Zhamanshin astrobleme provides evidence for carbonaceous chondrite and post-impact exchange between ejecta and Earth's atmosphere

Tomáš Magna, Karel Žák, Andreas Pack, Frédéric Moynier, Bérengère Mougel, Stefan Peters, Roman Skála, Šárka Jonášová, Jirí Mizera, Zdenek Randa

Rannsóknarafurð: Framlag til fræðitímaritsGreinritrýni

13 Tilvitnanir (Scopus)

Útdráttur

Chemical fingerprints of impacts are usually compromised by extreme conditions in the impact plume, and the contribution of projectile matter to impactites does not often exceed a fraction of per cent. Here we use chromium and oxygen isotopes to identify the impactor and impact-plume processes for Zhamanshin astrobleme, Kazakhstan. e54Cr values up to 1.54 in irghizites, part of the fallback ejecta, represent the 54Cr-rich extremity of the Solar System range and suggest a CI-like chondrite impactor. Δ17O values as low as -0.22% in irghizites, however, are incompatible with a CI-like impactor. We suggest that the observed 17O depletion in irghizites relative to the terrestrial range is caused by partial isotope exchange with atmospheric oxygen (Δ17O = -0.47%) following material ejection. In contrast, combined δ17O-e54Cr data for central European tektites (distal ejecta) fall into the terrestrial range and neither impactor fingerprint nor oxygen isotope exchange with the atmosphere are indicated.

Upprunalegt tungumálEnska
Númer greinar227
FræðitímaritNature Communications
Bindi8
Númer tölublaðs1
DOI
ÚtgáfustaðaÚtgefið - 1 des. 2017

Athugasemd

Publisher Copyright:
© The Author(s) 2017.

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