Abstract
It is well-known that the asteroid mean opposition magnitude ℄ B(a,0) ℄ represent a crude approximation of asteroid average opposition brightness, especially for objects of high eccentricity and/or inclination. In the paper we propose a new simple method of calculating the “quasi-median opposition magnitude”, which very closely matches the median apparent brightness of an asteroid in opposition.
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References
Kiang,T.: 1966, Icarus, 5, pp. 437–449.
Kneževié, Z.: 1981, submitted to Bull.Astron.Inst.Czech.
Kresák, L.: 1967, BUll.AStron.Inst.CZech., 18, pp. 27–36.
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© 1982 D. Reidel Publishing Company
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Knežević, Z., Zappalà, V. (1982). An Improved Representation of the Average Opposition Magnitudes of Asteroids. In: Fricke, W., Teleki, G. (eds) Sun and Planetary System. Astrophysics and Space Science Library, vol 96. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7846-1_81
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DOI: https://doi.org/10.1007/978-94-009-7846-1_81
Publisher Name: Springer, Dordrecht
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