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Inventing a Space Mission: The Story of the Herschel Space Observatory 1st ed. 2017 [Hardback]

  • Formāts: Hardback, 280 pages, height x width: 235x155 mm, weight: 720 g, 69 Illustrations, color; 22 Illustrations, black and white; XII, 280 p. 91 illus., 69 illus. in color., 1 Hardback
  • Sērija : ISSI Scientific Report Series 14
  • Izdošanas datums: 11-Dec-2017
  • Izdevniecība: Springer International Publishing AG
  • ISBN-10: 3319600230
  • ISBN-13: 9783319600239
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  • Formāts: Hardback, 280 pages, height x width: 235x155 mm, weight: 720 g, 69 Illustrations, color; 22 Illustrations, black and white; XII, 280 p. 91 illus., 69 illus. in color., 1 Hardback
  • Sērija : ISSI Scientific Report Series 14
  • Izdošanas datums: 11-Dec-2017
  • Izdevniecība: Springer International Publishing AG
  • ISBN-10: 3319600230
  • ISBN-13: 9783319600239
This book describes prominent technological achievements within a very successful space science mission: the Herschel space observatory. Focusing on the various processes of innovation it offers an analysis and discussion of the social, technological and scientific context of the mission that paved the way to its development. It addresses the key question raised by these processes in our modern society, i.e.: how knowledge management of innovation set the conditions for inventing the future? In that respect the book is based on a transdisciplinary analysis of the programmatic complexity of Herschel, with inputs from space scientists, managers, philosophers, and engineers.





