Published August 24, 2010 | Version Supplemental Material + Published
Journal Article Open

Filtration of submicrometer particles by pelagic tunicates

  • 1. ROR icon Woods Hole Oceanographic Institution
  • 2. ROR icon Massachusetts Institute of Technology

Abstract

Salps are common in oceanic waters and have higher per-individual filtration rates than any other zooplankton filter feeder. Although salps are centimeters in length, feeding via particle capture occurs on a fine, mucous mesh (fiber diameter d ~0.1 μm) at low velocity (U = 1.6 ± 0.6 cm•s^(−1), mean ± SD) and is thus a low Reynolds-number (Re ~10^(−3)) process. In contrast to the current view that particle encounter is dictated by simple sieving of particles larger than the mesh spacing, a low-Re mathematical model of encounter rates by the salp feeding apparatus for realistic oceanic particle-size distributions shows that submicron particles, due to their higher abundances, are encountered at higher rates (particles per time) than larger particles. Data from feeding experiments with 0.5-, 1-, and 3-μm diameter polystyrene spheres corroborate these findings. Although particles larger than 1 μm (e.g., flagellates, small diatoms) represent a larger carbon pool, smaller particles in the 0.1- to 1-μm range (e.g., bacteria, Prochlorococcus) may be more quickly digestible because they present more surface area, and we find that particles smaller than the mesh size (1.4 μm) can fully satisfy salp energetic needs. Furthermore, by packaging submicrometer particles into rapidly sinking fecal pellets, pelagic tunicates can substantially change particle-size spectra and increase downward fluxes in the ocean.

Additional Information

© 2010 by the National Academy of Sciences. Edited by Mimi A. R. Koehl, University of California, Berkeley, CA, and approved July 14, 2010 (received for review March 17, 2010). Published online before print August 9, 2010. We thank those who facilitated our work at the Liquid Jungle Lab, Panama, especially Ellen Bailey, Luis Camilli, and numerous SCUBA divers. Mark Wells, Hugh Ducklow, and Dariusz Stramski, as well as two anonymous reviewers, provided insightful comments relating to the manuscript. This work was supported by National Science Foundation Grants OCE-0647723 (to L.P.M.) and OCE-074464-CAREER (to R.S.) and the Woods Hole Oceanographic Institution Ocean Life Institute. Author contributions: K.R.S, L.P.M., and R.S. designed research; K.R.S., L.P.M., and R.S. performed research; K.R.S. analyzed data; and K.R.S, L.P.M., and R.S. wrote the paper.

Attached Files

Published - Sutherland2010p11306P_Natl_Acad_Sci_Usa.pdf

Supplemental Material - pnas.201003599SI.pdf

Supplemental Material - sapp.pdf

Supplemental Material - sm01.avi

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Additional details

Identifiers

PMCID
PMC2930554
Eprint ID
19909
Resolver ID
CaltechAUTHORS:20100913-113946215

Funding

NSF
OCE-0647723
NSF
OCE-074464
Woods Hole Oceanographic Institution

Dates

Created
2010-09-15
Created from EPrint's datestamp field
Updated
2021-11-08
Created from EPrint's last_modified field