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Benares (a) meteorite, Varanasi District, Uttar Pradesh, Indiai
Regional Level Types
Benares (a) meteoriteMeteorite Fall Location
Varanasi DistrictDistrict
Uttar PradeshState
IndiaCountry

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PhotosMapsSearch
Latitude & Longitude (WGS84):
25° 22' North , 82° 55' East
Latitude & Longitude (decimal):
Nearest Settlements:
PlacePopulationDistance
Varanasi1,164,404 (2014)10.9km
Barāgaon11,362 (2016)12.2km
Rāmnagar44,277 (2016)15.7km
Mughal Sarāi98,043 (2015)22.4km
Chunār36,459 (2015)26.8km
Mindat Locality ID:
270484
Long-form identifier:
mindat:1:2:270484:8
GUID (UUID V4):
ff0fad18-dcd6-49f1-aeb3-2f7f0660c147


Ordinary chondrite, (LL4; S4; W0)
Fell, 19 December 1798; 3.7 kg

After the appearance of a luminous meteor and detonations, many stones fell at Krakhut including a 900 g stone which fell through the roof of a home. Many stones were destroyed, but a number of spherical stones covered with a black fusion crust were preserved. The interiors consist of well delineated 'slate gray' chondrules, relict chondrules, chondrule fragments, and opaques within a light gray matrix rich in olivine and orthopyroxene. A few of the larger crystals have become isolated from the chondrules. Olivine composition (Fa28) is uniform, but the low-Ca pyroxene is quite variable (Fs12-24). Fe-Ni metal and troilite are found as polycrystalline grains and as partial rims around chondrule fragments. Olivine grains are fractured and mosaicized consistent with S4 level shock. A cosmic ray exposure (CRE) age of ~16 Ma has been reported for Benares (a). Benares (a) may be one of many LL chondrites (perhaps 1/3rd of all LL chondrites) apparently produced by the catastrophic disruption of a parent asteroid/meteoroid ~15 million years ago.

Historically, Benares (a) was an important meteorite in the story of the scientific acceptance of meteorites as extra-terrestrial objects. In 1802 Edward C. Howard found that the peculiar Ni-bearing iron found in Benares (a) and other meteorites was different from all known sources of natural terrestrial iron. Today, Benares (a) is classified as a member of the LL geochemical group of ordinary chondrites (ordinary chondrites very low in total iron). The LL chondrites are the smallest group of ordinary chondrites (~10% of all fully classified witnessed meteorite falls). The LL4 petrologic type of LL chondrites themselves are relatively rare. Only 7 meteorite falls were classified exactly as an 'LL4' chondrites at the Meteoritical Bulletin Database (as of early 2016). Only the 80 kg Soko-Banja fall of 1877 has had a significantly larger mass. According to the Catalogue of Meteorites (2000) a number of specimens of small and moderate mass are still held by different institutions, but the mislabeling of some specimens suggests that additional caution may be needed in interpreting future studies.

What's in a name? 'Benares (a)' is a well-established witnessed meteorite fall. 'Benares (b)' is the name of a more poorly documented and artificially heated iron meteorite discovered somewhat later in the same region of India.

Select Mineral List Type

Standard Detailed Gallery Strunz Chemical Elements

Mineral List


2 valid minerals.

Meteorite/Rock Types Recorded

Note: data is currently VERY limited. Please bear with us while we work towards adding this information!

Select Rock List Type

Alphabetical List Tree Diagram

Detailed Mineral List:

