Dung Beetles Use the Milky Way for Orientation

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Dung Beetles and The Milky Way
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Dung Beetles Use the Milky Way for Orientation Marie Dacke, Emily Baird, Marcus Byrne, Clarke H. Scholtz, Eric J. Warrant  Current Biology  Volume 23, Issue 4, Pages 298-300 (February 2013) DOI: 10.1016/j.cub.2012.12.034 Copyright © 2013 Elsevier Ltd Terms and Conditions

Figure 1 The Effect of Celestial Input on the Straight-Line Orientation of Dung Beetles Paths of the dung beetle S. satyrus rolling outward from the center of a circular arena (3 m diameter, black circle) under an unobstructed (A) or an occluded (B) view of a moonless starry sky. So that the view of the sky could be blocked, small “caps” were attached to the thorax of the beetle (C). The tracking of the beetle began once it had rolled out from an inner, 30 cm diameter circle (gray circle). Current Biology 2013 23, 298-300DOI: (10.1016/j.cub.2012.12.034) Copyright © 2013 Elsevier Ltd Terms and Conditions

Figure 2 The Effect of Stars on the Orientation Performance of Ball-Rolling Dung Beetles The time taken for beetles to roll from the center of a circular arena (2 m diameter) to its edge was recorded as a measure of orientation performance in the field and in a planetarium. In the field (left panel), times were recorded on a moonlit night (moon), a moonless starlit night (starry sky), a moonless starlit night with the sky occluded by a cap (cap), and an overcast night (overcast). In the planetarium, times were recorded under four ceiling projection conditions: a complete starry sky (starry sky), a diffuse streak of light that imitates the Milky Way (Milky Way), 4,000 dim stars excluding the Milky Way (4000 dim stars), 18 brightest stars excluding the Milky Way (18 bright stars), or complete darkness (black). Asterisks indicate the results of a comparison between the orientation performance under a full starry sky (gray bars) and the other experimental conditions, either in the field or in the planetarium (∗p < 0.05, ∗∗∗p < 0.001). Error bars indicate the SEM. Current Biology 2013 23, 298-300DOI: (10.1016/j.cub.2012.12.034) Copyright © 2013 Elsevier Ltd Terms and Conditions