 9. CHRONOMETRY 10. MECHANICS 11. OPTICS 12. ACOUSTICS 13. TERMOPHYSICS 14. ATOMIC PHYSICS 15. ELECTRICITY AND MAGNETISM 16. GEOLOGY AND GEOPHYSICS Table 2: Sections and Types 1. MATHEMATICS 1. Drawing instruments 2. Analog measuring instruments and computing machines 3. Digital computers 4. Models 2. METROLOGY 1. Lenght measuring instruments 2. Mass and/or weight measuring instruments 3. Volume measuring instruments 4. Comparators 3. TOPOGRAPHY AND GEODESY 4
5 1. Direct distance measuring instruments 2. Aligning instruments 3. Angle measuring instruments 4. Drawing instruments 5. Measuring and computing instruments 6. Instruments for photographic surveys 7. Models 4. GEOGRAPHY 1. Terrestrial globes 2. Maps and atlases 3. Mapping instruments 5. NAVIGATION 1. Charts and portolanos 2. Plotting instruments 3. Compasses 4. Celestial body altitude measuring instruments 5. Hourglasses 6. Chronometers 7. Instruments for hydrometric measures 8. Ship's telescopes and binoculars 9. Models 6. ASTRONOMY 1. Astrometric instruments 2. Refracting telescopes 3. Reflecting telescopes 4. Solar telescopes 5. Eyepieces 6. Micrometers 7. Filters 8. Focal plane photographic instruments 9. Stellar photometers and bolometers 10. Solar photometers and bolometers 11. Stellar spectrometers 12. Solar spectrometers 13. Polarimeters 14. Radiotelescopes and detectors 15. Gamma-ray, X-ray and Infrared radiation detectors and telescopes 16. Photographic observations reduction instruments 17. Photoelectric observations reduction instruments 18. Celestial and planetary globes 19. Sky maps, planetary maps, atlases, celestial phenomena representations, calendars 20. Celestial and/or planetary representation instruments 21. Domes 22. Slide rules or machines for astronomical reductions 23. Furniture 24. Models 7. METEOROLOGY 1. Temperature measuring instruments 2. Atmospheric pressure measuring instruments 3. Atmospheric umidity measuring instruments 4. Wind measuring instruments 5. Rainfall measuring instruments 6. Atmospheric electricity measuring instruments 7. Sunshine recorders and solar radiation measuring instruments 8. Weather stations 9. Furniture 8. GNOMONICS 1. Meridian lines 2. Fixed sundials 3. Portable sundials 9. CHRONOMETRY 1. Hourglasses and water clocks 2. Mechanical weight-driven clocks 3. Mechanical spring-driven clocks 4. Electrically-driven clocks 5. Atomic and molecular clocks 6. Time signal receivers and chronographs 5
6 10. MECHANICS 1. Mechanical phenomena studying and measuring instruments 2. Materials processing machines 3. Engines and pumps 4. Models 11. OPTICS 1. Optical benches, supports, fittings 2. Lenses, mirrors and eyepieces 3. Prisms, gratings, polarizers and filters 4. Laboratory photometers, spectrometers and polarimeters 5. Sources 6. Photographic cameras and darkroom equipments 7. Optical projection systems 8. Camerae obscurae and camerae lucidae 9. Refractometric measuring instruments 10. Spherometric measuring instruments 11. Microscopes 12. Interferometers 13. Models 12. ACOUSTICS 1. Acoustic phenomena studying and measuring instruments 2. Sound reproducers 3. Models 13. TERMOPHYSICS 1. Thermal radiation measuring devices 2. Heat quantities measuring devices 14. ATOMIC PHYSICS 1. Particle sources 2. Particle detectors 3. Models 15. ELECTRICITY AND MAGNETISM 1. Magnetic and electric phenomena studying and measuring instruments 2. Laboratory instruments 3. Electronic or electrotechnical components 4. Models 16. GEOLOGY AND GEOPHYSICS 1. Instruments for seismic surveys 2. Terrestrial gravitation measuring instruments 3. Instruments for measuring the deviation from the vertical line 4. Electric and magnetic terrestrial phenomena measuring