Diopside
Formula: CaMgSi2O6
Reference: Dunn, T.L., Cressy, G., McSween Jr, H.Y. & McCoy, T.J. (2010) Analysis of ordinary chondrites using powder X-ray diffraction: 1. Modal mineral abundances. Meteoritics & Planetary Science 45(1):123-134. (Jan 2010). (Jan 2010).
'Fayalite-Forsterite Series'
Description: Olivine of uniform composition (Fa28).
Reference: Mason, B. (1963) Olivine in ordinary chondrites. Geochimica et Cosmochimica Acta 27(9): 1011-1023. (Sept 1963).; Mason, B. (1986) Classification of the Benares Chondrite: Meteoritics 21 (1): 131-132. (Mar 1986).; Dunn, T.L., Cressy, G., McSween Jr, H.Y. & McCoy, T.J. (2010) Analysis of ordinary chondrites using powder X-ray diffraction: 1. Modal mineral abundances. Meteoritics & Planetary Science 45(1):123-134. (Jan 2010). (Jan 2010).; Grady, M.M., Pratesi, G. & Moggi-Cecchi, V. (2015) Atlas of Meteorites. Cambridge University Press: Cambridge, United Kingdom. 373 pages.
'Meteoritic Iron'
Reference: Grady, M.M., Pratesi, G. & Moggi-Cecchi, V. (2015) Atlas of Meteorites. Cambridge University Press: Cambridge, United Kingdom. 373 pages.
'Orthopyroxene Subgroup'
Reference: Dunn, T.L., Cressy, G., McSween Jr, H.Y. & McCoy, T.J. (2010) Analysis of ordinary chondrites using powder X-ray diffraction: 1. Modal mineral abundances. Meteoritics & Planetary Science 45(1):123-134. (Jan 2010). (Jan 2010).; Grady, M.M., Pratesi, G. & Moggi-Cecchi, V. (2015) Atlas of Meteorites. Cambridge University Press: Cambridge, United Kingdom. 373 pages.
'Plagioclase'
Formula: (Na,Ca)[(Si,Al)AlSi2]O8
Reference: Mason, B. (1986) Classification of the Benares Chondrite: Meteoritics 21 (1): 131-132. (Mar 1986).; Dunn, T.L., Cressy, G., McSween Jr, H.Y. & McCoy, T.J. (2010) Analysis of ordinary chondrites using powder X-ray diffraction: 1. Modal mineral abundances. Meteoritics & Planetary Science 45(1):123-134. (Jan 2010). (Jan 2010).
'Pyroxene Group'
Formula: ADSi2O6
Description: Low-Ca pyroxene (mostly or entirely orthopyroxene) is polysynthetically twinned with variable composition (Fs12-24). Diopside also present.
Reference: Mason, B. (1986) Classification of the Benares Chondrite: Meteoritics 21 (1): 131-132. (Mar 1986).
Troilite
Formula: FeS
Reference: Mason, B. (1986) Classification of the Benares Chondrite: Meteoritics 21 (1): 131-132. (Mar 1986).; Dunn, T.L., Cressy, G., McSween Jr, H.Y. & McCoy, T.J. (2010) Analysis of ordinary chondrites using powder X-ray diffraction: 1. Modal mineral abundances. Meteoritics & Planetary Science 45(1):123-134. (Jan 2010). (Jan 2010).; Grady, M.M., Pratesi, G. & Moggi-Cecchi, V. (2015) Atlas of Meteorites. Cambridge University Press: Cambridge, United Kingdom. 373 pages.

Gallery:

List of minerals arranged by Strunz 10th Edition classification

Group 2 - Sulphides and Sulfosalts
Troilite2.CC.10FeS
Group 9 - Silicates
Diopside9.DA.15CaMgSi2O6
Unclassified Minerals, Rocks, etc.
'Fayalite-Forsterite Series'-
'Meteoritic Iron'-
'Orthopyroxene Subgroup'-
'Plagioclase'-(Na,Ca)[(Si,Al)AlSi2]O8
'Pyroxene Group'-ADSi2O6

List of minerals for each chemical element

OOxygen
O Plagioclase(Na,Ca)[(Si,Al)AlSi2]O8
O Pyroxene GroupADSi2O6
O DiopsideCaMgSi2O6
NaSodium
Na Plagioclase(Na,Ca)[(Si,Al)AlSi2]O8
MgMagnesium
Mg DiopsideCaMgSi2O6
AlAluminium
Al Plagioclase(Na,Ca)[(Si,Al)AlSi2]O8
SiSilicon
Si Plagioclase(Na,Ca)[(Si,Al)AlSi2]O8
Si Pyroxene GroupADSi2O6
Si DiopsideCaMgSi2O6
SSulfur
S TroiliteFeS
CaCalcium
Ca Plagioclase(Na,Ca)[(Si,Al)AlSi2]O8
Ca DiopsideCaMgSi2O6
FeIron
Fe TroiliteFeS

References

Sort by

Year (asc) Year (desc) Author (A-Z) Author (Z-A)
Mason, B. (1963) Olivine in ordinary chondrites. Geochimica et Cosmochimica Acta 27(9): 1011-1023. (Sept 1963).
Mason, B. (1986) Classification of the Benares Chondrite: Meteoritics 21 (1): 131-132. (Mar 1986).
Burke, J.G. (1986) Cosmic Debris: Meteorites in History. University of California Press: Berkeley; Los Angeles. 441 pages.
Graf, T. & Marti, K. (1994) Collisional records in LL-chondrites. Meteoritics 29(5): 643–648. (Sept 1994).
Grady, M.M. (2000). Catalogue of Meteorites (5/e). Cambridge University Press: Cambridge; New York; Oakleigh; Madrid; Cape Town. 689 pages.
Dunn, T.L., Cressy, G., McSween Jr, H.Y. & McCoy, T.J. (2010) Analysis of ordinary chondrites using powder X-ray diffraction: 1. Modal mineral abundances. Meteoritics & Planetary Science 45(1):123-134. (Jan 2010).
Grady, M.M., Pratesi, G. & Moggi-Cecchi, V. (2015) Atlas of Meteorites. Cambridge University Press: Cambridge, United Kingdom. 373 pages.

External Links


Other Regions, Features and Areas containing this locality

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