Haberer-Meteorites Gifts of the sky

 

 

 

Home

 

 

 

General Information

 

Origin

 

History

 

Culture & Religion

 

Records

 

Sensations

 

FAQs

 

Index

 

Classification

 

Iron-meteorites

 

Stony-iron-meteorites

 

Stony-meteorites

News

About us

 

Background

 

Certificates

   
 
Sales Chondrites
 

 

Sales

   

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Chondrites

 

Chondrites are the oldest known matter. These meteorites developed simultaneously with our central star, the Sun, by crystalizing out in the presolar primeval nebula in form of ball-like spezies, the so-called chondrules. These chondrules condensed together with other presolar matterl to smaller and larger rocks and remained the following 4,5 billions years more or less unchanged.

Chemically the Chondrites resemble the Sun if one refrains from the missing of all fleeting elements as well as helium and hydrogen. But according to the place, in which the respective Chondrites crystalized out in the presolar primeval nebula they are significantly different, thus numerous groups and clans are distinguished, which further below are described individually.

Next to the separation in clans and groups, Chondrites are generally distinguished according to so-called petrological classes, a scale of 1 to 7 that gives information about the differentiation degree of the individual Chondrites. The classes 1 and 2 occur only in Carbonaceous Chondrites and designate meteorites with sparse, little chondrules in which a change took place through oxidising and water. The class 3 designates meteorites with large, clear chondrules that remained almost unchanged while the classes 4 to 6 designate Chondrites, that increasingly got heated in their history and hereby were changed. The chondrules with higher petrological degree become more and more undifferentiated and fuse with the matrix. The class 7 finally comprises meteorites whose chondric nature becomes clear only through their chemical compound. They contain no more chondrules and form a kind of transition to the Achondrites.

 

Jiddat al Harasis Jah Chondrites:

Research of the Jiddat al Harasis Chondrite:

Meteoritical Bulletin

Proposed Name

Jiddat al Harasis xxx

Abbreviation

JaH xxx

Pseudonyms or field names

SH107-39

Location of Recovery (description)

desert

Date of Recovery

07.03.2003

 

Country

Oman

State or province

Al Wusta

Latitude

19°21.531

Longitude

055°32.906

 

Mass (g)

16879.1

Type spec (g)

26.6

Type spec locatio

Univ. Kiel 

 

Number of Pieces

70

Classifier and institution

Barto

 

Class

L ~6

Shock

4

WG

4.42


234 g 90 Euro  
sold

248 g 100 Euro  
sold

412 g 160 Euro

442 g 170 Euro  
sold

159,3 g 80 Euro  
sold

151,7 g 70 Euro  

136,3 g 60 Euro  
sold

128 g 55 Euro  
sold

111,9 g 50 Euro  
sold

80.9 g 45 Euro  
sold

78,9 g 45 Euro  
sold

41,9 g 25 Euro  sold

30,4 g 18 Euro  
sold

25,4 g 15 Euro  
sold

 

Dhofar Chondrites:

 


Dho 408 L 6 161,2 g 90 Euro

 


Dho 616 H 5/6 11,3 g 8 Euro  sold

 


Dho 649 L6 25,5 g 15 Euro  sold

 


Dho 446 12,7 g 8 Euro

       

 

Please click on images to enlarge

(the backside of each meteorite is shown)

 

 

 
 
 
Inquiry and sales