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Text File  |  1992-11-19  |  1.0 KB  |  26 lines

  1. Newsgroups: sci.space
  2. Path: sparky!uunet!cis.ohio-state.edu!news.sei.cmu.edu!fs7.ece.cmu.edu!crabapple.srv.cs.cmu.edu!roberts@cmr.ncsl.nist.gov
  3. From: roberts@cmr.ncsl.nist.gov (John Roberts)
  4. Subject: Scientific method (followup)
  5. Message-ID: <By05HH.uv.1@cs.cmu.edu>
  6. X-Added: Forwarded by Space Digest
  7. Sender: news+@cs.cmu.edu
  8. Organization: National Institute of Standards and Technology formerly National Bureau of Standards
  9. Original-Sender: isu@VACATION.VENARI.CS.CMU.EDU
  10. Distribution: sci
  11. Date: Fri, 20 Nov 1992 06:45:21 GMT
  12. Approved: bboard-news_gateway
  13. Lines: 11
  14.  
  15.  
  16. For those who *insist* on the classical method of development of theory
  17. followed by testing for previously unobserved supporting phenomena, the
  18. current condition of HST offers a priceless opportunity. They can develop
  19. their hypotheses now, then after the installation of WF/PC II and COSTAR,
  20. they can look again in more detail. (This was discussed on Thursday with
  21. respect to the discovery of the accretion disk.)
  22.  
  23. John Roberts
  24. roberts@cmr.ncsl.nist.gov
  25.  
  26.