The Dar al Gani meteorite field (Libyan Sahara): Geological setting, pairing of meteorites, and recovery density

  title={The Dar al Gani meteorite field (Libyan Sahara): Geological setting, pairing of meteorites, and recovery density},
  author={Jochen Schl{\"u}ter and L. K. Schultz and Friedhelm Thiedig and Bertrina Olivia West Al-Mahdi and A. E. Abu Aghreb},
  journal={Meteoritics \& Planetary Science},
Abstract— As of July 2001, 1238 Libyan meteorites have been reported. Most were found in two areas called Dar al Gani and Hamadah al Hamra. Dar al Gani is located on a plateau of marine carbonate rocks with marly components. Eight‐hundred and sixty‐nine meteorites between 6 g and 95 kg totalling 687 kg have been found here but the calculated mean recovery density is comparatively low with one meteorite on 6.5 km2. 

Shişr 043 (IIIAB medium octahedrite): The first iron meteorite from the Oman desert

Abstract— The iron meteorite Shişr 043 is a single mass of 8267 g found in the south Oman desert 42 km NE of the Shişr village. It is the first iron identified among the >1400 individual meteorites

Characteristics of the Sahara as a meteorite recovery surface

We describe the geological, geomorphological, and paleoclimatic setting of the Sahara of North Africa in particular, focused on the main meteorite dense collection areas (DCA; Morocco, Algeria,

The new polymict eucrite Dar al Gani 983: Petrography, chemical composition, noble gas record, and evolution

Abstract— Mineralogical and chemical studies of Dar al Gani 983 show that this meteorite is a eucrite. Its texture is that of an impact breccia. It contains cumulate pyroxene and feldspar megacrysts,

Meteorites from the Lut Desert (Iran)

We present for the first time a detailed report on the discovery of a new meteorite collection region in the Lut Desert, eastern–southeastern Iran, describing its geological, morphological, and

Description of a very dense meteorite collection area in western Atacama: Insight into the long‐term composition of the meteorite flux to Earth

We describe the geological, morphological, and climatic settings of two new meteorite collections from Atacama (Chile). The “El Médano collection” was recovered by systematic on‐foot search in El

Meteorite reconnaissance in Saudi Arabia

Meteorite searches in Saudi Arabia between 2008 and 2014 yielded 46 meteorites from the Yabrin area (23°N 49°E), 35 meteorites from the Rub' al‐Khali sand desert (19°–20°N, 48°–51°E), and 1 meteorite

The densest meteorite collection area in hot deserts: The San Juan meteorite field (Atacama Desert, Chile)

Abstract– We describe the geological, morphological, and climatic setting of the San Juan meteorite collection area in the Central Depression of the Atacama Desert (Chile). Our recovery activities

Desert meteorites: a history

  • A. Bevan
  • Environmental Science, Geology
    Geological Society, London, Special Publications
  • 2006
Abstract During the last 35 years, the number of meteorites available for study has increased by an order of magnitude (from around 2000 to nearly 30 000). The largest contribution has come from

Meteorites from the United Arab Emirates: Description, weathering, and terrestrial ages

We report on the first meteorite search campaign in the United Arab Emirates (UAE). The geology and proximity of our search region suggest that it is the north‐western extension of the Oman meteorite



Meteorites from the Sahara: Find locations, shock classification, degree of weathering and pairing

— The Sahara is an extraordinary area for recovering meteorites. Between 1989 and 1993, 471 meteorites were collected in Algeria and Libya. Studies of 465 samples have been done. In addition to the

Geophysical Studies of North African Cenozoic Volcanic Areas I: Haruj Assuad, Libya

This study is the first of a series in which a main concern will be to establish the Neogene absolute motion of the African Plate. A combined palaeomagnetic and K–Ar whole rock age dating study has

Meteorite flux on the Nullarbor Region, Australia

Abstract The Nullarbor Region of Australia is one of the most prolific sites for meteorite recoveries outside of Antarctica. Reported 14C terrestrial ages for chondritic meteorites from the Nullarbor

The Meteoritical Bulletin, No. 85, 2001 September

Abstract— Meteoritical Bulletin No. 85 lists information for 1376 newly classified meteorites, comprising 658 from Antarctica, 409 from Africa, 265 from Asia (262 of which are from Oman), 31 from

Ancient Meteorite Finds and the Earth's Surface Environment

Abstract The flux of meteorites to the Earth over the last 50,000 yr has remained approximately constant. Most meteorites that fall in temperate or tropical areas are destroyed on a time scale which

Meteorite Infall as a Function of Mass: Implications for the Accumulation of Meteorites on Antarctic Ice

  • G. Huss
  • Geology, Environmental Science
  • 1990
Antarctic meteorites are considerably smaller, on average, than those recovered elsewhere in the world, and seem to represent a different portion of the mass distribution of infalling meteorites.

Noble gas record, collisional history, and pairing of CV, CO, CK, and other carbonaceous chondrites

Abstract— Concentration and isotopic composition of the light noble gases as well as of 84Kr, 129Xe, and 132Xe have been measured in bulk samples of 60 carbonaceous chondrites; 45 were measured for

Exposure History of Shergottites Dar Al Gani 476/489/670/735 and Sayh Al Uhaymir 005

Four basaltic shergottites, Dar al Gani (DaG) 476, 489, 670, and 735 were found in the Libyan Sahara [1-3]; two basaltic shergottites, Sayh al Uhaymir (SaU) 005 and 008 were found in Oman [4].