instruments 5. Instruments for hydrometric and hydrographic measures Table 3: Example of the subdivision in Types and Objects, for Section 6 'Astronomy': Types ASTRONOMY 1. Astrometric instruments 1. astrolabe 2. cross-staff also Jacob's staff 3. baculus also arbaletum 4. diopter 1. Hipparchus' diopter 5. nocturnal 6. altitude quadrant 7. astronomical ring 8. triquetrum also Ptolemy's ruler also parallactic ruler 9. torquetum also turquet 10. movable astronomical quadrant 11. ring dial also armilla 1. equatorial ring dial 2. zodiacal ring dial 3. universal equinoctial ring dial 12. meridian circle 13. repeating circle 14. theodolite 1. circumferentor 2. repeating circle 6
7 15. astronomical compendium 16. octant 17. mural quadrant 18. mural semicircle 19. transit telescope 20. zenith telescope 21. parallactic telescope 2. Refracting telescopes 1. astrograph 2. Baker-Nunn camera 3. hand held telescope 1. astronomical telescope also Keplerian telescope 2. Galilean telescope also terrestrial telescope 4. refracting telescope 1. with non achromatic object glass 2. with achromatic object glass - the following divisions are not associated to the last entry, but they are hierarchical combinations of all the preceding entries - 1. with astronomical optical system also with Keplerian optical system 2. with Galilean optical system also with terrestrial optical system 1. in aerial mounting 2. in altazimuth mounting 3. in ecliptic mounting 4. in zenith mounting 5. in equatorial 1. English mounting 2. German mounting 3. fork mounting 3. Reflecting telescopes 1. reflecting telescope 1. with spherical mirror 2. with parabolic mirror 3. with hyperbolic mirror 4. multi-mirror telescope 5. Schmidt telescope also Schmidt camera 6. Ritchey-Chrétien telescope - the following divisions are not associated to the last entry, but they are hierarchical combinations of all the preceding entries - 1. with primary focus 2. with Cassegrain focus 3. with Newtonian focus 4. with Gregorian focus 5. multi-focus 1. in herschelian mounting 2. in altazimuth mounting 3. in equatorial 1. English mounting 2. German mounting 3. fork mounting 4. yoke mounting Table 4: Example of the list of objects, which appear in section 6 'Astronomy' (types 1-3), alphabetically, and indexes related to sections and types arbaletum... use baculus armilla... use ring dial astrograph astrolabe eclipse computing astrolabe Danjon's astrolabe... use impersonal astrolabe impersonal astrolabe also prismatic astrolabe also Danjon's astrolabe mariner's astrolabe pendulum astrolabe prismatic astrolabe... use impersonal astrolabe astronomical compendium astronomical ring Baker-Nunn camera backstaff also Davis's quadrant baculus also arbaletum cross-staff also Jacob's staff diopter Hipparchus' diopter Jacob's staff... use cross-staff meridian circle
8 mural semicircle octant parallactic ruler... use triquetrum Ptolemy's ruler... use triquetrum quadrant sinical quadrant altitude quadrant Davis's quadrant... use backstaff mariner's quadrant movable astronomical quadrant mural quadrant nocturnal repeating circle ring dial equatorial ring dial universal equinoctial ring dial zodiacal ring dial telescope, hand held astronomical telescope also Keplerian telescope Galilean telescope also terrestrial telescope Keplerian telescope... use astronomical telescope ship's telescope terrestrial telescope... use Galilean telescope telescope, parallactic telescope, reflecting the following divisions are not associated to the last entry, but they are hierarchical combinations of all the preceding entries, therefore only indexes subsequent to the first one (6.3.1) are reported here - with spherical mirror with parabolic mirror