Stellar performance: mechanisms underlying Milky Way orientation in dung beetles
Author(s) -
James J. Foster,
Basil el Jundi,
Jochen Smolka,
Lana Khaldy,
Dan-Eric Nilsson,
Marcus J. Byrne,
Marie Dacke
Publication year - 2017
Publication title -
philosophical transactions of the royal society b biological sciences
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.753
H-Index - 272
eISSN - 1471-2970
pISSN - 0962-8436
DOI - 10.1098/rstb.2016.0079
Subject(s) - milky way , context (archaeology) , physics , orientation (vector space) , ecology , biology , astronomy , paleontology , geometry , galaxy , mathematics
Nocturnal dung beetles (Scarabaeus satyrus ) are currently the only animals that have been demonstrated to use the Milky Way for reliable orientation. In this study, we tested the capacity ofS. satyrus to orient under a range of artificial celestial cues, and compared the properties of these cues with images of the Milky Way simulated for a beetle's visual system. We find that the mechanism that permits accurate stellar orientation under the Milky Way is based on an intensity comparison between different regions of the Milky Way. We determined the beetles' contrast sensitivity for this task in behavioural experiments in the laboratory, and found that the resulting threshold of 13% is sufficient to detect the contrast between the southern and northern arms of the Milky Way under natural conditions. This mechanism should be effective under extremely dim conditions and on nights when the Milky Way forms a near symmetrical band that crosses the zenith. These findings are discussed in the context of studies of stellar orientation in migratory birds and itinerant seals.This article is part of the themed issue ‘Vision in dim light’.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom