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Chinese Name:雪辰橄欖隕鐵, 橄欖石天鐵
English Name:Seymchan Pallasite Meteorite
Chemical Composition:Mainly consists of peridot, nickel& iron.
Lustre:Metallic
SG:
8.67 (nickel) 7.21 (iron)
Related Chakra:Get through all chakras especially heart chakra
Colour:Silverly gray, redish brown together with yellow green to brownish green
Locality: Magadan Oblast, Russia, other Pallasite Meteorites and be found from other parts of Russia, Argentina,Australia,Chile,China & United States
Remarks:A pallasite is a class of stony-iron meteorite

Pallasites are a rare type of meteorite. Only 61 are known to date, including 10 from Antarctica, with four being observed falls.

Meteorite that contain fragments of gemmy olivine and/or peridot crystal are called "pallasite", or "stony-iron meteorite." When sliced into thin layers, these olivine and peridot fragments are transparent next to the opaque nickel-iron matrix they are contained in.

Krasnojarsk, Yeniseisk, Russia. A mass of about 700 kg was detected in 1749 about 145 miles (233 km) south of Krasnojarsk. It was seen by P. S. Pallas in 1772 and transported to Krasnojarsk (see above) The main mass of 515 kg is now in Moscow at the Academy of Sciences. Pallasites are named after Peter Pallas for his study of this meteorite

Marjalahti, Karelia, Russia. After the appearance of a bright meteor and detonations, a large mass was seen to fall and 45 kilograms (99 lb) were recovered in June 1902. At this date the fall site belonged to Finland, and the main mass of Marjalahti is now at the Geological Museum of the University of Helsinki.

Pallasovka, Pallasovka, Russia. A single mass of 198 kg was found near Pallasovka, Russia in 1990. Coincidentally, both the town of Pallasovka and pallasite meteorites were named after the naturalist, Peter Pallas.
 
hot sell
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Classification of Meteorites:
1. Iron Meteorites
2. Stony Meteorites
3. Stony-iron meteorites
  1.1 Kamacite
1.2 Taenite

 

2.1 Chondrites
2.2 Achondrites
  3.1 Pallasites
3.2 Mesosiderites


Classification of Meteorites
1. Iron Meteorites
  Iron meteorites are composed of iron and nickel and are extremely dense. They are pieces of the cores of asteroids. Early in Solar System history, asteroids melted and the dense iron-nickel metal sank to the center to form a core - much like the Earth has a core.
One of the most distinguishing features of meteorites is the presence of the Widmanstatten pattern - the distinctive series of bands in geometric patterns. This pattern is created by the intergrowth of two different iron-nickel minerals formed during very slow cooling (a few degrees every million years) in the core of the asteroid. The presence of nickel is a universal feature of iron meteorites.
Iron meteorites are subdivided into classes both by chemical composition and structure. Structural classes are determined by studying their 2 component iron-nickel alloys: Kamacite and Taenite.
 
  1.1 Kamacite  
  Kamacite is an alloy of iron and nickel, the proportion iron:nickel is beteween 90:10 to 95:5; small quantities of other elements, such as cobalt or carbon may also be present.
It is a major constituent of iron meteorites (octahedrite and hexahedrite types).
In the octahedrites it is found in bands interleaving with taenite forming Widmanstatten patterns.
In hexahedrites, fine parallel lines called Neumann lines are often seen, which are evidence for structural deformation of adjacent kamacite plates due to shock from impacts.
Hardness: around 4
 
  1.1.1
Gibeon Meteorites
hot sell
The Giben Meteorite is a fine octahedrite iron meteorite which flamed into our atmosphere as a visible star-like streak an estimated 30,000 years ago, landing in what is present day Namibia. Prior to this, the Gibeon meteorite traveled through space for over 4 billion years before it was finally trapped by the Earth's gravitational field and pulled to earth as a fire ball.  
Location Found
Classification

Age

Year Found

Rough

After Polished

 
Gibeon (Namibia) Kamacite

Fine Octahedrite
(IVA)
4 billion years

Time of Fall: ~ 30,000 years ago
1838
hot sell
  1.1.2
Muonionalusta Meteorite
hot sell
The Muonionalusta is a meteorite classified as fine octahedrite, type IVA (Of) which impacted in northern Scandinavia, west of the border between Sweden and Finland, about one million years BCE.  
Location
Classification
Age
Year Found
Rough
After Polished
 
Norrbotten (Sweden) Kamacite

Fine Octahedrite
(IVA)
4 billion years

Time of Fall: about one millions years BCE.
1906
hot sell
  1.1.3
Sikhote-Alin Meteorite
hot sell
A conical meteorite fell in a corn field near the village of Bogga Dingare after a bright fireball was witnessed moving west to east and an explosion was heard. The local people hammered the meteorite into many pieces, and most of the material was dispersed.  
Location
Type
Age
Year Found
Rough
After Polished
 

Sikhote-Alin Mountains, Maritime Province, Russia

Kamacite

coarse octahedrite (IIAB)
4.5 Billion years

Time of Fall: 1947, February 12
1956
hot sell
  1.1.4
Agoudal Iron Meteorite

Also Known As: Imilchil. In 2000 two small pieces of "iron" were collected in the Agoudal area, High Atlas Mountains, Morocco. Later in September 2011, one piece was sold to a dealer who recognized it as an iron meteorite. Since then many more pieces have been collected. Type IIAB iron meteorites are also called hexahedrites. Hexahedrites are low nickel iron meteorites.

 
Location
Type
Age
Year Found
Rough
After Polished
 

Centre-South, Morocco

Iron

Hexahedrite
(IIAB)
4 billion years

Time of Fall: 40,000 years ago
2000
 
  1.2 Taenite  
 
Taenite (Fe,Ni) is a mineral found naturally on Earth mostly in iron meteorites. It is an alloy of iron and nickel, with nickel proportions of 20% up to 65%. Taenite is a major constituent of iron meteorites.
In octahedrites it is found in bands interleaving with kamacite forming Widmanstatten patterns
Hardness: 5 -5.5
 
  Name Location Classification Age
Year Found
Rough
After Polished
 
  1.2.1
Campo del Cielo Meteorites
hot sell
Argentina Taenite

Coarse Octahedrite
(IAB)
4.5 billion years

Time of Fall: between 4,000-6,000 years ago
1576
hot sell
  1.2.2
Henbury Meteorites
west-southwest of Henbury, Northern Territory, central Australia Taenite

medium octahedrite
(IIIAB)
4.56 billion years

Time of Fall: 4,700 years ago
1931
 
  1.2.3
Canyon Diablo Meteorites
Arizona Taenite

coarse octahedrite
(IA)
between 4.53 to 4.58 billion years

Time of Fall: 49,000 years ago
1891
 
2. Stony Meteorites
 
  More than 95% of meteorites observed to fall to Earth are stony.
They can be divided into chondrites and achondrites.
Both types are composed mostly of silicate minerals, but the great majority also contain metallic iron in small-scattered grains.
 
  2.1 Chondrites
  Chondrites are named for their most prominent feature - millimeter-sized spherical bodies called chondrules. These chondrules (from the Greek for small sphere) formed 4.5 billion years ago in the Solar Nebula - the cloud of gas and dust from which the Sun, planets, asteroids, and comets formed.  
  2.1.1
NWA 869
hot sell
These meteorites are found in the middle of the desert near no post office! So a numbering system used by the Meteoritical Society (An non-profit organization founded in 1933 by American) incorporates the order of recovery for specimens and their GPS locations.  
Location Classification Age
Year Found
Rough
After Polished
 
Northwest Africa Chondrites

(L4-6)
4.55 billion years
2000
hot sell
  2.1.2
Gujba Meteorite
Location
Classification
Age
Year Found
Rough
After Polished
 
Bogga Dingare, Yobe State, Nigeria Chondrites

bencubbinite (class CBa)
4.56 billion years
1984
 
  2.1.3
Chelyabinsk Meteorite
hot sell
  The Chelyabinsk meteorite (Russian: Челябинский метеорит) is the fragmented remains of the large Chelyabinsk meteor of 15 February 2013 which reached the ground after the meteor's passage through the atmosphere. The descent of the meteor, visible as a brilliant superbolide in the morning sky, caused a series of shock waves that shattered windows, damaged approximately 7,200 buildings and left 1,500 people injured. The resulting fragments were scattered over a wide area.  
Location Classification Age
Year Found
Rough
After Polished
 