with hyperbolic mirror multi-mirror telescope Schmidt telescope also Schmidt camera Ritchey-Chrétien telescope with primary focus with Cassegrain focus with Newtonian focus with Gregorian focus multi-focus in herschelian mounting....1 in altazimuth mounting....2 in equatorial English mounting....1 German mounting....2 fork mounting....3 yoke mounting....4 telescope, refracting the following divisions are not associated to the last entry, but they are hierarchical combinations of all the preceding entries, therefore only indexes subsequent to the first one (6.2.4) are reported here - with non achromatic object glass with achromatic object glass with astronomical optical system also with Keplerian optical system with Galilean optical system also with terrestrial optical system in aerial mounting in altazimuth mounting in ecliptic mounting in zenith mounting in equatorial English mounting....1 German mounting....2 fork mounting....3 telescope, zenith theodolite circumferentor repeating thedolite torquetum also turquet transit telescope triquetrum also Ptolemy's ruler also parallactic ruler turquet... use torquetum References 1. M. Holbrook, Science preserved. A directory of scientific instruments in collections in the United Kingdom and Eire (London, 1992). 8
9 2. Union internationale d'histoire et philosophie des sciences. Division d'histoire des sciences. Commission pour l'inventaire mondial des appareil scientifiques d'intérêt historique. Inventaire des instruments conservés en Italie, five volumes, Museo Nazionale della Scienza e della Tecnica Leonardo da Vinci Milan ( ). 3. H. Michel, "Note sur l'inventaire mondial des instruments scientifique d'intérêt historique", Archives internationales d'historie des sciences, xi (1958), Centre national d'histoire des sciences. Inventaire des instruments scientifiques historiques conservés en Belgique, two parts (Brussel, 1959, 1960). 5. D. Bearman, Vocabulary Control, Archives and Museum Informatics, vol. 7, no 4, p. 6, (1993) 6. M. Calisi, Catalogazione della strumentazione storico-scientifica esistente nell'osservatorio Astronomico di Roma, Museologia Scientifica, viii (1991), F. Bònoli, M. Calisi, E. Proverbio, P. Ranfagni, Una proposta di classificazione della strumentaria storica astronomica, in "Atti del Seminario sui problemi del recupero e della valorizzazione del patrimonio strumentale, archivistico e bibliografico di interesse storico degli Osservatori Astronomici e Astrofisici Italiani", Società Astronomica Italiana, p. 9 (1994) 8. S. Pilloni, P. Ranfagni, M. Calisi, F. Bònoli, Progetto di informatizzazione delle schede catalografiche degli strumenti di interesse storico degli Osservatori Astronomici Italiani, in "Atti del Seminario sui problemi del recupero e della valorizzazione del patrimonio strumentale, archivistico e bibliografico di interesse storico degli Osservatori Astronomici e Astrofisici Italiani", Società Astronomica Italiana, p. 51 (1994) 9. R.G.W. Anderson, J.A. Bennett, W.F. Ryan (Edts), Making Instruments Count, Variorum Collected Studies Series (Aldershot, 1993) 10. E. Baiada, F. Bònoli, A. Braccesi, Museo della Specola. Catalogo, Bologna University Press (1995). 11. J.A. Bennett, The Divided Circle, Phaidon Christie's (Oxford, 1987). 12. J.A. Bennett, From Pleasure and Profit to Science and Security. Etienne Lenoir and the transformation of precision instrument-making in France: , The Whipple Museum of the History of Science (Cambridge, 1989). 13. N. Bion, Traité de la construction et des principaux usages des instruments de mathématique (La Haye, IV ed. Jonbert e Nion, 1752). 14. G. Boffito, Gli strumenti della scienza e la scienza degli strumenti, L.G.Seeber (Florence, 1929). 