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Steps Toward the HST. NASM 18 November 2009

Steps Toward the HST. NASM 18 November 2009. C. R. O’Dell Vanderbilt University- Distinguished Research Professor of Physics and Astronomy Rice University -Andrew Hayes Buchanan Professor of Astrophysics-Emeritus. Steps Toward the HST.

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Steps Toward the HST. NASM 18 November 2009

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  1. Steps Toward the HST.NASM18 November 2009 C. R. O’Dell Vanderbilt University-DistinguishedResearch Professor of Physics and Astronomy Rice University-Andrew Hayes Buchanan Professor of Astrophysics-Emeritus

  2. Steps Toward the HST. • 1971-1972 Feasibility Studies (HQ Group, GSFC, MSFC, Contractors).

  3. From Eric Chaisson & Ray Villard’s April, 1990 Sky&Tel article.

  4. 1972-GSFC-3mCrossSection

  5. 1972-MSFC-3mConfiguration

  6. Steps Toward the HST. • 1971-1972 Feasibility Studies (HQ Group, GSFC, MSFC, Contractors). • 1973-1977 Preliminary Design (SWG,MSFC,GSFC,Contractors).

  7. 1973-A broad Scientific Base is established. • I came on-board in September, 1972. • In December NASA issued an AO for creation of Instrument Definition Teams, the leaders plus a few generalists would form a Science Working Group. • January, 1973 a dog-and-pony show was presented at CalTech, Chicago, and Harvard advertising the AO.

  8. 1974 • However, we needed an even broader constituency. • This was done in part by having special sessions at the American Astronomical Society meetings. • The watershed event was the January 30 American Institute of Aeronautics and Astronautics meeting.

  9. AIAA ScienceSpeakers.

  10. HST CutawayCropped

  11. Supermanto the Rescue.

  12. NBSAxial SI Replacement

  13. Steps Toward the HST. • 1971-1972 Feasibility Studies (HQ Group, GSFC, MSFC, Contractors). • 1973-1977 Preliminary Design (SWG,MSFC,GSFC,Contractors). • 1978-1990 Design and Development (New SWG, MSFC,GSFC,Lockheed-Martin,Perkin-Elmer, SI Contractors).

  14. Schedule History From Richard Tresch Fienberg’s April 1990 Sky&Tel article.

  15. JAW Cartoon

  16. Backup Material Follows.

  17. 1971-72 Feasibility Studies and the Roman Group. • One of the first things NASA did was to establish if the project was feasible (a Phase-A Study). • In parallel with studies by multiple contractors a group of scientists was convened at NASA HQ by Nancy G.Roman to provide feedback.

  18. Lyman Spitzer

  19. AIAA Cover

  20. AIAA Participants

  21. Fletcher-Petrone-CRO

  22. 1975-Seeking Funding for Actual Construction (Phase C/D) • The escalating identified costs caused many in the Congress to balk. Several times the program was considered dead. • NASA negotiates its budgets internally, then with the White House, and then the Congress approves-modifies-rejects the submitted presidential budget. • NASA employees must support the submitted budget and DO NOT make end-runs to Capitol Hill.

  23. Convincing the Congress • Non-NASA scientists COULD go directly to the key members of the House and Senate. • This was done with wisdom and vigor by Lyman Spitzer and John Bahcall. • The truth of their arguments won the day, which may not have been the case without them. • In the early years these efforts kept HST alive as congress stretched out the Phase B activities. • In the final years, the lobbying efforts resulted in the HST being included in the FY1978 budget almost in spite of NASA.

  24. 1976-European Participation • The first major joint NASA-ESA venture was the IUE (launched in 1978). • Negotiations with the ESA started in Phase B as soon as we started having cost problems. • The areas of participation were finally narrowed down to the Solar Arrays and a Scientific Instrument (the FOC). • Although probably financially and scientifically attractive, the primary determinant was the will of the Congress. • A NASA-ESA agreement was reached in late 1976.

  25. How was the Science Data to be managed? • Traditionally astronomer’s data didn’t transport well (mostly photographic). • NASA’s experience was similar, with the instrument teams exclusively using the results from the spacecraft. • Clearly, these were NOT the ways to do the HST.

  26. Data Rights and Distribution • Very early we established that the GTO’s were to have a rapidly decreasing reward in use of the SI’s. • This meant that GO’s would be the primary users of the SI’s. • It was clear that there had to be a central facility(ies) for routine processing and archiving the data.

  27. How was the Science to be Managed? • Astronomers were used to the national facilities being run by consortia of universities. • KPNO+CTIO-AURA, NRAO-AUI. • The idea of the STScI was first advocated by the ad hoc Ramsey Committee in 1965, before HST was started, but then forgotten. • Within the HST project, an STScI was first advocated by the Project Scientist in 1972, eventually this idea was embraced by the Phase B SWG. • A National Academy of Science study in July, 1976 endorsed the concept and NASA reluctantly accepted it.

  28. HST SWGPhase C/D

  29. The SI’s Selected. • The Wide Field/Planetary Camera; PI, Jim Westphal of CalTech. • The Faint Object Spectrograph; PI, Richard Harms of UC San Diego. • The Goddard High Resolution Spectrograph; PI, Jack Brandt (Sally Heap). • The High Speed Photometer; PI, Bob Bless of the University of Wisconsin. • The Faint Object Camera; ESA (preselected) PI Duccio Macchetto & Henk van de Hulst. • Astrometry with the FGS; Leader,BillJeffereys

  30. The Phase C/D SWG. • NASA-Project Scientist (O’Dell, Brown, Boggess),and Program Scientist Ed Weiler. • SI Team Leaders (seven in all, John Trauger of JPL added later). • Telescope Scientists: Dan Schroeder -Beloit College & Bill Fastie-JHU) • At Large Members: John Caldwell-Toronto,Malcolm Longair-Edinburgh,Ed Groth-Princeton(Physics), David Lambert-Texas,John Bahcall, and Riccardo Giacconi (added).

  31. Spherical Aberration • This was discovered as the first images were made. • The cause was a misaligned optical device used to measure the shape of the primary mirror. • This device was intended to make the mirror appear to be flat when it was of the right shape.

  32. Contributing Factors • The primary mirror was not considered the most demanding part of the HST. • The program was very cost-constrained and the method of testing was considered straightforward. • Management was concentrating on a redesign of the FGS, which WAS new. • The resident MSFC QA person had not been changed because of manpower constraints. • The report on the anomaly with the alignment was not forwarded to MSFC.

  33. SM1Axial SI Replacement

  34. Reading Material • “The Space Telescope” by Robert W. Smith. Cambridge University Press, 1989(pre-launch) & 1993(post-launch). • “The Orion Nebula” by C. Robert O’Dell, Harvard University Press, 2003 (Chapter 10). • “Alice and the Space Telescope” by Malcolm Longair, JHU Press, 1989.

  35. Don’t you just love a story with a happy ending?

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