Antarctic Meteorite Newsletter, Volume 29, No. 1 - February 2006
Volume 29, No. 1 - February 2006

Petrographic Descriptions            Go to Pet. Desc. Page 1 of 2

Sample No.: LAP 031173;
LAP 04642
Location: LaPaz Ice Field
Field No.: 16105; 17406
Dimensions (cm):   1.5x1.0x0.5
1.0x1.0x0.5
Weight (g): 1.360; 1.196
Meteorite Type: H Chondrite (Impact Melt)
LAP 031173


Macroscopic Description: Kathleen McBride
The exteriors are covered with brown/black fusion crust with oxidation halos. The interiors are rusty brown with a brittle texture.

Thin Section (,2) Description: Tim McCoy and Linda Welzenbach
These sections are so similar that a single description suffices. The meteorites exhibit a microcrystalline silicate matrix including rounded metal-sulfide blebs reaching 20 microns and relict grains, chondrules and clasts reaching up to a few mm. Mafic silicate compositions (Fa19, Fs17) indicate they are of H chondrite parentage and textures suggest they are impact melt breccias.

Cross-Polarized LightPlane-Polarized LightReflected Light
LAP 031173 - Cross-Polarized Light LAP 031173 - Plane-Polarized Light LAP 031173 - Reflected Light

Cross-Polarized LightReflected Light
LAP 04642 - Cross-Polarized Light LAP 04642 - Reflected Light



Sample No.: LAP 031214
Location: LaPaz Ice Field
Field No.: 16820
Dimensions (cm):   3.0x2.0x2.0
Weight (g): 9.504
Meteorite Type: CM 1-2 Chondrite
LAP 031214 LAP 031214
LAP 031214   


Macroscopic Description: Kathleen McBride
Thick purple-black fusion crust covers 40% of the exterior. Polygonal fractures are visible. The interior is a dark gray to black matrix with an oxidation rind.

Thin Section (,2) Description: Tim McCoy and Linda Welzenbach
The sections consist of a few isolated mineral grains in a black matrix; rare metal and sulfide grains are present. Olivine compositions are Fa1-41. The meteorite is a CM chondrite and is intermediate between type 1 and type 2.

Plane-Polarized LightReflected LightReflected Light
LAP 031214 - Plane-Polarized Light LAP 031214 - Reflected Light
LAP 031214 - Reflected Light



Sample No.: LAP 031280
Location: LaPaz Ice Field
Field No.: 16046
Dimensions (cm):   4.0x2.75x1.0
Weight (g): 17.752
Meteorite Type: Eucrite (Brecciated)
LAP 031280


Macroscopic Description: Kathleen McBride
Shiny, rough brown/black fusion crust covers 50% of this achondrite's exterior. The interior is a sandy textured, tan colored matrix with gray inclusions.

Thin Section (,2) Description: Tim McCoy and Linda Welzenbach
The meteorite is a dominated by a fine-grained (50-100 micron grain size) basaltic host with coarser-grained areas that may be clasts incorporated prior to metamorphism. Pyroxene is exsolved on a 1-20 micron scale. Orthopyroxene analyses range to Fs60Wo5 and augite to Fs32Wo40. Plagioclase is An88Or0.5. The Fe/Mn ratio of the pyroxene is ~30. The meteorite is a eucrite.

Cross-Polarized LightPlane-Polarized LightCross-Polarized LightPlane-Polarized Light
LAP 031280 - Cross-Polarized Light LAP 031280 - Plane-Polarized Light
LAP 031280 - Cross-Polarized Light LAP 031280 - Plane-Polarized Light



Sample No.: LAP 031323
Location: LaPaz Ice Field
Field No.: 16647
Dimensions (cm):   1.5x1.5x1.0
Weight (g): 3.125
Meteorite Type: Acapulcoite
LAP 031323


Macroscopic Description: Kathleen McBride
50% of the exterior has brown/black fusion crust. The rusty, granular textured interior has a high metal content.

Thin Section (,2) Description: Tim McCoy and Linda Welzenbach
The section consists of an equigranular mixture of olivine (Fa13), orthopyroxene (Fs12Wo2), clinopyroxene (Fs5Wo43), plagioclase (An15Or4), metal and troilite. Mafic grain sizes are ~100 microns, triple junctions are common and plagioclase is interstitial to and includes mafic silicates. The rock is an acapulcoite, but similar in texture to the intermediate members of the acapulcoite-lodranite clan EET 84302 and GRA 95209.

Cross-Polarized LightPlane-Polarized LightCross-Polarized LightPlane-Polarized Light
LAP 031323 - Cross-Polarized Light LAP 031323 - Plane-Polarized Light
LAP 031323 - Cross-Polarized Light LAP 031323 - Plane-Polarized Light



Sample No.: CMS 04016
Location: Cumulus Hills
Field No.: 14674
Dimensions (cm):   5.0x4.0x3.0
Weight (g): 162.069
Meteorite Type: L3 Chondrite
CMS 04016 CMS 04016


Macroscopic Description: Kathleen McBride
The exterior and interior of this meteorite is rusty with a high metal content.

Thin Section (,2) Description: Tim McCoy and Valerie Reynolds
Cross-Polarized LightPlane-Polarized Light
CMS 04016 - Cross-Polarized Light CMS 04016 - Plane-Polarized Light
The section exhibits numerous well-defined chondrules (up to 1.5 mm) in a black matrix of fine-grained silicates, metal and troilite. Weak shock effects are present. Polysynthetically twinned pyroxene is abundant. The meteorite is moderately weathered. Silicates are unequilibrated; olivines range from Fa1-26, with most grains Fa20-26, and pyroxenes from Fs5-12. The meteorite is an L3 chondrite (estimated subtype 3.8).



Sample No.: LAP 04840
Location: LaPaz Ice Field
Field No.: 17198
Dimensions (cm):   5.0x3.0x1.75
Weight (g): 50.405
Meteorite Type: R Chondrite
LAP 04840 LAP 04840


Macroscopic Description: Kathleen McBride
Rough, black fusion crust with polygonal fractures is present on the exterior surface. The interior is a fine grained crystalline matrix with black and white crystalline inclusions. The meteorite was very hard with no rusting or apparent metal.

Thin Section (,4) Description: Tim McCoy
The section is texturally heterogeneous, containing relict chondrules up to 1 mm, isolated mineral grains of 100-200 microns and microcrystalline areas reaching 1 mm with mafic silicate grain sizes of 5-10 microns. Shock effects are pervasive, particularly in plagioclase. The rock consists of FeO-rich olivine (Fa38) and orthopyroxene (Fs30Wo1). Plagioclase is An7Or3. A brown, strongly pleochroic mineral comprises ~15% of the section. Microprobe analyses suggest hornblende with approximately 48% SiO2, 3% Na2O, 6% Al2O3, 16.5% MgO, 11% FeO, 10% CaO and < 0.5% TiO2, MnO and K2O. Low totals and the strong pleochroism may be due to structurally bound OH, as no Cl was noted in EDS analyses. Opaques include troilite, pentlandite and chromite. The meteorite is an R chondrite of petrologic type 6.

Oxygen isotope analysis laser fluorination: D. Rumble
The analysis of two silicate-rich fractions yielded δ18Ο=+4.28, δ17Ο=+4.37, and δ18Ο=+4.76, δ17Ο=+5.76, similar to other R-chondrites.

Cross-Polarized LightPlane-Polarized LightCross-Polarized LightPlane-Polarized LightReflected Light
LAP 04840 - Cross-Polarized Light LAP 04840 - Plane-Polarized Light
LAP 04840 - Cross-Polarized Light LAP 04840 - Plane-Polarized Light
LAP 04840 - Reflected Light



Sample No.: LAP 04843
Location: LaPaz Ice Field
Field No.: 17006
Dimensions (cm):   5.0x5.0x2.5
Weight (g): 108.639
Meteorite Type: CV3 Chondrite
LAP 04843 LAP 04843


Macroscopic Description: Kathleen McBride
The exterior has rough, black fusion crust with purple shiny areas. Vugs of plucked areas are visible. The muddy gray matrix has white clasts with evaporites. This meteorite was very hard.

