Showing 109–126 of 155 results

Out of stock

Orconuma H3-4 #2 – 1.2 g

78,48 $

The Orcunama meteorite fell in the Philippines in 2011.

It has been classified chondrite type H3-4.

A single stone of 7800 g covered with a dark fusion crust was discovered.

On the clear and sunny morning of March 7, 2011, three farmers (Fredo Manzano, Edgar Francisco Senior and Enrico Camacho Junior) in Orconuma, Bongabonga, Philippines were clearing their field when they were startled by six consecutive loud explosions. The sound of the explosions seemed to last for half a minute. At first they thought it was thunder because the ground was shaking. As they looked up to the sky, they saw a “burning red object with sparks coming out of it”, leaving a thick trail of smoke and making a characteristic hissing sound before it hit the ground. By their own admission, the farmers initially thought it was a bomb and considered that it might be “the end of the world.” They remember that the birds flew away immediately at the sound of the explosions. They went to look, and less than 10 meters away, they found a hole in the ground, surrounded by stirred up dirt and what looked like burnt grass. Inside the hole, about 1 m deep, they saw a stone object and, lacking tools, they used a piece of wood lying nearby and their bare hands to dig it up. Not knowing what this strange stone was, they started asking around, and showing the stone to the locals, but then they were afraid someone would try to take it from them. This fear led them to wrap it in a sealed plastic container before burying it underground for a year. They finally decided that no one would come looking for it, so they dug up the stone and stored it in Fredo Manzano’s closet for the next 8 years. In 2020, they were interviewed for a local TV newscast (later posted on YouTube with over 5 million views), and during the filming, the stone was visually examined by geologist Jocelyn Villanueva, who concluded that it might be a type of basaltic volcanic rock. The farmers, however, remained convinced that it could be a meteorite and hired Ramelle Baquil Ramirez to help them find a buyer. Subsequently in April 2021, with the assistance of an experienced tektite dealer (Carmelita Cepe), the stone was acquired jointly by John Higgins and Jasper Spencer.

Out of stock

Orconuma H3-4 #1 – 2.3 g

136,74 $

The Orcunama meteorite fell in the Philippines in 2011.

It has been classified chondrite type H3-4.

A single stone of 7800 g covered with a dark fusion crust was discovered.

On the clear and sunny morning of March 7, 2011, three farmers (Fredo Manzano, Edgar Francisco Senior and Enrico Camacho Junior) in Orconuma, Bongabonga, Philippines were clearing their field when they were startled by six consecutive loud explosions. The sound of the explosions seemed to last for half a minute. At first they thought it was thunder because the ground was shaking. As they looked up to the sky, they saw a “burning red object with sparks coming out of it”, leaving a thick trail of smoke and making a characteristic hissing sound before it hit the ground. By their own admission, the farmers initially thought it was a bomb and considered that it might be “the end of the world.” They remember that the birds flew away immediately at the sound of the explosions. They went to look, and less than 10 meters away, they found a hole in the ground, surrounded by stirred up dirt and what looked like burnt grass. Inside the hole, about 1 m deep, they saw a stone object and, lacking tools, they used a piece of wood lying nearby and their bare hands to dig it up. Not knowing what this strange stone was, they started asking around, and showing the stone to the locals, but then they were afraid someone would try to take it from them. This fear led them to wrap it in a sealed plastic container before burying it underground for a year. They finally decided that no one would come looking for it, so they dug up the stone and stored it in Fredo Manzano’s closet for the next 8 years. In 2020, they were interviewed for a local TV newscast (later posted on YouTube with over 5 million views), and during the filming, the stone was visually examined by geologist Jocelyn Villanueva, who concluded that it might be a type of basaltic volcanic rock. The farmers, however, remained convinced that it could be a meteorite and hired Ramelle Baquil Ramirez to help them find a buyer. Subsequently in April 2021, with the assistance of an experienced tektite dealer (Carmelita Cepe), the stone was acquired jointly by John Higgins and Jasper Spencer.

Out of stock

Nuevo Mercurio H5 #7 – 2.7 g

39,24 $

The Nuevo Mercurio meteorite is a type H5 meteorite that fell in Mexico in 1978.

About 50 kg of this meteorite were found near the village of Nuevo Mercurio.

Nuevo Mercurio H5 #6 – 5 g

71,34 $

The Nuevo Mercurio meteorite is a type H5 meteorite that fell in Mexico in 1978.

About 50 kg of this meteorite were found near the village of Nuevo Mercurio.

Out of stock

Nuevo Mercurio H5 #5 – 5,8 g

68,96 $

The Nuevo Mercurio meteorite is a type H5 meteorite that fell in Mexico in 1978.

About 50 kg of this meteorite were found near the village of Nuevo Mercurio.

Out of stock

Nuevo Mercurio H5 #4 – 3,4 g

40,43 $

The Nuevo Mercurio meteorite is a type H5 meteorite that fell in Mexico in 1978.

About 50 kg of this meteorite were found near the village of Nuevo Mercurio.

Out of stock

Nuevo Mercurio H5 #3 – 4,3 g

51,13 $

The Nuevo Mercurio meteorite is a type H5 meteorite that fell in Mexico in 1978.

About 50 kg of this meteorite were found near the village of Nuevo Mercurio.

Out of stock

Nuevo Mercurio H5 #2 – 3,4 g

40,43 $

The Nuevo Mercurio meteorite is a type H5 meteorite that fell in Mexico in 1978.

About 50 kg of this meteorite were found near the village of Nuevo Mercurio.

Out of stock

Nuevo Mercurio H5 #1 – 6,2 g

83,23 $

The Nuevo Mercurio meteorite is a type H5 meteorite that fell in Mexico in 1978.

About 50 kg of this meteorite were found near the village of Nuevo Mercurio.

VINALES L6 #8 – 19,2 g

228,29 $

In a clear sky, a fireball, followed by a trail of smoke was seen over Havana, Cuba, and then fell to the ground in a shower of fragments in the Vinales Valley, 180 km from the capital, in the west of the country… Falling around 1:30 pm local time, on February 1, without causing any casualties, the fall of the meteorite was accompanied by a lightning bolt and a strong explosion. This meteorite was classified as an ordinary chondrite type L6, about 50 kg of this meteorite were found.

 

Out of stock

Sidi Ali #1 L4 – 44,5 g

630,19 $

Sidi Ali is a meteorite that fell in Morocco on July 28, 2015 near Tissint.

Meteorites of 5 to 100 grams were discovered in a fall ellipse of about 4 km.

The analysis determined that this meteorite is of the ordinary L4 chondrite type.

Writeup from MB 105:

Sidi Ali Ou Azza 29°47’2.9″N, 7°23’21.8″W

Guelmim-Es-Semara, Morocco

Confirmed fall: 28 Jul 2015

Classification: Ordinary chondrite (L4)

History: (H. Chennaoui Aoudjehane FSAC, A. Aaranson, A. Bouragaa, A. Bouferra). On Tuesday, 28 July 2015, around 5:30 pm local time (6:30 pm GMT), many people from Tissint and its vicinity heard three sonic booms in the direction of Sidi Ali Ou Azza. Immediately, numerous people begin searching for the meteorite in the area. Two days after the fall, many small pieces from 5 to 109 g (so far: 109, 100, 75, 50, 40, 37, 20, 10, 7, and 5.7 g) were recovered close to Sidi Ali Ou Azza and El Kharoua’ well, a few km west of Tissint. Most pieces are complete and mostly covered by black fusion crust. The interior is dark and brecciated, with a few clear gray zones. Numerous small and well-defined chondrules are visible as well as sulfides and metals. The direction of the fall was from north to south; the strewnfield is ~4 km long.

Physical characteristics: Black and brown patchy fusion crust. A saw cut reveals numerous, distinct chondrules and fine grained metal/sulfide. A dark angular clast, ~5 mm, was also observed.

Petrography: (C. Agee, UNM) Microprobe examination of a polished mount shows numerous porphyritic chondrules, a few BO chondrules, and an enstatite-rich chondrule. Mesostasis and very fine-grained plagioclase is ubiquitous. Kamacite, taenite, troilite, chromite, and a phosphate phase were observed throughout. The dark angular clast described above has an igneous texture with ~50% zoned euhedral olivines (up to 50 μm) and ~50% fine spinifex quench crystals, with sparse scattered metal or sulfide blebs (up to 10 μm).

Geochemistry: (C. Agee and N. Muttik, UNM) Chondrule olivine Fa25.7±0.9, Fe/Mn=50±3, Cr2O3=0.03±0.03 (wt%), n=24; chondrule low-Ca pyroxene Fa20.4±1.7, Fe/Mn=29±1, n=10; chondrule enstatite Fs2.1±0.2Wo0.6±0.2, n=2; plagioclase An8.3±3.9Ab86.9±3.1Or4.9±0.9. Clast olivine Fa19.3±4.1, Fe/Mn=47±4, Cr2O3=0.45±0.21 (wt%), n=6.

Classification: Ordinary chondrite, L4

Specimens: 20.8 g, UNM; 10.7 g, FSAC

 

Out of stock

Tatahouine #1 Diogénite – 2,4 g

53,51 $

The Tatahouine meteorite is a very beautiful achondrite diogenite meteorite, which fell on June 27, 1931 at 01:30 am, 4 kilometers northeast of the village of Foum Tataouine in Tunisia. The explosion woke up the whole population and also the French garrison. The next day French legionnaires found some fragments.

The diogenite meteorites come from the asteroid Vesta.
Out of stock

Allende CV3 #9 – 3,4 g

141,49 $

The Allende meteorite fell in Mexico in 1969.

It is often considered as the “Rosetta Stone” of planetologists, because it has improved our knowledge on the origins of our solar system. This meteorite was formed before our planet, in the very first moments of the solar system. It preserves in its heart the traces of the nebula which generated the Sun and its procession of planets.

Out of stock

Allende CV3 #8 – 2,8 g

116,52 $

The Allende meteorite fell in Mexico in 1969.

It is often considered as the “Rosetta Stone” of planetologists, because it has improved our knowledge on the origins of our solar system. This meteorite was formed before our planet, in the very first moments of the solar system. It preserves in its heart the traces of the nebula which generated the Sun and its procession of planets.

Out of stock

Allende CV3 #7 – 1,6 g

68,96 $

The Allende meteorite fell in Mexico in 1969.

It is often considered as the “Rosetta Stone” of planetologists, because it has improved our knowledge on the origins of our solar system. This meteorite was formed before our planet, in the very first moments of the solar system. It preserves in its heart the traces of the nebula which generated the Sun and its procession of planets.

Out of stock

Allende CV3 #6 – 1,8 g

77,29 $

The Allende meteorite fell in Mexico in 1969.

It is often considered as the “Rosetta Stone” of planetologists, because it has improved our knowledge on the origins of our solar system. This meteorite was formed before our planet, in the very first moments of the solar system. It preserves in its heart the traces of the nebula which generated the Sun and its procession of planets.

Out of stock

Allende CV3 #5 – 3,3 g

136,74 $

The Allende meteorite fell in Mexico in 1969.

It is often considered as the “Rosetta Stone” of planetologists, because it has improved our knowledge on the origins of our solar system. This meteorite was formed before our planet, in the very first moments of the solar system. It preserves in its heart the traces of the nebula which generated the Sun and its procession of planets.

Out of stock

Allende CV3 #4 – 3,7g

154,57 $

The Allende meteorite fell in Mexico in 1969.

It is often considered as the “Rosetta Stone” of planetologists, because it has improved our knowledge on the origins of our solar system. This meteorite was formed before our planet, in the very first moments of the solar system. It preserves in its heart the traces of the nebula which generated the Sun and its procession of planets.