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NO. 172 THE LUNAR AND PLANETARY LABORATORY AND ITS TELESCOPES by Gerard P. Kuiper December 31, 1972 1. Introduction In "Organization and Programs of the Laboratory", LPL Communication No. 1 (1962), I projected a set of aims and objectives for this Laboratory. This in cluded the telescopes planned for the immediate future and a brief description of the facilities on this Campus. A number of early results were also mentioned: the ORTHOGRAPHIC ATLAS OF THE MOON (1961); the RECTIFIED LUNAR ATLAS, to be issued 1963; and near-infrared spectra of planets and red stars. Late 1963 I summarized elsewhere (Sky and Telescope, Jan, Feb, 1964) the activities of this Laboratory for its first three years of operation. I stressed especially the interdisciplinary nature of planetary astronomy with its demands on staff and facilities. The present Communication describes the LPL Campus and Observatory facilities as of 1972. Our several test programs toward the discovery of optimum observatory sites, both in Arizona and elsewhere, are recorded in LPL Communication No. 199. That issue also covers the acquisition in 1970 of the 20-acre well-developed Mt. Lemmon summit. Its favorable elevation (9157 ft or 2800 m), latitude (32°N), climate, and accessibility, make it ideally suited for an inter-university Infra red Observatory. 199

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Page 1: NO. 172 THE LUNAR AND PLANETARY LABORATORY AND ITS TELESCOPES › sites › default › files › sic › collection › jo… · 1963; and near-infrared spectra of planets and red

NO. 172 THE LUNAR AND PLANETARY LABORATORY AND ITS TELESCOPES

by Gerard P. Kuiper

December 31, 1972

1 . I n t r o d u c t i o n

In "Organization and Programs of the Laboratory", LPL Communication No. 1(1962), I projected a set of aims and objectives for this Laboratory. This included the telescopes planned for the immediate future and a brief descriptionof the facilities on this Campus. A number of early results were also mentioned:the ORTHOGRAPHIC ATLAS OF THE MOON (1961); the RECTIFIED LUNAR ATLAS, to be issued1963; and near-infrared spectra of planets and red stars. Late 1963 I summarizedelsewhere (Sky and Telescope, Jan, Feb, 1964) the activities of this Laboratory fori ts first three years of operat ion. I stressed especial ly the interdiscipl inarynature of planetary astronomy with its demands on staff and facilities.

The present Communication describes the LPL Campus and Observatory facilitiesas of 1972. Our several test programs toward the discovery of optimum observatorysites, both in Arizona and elsewhere, are recorded in LPL Communication No. 199.That issue also covers the acquisition in 1970 of the 20-acre well-developed Mt.Lemmon summit. Its favorable elevation (9157 ft or 2800 m), latitude (32°N),cl imate, and accessibi l i ty, make i t ideal ly suited for an inter-university Infrared Observatory.

199

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THE LABORATORY AND ITS TELESCOPES

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THE LABORATORY AND ITS TELESCOPES

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T H E L A B O R AT O R Y A N D I T S T E L E S C O P E S 2 4 3

Lunar and Planetary Surfaces (Dr. Kuiper and Mr. Strom):

Charles A. Wood, M. S.Ralph Turner, Sculptor (p)2 Assistants (p)

Library - Sue Morris, B. A. (p)

Editorial Department:

Gerard P. Kuiper, EditorElizabeth Roemer, Associate EditorMicheline Wilson, B. A., Assistant Editor (p)

LPL STAFF:

Administrat ive:

Melvin J. Simmons, Assistant to the Director and Business Manager(Mr. Simmons is responsible for managing the contracts and the financialstructure of LPL and the Observatories, generally including direction ofthe LPL Observatory Staff and supervision of much of the Shop work).

