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The lightcurve describes the temporal variation of the brightness of an object.
Overview
The lightcurve shows the temporal variation of the brightness of a celestial body at a given wavelength. When due to the rotation of an object, the lightcurve generally has a sinusoidal periodic behavior with two maxima and two minima. In planetary science, the lightcurve is the most useful tool for investigating the rotational properties and the shape of a body, mainly of small ones: asteroids, satellites, comets, and transneptunian objects.
Most small bodies cannot be resolved since the apparent angular size of the object is in general smaller than the observer’s angular resolution; therefore, analysis of the lightcurve can be used to determine the shape and the surface spots of the observed body.
For an airless body each point of the lightcurve represents the fraction of the sunlight reflected by the illuminated portion of the body surface in the direction of...
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References and Further Reading
Kaasalainen M, Mottola S, Fulchignoni M (2002) Asteroid models from disk-integrated data. In: Bottke WF, Cellino A, Paolicchi P, Binzel RP (eds) Asteroids III. University of Arizona Press, Tucson, pp 139–150
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© 2011 Springer-Verlag Berlin Heidelberg
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Barucci, M.A. (2011). Lightcurve (Planetary Science). In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-11274-4_883
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DOI: https://doi.org/10.1007/978-3-642-11274-4_883
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-11271-3
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