Thin Section (,4) Description: Tim McCoy and Linda Welzenbach
The section exhibits large chondrules (up to 3 mm) and CAIs in a dark matrix. Olivines range from Fa1-46 and a single pyroxene is Fs1. The meteorite is an oxidized CV3.

Cross-Polarized LightPlane-Polarized LightCross-Polarized LightPlane-Polarized Light
LAP 04843 - Cross-Polarized Light LAP 04843 - Plane-Polarized Light
LAP 04843 - Cross-Polarized Light LAP 04843 - Plane-Polarized Light



Sample No.: LAP 04844
Location: LaPaz Ice Field
Field No.: 17074
Dimensions (cm):   2.0x2.0x1.5
Weight (g): 6.831
Meteorite Type: Diogenite
LAP 04844


Macroscopic Description: Kathleen McBride
The exterior has some patchy brown/black fusion crust. The tan to yellowish fine grained matrix has green and brown clasts of various sizes.

Thin Section (,2) Description: Tim McCoy and Linda Welzenbach
Cross-Polarized LightPlane-Polarized Light
LAP 04844 - Cross-Polarized Light LAP 04844 - Plane-Polarized Light
The section shows a groundmass of coarse (up to 1.5 mm) comminuted pyroxene. Orthopyroxene has a composition of Fs23Wo2. The meteorite is a diogenite and is probably paired with the LAP 91900 pairing group.



Sample No.: MAC 04930
Location: MacAlpine Hills
Field No.: 15086
Dimensions (cm):   0.5x0.7x0.4
Weight (g): 0.880
Meteorite Type: H3 Chondrite


Macroscopic and Thin Section (,2) Description: Tim McCoy and Linda Welzenbach
Cross-Polarized LightPlane-Polarized Light
MAC 04930 - Cross-Polarized Light MAC 04930 - Plane-Polarized Light
This pea sized rusty ordinary chondrite exhibits numerous small chondrules (up to 1 mm) in a black matrix with irregular metal and troilite. The meteorite is highly weathered. Silicates are unequilibrated; olivines range from Fa2-24 and pyroxenes from Fs3-12. The meteorite is an H3 chondrite (estimated subtype 3.6).



Sample No.: MAC 041169
Location: MacAlpine Hills
Field No.: 15371
Dimensions (cm):   1.75x1.5x0.75
Weight (g): 3.187
Meteorite Type: Eucrite (Unbrecciated)
MAC 041169


Macroscopic Description: Kathleen McBride
40% rough, black fusion crust covers the exterior of this meteorite. The interior is a coarse grained black and white matrix with rusty areas.

Thin Section (, 3) Description: Tim McCoy
Cross-Polarized LightPlane-Polarized Light
MAC 041169 - Cross-Polarized Light MAC 041169 - Plane-Polarized Light
The meteorite is a medium-grained (100-200 micron grain size), unbrecciated basalt with numerous late-stage interstitial melt pockets that can reach several hundreds of microns. Mineral compositions are relatively homogeneous with orthopyroxene (Fs57-64Wo2-5), with 1-5 micron lamellae of augite (Fs32Wo39), and plagioclase (An89Or0.5). The Fe/Mn ratio of the pyroxene is ~30. The meteorite is an unbrecciated eucrite.



Sample No.: MAC 041269
Location: MacAlpine Hills
Field No.: 15820
Dimensions (cm):   2.0x1.5x1.0
Weight (g): 4.509
Meteorite Type: Howardite


Macroscopic Description: Kathleen McBride
50% of the exterior surface is covered with black shiny (like glass) fusion crust. The interior is a black and gray, fine grained matrix with black and white inclusions. Very minor amount of rust is present.

Thin Section (,2) Description: Tim McCoy and Linda Welzenbach
Cross-Polarized LightPlane-Polarized Light
MAC 041269 - Cross-Polarized Light MAC 041269 - Plane-Polarized Light
The section shows a groundmass of comminuted pyroxene and plagioclase (up to 0.5 mm) with fine- to coarse-grained basaltic clasts ranging up to 5 mm. Pyroxene ranges from pigeonite composition (possibly finely exsolved) of Fs56Wo6 to augite of Fs28Wo40. Plagioclase is An89Or0.5. The meteorite is a howardite.



Go to Pet. Desc. Page 1 of 2