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Asteroid Albedos and Diameters

Published online by Cambridge University Press:  19 July 2016

Edward F. Tedesco
Edward F. Tedesco*
Affiliation:
Mission Research Corporation, One Tara Boulevard, Nashua, NH 03062 USA E-mail etedesco@pldac.plh.af.mil

Abstract

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This paper discusses the status of our knowledge regarding asteroid sizes and albedos. It presents a brief discussion of the methods used to determine sizes and albedos beginning with attempts using filar micrometers as early as 1802 and culminating with the 1993 publication of the IRAS Minor Planet Survey. It addresses the completeness and reliability of the IRAS Minor Planet Survey, summarizes the statistical adjustments made to the derived results, and considers the implications of those results.

Information

Type
Populations of Small Bodies
Information
Symposium - International Astronomical Union , Volume 160: Asteroids, Comets, Meteors 1993 , 1994 , pp. 55 - 74
Copyright
Copyright © Kluwer 1994 

References

Allen, D.A.: 1971, “The method of determining infrared diameters”. In Physical Studies of Minor Planets (Gehrels, T., Ed.), NASA SP-267, pp. 41–44.Google Scholar
Barnard, E.E.: 1894, “On the diameters of Ceres, Pallas, and Vesta”. Astron. & Astrophys. 13, 341–344.Google Scholar
Barnard, E.E.: 1895, “Micrometrical determinations of the diameters of the minor plan ets Ceres (1), Pallas (2), Juno (3), and Vesta (4), made with the filar micrometer of the 36-inch equatorial of the Lick Observatory, and on the albedos of those planets”. Monthly Not. Roy. Astron. Soc. 56, 55–63.Google Scholar
Barnard, E.E.: 1900a, “On the diameter of Ceres and Vesta”. Monthly Not. Roy. Astron. Soc. 60, 261–263.Google Scholar
Barnard, E.E.: 1900b, “The diameter of the asteroid Juno (3) determined with the micrometer of the 40-inch refractor of the Yerkes Observatory, with remarks on some of the other asteroids”. Monthly Not. Roy. Astron. Soc. 61, 68–69.Google Scholar
Cellino, A., Zappala, V., and Farinella, P.: 1991, “The size distribution of main-belt asteroids from IRAS data”. Monthly Not. Roy. Astron. Soc. 253, 561–574.CrossRefGoogle Scholar
Cohen, M., Schwartz, D.E., Chokshi, A., and Walker, R.G.: 1987, “IRAS colors of normal stars”. Astron. J. 93, 1199–1219.Google Scholar
Dollfus, A.: 1971, “Diameter measurements of asteroids”. In Physical Studies of Minor Planets (Gehrels, T., Ed.), NASA SP-267, pp. 25–32.Google Scholar
Dollfus, A., Wolff, M., Geake, J.E., Lupishko, D.F., and Dougherty, L.M.: 1989, “Photopolarimetry of asteroids”. In Asteroids II (Binzel, R.P., Gehrels, T., and Matthews, M.S., Eds.), University of Arizona Press, Tucson, pp. 594–616.Google Scholar
Drummond, J.D. and Hege, E.K.: 1989, “Speckle interferometry of asteroids”. Ibid, pp. 171–191.Google Scholar
Dunham, D.W.: 1991, “Asteroid news”. Occultation Newsletter 5, 93.Google Scholar
Dunham, D.W. and 45 others: 1990, “The size and shape, of (2) Pallas from the 1983 occultation of 1 Vulpeculae”. Astron. J. 99, 1636–1662.Google Scholar
Gradie, J. and Tedesco, E.F.: 1988, “Albedos and diameters for 350 asteroids from the IRTF 10 μm and 20 μm radiometry survey”. Bull. Amer. Astron. Soc. 20, 866.Google Scholar
The IRAS Minor Planet Survey, 1992, edited by Tedesco, E. F. Phillips Laboratory Technical Report No. PL-TR-92-2049. Hanscom Air Force Base, MA.Google Scholar
Infrared Astronomical Satellite Asteroid and Comet Survey: Preprint Version No. 1, 1986, edited by Matson, D.L., JPL Internal Document No. D-3698. (Jet Propulsion Laboratory, Pasadena)Google Scholar
IRAS Catalogs and Atlases, Volume 1, Explanatory Supplement, 1988, edited by Beichman, C.A., Neugebauer, G., Habing, H.J., Clegg, P.E. and Chester, T.J. (NASA Publication No. RP-1190, Washington D.C.: U.S. Government Printing Office).Google Scholar
KenKnight, C.E., Rosenberg, D.L., and Wehner, G.K.: 1967. “Parameters of the optical properties of the lunar surface powder in relation to solar wind bombardment”. J. Geophys. Res. 72, 3105–3117.Google Scholar
