Grains formed by impact reaction found at spherules of various impact craters, meteorite showers and geological boundaries

In situ analysis of residues resulting from laboratory impacts into aluminum 1100 foil: Implications for Stardust crater analyses

Wozniakiewicz, P. J.
Kearsley, A. T.
Burchell, M. J.
Foster, N. J.
Cole, M. J.
Bland, P. A.
Russell, S. S.

January 2009

The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...

A Classification of Extraterrestrial Spherules Found in Sedimentary Rocks and Till

Lougheed, M. S.

May 1966

Author Institution: Department of Geology, Bowling Green State University, Bolwing Green, OhioExtrat...

Ni-rich spinels and platinum group element nuggets condensed from a Late Archaean impact vapour cloud

Goderis, Steven
Simonson, Bruce M.
McDonald, Iain
Hassler, Scott W.
Izmer, Andrei
Belza, Joke
Terryn, Herman
Vanhaecke, Frank
Claeys, Philippe

January 2013

Deciphering Earthʼs impact history before ∼2 Ga relies heavily on the lunar record and terrestrial s...

New impact fragments of Fe-Ni-Si spherules at Takamatsu Crater, Japan

Miura, Y.
Fukuyama, S.
Gucsik, Arnold

January 1999

Fe-Ni-Si grains trapped in vacant regions formed by impact events on granitic rock are found in sphe...

Chemical separation of Fe-Ni particles after impact

Miura, Y.
Fukuyama, S.
Kedves, M. A.
Yamori, A.
Okamoto, M.
Gucsik, Arnold

January 2000

Tiny grains of Fe-Ni system originated from planetesimals or meteoroids can remain under solid (or m...

The mineralogy and petrology of I-type cosmic spherules:Implications for their sources, origins and identification in sedimentary rocks

Genge, Matthew John
Davies, Bridie
Suttle, Martin D.
van Ginneken, Matthias
Tomkins, Andrew G.

December 2017

I-type cosmic spherules are micrometeorites that formed by melting during atmospheric entry and cons...

The mineralogy and petrology of I-type cosmic spherules: Implications for their sources, origins and identification in sedimentary rocks

Genge, Matthew J.
Davies, Bridie
Suttle, Martin D.
van Ginneken, Matthias
Tomkins, Andrew G.

September 2017

I-type cosmic spherules are micrometeorites that formed by melting during atmospheric entry and cons...

Impact metamorphosed compositions of the Fe-Si-Ni-S system

Miura, Y.
Fukuyama, S.
Gucsik, Arnold

January 1999

The characterization of impact materials is discussed from the point of view of compositional change...

Spherule layers—records of ancient impacts

Simonson, Bruce M.
Glass, Billy P.

May 2004

A large extraterrestrial object striking Earth at cosmic velocity melts and vaporizes silicate mater...

Microscopic impactor debris at Kamil crater (Egypt): the origin of the Fe,Ni-oxide microscopic spherules

CARONE, LAURA

November 2017

Il cratere di Kamil è un piccolo (45 metri in diametro) cratere da impatto situato nell’Egitto sud-o...

Description, chemical composition, and origin of six microscopic spherules collected from the meteorite moraine in Antarctica: an SEM study

Wight, Shawn

March 1995

Microscopic spherules (100-1000 micrometers) have been found in glacial moraine deposits in Antarcti...

Moderate velocity oblique impact sliding: Production of shocked meteorite textures and palaeomagnetically important metallic spherules in planetary regoliths

Potter, David K.
Ahrens, Thomas J.

April 2013

We detail the production of metallic spherules in laboratory oblique shock impact experiments, and t...

Origin and formation of iron silicide phases in the aerogel of the Stardust mission

Rietmeijer, F. J. M.
Nakamura, T.
Tsuchiyama, A.
Uesugi, K.
Nakano, T.
Leroux, H.

January 2008

Suessite along with hapkeite and more Fe-rich iron-silicides up to Fe7Si2 formed near the entrance o...

Shock Metamorphism and Impact Melting at Kamil Crater, Egypt

FAZIO, AGNESE

March 2015

Shock effects in small terrestrial impact craters (diameter < 300 m) have been poorly studied becaus...

Trace element concentrations in iron type cosmic spherules determined by the SR-XRF method

Nozaki,Wataru
Nakamura,Tomoki
Iida,Atsuo
Matsuoka,Kenji
Takaoka,Nobuo

March 1999

The X-ray fluorescence method using synchrotron radiation (SR-XRF) was applied to determine trace el...

In situ analysis of residues resulting from laboratory impacts into aluminum 1100 foil: Implications for Stardust crater analyses

Wozniakiewicz, P. J.
Kearsley, A. T.
Burchell, M. J.
Foster, N. J.
Cole, M. J.
Bland, P. A.
Russell, S. S.

January 2009

The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...

A Classification of Extraterrestrial Spherules Found in Sedimentary Rocks and Till

Lougheed, M. S.

May 1966

Author Institution: Department of Geology, Bowling Green State University, Bolwing Green, OhioExtrat...