Ida A. Edwards, Secretary to the DirectorKathryn Osburn, Secretary, AccountantRuth Ash, Secretary

Observatories:Optical Shop:

Arnold D. Evans, Super intendentR o b e r t L . Wa l a n d , C h i e f O p t i c i a n L e l a n d E v a n s , R e s i d e n t E n g i n e e rR o b e r t G . C r a w f o r d , O p t i c i a n " " l i e o n a r d H . K e l l e y , A s s i s t a n tE d w a r d J . P l a m o n d o n , O p t i c i a n J o s e E . G a r c i a

Electronics Shop:

James R. PercyB. L. BelschnerBarry L. McClendon

Machine Shop:

Harold Mil lerRonald J. James

Drafting - Charles L. Edwards (p)

Computer Room:

Allen S. LathamRichard F. Poppen (p)

Research Assistantships are normally, but not exclusively, assigned to advanced graduate students. Research done as part of the Assistant's duties may,under appropriate conditions, be used for a thesis or as part of a thesis.

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T H E L A B O R A T O R Y A N D I T S T E L E S C O P E S 2 4 5

Acknowledgments. I must record my deep indebtedness to President EmeritusRichard Harvill, the late Vice President David Patrick, Provost Bowen Dees, andthe present University Administration for their continued interest in and support of this Laboratory and its programs. Our debt to the National Aeronauticsand Space Administration is beyond measure. NASA not only assisted the Laboratory with telescopic equipment, the Space Sciences Building, and researchsupport, but through NASA, my associates and I have been privileged to participate in the greatest scientific venture of history.

REFERENCES

1. Descriptive, supplementary to text

Coffeen, D. L. and Gehrels, T. 1970, "Ultraviolet Polarimetry of the Planets",SPACE RESEARCH X - North-Holland Publishing Co., Holland, 1936-1942.

Coffeen, D. L. and Hansen, J. E. 1972, "Airborne Infrared Polarimetry", Proceedings of the Eighth International Symposium on Remote Sensing of Environment.

Coyne, G. V. and Gehrels, T. 1968, "Polarimetry from High-Altitude Balloons",LPL Comm. No. 108, 7, 33-38.

Gehrels, T. et at. 1960-1969, "The Wavelength Dependence of Polarization,I to XV", Astron. J.

Gehrels, T. 1970, "Photometry of Asteroids", Chap. 6, SURFACES AND INTERIORSOF PLANETS AND SATELLITES, ed. Dollfus, A., Academic Press, 317-375.

Gehrels, T. 1972, "The Polariscope Program", Space Science Reviews, 13, 319.Gehrels, T., Suomi, V., and Krauss, R. J. 1972, "On the Capabilities of the

Spin-Scan Imaging Technique", SPACE RESEARCH XII, Akademie-Verlag, Berlin.Gehrels, T. 1973, "Photopolarimetry of Planets and Stars", VISTAS IN ASTRO

NOMY, Vol. 15, ed. Beer, A., Pergamon Press, Oxford.Kuiper, G. P. 1973, "High Resolution Planetary Observation", SPACE RESEARCH

XII, Akademie Verlag, Berlin, 1683-1687.Kuiper, G. P.1973, "The Origin of the Solar System", Celestial Mechanics,

in press.Larson, H. P. and Fink, U. 1973, "The NASA CV-990 1971 Mars Flights", in

preparation.Larson, S. M. /972, "The Tumamoc Hill Site Near Tucson, Arizona", The Kiva,

38, No. 2.Low, F. J., Aumann, H. H., and Gillespie, C. M. 1970, "Closing Astronomy's

Last Frontier - Far Infrared", Astronautics & Aeronautics, 7, 26-30.Low, F. J. et al. 1973, "Infrared Astronomy", Chap. 3, ASTRONOMY AND ASTRO

PHYSICS FOR THE 1970*S, Rept. by the Greenstein Committee, National Academyof Sciences, 50-93.

Michel, G. 1972, "Real-Time Computer for Monitoring a Rapid Scanning FourierSpectrometer", App. Optics, 11, 2671-2675.

Strom, R. G. 1972, "Lunar Mare Ridges, Rings and Volcanic Ring Complexes", inIAU Symposium No. 47, THE MOON, eds. Runcorn, S. K. and Urey, H. C, D.Reidel Publishing Co.

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