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1.1.5 Star Counts in the Background Sky Observed from Pioneer 10

Published online by Cambridge University Press:  12 April 2016

H. Tanabe
Affiliation:
Tokyo Astronomical Observatory, Mitaka, Tokyo, Japan
K. Mori
Affiliation:
Tokyo Astronomical Observatory, Mitaka, Tokyo, Japan

Abstract

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Star counts in the sky region observed by Pioneer 10 at 4.64AU from the sun, where the contribution of zodiacal light is negligible, were made using the Palomar Sky Survey Atlas. Brightness of the integrated starlight derived from our star counts agrees, in general, with the Pioneer 10’s observation.

Type
1 Zodiacal Light
Copyright
Copyright © Springer-Verlag 1976

References

Allen, C.W.(1973) “Astrophysical Quantities 3rd ed.”, p.162, p. 203, University of London, the Athlone Press.Google Scholar
Hanner, M.S., Weinberg, J.L., DeShields, L.M. II, Green, B.A. and Toller, G.N.(1974) J. Geophys. Res., 79, 3671.Google Scholar
Roach, F.E. and Megill, L.R.(1961) Astrophys. J., 133, 228.CrossRefGoogle Scholar
Seares, F.H.(1925) Astrophys. J., 61, 114.CrossRefGoogle Scholar
Smithsonian Astrophysical Observatory Star Catalog(1966) Smithsonian Institution, Washington, D.C. Google Scholar
Tanabe, H. and Mori, K.(1971) Publ. Roy. Obs. Edinburgh, 8, 173.Google Scholar
Tanabe, H.(1973) “Papers on the Night Sky Light and Airglow Data at Chichijima”, p.48, Tokyo Astronomical Observatory.Google Scholar
van Rhijn, P.J.(1925) Groningen Publ., No.43.Google Scholar
Weinberg, J.L., Hanner, M.S., Beeson, D.E., DeShields, L.M. II and Green, B.A.(1974) J. Geophys. Res., 79, 3665.CrossRefGoogle Scholar
Weinberg, J.L.(1975) private communication.Google Scholar