Porosity of an Anhydrous Chondritic Interplanetary Dust Particle

Details Porosity of an Anhydrous Chondritic Interplanetary Dust Particle Porosity of an Anhydrous Chondritic Interplanetary Dust Particle

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995metic..30r.583s&link_type=abstract

Meteoritics, vol. 30, no. 5, page 583

Computer Science

Graphics

2

Chondritic, Dust Particles, Interplanetary, Porosity

Scientific paper

Determination of the density and porosity of Interplanetary Dust Particles (IDPs) is important in the dynamics of collisional and orbital evolution of small-sized particles. These measurements are also useful to suggest possible sources for IDPs based on comparisons with known extraterrestrial materials (e.g., chondrites). Previous work on IDPs shows a wide range of densities from very low (0.08 g/cm3 [1]) through low (0.3 g/cm3 [2]) to high (6.2 g/cm3 [3]), with an average density at 2.0 g/cm3 for 150 particles [2]. In another study, IDPs fall into two distinct density groups with mean values of 0.6 g/cm3 and 1.9g/cm3 [3]. In general, chondritic IDPs with lower density values most likely have appreciable porosity, suggesting they are primitive, uncompacted particles. It is believed that porosities greater than 70% are rare [2]. Sample In this study, porosity measurements were determined for one IDP, Clu17. This chondritic particle is a fragment of a large-sized IDP (L2008#5) known as a cluster particle. The cluster is composed of 53 fragments >5 micrometers in diameter; a detailed description of the cluster is given in [4]. IDP Clu17 has ~12 wt.% C and contains chondritic abundances (within 2xCI) for major elements. This fragment is dominated by fine-grained aggregates, also known as GEMS (glass with embedded metal and sulfide [5]), and contains some olivine, pyroxene, Fe-Ni sulfides, and carbonaceous material. Methods IDP Clu17 was analyzed for light elements quantitatively analysis using scanning electron microscopy and thin-window energy dispersive spectrometry [details of technique in 4]. Following the initial bulk chemical analysis, the particle was embedded in epoxy, thin sectioned using an ultramicrotome, and examined with a JEOL 2000 FX transmission electron microscope. Many of the sections were not complete; individual grains in some sections are lost during microtoming. Photos from nine of the best sections were digitized by scanning at 1200 dpi. The images were cropped and reduced in size to fit the memory capabilities of the computer analysis program. The digitized images were measured using NIH Image on a Macintosh computer. Results Using a combination of tools, including density slicing, area selection and a graphics tablet, to measure porosity, the sections give values from 9 to 15% porosity. There are a variety of errors that can enter into the measurement process: (1) defining exterior surface boundaries, which can vary between sections, (2) presence of holes in the sections where grains fell out during microtoming, and (3) differentiation between the mounting medium (epoxy) and extraterrestrial components (carbonaceous material can look similar to epoxy). As noted in earlier work [6], image processing is somewhat subjective and requires careful judgment in setting the conditions for electron microscopy and digital scanning. Conclusions Typical published anhydrous IDP porosities are in the 40% range [2], a value significantly higher than the 9-15% porosity range for IDP Clu17. The porosity values for cluster particles may be more difficult to determine because both the inter- and intra-fragment porosities must be considered. The inter-fragment porosity of ~10% for Clu17 is probably much lower than the intra-fragment porosity for cluster L2008#5 because this IDP remained intact on the collection surface while the cluster particle was fragmented into hundreds of smaller units, likely reflecting an high initial cluster porosity and low coherence. We conclude that image analysis combined with microtome sectioning offers a useful new tool for porosity measurements of IDPs and other kinds of extraterrestrial materials. Acknowledgments: This work was supported by NASA/JOVE Grant #NAG8-999. References: [1] Rietmeijer F. (1993) EPSL, 117, 609. [2] Love S. et al. (1994) Icarus, 111, 227. [3] Flynn G. and Sutton S. (1991) Proc. LPS, Vol. 21, 541. [4] Thomas K. et al. (1995) GCA, in press. [5] Bradley J. (1994) Science, 265, 925. [6] Strait M. et. al. (1994) Meteoritics, 29, 537.

Affiliated with

Also associated with

No associations

Rating

Porosity of an Anhydrous Chondritic Interplanetary Dust Particle does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Porosity of an Anhydrous Chondritic Interplanetary Dust Particle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Porosity of an Anhydrous Chondritic Interplanetary Dust Particle will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-830943