Data obtained by the Cassini spacecraft show that the plume of ice particles at the south pole of Saturn's moon Enceladus is four times brighter when the moon is farthest away from the planet than when it is closest. See Letter p.182
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*This article and the paper under discussion1 were published online on 31 July 2013.
Hedman, M. M. et al. Nature 500, 182–184 (2013).
Hurford, T. A., Helfenstein, P., Hoppa, G. V., Greenberg, R. & Bills, B. G. Nature 447, 292–294 (2007).
Spencer, J. R. & Nimmo, F. Annu. Rev. Earth Planet. Sci. 41, 693–717 (2013).
Postberg, F., Schmidt, J., Hillier, J., Kempf, S. & Srama, R. Nature 474, 620–622 (2011).
Waite, J. H. et al. Nature 460, 487–490 (2009).
Spitale, J. N. & Porco, C. C. Nature 449, 695–697 (2007).
Roberts, J. H. & Nimmo, F. Icarus 194, 675–689 (2008).
Collins, G. C. & Goodman, J. C. Icarus 189, 72–82 (2007).
Porco, C., DiNino, D. & Nimmo, F. 44th Lunar Planet. Sci. Conf. abstr. 1775 (2013).
Crow-Willard, E. & Pappalardo, R. T. EPSC Abstr. 6, EPSC-DPS2011-635-1 (2011).
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Spencer, J. Saturn's tides control Enceladus' plume. Nature 500, 155–156 (2013). https://doi.org/10.1038/nature12462