Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-43723
Scott, A C; Pinter, N; Collinson, M E; Hardiman, M; Anderson, R. S; Brain, A P R; Smith, S Y; Marone, F; Stampanoni, M (2010). Fungus, not comet or catastrophe, accounts for carbonaceous spherules in the Younger Dryas “impact layer”. Geophysical Research Letters, 37(14):L14302.
A claim attributes the onset of the Younger Dryas climate interval and a range of other effects ∼12,900 years ago to a comet airburst and/or impact event. One key aspect of this claim centers on the origin of carbonaceous spherules that purportedly formed during intense, impact-ignited wildfires. Samples from Pleistocene-Holocene sedimentary sequences in the California Channel Islands and other sites show that carbon spherules and elongate forms are common in samples dating to before, during, and well after the 12,900-year time horizon, including from modern samples. Microscopic studies show that carbon spherules have morphologies and internal structures identical to fungal sclerotia (such as Sclerotium and Cenococcum). Experimental charring of fungal sclerotia shows that their reflectance increases with temperature. Reflectance measurements of modern and late Pleistocene spherules show that the latter indicate, at most, low-intensity burning. These data cast further doubt upon the evidence suggesting a catastrophic Younger Dryas impact event.
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||04 Faculty of Medicine > Institute of Biomedical Engineering|
610 Medicine & health
|Deposited On:||30 Jan 2011 22:45|
|Last Modified:||27 Nov 2013 23:27|
|Publisher:||American Geophysical Union|
|Citations:||Web of Science®. Times cited: 14|
Users (please log in): suggest update or correction for this item
Repository Staff Only: item control page