Abstract

A basic question concerning the monarch butterflies’ fall migration is which monarchs succeed in reaching overwintering sites in Mexico, which fail—and why. We document the timing and pace of the fall migration, ask whether the sun’s position in the sky is associated with the pace of the migration, and whether timing affects success in completing the migration. Using data from the Monarch Watch tagging program, we explore whether the fall monarch migration is associated with the daily maximum vertical angle of the sun above the horizon (Sun Angle at Solar Noon, SASN) or whether other processes are more likely to explain the pace of the migration. From 1998 to 2015, more than 1.38 million monarchs were tagged and 13,824 (1%) were recovered in Mexico. The pace of migration was relatively slow early in the migration but increased in late September and declined again later in October as the migrating monarchs approached lower latitudes. This slow-fast-slow pacing in the fall migration is consistent with monarchs reaching latitudes with the same SASN, day after day, as they move south to their overwintering sites. The observed pacing pattern and overall movement rates are also consistent with monarchs migrating at a pace determined by interactions among SASN, temperature, and daylength. The results suggest monarchs successfully reaching the Monarch Butterfly Biosphere Reserve (MBBR) migrate within a “migration window” with an SASN of about 57° at the leading edge of the migration and 46° at the trailing edge. Ninety percent of the tags recovered in Mexico were from monarchs tagged within this window. Migrants reaching locations along the migration route with SASN outside this migration window may be considered early or late migrants. We noted several years with low overwintering abundance of monarchs, 2004 and 2011–2014, with high percentages of late migrants. This observation suggests a possible effect of migration timing on population size. The migration window defined by SASN can serve as a framework against which to establish the influence of environmental factors on the size, geographic distribution, and timing of past and future fall migrations.

Highlights

  • The eastern North American migratory population of monarch butterflies (Danaus plexippus) can migrate more than 4,000 km in late summer and early fall from breeding areas encompassing hundreds of millions of hectares across the eastern U.S and Canada to reach Mexican overwintering sites comprising fewer than 20 hectares (Brower, 1997)

  • Whether a causal relationship exists between Sun Angle at Solar Noon (SASN) and monarchs is not known and requires further study; SASN is associated with migratory success, since 90% of the recovered tags across all latitudes were tagged within a migration window defined by SASN values of 56.8◦–46.0◦

  • Whether a causal relationship exists between SASN and monarchs is not known and requires further study; however, SASN is associated with migratory success, since 90% of the recovered tags across all latitudes were tagged within a migration window defined by SASN values of 56.8◦–46.0◦

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Summary

Introduction

The eastern North American migratory population of monarch butterflies (Danaus plexippus) can migrate more than 4,000 km in late summer and early fall from breeding areas encompassing hundreds of millions of hectares across the eastern U.S and Canada to reach Mexican overwintering sites comprising fewer than 20 hectares (Brower, 1997). Pace here refers to the distance advanced per day and timing refers to the date at which a monarch was recorded within the migration To address these questions, we use data from the long-term monarch tagging program created by Monarch Watch (MW) to explore whether the fall migration from the eastern U.S and Canada to Mexico is an orderly and predictable process, possibly associated with the daily maximum vertical angle of the sun above the horizon (Sun Angle at Solar Noon, SASN). There are many possible cues for monarch migration initiation and pacing, solar cues, weather effects, and daylength may be related to changes in monarch physiology and behavior that initiate and affect the pace of the migration south to Mexico (Barker and Herman, 1976; Reppert and de Roode, 2018). We compare the pacing of the migration determined from MW tagging records to the pace that might be associated with monarchs following spatial and temporal variation in temperature, daylength, and SASN across latitudes

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