15. R.C. Brooks, The development of micrometers in the seventeenth, eighteenth and nineteenth centuries, Journal Hist. Astron., XXIII, p. 146 (1991). 16. M. Calisi, Guida alla visita del Museo Astronomico e Copernicano di Roma, Osservatorio Astronomico di Monte Mario Ed. (Rome, 1991). 17. A. Chapman, Dividing the Circle, Ellis Orwood Limited (Chichester, 1988). 18. M. Daumas, Les instruments scientifiques aux XVIIe et XVIIIe siecles, Presses Universitaires de France (Paris, 1953) 19. D.J. de Solla Price, Clockwork before the clock (1955). 20. D. Diderot, J-B. le Rond d'alembert, Encyclopédie ou dictionnaire raisonné des sciences, des arts et des métiers. Recueil de planches, sur les sciences, les artes libéraux, et les arts méchaniques, avec leur explication. Third edition (Livorno 1750). 21. E. Engberts, Descriptive Catalogue of Telescopes, Communication No. 138 from the a.m. Museum (Leiden, 1970). 22. Ephemerides Societatis Meteorologicae Palatinae. Annorum (Mannheim, ). 23. G. Ferrari, Tromometri, avvisatori, sismografi: osservazioni e teorie dal 1850 al 1880, SGA Storia-Geofisica-Ambiente Ed. (Bologna, 1991). 24. M. Fiorini, Sfere terrestri e celesti di autore italiano, oppure fatte e conservate in Italia, Società Geografica Italiana (Rome, 1899). 25. S. Gibbs, G. Saliba, Planispheric Astrolabes from the National Museum of American History, Smithsonian Institution Press (City of Washington, 1984). 26. K. Higgins, The Classification of Sundials, Annals of Science, Vol.9, No. 4 (1953). 27. M. Holbrook, Science Preserved. A directory of scientific instruments in collections in the United Kingdom and Eire, HMSO (London, 1992). 28. An Inventory of the Navigation and Astronomy collections in the National Maritime Museum Greenwich, Department of 9
10 Navigation, Department of Astronomy, National Maritime Museum, Greenwich (London, ). 29. D.A. King, Strumentazione astronomica nel mondo islamico, in Storia delle Scienze: Vol. I - Gli strumenti, Einaudi, (1991) p H.C. King, The History of the Telescope, Charles Griffin & Co. Ltd. (London, 1955). 31. McGraw-Hill Dictionary of Scientific and Technical Terms (New York, 1978). 32. J.R. Millburn, Misurazione del tempo in Storia delle Scienze: Vol. I - Gli strumenti, Einaudi (1991) pp M. Miniati (a cura di), Catalogo del Museo di Storia della Scienza di Firenze, Giunti (Florence, 1991). 34. H. Minow, Historische Vermessungsinstrumente, Verlag Chmielorz GmbH (Wiesbaden, 1990). 35. E. Miotto, G. Tagliaferri, P. Tucci, La strumentazione nella storia dell'osservatorio Astronomico di Brera, Edizioni Unicopli (Milan, 1990). 36. J.A. Repsold, Zur Geschichte der Astronomischen Messwerkzeuge von Purbach bis Reichenbach, 1450 bis 1830, Verlag von Wilhelm Engelmann (Leipzig, 1908). 37. J.A. Repsold, Zur Geschichte der Astronomischen Messwerkzeuge, von 1830 bis um 1900, Verlag von Emmanuel Reinicke (Leipzig, 1914). 38. E.L. Stevenson, Terrestrial and Celestial Globes (New York, 1921). 39. A.J.Turner, Le Citoyen Lenoir. Scientific instrument making in revolutionary France, The Whipple Museum of the History of Science (Cambridge, 1989). 40. A.J. Turner ed., Time (The Hague, 1990). 41. G. L'E. Turner, Antique Scientific Instruments, Blandford Press (Poole, 1980) 42. G. L'E. Turner, Scientific Instruments and Experimental Philosophy , Variorum Collected Studies Series (Aldershot, 1991) 43. G. L'E. Turner (a cura di), Storia delle Scienze: Vol. I - Gli strumenti (Einaudi, 1991). 44. D.P. Wheatland, The Apparatus of Science at Harvard: (Harvard University Press, 1968). [*] Dipartimento di Astronomia, Università degli Studi di Bologna; [**] Osservatorio Astronomico di Roma [***] Osservatorio Astrofisico di Arcetri, Firenze Istituto di Fisica Generale Applicata Università degli Studi di Milano via Brera Milano, tel fax