  Lake Chebarkul, Chelyabinsk Oblast, Russia Chondrites

(LL5)
4.55 billion years

Time of Fall:
15 February 2013
27 February 2013
hot sell
  2.2 Achondrites
  Less common, comprising only a few percent of all meteorites, are achondrites. These are also stony meteorites composed primarily of silicates, but these meteorites have experienced familiar geologic processes of melting and differentiation - although these happened long ago. Most achondrites formed on asteroids during the birth of the Solar System, but a small number formed on Mars and the Moon.  
  2.2.1
NWA 4664
Location Classification Age
Year Found
Rough
After Polished
 
Algeria, Northwest Africa Achondrites

(diogenite, polymict breccia)
over 4 billion years
2006
 
  2.2.2
Johnstown
Colorado, United States Achondrite

(a calcium-poor diogenite)
4.43 - 4.55 
billion years
1924
 
3. Stony-iron meteorites  
  Stony-iron meteorites, contain about equal proportions of metal and silicate material, and are rare (less than 2% of all known meteorites). Stony-iron meteorites form in places where metal and silicate are mixed. They are divided into two groups: the pallasites and the mesosiderites  
  3.1 Pallasites
  One type of stony-iron are pallasites - rocks composed of a network of iron-nickel metal surrounding a greenish, silicate mineral called olivine. Pallasites probably form when the olivine-rich mantle of an asteroid mixes with the metallic core.  
  3.1.1
Seymchan
hot sell
Location Classification Age
Year Found
Rough
After Polished
 
Magadan Oblast, Russia Pallasite

Coarse octahedrite
(IIE)
over 4 billion years
1967
hot sell
  3.1.2
Brahin
Belarus, Russia Pallasite

Medium octahedrite
4.5 billion years
1807
 
  3.1.3
Imilac
Atacama Desert (Chile) Pallasite 4.5 billion years
1822
 
  3.14
Sericho
hot sell
(Habaswein),North-Eastern, Kenya Pallasite 4.5 billion years
2016
hot sell
  3.2 Mesosiderites  
  Mesosiderites are mixtures of iron-nickel metal and basalt and probably formed by the collision of two asteroids.  
    Location Type Age
Year Found
Rough
After Polished
 
  3.2.1
Vaca Muerta
Atacama Desert, (Chile) Mesosiderite

(AI)
over 4 billion years
1861
 
  3.2.2
NWA 2932
Northwest Africa (Morocco) Mesosiderite over 4 billion years
2005
 

References: [1] Meteoritical Bulletin 106 (2018) Meteoritics & Planet. Sci, 53, in prep. [2] https://www.lpi.usra.edu/meteor/metbull.php?code=65717; https://www.hou.usra.edu/meetings/lpsc2018/pdf/1556.pdf; http://geology.com; http://www.mindat.org; http://www.meteorites.com.au; www.collectingmeteorites.com; www.arizonaskiesmeteorites.com;http://www.lpi.usra.edu; www.meteoriteguy.com; geology.com; www.meteorite-pictures.org; http://www.freeexistence.org; www.reporterherald.com; http://www.meteorite-recon.com; http://www.encyclopedia-of-meteorites.com; http://www.meteorite.fr; https://meteorites.asu.edu; http://meteorite.museums.ualberta.ca; The Book of Stones by Robert Simmons & Naisha Ahsian
Functions:
1. Stimulates the loving energies of the heart chakra, along with the visionary capacities of the third eye.
2. Pallasite opens the emotional gateway of the heart along with the inner eye of wonder and expanded awareness, for the purpose of allowing one to experience the link between oneself and the cosmos.
3. It can calm the fear of flying and can also assist those who suffer from agoraphobia.
4. Pallasite can also assist one in manifesting prosperity and abundance in one's material life.
5. For opening the heart more fully, one can combine Pallasite with Dioptase, Morganite, Emerald and/or Kunzite.
6. Hematite, Black Tourmaline, and Smoky Quartz are all excellent choices if one feels that a grounding influence is needed.
   
General care:
 
1. Meteorite can be scratched easily, so wear with caution.
2. Do not soak in water.
3. Do not soak in jewellery cleaner.
4 Avoid contact with household cleaners.
5. Avoid using ultrasonic and steam cleaners.
6. Cleaning: Clean using lukewarm plain water and soft brush, then dry using a soft cloth. (Do remember to dry it cause meteorite might oxidize easily!)
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