Does interplanetary dust control 100 kyr glacial cycles?

LDEO Publication: 
Publication Type  Journal Article
Year of Publication  2004
Authors  Winckler, G.; Anderson, R. F.; Stute, M.; Schlosser, P.
Journal Title  Quaternary Science Reviews
Volume  23
Issue  18-19
Pages  1873-1878
Journal Date  Oct
ISBN Number  0277-3791
Accession Number  ISI:000223906400001
LDEO Publication Number  6623
Key Words  equatorial pacific-ocean; extraterrestrial he-3; sea-floor; orbital inclination; sediment; accumulation; ice; eccentricity; periodicity; particles

The cause of the 100 kyr glacial-interglacial cycles during the past 800 kyr is one of the fundamental puzzles in paleoclimatology. The widely accepted Milankovitch theory, relating earth's climate cycles to variations in insolation caused by periodic changes in orbital parameters, has difficulties to explain the predominant 100 kyr rhythm. Although earth's eccentricity varies with a period of 100 kyr, the resulting change in insolation is too small to produce the corresponding climate cycle by direct forcing (Imbrie et al., Paleoceanography 8 (1993) 699). In order to solve the '100 kyr problem', Muller and MacDonald (Nature 377 (1995) 107; Science 277 (1997a) 215; Proc. Nat. Acad. Sci. USA 94 (1997b) 8329) proposed an alternative orbital but non-Milankovitch mechanism attributing the glacial cycles to regular variations in the accretion of interplanetary dust particles (IDP) caused by 100 kyr cycles in the orbital inclination of the earth. To test this controversial hypothesis, we study the IDP accumulation in deep-sea sediments from a period in the early Pleistocene. We find apparent 41 kyr cycles but no 100 kyr periodicity in the IDP accumulation rate. As there is no known mechanism to produce 41 kyr cycles in IDP supply from space, we conclude that the 41 kyr cycles are caused by the dynamics of sediment accumulation, and that changes in the IDP flux do not drive the Pleistocene glacial cycles. (C) 2004 Elsevier Ltd. All rights reserved.


854METimes Cited:9Cited References Count:24

URL  <Go to ISI>://000223906400001
DOI  DOI 10.1016/j.quascirev.2004.05.007