This book is addressed to decision makers, not only in space science, but also in other industries and sciences using or building large machines. It is also addressed to space engineers and scientists as well as students in science and management.
1 Inventing a Space Machine: Breaking the Borders of Knowledge, Technology and Management
1(8)
1.1 Why Choose a Space Science Mission for a Study About Innovation
2(3)
1.2 Why Herschel?
5(1)
1.3 Our Approach
6(3)
2 Creating the Historical and Strategic Framework for Herschel
9(36)
2.1 The Birth of Infrared and Submillimetre Astronomy
9(10)
2.1.1 The Military Connection
12(1)
2.1.2 The Emerging Infrared Astronomy Community
13(2)
2.1.3 The Space Connection
15(4)
2.2 The Birth of Space Infrared and Submillimetre Astronomy in Europe
19(26)
2.2.1 Creation of a European Space Research Organisation
19(2)
2.2.2 Infrared Astronomy and the ESRO Programme
21(1)
2.2.3 From ESRO to ESA: A 14-Year Stagnation Period in Space Science
22(2)
2.2.4 Fighting to Recover ESRO's Lost Science Budget
24(2)
2.2.5 Formulation of an ESA Strategic Long-Term View: Horizon 2000
26(3)
2.2.6 The Horizon 2000 Philosophy: Scientific Excellence, Schedule Respect and Design-to-Cost
29(2)
2.2.7 Paving the Way to Success
31(2)
2.2.8 Implementation of Horizon 2000
33(2)
2.2.9 Problems on the Horizon
35(6)
2.2.10 Conclusion
41(1)
References
42(3)
3 Herschel Mission Overview
45(38)
3.1 Introduction
45(1)
3.2 FIRST in the Pre- and Post-Horizon 2000 Period (1974--1986)
46(5)
3.3 The Race to the CS3 H 2000 Position: From Community Wishes to SPC Adoption
51(5)
3.3.1 Mission Definition Study (1987--1990)
51(1)
3.3.2 System Definition Study (1990--1992)
52(2)
3.3.3 Rider Study (1992--1993)
54(1)
3.3.4 Selection of FIRST as Cornerstone 4 of Horizon 2000 (1993)
55(1)
3.4 FIRST in the New Horizon 2000 Plan (1993--1997)
56(7)
3.4.1 The Traumatic 1994--1997 Series of Crises
56(1)
3.4.2 Managing the Crises (1994--1997)
57(1)
3.4.3 Selection of the Combined FIRST/Planck Option (1997--1998)
58(2)
3.4.4 Optimization Studies of Mission Critical Elements (1994--2000)
60(3)
3.5 Selecting the FIRST Scientific Payload (1997--1999)
63(4)
3.5.1 The Announcement of Opportunity for the Combined FIRST/Planck Mission
63(2)
3.5.2 Selection of the FIRST/Planck Scientific Payload
65(2)
3.6 Project Development (2000--2009)
67(4)
3.6.1 Preparation of the FIRST/Planck Industrial Project Development (2000--2001)
67(1)
3.6.2 Herschel/Planck Last Race Towards Launch (2001--2009)
68(3)
3.7 Herschel In-orbit (2009--2013) and the Post-operations Phase (2013--2017)
71(3)
3.8 Evolution of the Cost Estimate Up to Completion of the Post-operations Phase
74(1)
3.9 Conclusion
75(8)
Appendix 1
76(1)
Appendix 2
77(1)
Appendix 3
78(1)
Appendix 4
79(1)
References
80(3)
4 Herschel Science Evolution and Results
83(40)
4.1 The Diagnostic Importance of the FIR and Submillimetre Spectral Range
84(2)
4.2 Evolution of FIRST/Herschel Science Objectives
86(3)
4.3 Herschel in Orbit
89(5)
4.4 A Selection of Scientific Results
94(16)
4.4.1 Star Formation in Our Milky Way Galaxy
94(6)
4.4.2 Evolution of Galaxies and Star Formation over Cosmic Time
100(5)
4.4.3 `Water Trail' and Solar System Studies
105(5)
4.5 Bibliometric Analysis of Herschel's Scientific Return
110(10)
4.5.1 Scientific Return on Investment: ESA Key Performance Indicators
111(4)
4.5.2 Structure of Herschel's Community: Co-citation Mapping
115(4)
4.5.3 Identification of the Most Important Groups Linked to Science Cases
119(1)
4.6 Conclusion
120(3)
References
121(2)
5 Innovation in Technology and Management
123(16)
5.1 What Is Innovation?
123(3)
5.2 Setting the Condition for `Coopetition'
126(2)
5.3 Promoting Sociality Between Science and Industry
128(1)
5.4 Concepts and Knowledge Leading to Innovation
129(1)
5.5 Mechanology and the Pace of Innovation
130(3)
5.6 Typology and Census of Innovations
133(2)
5.7 Plurality of Functionalities and Relativity of Criteria
135(4)
References
137(2)
6 Silicon Carbide Telescope: Radical Innovation
139(20)
6.1 Telescope Principle
140(1)
6.2 FIRST: An `Undecidable' Initial Concept
141(3)
6.3 Competition Between Various Industrial Concepts
144(4)
6.4 JPL/NASA Concept
148(2)
6.5 Plan B: The SiC Telescope
150(2)
6.6 Invention of a Technical Lineage: From Herschel to Euclid
152(4)
6.7 Conclusion and Future Perspective
156(3)
References
157(2)
7 Far-Infrared Bolometers: Technical Lineages
159(24)
7.1 Bolometric Detectors
159(2)
7.2 Early Bolometer Instruments for Astronomy
161(1)
7.3 3He-Cooled Bolometers
162(3)
7.4 The Development of Ground-Based Bolometer Array Instruments
165(4)
7.5 The Herschel SPIRE Instrument
169(1)
7.6 Superconducting Transition Edge Bolometers
170(1)
7.7 Micromachined Silicon Bolometers
171(1)
7.8 Absorber-Coupled vs Feedhorn-Coupled Arrays
172(1)
7.9 The SPIRE Detector Development Programme
173(3)
7.10 CEA Silicon Bolometers: From SPIRE to PACS
176(1)
7.11 Bolometer Technical Lineages
176(3)
7.12 Conclusions
179(4)
References
180(3)
8 Heterodyne Technology in Submillimetre Astronomy: Towards Implementation in Herschel
183(30)
8.1 Principle of the Heterodyne Technique
184(2)
8.2 Technical Lineages, Risk and Innovation
186(3)
8.3 Developments on Mixers and LOs (1970--1997)
189(9)
8.4 From the Heterodyne Model Payload Instrument (HET) to HIFI
198(3)
8.5 Ultimate Technological Developments for HIFI
201(4)
8.5.1 Mixer Developments
201(2)
8.5.2 Local Oscillator Developments
203(2)
8.6 HIFI as Built
205(4)
8.7 Conclusion
209(4)
References
210(3)
9 Super fluid Helium Cryostat Customisation
213(18)
9.1 Principles of Cryogenic Devices
214(3)
9.2 Initial Concepts: From Cryocoolers to Superfluid Helium Cryostat
217(2)
9.3 Liquid Helium Cryostat Lineage
219(3)
9.4 Customisation and Innovation
222(4)
9.5 Mission Lifetime and Cryostat Volume
226(1)
9.6 Conclusion
227(4)
References
229(2)
10 Management and Organisation of Science Instruments
231(30)
10.1 ESA/Herschel Organisation
232(3)
10.2 Management of Instrument and Science Consortia
235(20)
10.2.1 Genesis of a Consortium Instrument: The Case of HIFI
236(8)
10.2.2 Science Organisation Within the HIFI Consortium
244(2)
10.2.3 Herschel, Industry and Innovation: Lessons Learned from the PACS Consortium
246(5)
10.2.4 Confronting the Management Organisation in HIFI, PACS and SPIRE
251(4)
10.3 Management of Data Products
255(2)
10.4 Conclusions
257(4)
References
259(2)
11 Conclusion: Risk-Based Innovation and Knowledge Management
261(8)
Acronyms 269(6)
Index 275
Roger-Maurice Bonnet graduated from Paris University. A space scientist and solar astronomer, he was in charge of the first French space astronomy rocket program. He led the Laboratoire de Physique Stellaire et Planétaire of CNRS (now renamed Institut dAstrophysique Spatiale) from1969 until 1983 when he was elected Director of the ESA Science Program. There he established the first long term scientific program of ESA Space Science Horizon 2000, a balanced mix of more than 20 large, medium and small missions, among which Herschel and Planck. In 2003 he became Executive Director of the International Space Science Institute (ISSI). He is the author of more than 150 scientific articles and several books, several of them published by Springer.