Lebofsky, L.A. and Spencer, J.R.: 1989. “Radiometry and thermal modeling of asteroids”. In Asteroids II (Binzel, R.P., Gehrels, T., and Matthews, M.S., Eds.), University of Arizona Press, Tucson, pp. 128–147.Google Scholar
Lebofsky, L.A., Matson, D.L., Veeder, G.J., and Tedesco, E.F.: 1986a. “The IRAS asteroid thermal model”. In Infrared Astronomical Satellite Asteroid and Comet Survey, Matson, D. L., ed. (JPL D-3698, Jet Propulsion Laboratory, Pasadena), pp. 7–1 to 7–18.Google Scholar
Lebofsky, L.A., Sykes, M.V., Tedesco, E.F., Veeder, G.J., Matson, D.L., Brown, R.H., Gradie, J.C., Feierberg, M.A. and Rudy, R.J.: 1986b. “A refined “standard” thermal model for asteroids based on observations of 1 Ceres and 2 Pallas”. Icarus 68, 239–251.CrossRefGoogle Scholar
Matson, D.L., Veeder, G.J., Tedesco, E.F., and Lebofsky, L.A.: 1989. “The IRAS Asteroid and Comet Survey”. In Asteroids II, Binzel, R., Gehrels, T. and Matthews, M., eds. (University of Arizona Press, Tucson), pp. 269–281.Google Scholar
Millis, R.L. and Dunham, D.W.: 1989. “Precise measurement of asteroid sizes and shapes from occultations”. In Asteroids II (Binzel, R.P., Gehrels, T., and Matthews, M.S., Eds.), University of Arizona Press, Tucson, pp. 148–170.Google Scholar
Millis, R.L. and 37 others: 1981. “The diameter of Juno from its occultation of AG +0° 1022”. Astron. J. 86, 306–313.Google Scholar
Millis, R.L. and 41 others: 1987, “The size, shape, density, and albedo of Ceres from its occultation of BD +8° 471”. Icarus 72, 507–518.Google Scholar
Morrison, D. and Zellner, B.: 1979, “Polarimetry and radiometry of the asteroids”. In Asteroids II (Binzel, R.P., Gehrels, T., and Matthews, M.S., Eds.), University of Arizona Press, Tucson, pp. 1090–1097.Google Scholar
Ostro, S.J.: 1989, “Radar observations of asteroids”. In Asteroids II (Binzel, R.P., Gehrels, T., and Matthews, M.S., Eds.), University of Arizona Press, Tucson, pp. 192–212.Google Scholar
Tedesco, E.F.: 1989a, “Introduction to the Asteroids II data base”. In Asteroids II, (Binzel, R., Gehrels, T. and Matthews, M., Eds.) pp. 997–1001, University of Arizona Press, Tucson.Google Scholar
Tedesco, E.F.: 1989b, “Asteroid magnitudes, UBV colors and IRAS albedos and diameters”. In Asteroids II, (Binzel, R., Gehrels, T. and Matthews, M., Eds.) pp. 1090–1138, University of Arizona Press, Tucson.Google Scholar
Tedesco, E.F. and Gradie, J.C.: 1988, “IRAS Vs. IRTF asteroid radiometric albedos”. Bull. Amer. Astron. Soc. 20, 865.Google Scholar
Tedesco, E.F., Gradie, J.C., and Lebofsky, L.A.: 1990, “Size dependence of radiometric diameters and albedos”. Bull. Amer. Astron. Soc. 22, 1113.Google Scholar
Tedesco, E.F., Fowler, J.W., and Chester, T.J.: 1992, “Summary”. In Infrared Astronomical Satellite Minor Planet Survey Catalog, 1992 (Tedesco, E.F., Ed.), pp. 127–148. Phillips Laboratory Technical Report No. PL-TR-92-2049. Hanscom Air Force Base, MA.Google Scholar
Tedesco, E.F., Matson, D.L. and Veeder, G.J.: 1989a, “Classification of IRAS asteroids”. In Asteroids II, Binzel, R., Gehrels, T. and Matthews, M., eds. (University of Arizona Press, Tucson), pp. 290–297.Google Scholar
Tedesco, E.F., Williams, J.G., Matson, D.L., Veeder, G.J., Gradie, J.C. and Lebofsky, L.A.: 1989b, “A three-parameter asteroid taxonomy”. Astron. J. 97, 580–606.Google Scholar
Veeder, G.J.: 1991, “Evidence against dusty regoliths on small main belt asteroids”. Bull. Amer. Astron. Soc. 23, 1155.Google Scholar
Veeder, G.J., Hanner, M.S., Matson, D.L., Tedesco, E.F., Lebofsky, L.A. and Tokunaga, A.T.: 1989a, “Radiometry of near-Earth asteroids”. Astron. J. 97, 1211–1219.Google Scholar
Veeder, G.J., Tedesco, E.F., and Matson, D.L.: 1989b, “Asteroid results from the IRAS survey”. In Asteroids II, Binzel, R., Gehrels, T. and Matthews, M., eds. (University of Arizona Press, Tucson), pp. 282–289.Google Scholar
Zellner, B. Leake, M., Le Bertre, T., Duseaux, M., and Dollfus, A.: 1977a, “The asteroid albedo scale. I - Laboratory polarimetry of meteorites”. Proc. Lunar Sci. Conf. 8, 1091–1100.Google Scholar
Zellner, B. Le Bertre, T., and Day, K.: 1977b, “The asteroid albedo scale. II – Laboratory polarimetry of dark carbon-bearing silicates”. Proc. Lunar Sci. Conf. 8, 1111–1117.Google Scholar