![]() |
||
|
Knardna 001 | |||||||||||||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Basic information | Name: Knardna 001 This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2012 Country: Australia Mass: ![]() | ||||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 6407 approved meteorites (plus 2 unapproved names) classified as H4. [show all] Search for other: H chondrites, H chondrites (type 4-7), Ordinary chondrites, and Ordinary chondrites (type 4-7) | ||||||||||||||||||||||||||||||||||||||
Comments: | Approved 18 Jul 2015 | ||||||||||||||||||||||||||||||||||||||
Writeup![]() |
Writeup from MB 104:
Knardna 001 31° 0’18.70"S, 130°54’18.60"E South Australia, Australia Purchased: 2012 May 16 Classification: Ordinary chondrite (H4) History: Fragment found by J. Kuyken on claypan. Physical characteristics: Broken desert-red fragment with 15% fusion crust. Petrography: (L. Bowlt, Monash) This sample contains chondrules that are highly fragmented and poorly defined, as well as chondrules that make sharp contact with the surrounding matrix. The chondrules range in size up to 2 mm (average 0.2-1 mm). There are distinct light/dark areas at the sub-centimeter scale corresponding to two differing types of matrix; the majority of the sample contains recrystallised matrix and there are two areas that have an optically opaque matrix associated with shock blackening. Minerals include olivine, pyroxene, plagioclase (1-2 microns), Fe-Ni metal and troilite. Chondrules are relatively abundant (20-25%) and chondrule types include RP, BO, PO, PP and POP. Olivine grains show undulose extinction and shock lamellae. 60-70% of metal and troilite have been oxidised with the remaining 30-40% divided up between 30-35% sulphides and 5-10% metal grains. Geochemistry: (L. Bowlt, Monash) Microprobe analyses show that olivine and pyroxene compositions are uniform: olivine Fa16.9-17.7, mean= 17.3 mol%, std= 0.38, n=4; Low-Ca pyroxene Fs 14.8-15.9, mean= 15.48 mol%, std= 0.45, n=4. Classification: Ordinary Chondrite (H4 , S3, W3) Specimens: Specimen and one thin-section held by A. Tomkins. | ||||||||||||||||||||||||||||||||||||||
Data from: MB104 Table 0 Line 0: |
|
||||||||||||||||||||||||||||||||||||||
Institutions and collections |
Monash: Building 28
School of Geosciences
Monash University
Victoria 3800
Australia, Australia (institutional address; updated 12 Dec 2012) |
||||||||||||||||||||||||||||||||||||||
Catalogs: |
| ||||||||||||||||||||||||||||||||||||||
References: | Published in Meteoritical Bulletin, no. 104, MAPS 52, 2284, Octover 2017, http://onlinelibrary.wiley.com/doi/10.1111/maps.12930/full
| ||||||||||||||||||||||||||||||||||||||
Geography:![]() |
Statistics: This is 1 of 240 approved meteorites from South Australia, Australia (plus 3 unapproved names) (plus 4 impact craters) This is 1 of 717 approved meteorites from Australia (plus 46 unapproved names) (plus 27 impact craters) | ||||||||||||||||||||||||||||||||||||||
Proximity search: |