3.34g CARANCAS Meteorite Fragment with Crust and Original Impact Crater I H4-5 Chondrite Rare Crater Maker
Description: A 3.34 gram partially crusted fragment of the Carancas H4-5 meteorite that entered the atmosphere over lake Titicaca and impacted the Earth on September 15th 2007 in Peru very near the border with Bolivia. This fragment of the Carancas meteorite is accompanied by a carefully collected piece of the impact crater under where the meteorite fragment was recovered. Both the meteorite and the piece of the crater were collected at the same time by a local villager very shortly after the impact.
Despite popular misconceptions, nearly all meteorites that hit the Earth breakup during their transit of the atmosphere and shed all of their "cosmic velocity" through aerial braking (drag). After losing this cosmic velocity they essentially "fall" from the sky reaching only terminal velocity, landing with minimal force and freezing cold. Stories of large impact craters, burning hot meteorites, noxious vapors, and strange illnesses are almost never actually true. In the case of the Carancas meteorite, some or perhaps even all of the above were corroborated and did indeed happen. A truly exceptional meteorite and impact event!
| Carancas | |||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Basic information |
This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: Yes Year fell: 2007 Country: Peru Mass: 342 g |
||||||||||||||||||
| Classification history: |
This is 1 of 82 approved meteorites classified as H4-5. |
||||||||||||||||||
| Comments: |
Revised 4 Aug 2008: final writeup; 2008-01-17 fix error in 17O |
||||||||||||||||||
| Writeup |
Writeup from MB 93
Carancas 16°39'52''S, 69°02'38''W Carancas, Chucuito, Puno, Peru Fall: 15 September 2007, ~16: 45 UTC Ordinary chondrite (H4-5) History: A large fireball was witnessed to impact near the community of Carancas, in the province of Chucuito, region of Puno in the country of Peru. It made a sizable impact crater, ~13.8 m in diameter (INGEMMET) or 11-12 m (L. Jackson, CGS). Local residents and many others have recovered numerous pieces of the impactor from the sides of the crater and the surrounding area. Mike Farmer brought several samples to the Lunar and Planetary Laboratory of the UAz for classification on October 5, 2007. The total mass is currently unknown. A preliminary report was published on the web by F. Luisa Macedo and O. José Macharé of INGIMMET, Peru. Physical characteristics: Most specimens are without fusion crust and have a gray color with some metal and chondrules visible, although the chondrules are not easily observed. At least one specimen had two different lithologies, the second white in color, indicating it is a breccia. Numerous black shock veins, often on more than one face of a specimen, were observed. At least one large (~2 cm) metal grain was also recovered, with a thin layer of stone attached to it. Petrography: (H. Connolly, KCCU, UAz; D. Hill, UAz, D. Schrader, UAz, K. Domanik, UAz, and D. Lauretta, UAz). One polished butt and one thin section, of two different samples, were examined. The polished butt contains some relict chondrules with well-defined margins and many textural types present. The thin section shows the rock to have experienced extensive recrystallization of the matrix with few relict chondrules present. Relict chondrules range in size from ~170 µm to 1 mm. Olivine and orthopyroxene were observed with abundant Fe, Ni-metal and Fe-rich sulfide. Mineral compositions: Olivine (Fa18.4±0.5) and pyroxene (Fs16.1±0.2). Oxygen isotopes: (R. Greenwood, OU; two analyses) δ17O = 3.017, 2.942; δ 18O = 4.519, 4.344; Δ17O = 0.667, 0.683 (all ‰). Classification: Ordinary chondrite (H4-5); W0, S3. Type specimens: A total of 22 g, including 5 thin sections, are on deposit at UAz. MFarmer holds 320 g. Submitted by: Harold C. Connolly Jr., KCCU and UAz. |
||||||||||||||||||
| Data from: MB107 Table 0 Line 0: |
|
||||||||||||||||||
We Also Recommend