Identification of a meteoritic component using chromium isotopic composition of impact rocks from the Lonar impact structure,India     

Berengere Mougel  Frederic Moynier  Christian Koeberl  Daniel Wielandt  Martin Bizzarro 《Meteoritics & planetary science》2019,54(10):2592-2599

The existence of mass‐independent chromium isotope variability of nucleosynthetic origin in meteorites and their components provides a means to investigate potential genetic relationship between meteorites and planetary bodies. Moreover, chromium abundances are depleted in most surficial terrestrial rocks relative to chondrites such that Cr isotopes are a powerful tool to detect the contribution of various types of extra‐terrestrial material in terrestrial impactites. This approach can thus be used to constrain the nature of the bolide resulting in breccia and melt rocks in terrestrial impact structures. Here, we report the Cr isotope composition of impact rocks from the ~0.57 Ma Lonar crater (India), which is the best‐preserved impact structure excavated in basaltic target rocks. Results confirm the presence of a chondritic component in several bulk rock samples of up to 3%. The impactor that created the Lonar crater had a composition that was most likely similar to that of carbonaceous chondrites, possibly a CM‐type chondrite.  相似文献   

Coagulation and settling of dust in a turbulent protoplanetary disk     

Michael F. Sterzik  Gregor E. Morfill  Berengere Dubrulle 《Astrophysics and Space Science》1995,224(1-2):567-568

We apply our analytic model for the dust diffusivity to calculate the vertical structure of the dust sub-disk in a turbulent protoplanetary nebula. We present a numerical solution of a vertical dust settling equationand a coagulation equation for dust grains covering four orders of magnitude in time and grain size.  相似文献   

Pantasma: Evidence for a Pleistocene circa 14 km diameter impact crater in Nicaragua     

P. Rochette  R. Ala  P. Beck  G. Brocard  A. J. Cavosie  V. Debaille  B. Devouard  F. Jourdan  B. Mougel  F. Moustard  F. Moynier  S. Nomade  G. R. Osinski  B. Reynard  J. Cornec 《Meteoritics & planetary science》2019,54(4):880-901

The circa 14 km diameter Pantasma circular structure in Oligocene volcanic rocks in Nicaragua is here studied for the first time to understand its origin. Geomorphology, field mapping, and petrographic and geochemical investigations all are consistent with an impact origin for the Pantasma structure. Observations supporting an impact origin include outward‐dipping volcanic flows, the presence of former melt‐bearing polymict breccia, impact glass (with lechatelierite and low H₂O, <300 ppm), and also a possible ejecta layer containing Paleozoic rocks which originated from hundreds of meters below the surface. Diagnostic evidence for impact is provided by detection in impact glass of the former presence of reidite in granular zircon as well as coesite, and extraterrestrial ε⁵⁴Cr value in polymict breccia. Two ⁴⁰Ar/³⁹Ar plateau ages with a combined weighted mean age of 815 ± 11 ka (2 σ; P = 0.17) were obtained on impact glass. This age is consistent with geomorphological data and erosion modeling, which all suggest a rather young crater. Pantasma is only the fourth exposed crater >10 km found in the Americas south of N30 latitude, and provides further evidence that a significant number of impact craters may remain to be discovered in Central and South America.  相似文献