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Fig. 6.4 Shoemaker-Levy 9 colliding into Jupiter in 1994. Eight impact sites are visible. From left
to right are the E/F complex (barely visible on the edge of the planet), the star-shaped H site, the
impact sites for tiny N, Q1, small Q2, and R, and on the far right limb the D/G complex. The D/G
complex also shows extended haze at the edge of the planet. The features are rapidly evolving on
timescales of days. The smallest features in this image are less than 200 km across. This image is
a color composite from three filters at 9,530, 5,550, and 4,100 A (Copyright free, image released
into the public domain by NASA)
Fig. 6.5 Interpretations
of the key evidence by
competing paradigms in the
KT debate
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