Track C44

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Stardust Catalog Track Information for Track C44

Information Details

Track Number: C44 Sample Name: C2004,1,44,0,0
Extraction Date: 02/22/2006 Extracted By: TB
Track Type:     Hedgehog / Crater
Track Length (µm): 8000.000 Entry Hole (EH) Diameter:
Bulb Width (BW): 0.000 Bulb Depth (BD):
Keystone Thickness: Terminal Particle (TP) Info:

Subsample List

Sample Name Description Allocation Status
C2004,1,44,1,0 Grain on glass fiber Available
C2004,1,44,2,0 Grain on glass fiber Available
C2004,1,44,3,0 Grain on glass fiber On Loan
C2004,1,44,4,0 Grain on glass fiber, then potted butt On Loan
C2004,1,44,4,1 C on Cu grid Available
C2004,1,44,4,2 C on Cu grid Available
C2004,1,44,4,3 C on Cu grid Available
C2004,1,44,4,4 C on Cu grid Available
C2004,1,44,4,5 C on Cu grid Available
C2004,1,44,4,6 Particle Fragment Ultramicrotomed TEM Grid On Loan
C2004,1,44,4,7 Particle Fragment Ultramicrotomed TEM Grid On Loan
C2004,1,44,4,8 Particle Fragment Ultramicrotomed TEM Grid On Loan
C2004,1,44,4,9 Particle Fragment Ultramicrotomed TEM Grid On Loan

Track Notes

Sample Name Notes Category
C2004,1,44,0,0 This is the largest impact feature in the cometary tray. The impact feature is large because the cometary particle struck the edge of the tray frame and then bounced into the adjacent aerogel. The cel ... