NWA 7811 is a fresh meteorite classified eucrite polymict breccia of only 95 grams.
It was discovered in 2011 and classified by Anthony Irving in 2012.
The eucrites come from the Asteroid Vesta.
Petrography: (A. Irving and S. Kuehner, UWS) Fresh fragmental breccia composed mainly of crystal debris from several different basaltic eucrite and gabbroic eucrite protoliths (with some polymineralic clasts of same), plus sparse clasts of diogenite and diogenitic orthopyroxene. Minerals include exsolved pigeonite, orthopyroxene, clinopyroxene, calcic plagioclase, silica polymorph, ilmenite, troilite, chromite, and fayalite.
NWA 7811 is a fresh meteorite classified eucrite polymict breccia of only 95 grams.
It was discovered in 2011 and classified by Anthony Irving in 2012.
The eucrites come from the Asteroid Vesta.
Petrography: (A. Irving and S. Kuehner, UWS) Fresh fragmental breccia composed mainly of crystal debris from several different basaltic eucrite and gabbroic eucrite protoliths (with some polymineralic clasts of same), plus sparse clasts of diogenite and diogenitic orthopyroxene. Minerals include exsolved pigeonite, orthopyroxene, clinopyroxene, calcic plagioclase, silica polymorph, ilmenite, troilite, chromite, and fayalite.
NWA 7811 is a fresh meteorite classified eucrite polymict breccia of only 95 grams.
It was discovered in 2011 and classified by Anthony Irving in 2012.
The eucrites come from the Asteroid Vesta.
Petrography: (A. Irving and S. Kuehner, UWS) Fresh fragmental breccia composed mainly of crystal debris from several different basaltic eucrite and gabbroic eucrite protoliths (with some polymineralic clasts of same), plus sparse clasts of diogenite and diogenitic orthopyroxene. Minerals include exsolved pigeonite, orthopyroxene, clinopyroxene, calcic plagioclase, silica polymorph, ilmenite, troilite, chromite, and fayalite.
NWA 7811 is a fresh meteorite classified eucrite polymict breccia of only 95 grams.
It was discovered in 2011 and classified by Anthony Irving in 2012.
The eucrites come from the Asteroid Vesta.
Petrography: (A. Irving and S. Kuehner, UWS) Fresh fragmental breccia composed mainly of crystal debris from several different basaltic eucrite and gabbroic eucrite protoliths (with some polymineralic clasts of same), plus sparse clasts of diogenite and diogenitic orthopyroxene. Minerals include exsolved pigeonite, orthopyroxene, clinopyroxene, calcic plagioclase, silica polymorph, ilmenite, troilite, chromite, and fayalite.
Zagora 003 is a fresh meteorite classified as eucrite of only 135 grams.
It was discovered near Zagora in Morocco by Ahmed Enaji on September 13, 2020.
The eucrites come from the Asteroid Vesta.
Writeup from MB 110 :
Zagora 003 30°20’51.94″N, 5°36’41.79″W
Morocco
Find: 2020 Sep 13
Classification: HED achondrite (Eucrite)
History: Found by Ahmed Enaji on September 13, 2020. Bought from Zaid Oualguirah in 2020.
Physical characteristics: Several fusion crusted pieces with grey interior.
Petrography: (J. Gattacceca, CEREGE) Igneous rock with grain size about 500 µm. It contains melt rock areas, and other areas with variolitic texture. Main minerals are pyroxene and plagioclase. Other minerals: metal, troilite, chromite.
Jdiriya 003 is a meteorite of eucrite type of only 21.4 grams, it was discovered by Zaid Oualguirah in 2019 in the Western Sahara.
Howardite meteorites come from the asteroid Vesta, an asteroid between Mars and Jupiter.
I am selling the main mass of 15.7 grams, a unique piece !
Writeup from MB 109:
Jdiriya 003 27°36’59.42″N, 10°26’48.85″W
Saguia el Hamra, Western Sahara
Find: 2019 Dec 18
Classification: HED achondrite (Eucrite)
History: Found by Zaid Oualguirah on 2019 Dec 18.
Physical characteristics: A single crusted stone. Cut surface reveals a light homogeneous interior with ~500 µm plagioclase and pyroxene grains.
Petrography: ( J. Gattacceca, CEREGE) Igneous rock with subophitic texture. Main minerals are pyroxene (with both fine- and large-scale exsolutions) and plagioclase, with typical grain size 400 µm. Other minerals: chromite, ilmenite, metal, troilite, silica.
NWA 7811 is a fresh meteorite classified eucrite polymict breccia of only 95 grams.
It was discovered in 2011 and classified by Anthony Irving in 2012.
The eucrites come from the Asteroid Vesta.
Petrography: (A. Irving and S. Kuehner, UWS) Fresh fragmental breccia composed mainly of crystal debris from several different basaltic eucrite and gabbroic eucrite protoliths (with some polymineralic clasts of same), plus sparse clasts of diogenite and diogenitic orthopyroxene. Minerals include exsolved pigeonite, orthopyroxene, clinopyroxene, calcic plagioclase, silica polymorph, ilmenite, troilite, chromite, and fayalite.
NWA 7831 was discovered in March 2013.
This meteorite is a very beautiful and rare diogenite of the same type as Tataouine.
About 20 kilograms of this meteorite were found in the Western Sahara about 100 km northeast of Laâyoune in a place called Chwichiya.
Awsserd is a rare chondrite rumuruti type R4.
There are only 53 meteorites of this type in the world today !
This meteorite was bought by Marc Henry during a trip in the Western Sahara.
This fresh rumuruti of 924 grams was found less than 5 km from the small village of Awsserd. An exceptional meteorite!
Awsserd is a rare chondrite rumuruti type R4.
There are only 53 meteorites of this type in the world today !
This meteorite was bought by Marc Henry during a trip in the Western Sahara.
This fresh rumuruti of 924 grams was found less than 5 km from the small village of Awsserd. An exceptional meteorite!
NWA 7831 was discovered in March 2013.
This meteorite is a very beautiful and rare diogenite of the same type as Tataouine.
About 20 kilograms of this meteorite were found in the Western Sahara about 100 km northeast of Laâyoune in a place called Chwichiya.
The meteorite NWA 7034 is an exceptional meteorite.
This meteorite is not alone because other stones of the same type have been found in the fall zone.
It is a Martian meteorite, certainly the rarest and most scientifically interesting meteorite ever found. It was discovered by meteorite hunters in the Western Sahara.
It is the oldest rock from Mars ever discovered and contains more water than any other known Martian meteorite. Its texture is brecciated, it is composed of an agglomerate of rocks of which each rock tells us a fascinating story.
The meteorite NWA 7034 is an exceptional meteorite.
This meteorite is not alone because other stones of the same type have been found in the fall zone.
It is a Martian meteorite, certainly the rarest and most scientifically interesting meteorite ever found. It was discovered by meteorite hunters in the Western Sahara.
It is the oldest rock from Mars ever discovered and contains more water than any other known Martian meteorite. Its texture is brecciated, it is composed of an agglomerate of rocks of which each rock tells us a fascinating story.
The meteorite NWA 7034 is an exceptional meteorite.
This meteorite is not alone because other stones of the same type have been found in the fall zone.
It is a Martian meteorite, certainly the rarest and most scientifically interesting meteorite ever found. It was discovered by meteorite hunters in the Western Sahara.
It is the oldest rock from Mars ever discovered and contains more water than any other known Martian meteorite. Its texture is brecciated, it is composed of an agglomerate of rocks of which each rock tells us a fascinating story.
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