A Guide to Telescopes How to choose the right telescope for you Telescopes What is a Telescope? A Telescope is an instrument that aids in the observation of remote objects by collecting electromagnetic
Astrophysical Techniques C R Kitchin University of Hertfordshire Observatory Third Edition SUB Gottingen 7 210 119 268 99 A 8843 Institute of Physics Publishing Bristol and Philadelphia Contents Preface
Mem. S.A.It. Vol. 82, 253 c SAIt 2011 Memorie della G. V. Schiaparelli and the Arcetri Observatory S. Bianchi, D. Galli, and A. Gasperini Istituto Nazionale di Astrofisica Osservatorio Astrofisico di Arcetri,
Examiners Report November 2011 GCSE Physics/Science 5PH1F/01 Edexcel is one of the leading examining and awarding bodies in the UK and throughout the world. We provide a wide range of qualifications including
The Lombardia Region Exploratorium Project 19 October 2011 -Turin 1 Space Exploration Promotion what why who Incentive the Public Interest Introduction to Space Science and Engineering Understand the Space
The Internationalization and the Royal Academy of Italy!! working partnerships with the International Union of Academies, with the International Institute for Intellectual Cooperation,! support guaranteed
Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal
ARTEFACTS XX SCIENTIFIC HERITAGE AT WORLD EXHIBITIONS AND BEYOND THE LONG XX CENTURY 20-22 SEPTEMBER 2015 SUNDAY SEP 20 15.00-15.30 Registration 15.30-16.00 Welcome Fiorenzo Galli, General Director Laura
1 CHAPTER 7 TIME In this chapter we briefly discuss the several time scales that are in use in astronomy, such as Universal Time, Mean Solar Time, Ephemeris Time, Terrestrial Dynamical Time, and the several
Chapter 6: SOLAR GEOMETRY Full credit for this chapter to Prof. Leonard Bachman of the University of Houston SOLAR GEOMETRY AS A DETERMINING FACTOR OF HEAT GAIN, SHADING AND THE POTENTIAL OF DAYLIGHT PENETRATION...
Congresso della SAIT Museo della Scienza e della Tecnologia di Milano 15 Maggio 2014 Francesca Esposito INAF Osservatorio Astronomico di Capodimonte (Napoli) ExoMars Mission The ExoMars Program is carried
Andrea Pedeferri Curriculum Vitae Personal Data 3601 Greenway apt 811 21218 Baltimore, MD USA +1 443 850 0092 firstname.lastname@example.org http://departments.columbian.gwu.edu/philosophy/people/172 Areas of Specializations
History of the telescope History of the Telescope Hans Lippershey The first practical telescopes appeared in the Netherlands about 1608, and were credited to a Dutch spectacle maker named Hans Lippershey.
Solar Tracking Application A Rockwell Automation White Paper Solar trackers are devices used to orient photovoltaic panels, reflectors, lenses or other optical devices toward the sun. Since the sun s position
ELENCO RIVISTE Presidenza New Scientist Science Scienze Laboratori Nazionali di Frascati Advances in Physics American Journal of Physics Annals of Physics Applied Physics Letters Astronomy and Astrophysics
Introduction Stefano Ferrari Università degli Studi di Milano email@example.com Elaborazione delle immagini (Image processing I) academic year 2011 2012 Image processing Computer science concerns
96 Lab Experiments Experiment-255 RESOLVING POWER OF A READING TELESCOPE S Dr Jeethendra Kumar P K KamalJeeth Instrumentation & Service Unit, No-60, TATA Nagar, Bangalore-560 092, INDIA. Email:firstname.lastname@example.org
Name: Class: Date: ID: A PS Chapter 1 Review Multiple Choice Identify the choice that best completes the statement or answers the question. 1. The two main branches of science are a. physics and chemistry.
