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Hammadah al Hamra 337 | |||||||||||||||||||||||
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Basic information | Name: Hammadah al Hamra 337 This is an OFFICIAL meteorite name. Abbreviation: HaH 337 Observed fall: No Year found: 2001 Country: Libya Mass: ![]() | ||||||||||||||||||||||
Classification history: |
This is 1 of 121 approved meteorites classified as CK4. [show all] Search for other: Carbonaceous chondrites, Carbonaceous chondrites (equilibrated), CK chondrites, CK chondrites (type 4-6), and CV-CK clan chondrites | ||||||||||||||||||||||
Comments: | Approved 3 Feb 2006 | ||||||||||||||||||||||
Writeup![]() |
Writeup from MB 90:
Hammadah al Hamra 337 29°00′00′′N, 12°07′40′′E Hammadah al Hamra region, Libya Find: 24 February 2001 Carbonaceous chondrite (CK4) History: A single stone weighing 198 g was found in February 2001 in the Hammadah al Hamra region of Libya by Giovanni Pratesi (MSP) during a scientific expedition. Physical Characteristics: (V. Moggi-Cecchi, A. Salvadori, and G. Pratesi, MSP) The main mass has a dark brown external surface with fusion crust in some areas. In hand sample the chondrules are set in a dark green matrix and CAIs (up to 1 mm) are present. Petrography: The thin section contains few chondrules (not perfectly delineated and sometimes altered) set in fine-grained matrix with several coarser-grained olivine crystals. Chondrules range from 380 to 1800 µm (mean value 700 µm on n = 25) and account for about 20% of the total volume. Chondrule textural types: POP = 72%, PO = 12%, and GOP = 16% (all vol%). Very rare and extremely altered AOIs (2 vol%) and abundant CAIs (~1 mm) are observed. Plagioclase crystals can be found in GO and PO chondrules. Metal alloys are extremely rare (<0.01 vol%). Magnetite (inside and outside chondrules) is abundant (~8 vol%). Sulfides (mainly pyrrhotite) are rare and are located in the matrix. Rare kamacite and moncheite (Pt,Pd)(Te,Bi)2 are also present. Chemistry: (EPMA) Olivine compositions are quite homogeneous (Fo68–75; mean Fo74), with the exception of rare zoned olivine crystals (Fo68–93) in PO chondrules. Low-Ca pyroxenes in GOP chondrules are En90-100. High-Ca pyroxenes in POP chondrules have an augitic composition (Wo50En50–60Fs0–10). Plagioclase and devitrified mesostasis is albitic (An25–50). Magnetite (Cr2O3 = 2–3 wt%): Sulfides (Ni = 1–2 wt%); kamacite with low Ni. Classification: Carbonaceous chondrite (CK4); S1, moderate to extensive weathering. Specimens: The main mass (174 g), a 24 g type specimen, and two thin sections are on deposit at MSP (inventory number MSP 1592). | ||||||||||||||||||||||
Data from: MB90 Table 1 Line 6: |
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Plots: | O isotopes: | ||||||||||||||||||||||
Institutions and collections |
MSP: Museo di Scienze Planetarie, Via Galcianese 20/H, 59100 Prato, Italy, Italy; Website (institutional address; updated 22 Oct 2022) OU: Planetary and Space Sciences Department of Physical Sciences The Open University Walton Hall Milton Keynes MK7 6AA United Kingdom, United Kingdom (institutional address; updated 8 Dec 2011) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 90, MAPS 41, 1383-1418 (2006)
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Geography:![]() |
Statistics: This is 1 of 214 approved meteorites from Gharyan, Libya (plus 16 unapproved names) This is 1 of 1538 approved meteorites from Libya (plus 23 unapproved names) (plus 2 impact craters) | ||||||||||||||||||||||
Proximity search: |