Ni-rich spinels and platinum group element nuggets condensed from a Late Archaean impact vapour cloud

Goderis, Steven
Simonson, Bruce M.
McDonald, Iain
Hassler, Scott W.
Izmer, Andrei
Belza, Joke
Terryn, Herman
Vanhaecke, Frank
Claeys, Philippe

January 2013

Deciphering Earthʼs impact history before ∼2 Ga relies heavily on the lunar record and terrestrial s...

New impact fragments of Fe-Ni-Si spherules at Takamatsu Crater, Japan

Miura, Y.
Fukuyama, S.
Gucsik, Arnold

January 1999

Fe-Ni-Si grains trapped in vacant regions formed by impact events on granitic rock are found in sphe...

Chemical separation of Fe-Ni particles after impact

Miura, Y.
Fukuyama, S.
Kedves, M. A.
Yamori, A.
Okamoto, M.
Gucsik, Arnold

January 2000

Tiny grains of Fe-Ni system originated from planetesimals or meteoroids can remain under solid (or m...

The mineralogy and petrology of I-type cosmic spherules:Implications for their sources, origins and identification in sedimentary rocks

Genge, Matthew John
Davies, Bridie
Suttle, Martin D.
van Ginneken, Matthias
Tomkins, Andrew G.

December 2017

I-type cosmic spherules are micrometeorites that formed by melting during atmospheric entry and cons...

The mineralogy and petrology of I-type cosmic spherules: Implications for their sources, origins and identification in sedimentary rocks

Genge, Matthew J.
Davies, Bridie
Suttle, Martin D.
van Ginneken, Matthias
Tomkins, Andrew G.

September 2017

I-type cosmic spherules are micrometeorites that formed by melting during atmospheric entry and cons...

Impact metamorphosed compositions of the Fe-Si-Ni-S system

Miura, Y.
Fukuyama, S.
Gucsik, Arnold

January 1999

The characterization of impact materials is discussed from the point of view of compositional change...

Spherule layers—records of ancient impacts

Simonson, Bruce M.
Glass, Billy P.

May 2004

A large extraterrestrial object striking Earth at cosmic velocity melts and vaporizes silicate mater...

Microscopic impactor debris at Kamil crater (Egypt): the origin of the Fe,Ni-oxide microscopic spherules

CARONE, LAURA

November 2017

Il cratere di Kamil è un piccolo (45 metri in diametro) cratere da impatto situato nell’Egitto sud-o...

Description, chemical composition, and origin of six microscopic spherules collected from the meteorite moraine in Antarctica: an SEM study

Wight, Shawn

March 1995

Microscopic spherules (100-1000 micrometers) have been found in glacial moraine deposits in Antarcti...

Moderate velocity oblique impact sliding: Production of shocked meteorite textures and palaeomagnetically important metallic spherules in planetary regoliths

Potter, David K.
Ahrens, Thomas J.

April 2013

We detail the production of metallic spherules in laboratory oblique shock impact experiments, and t...

Origin and formation of iron silicide phases in the aerogel of the Stardust mission

Rietmeijer, F. J. M.
Nakamura, T.
Tsuchiyama, A.
Uesugi, K.
Nakano, T.
Leroux, H.

January 2008

Suessite along with hapkeite and more Fe-rich iron-silicides up to Fe7Si2 formed near the entrance o...

Shock Metamorphism and Impact Melting at Kamil Crater, Egypt

FAZIO, AGNESE

March 2015

Shock effects in small terrestrial impact craters (diameter < 300 m) have been poorly studied becaus...

Trace element concentrations in iron type cosmic spherules determined by the SR-XRF method

Nozaki,Wataru
Nakamura,Tomoki
Iida,Atsuo
Matsuoka,Kenji
Takaoka,Nobuo

March 1999

The X-ray fluorescence method using synchrotron radiation (SR-XRF) was applied to determine trace el...

In situ analysis of residues resulting from laboratory impacts into aluminum 1100 foil: Implications for Stardust crater analyses

Wozniakiewicz, P. J.
Kearsley, A. T.
Burchell, M. J.
Foster, N. J.
Cole, M. J.
Bland, P. A.
Russell, S. S.

January 2009

The encounter between the Stardust spacecraft and particles from comet 81P/Wild 2 gave impacts at a ...

A Classification of Extraterrestrial Spherules Found in Sedimentary Rocks and Till

Lougheed, M. S.

May 1966

Author Institution: Department of Geology, Bowling Green State University, Bolwing Green, OhioExtrat...

Ni-rich spinels and platinum group element nuggets condensed from a Late Archaean impact vapour cloud

Goderis, Steven
Simonson, Bruce M.
McDonald, Iain
Hassler, Scott W.
Izmer, Andrei
Belza, Joke
Terryn, Herman
Vanhaecke, Frank
Claeys, Philippe

January 2013

Deciphering Earthʼs impact history before ∼2 Ga relies heavily on the lunar record and terrestrial s...

Grains formed by impact reaction found at spherules of various impact craters, meteorite showers and geological boundaries

Abstract

Extracted data

Grains formed by impact reaction found at spherules of various impact craters, meteorite showers and geological boundaries

Abstract

Extracted data

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