THE USE OF OFFICIAL STATISTICS IN TEACHING UNIVERSITY GEOGRAPHY STUDENTS IN ITALY Enrica Aureli and Riccardo Russo Università La Sapienza, Italia This paper intends to be a report on the statistical methods
AS102 - Day Laboratory Exercise #3: Optics and Telescopes Page 1 DAY LABORATORY EXERCISE #3: OPTICS AND TELESCOPES Goals: To explore the functions of simple lenses To construct and use a refracting telescope
Satellite Meeting "Conservation and preservation of library material in a cultural-heritage oriented context" 31 August - 1 September 2009 Rome, Italy Organized by IFLA Core Activity on Preservation and
Mem. S.A.It. Suppl. Vol. 12, 77 c SAIt 2008 Memorie della Supplementi The Optical Design of the High Resolution Imaging Channel for the SIMBIO-SYS experiment on the BepiColombo Mission to Mercury G. Marra
ACTIVITY-1 Which month has larger and smaller day time? Problem: Which month has larger and smaller day time? Aim: Finding out which month has larger and smaller duration of day in the Year 2006. Format
There is a theory which states that if ever anybody discovers exactly what the Universe is for and why it is here, it will instantly disappear and be replaced by something even more bizarre and inexplicable.
6/24 Discussion of the first law. The first law appears to be contained within the second and it is. Why state it? Newton s laws are not always valid they are not valid in, say, an accelerating automobile.
Where Astronomy is looking up Choosing a Telescope There is no best telescope for everyone. The one that s right for you will depend on your lifestyle and your astronomy goals. The best telescope is the
Sixth Grade Science Curriculum One Stop Shop For Educators The Georgia Performance Standards are designed to provide students with the knowledge and skills for proficiency in science at the sixth grade
Scale of the Solar System Scale of the Universe How big is Earth compared to our solar system? How far away are the stars? How big is the Milky Way Galaxy? How big is the Universe? How do our lifetimes
Round Table Italy-Russia at Dubna Efforts in Fundamental Research and Perspectives for Applied S&T and Business Development Report by Marco Boiti President of Consortium E.I.N.S.T.E.IN. on Scientific cooperation
VOL. I NO. II JUNE 2006 TECHNICAL INFORMATION & PRODUCT NEWS 1 Technical Information No. 40: Optical glass for precision molding 2 New 0.9 mm FAC Lens offers potential for cost reduction in the fabrication
Associate Degree Program Department of Civil and Architectural Technology Major : Survey Technology First Semester NO 5 6 Code SRV 0 SRV 0 SRV 0 ENG 0 MTH 7 CMT 0 Course Title Land survey Survey drawing
Tips when buying a telescope You have gotten the Astronomy bug and decided that you must buy your first telescope. Well hopefully you have come to the right place. Have a word with our observations officers
CPO Science and the NGSS It is no coincidence that the performance expectations in the Next Generation Science Standards (NGSS) are all action-based. The NGSS champion the idea that science content cannot
Günter Seeber Satellite Geodesy 2nd completely revised and extended edition Walter de Gruyter Berlin New York 2003 Contents Preface Abbreviations vii xvii 1 Introduction 1 1.1 Subject of Satellite Geodesy...
