2017
DOI: 10.1130/focus012017.1
|View full text |Cite
|
Sign up to set email alerts
|

Do mercury isotopes record the signature of massive volcanism in marine sedimentary records?

Abstract: Large Igneous Provinces (LIPs) are associated with a significant number of mass extinctions and ocean anoxic events (OAEs) during the Phanerozoic. However, the role of LIPs in triggering and sustaining biotic and environmental crises is controversial (e.g., Bond and Wignall, 2014).

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

1
55
0

Year Published

2017
2017
2021
2021

Publication Types

Select...
4
2
1

Relationship

1
6

Authors

Journals

citations
Cited by 63 publications
(56 citation statements)
references
References 20 publications
1
55
0
Order By: Relevance
“…Further tests of our hypothesis will be possible via tighter constraints on the geochronology of the Sturtian glaciation and the Franklin LIP, and better estimates of sulfur release with melt inclusion studies along with three‐dimensional coupled ocean‐atmosphere modeling of the climate effect of stratospheric aerosol emissions. Mercury anomalies have been observed in sedimentary records that span the Permian‐Triassic and Triassic‐Jurassic boundaries and have been attributed to the Siberian Traps and CAMP, respectively [ Thibodeau and Bergquist , , and references therein]. Our model predicts that similar mercury signals will be present in sedimentary successions deposited during onset of the Sturtian glaciation.…”
Section: Resultsmentioning
confidence: 99%
“…Further tests of our hypothesis will be possible via tighter constraints on the geochronology of the Sturtian glaciation and the Franklin LIP, and better estimates of sulfur release with melt inclusion studies along with three‐dimensional coupled ocean‐atmosphere modeling of the climate effect of stratospheric aerosol emissions. Mercury anomalies have been observed in sedimentary records that span the Permian‐Triassic and Triassic‐Jurassic boundaries and have been attributed to the Siberian Traps and CAMP, respectively [ Thibodeau and Bergquist , , and references therein]. Our model predicts that similar mercury signals will be present in sedimentary successions deposited during onset of the Sturtian glaciation.…”
Section: Resultsmentioning
confidence: 99%
“…The positive  199 Hg shift is consistent with increased direct atmospheric deposition of volcanically derived Hg 2+ to the ocean (Thibodeau and Bergquist, 2017). This shift also coincides with the reef demise, implying that onset of ELIP eruption, marked by increased Hg 2+ , may have caused reef development to cease through significant CO2 release triggering greenhouse warming, as seen in conodont oxygen isotopes record (Chen et al, 2011).…”
Section: Environment Perturbationsmentioning
confidence: 53%
“…DR4) suggests that the stratigraphic pattern of Hg concentration is not due to 176 variation in TOC content. With respect to Hg sources, volcanic Hg has insignificant MIF 177 ( 199 Hg 0 ‰) (Thibodeau and Bergquist, 2017). Once emitted to the environment, MIF 178 ( 199 Hg) mostly occurs and results in positive  199 Hg values (Blum et al, 2014).…”
Section: Environment Perturbationsmentioning
confidence: 99%
“…Mercury can undergo complex geochemical transformation processes in the environment, that may induce mass dependent fractionation (MDF) and mass independent fractionation (MIF) of Hg isotopes 25,45,46 . MDF can occur during various physical, chemical, or biological transformations of Hg, whereas MIF is generated through a more limited set of pathways (mostly photochemical), making it a more conservative tracer 46 . Generally, Hg derived from volcanic eruptions or geogenic sources has insignificant MIF (Δ 199 Hg ~ 0‰) with δ…”
Section: A Late Ordovician Lip Eventmentioning
confidence: 99%
“…When released to the environment, Hg cycles through the atmospheric, marine, and terrestrial reservoirs 46 . In the atmosphere, odd-isotope MIF can be generated through the aqueous photoreduction of Hg 2+ 48 , such as in surface waters and cloud droplets, resulting in excess odd-isotope (i. Hg values at two extinction levels are negligible, suggesting that the Hg spikes are not related to changes in the background Hg source, but rather just enhanced loading from those sources (volcanoes).…”
mentioning
confidence: 99%