Frank Helmich studied at the University of Groningen and obtained his PhD at the University of Leiden. After a short excursion to stratospheric chemistry at SRON in Utrecht, he moved to SRON Groningen to work on HIFI calibration and science. In 2007 he became Head of SRONs Low Energy Astrophysics Division and took over as Principal Investigator for Herschel/HIFI. In 2015 he became Leader of the Astrophysics Program of SRON. He is (co-) author of 70-refereed papers.

Vincent Bontems graduated from École Normale Supérieure de Lettres et Sciences Humaines and earned a PhD in philosophy at the École des Hautes Études en Sciences Sociales. He works at the laboratory Larsim of the CEA on epistemology of physics, technology and innovation, and sociology of sciences. He is a member of the Physics and Fundamental Questions committee of the French Society of Physics. He has written a book on Gaston Bachelard (Bachelard, Belles Lettres, 2010) and many articles, including Gilbert Simondons genetic mécanologie and the understanding of laws of technical evolution (Techne, 13: 1, 2009) and What does innovation stand for? Review of a watchword in research policies (Journal of Innovation Economics, 15, 2014).



ESA Herschel Project Scientist Göran Pilbratt received his PhD from Onsala Space Observatory, Chalmers University of Technology, Göteborg, Sweden in 1986. His thesis topic was Very Long Baseline Interferometry (VLBI) observations of superluminal sources. In the same year, he joined ESA as a Research Fellow and was initially involved in ESA studies on space-based VLBI missions. He was appointed ESA Staff Scientist in 1988.  In 1991, he was appointed Study Scientist for FIRST, and became Project Scientist for the mission in 1995, a position he still holds. Following his proposal, the mission was renamed Herschel in December 2000 to celebrate the bicentenary of the discovery of infrared light by William Herschel.

Sergio Volonte graduated in physics at Université de Ličge in 1967. From 1968 to 1971 he was ESRO research fellow at the Culham Laboratory (UK) and obtained is PhD from University College London in 1972. He returned to Belgium at Departement dAstrophysique, Université de Mons where he lectured in Astronomy and Spectroscopy. In 1986, he joined ESA as Coordinator for Astronomy missions in the Directorate of the Science Programme at the Paris Headquarters. He retired in 2008 as Head of the ESA Science Programme Planning & Coordination Office. He is the author or co-author of some 80 scientific papers and a member of various societies, in particular, the International Astronomical Union, Cospar, the International Astronautical Federation as well as fellow of the Royal Astronomical Society. Vincent Minier received his PhD in astrophysics from Chalmers University of Technology, Gothenburg, Sweden. After a two-year research position at UNSW in Sydney, he came back to France in 2003 to work at CEA / Paris Saclay University. Star formation is his main field of expertise, and he has conducted observations with word-class telescopes both on Earth (Chile, Australia, US, Europe) and in space(Herschel space observatory). Besides fundamental science, he leads the ExplorNova research project on philosophy of innovation within Big science instruments and on information technologies to disseminate science through astrophysics. He is the author of more than 100 scientific articles, the MOOC ExplorUnivers on popular astronomy, Web sites dedicated to space missions and science videos.

Thijs (Mattheus) de Graauw studied at the University of Utrecht. After graduation he became staff member of ESAs Space Science Department at ESTEC where he started a submm instrumentation development, in collaboration with a number of European laboratories, with the aim to prepare for an astronomy  space mission. He was study scientist for several optical, ir and submm space projects and technical research programs (TRP) for future missions. He was member of the FIRST study team from 1982 till 1986. In 1983 he became director of SRONs space research laboratory in Groningen to lead the Dutch IR and submm space program. He was principal investigator for the Short Wavelength Spectrometer (SWS) of the Infrared Space Observatory (ISO) and for Herschels Heterodyne Instrument for the Far Infrared (HIFI). After delivery of the instrument to ESA (2008) he left HIFI to become director of the Atacama Large Millimeter/submillimeter Array (ALMA) to lead the construction of the ALMA Observatory. Since 2013, in his second retirement, he is engaged in fostering development of submm instrumentation and science in Brasil/Argentina and Russia. He is (co-) author of more than 150-refereed scientific papers.

Matt Griffin studied Electrical Engineering at University College Dublin and Astrophysics at Queen Mary College London, graduating with a PhD in 1985. He remained at Queen Mary until 2001, when he joined the Astronomy Instrumentation Group at Cardiff University. His research work has included the development of instruments for both ground-based and space-borne observatories, and study of planetary atmospheres, star formation, galaxy evolution, and the Earths atmosphere. He has worked on many ground-based and space-borne instrument projects. He was a Co-Investigator in the team that built the Long Wavelength Spectrometer for ESA's Infrared Space Observatory, and was the Principal Investigator for the Herschel-SPIRE instrument. He is the author of over 200-refereed publications.