Pre and post-visit activities - Navigating by the stars Vocabulary List Adult Education at Scienceworks Pre-visit Activity 1: What is longitude and latitude? Activity 2: Using the Southern Cross to find
Chapter 1 Parts C. Robert Bagnell, Jr., Ph.D., 2012 Figure 1.1 illustrates the parts of an upright compound microscope and indicates the terminology that I use in these notes. Figure 1.1. Parts of a Compound
Objective Geometric Optics Converging Lenses and Mirrors Physics Lab IV In this set of lab exercises, the basic properties geometric optics concerning converging lenses and mirrors will be explored. The
Ray Optics Minicourse COMSOL Tokyo Conference 2014 What is the Ray Optics Module? Add-on to COMSOL Multiphysics Can be combined with any other COMSOL Multiphysics Module Includes one physics interface,
Testing and Performance of the Convex Lens Concentrating Solar Power Panel Prototype Ankit S. Gujrathi 1, Prof. Dilip Gehlot 2 1 M.tech (2 nd Year), 2 Assistant Professor, Department of Mechanical Engg.,
Data Provided: A formula sheet and table of physical constants is attached to this paper. DEPARTMENT OF PHYSICS AND ASTRONOMY Autumn Semester (2014-2015) DARK MATTER AND THE UNIVERSE 2 HOURS Answer question
LIBRARY OF CONGRESS COLLECTIONS POLICY STATEMENTS ±² Collections Policy Statement Index Geography and Cartography Contents I. Scope II. Research Strengths III. Collecting Policy IV. Acquisitions Sources:
Chapter 5 Light and Matter: Reading Messages from the Cosmos Messages Interactions of Light and Matter The interactions determine everything we see, including what we observe in the Universe. What is light?
UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics Physics 111.6 MIDTERM TEST #4 March 15, 2007 Time: 90 minutes NAME: (Last) Please Print (Given) STUDENT NO.: LECTURE SECTION (please
An Automated Solar Shading Calculator M.K.Dennis Centre for Sustainable Energy Systems Australian National University Canberra ACT 0200 AUSTRALIA Telephone: +61 02 6125 3976 Facsimile: +61 02 6125 0506
CATALOG PLANETARIUM COLUMBIA OPTICS We have the honor to show you some of our products in the field of digital planetariums. PROJECTOR FOR PLANETARIUM DIGITAL DIGITAL PROJECTOR FULL-DOME Particular system
Science and Technology Chapter 1. What Is Science? 1. Science and the Natural World 2.Thinking Like a Scientist 3. Scientific Inquiry Scope and Sequence Interactive Science grades 6-8 Chapter 2. Science,
FRANCESCO BELLOCCHIO S CURRICULUM VITAE ET STUDIORUM April 2011 Index Personal details and education 1 Research activities 2 Teaching and tutorial activities 3 Conference organization and review activities
Telescopic Observations Materials: Paper, pencil, camera, Telescope or Binoculars In this project, you will be observing at least three objects with a telescope or binoculars, and drawing what you see.
The Science Education System in Oxford and the UK David Andrews 1 Outline of this talk High school education (brief) Undergraduate education Oxford Physics Other sciences at Oxford Other universities Postgraduate
California Standards Grades 912 Boardworks 2009 Science Contents Standards Mapping Earth Sciences Earth s Place in the Universe 1. Astronomy and planetary exploration reveal the solar system s structure,
THE 2014 EQUATORIAL SUNDIAL GEOGRAPHIC SOUTH POLE MARKER J. Dana Hrubes Design Steele Diggles Fabrication An equatorial sundial is the simplest sundial to construct and visualize. The sundial surface is
Optical Differences Between Telescopes and Microscopes Robert R. Pavlis, Girard, Kansas USA icroscopes and telescopes are optical instruments that are designed to permit observation of objects and details
9/6 Optics / GEOMETRIC OPTICS PURPOSE: To review the basics of geometric optics and to observe the function of some simple and compound optical devices. APPARATUS: Optical bench, lenses, mirror, target
name The Size & Shape of the Galaxy The whole lab consists of plotting two graphs. What s the catch? Aha visualizing and understanding what you have plotted of course! Form the Earth Science Picture of
SAINT PETERSBURG STATE ELECTROTECHNICAL UNIVERSITY LETI Laser Measurement and Navigation Systems department Master Degree Program ETU LETI TRADITIONS AND INNOVATIONS ETU LETI is the oldest Electrotechnical
Prof. Alberto CARPINTERI Chair of Structural Mechanics Politecnico di Torino 10129 - Torino - Italy Tel. : +39 011 564 4850 Fax: +39 011 564 4899 E-mail: email@example.com Homepage: http://staff.polito.it/alberto.carpinteri
Friday 18 January 2013 Morning AS GCE PHYSICS B (ADVANCING PHYSICS) G492/01 Understanding Processes / Experimentation and Data Handling *G411640113* Candidates answer on the Question Paper. OCR supplied
CURRICULUM VITAE Christian Rossi POLITICAL AND SOCIAL SCIENCE HISTORY OF INTERNATIONAL RELATIONS February 2011 I. PERSONAL INFORMATIONS Name and Surname: Christian Rossi Place and Date of Birth: Cagliari,
Curriculum for the Degree of Bachelor of Science In Nautical Science 1 1.Name :Bachelor of Science ( Nautical Science ) Abbreviation : B.Sc.( Nautical Science ) 2.Program of Study The Bachelor of Nautical
INDEX SR NO NAME OF THE PRACTICALS Page No 1 Measuring the bearing of traverse lines, calculation of included angles and check. 1 2 To study the essential parts of dumpy level & reduction of levels 3 To
Indiana Content for Educators SCIENCE PHYSICAL SCIENCE teachers are expected to have a broad understanding of the knowledge and skills needed for this educator license, and to use that knowledge to help
ERMES. Monitoring of radon in geogas at the Gran Sasso National Laboratory G. De Luca a and W. Plastino b a Istituto Nazionale di Geofisica e Vulcanologia (INGV) Centro Nazionale Terremoti (CNT), Via di
OVERVIEW More than ever before, Physics in the Twenty First Century has become an example of international cooperation, particularly in the areas of astronomy and cosmology. Astronomers work in a number
Spring Term Lecturer: Assoc. Prof. Dr. M. Zeki COŞKUN Department of Geomatics Engineering e-mail : firstname.lastname@example.org THEODOLITE What is Theodolite? Use of Theodoite Theodolite Terminology THEODOLITE Types
Virtual digital libraries: The DILIGENT Project Donatella Castelli ISTI-CNR, Italy The DLs evolution Dynamic Universal Knowledge Environment 2005 Repository of digital texts + search service 1996 Large
CELESTIAL MOTIONS Stars appear to move counterclockwise on the surface of a huge sphere the Starry Vault, in their daily motions about Earth Polaris remains stationary. In Charlottesville we see Polaris
Chapter 6 Telescopes: Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning:! How does your eye form an image?! How do we record images? How does your eye form an image?
Astrock, t he A stronomical Clock The astronomical clock is unlike any other clock. At first glance you ll find it has similar functions of a standard clock, however the astronomical clock can offer much
SIXTH GRADE WEATHER 1 WEEK LESSON PLANS AND ACTIVITIES WATER CYCLE OVERVIEW OF SIXTH GRADE WATER WEEK 1. PRE: Evaluating components of the water cycle. LAB: Experimenting with porosity and permeability.
National Aeronautics and Space Administration Einstein Rings: Nature s Gravitational Lenses Leonidas Moustakas and Adam Bolton Taken from: Hubble 2006 Science Year in Review The full contents of this book
Measuring Your Latitude from the Angle of the Sun at Noon Background: You can measure your latitude in earth's northern hemisphere by finding out the altitude of the celestial equator from the southern
Telescope Types and Designs There are three basic types of optical telescopes Refractor, Newtonian reflector and Catadioptric. All of these telescopes are designed to collect light and bring it to a focus
Eighth Grade Science Curriculum Approved July 12, 2004 The Georgia Performance Standards are designed to provide students with the knowledge and skills for proficiency in science at the eighth grade level.
Star Counts in the Milky Way: a Research Experience Designed for High School Competences Conrad A. Böhm, Giulia Iafrate Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Trieste email@example.com,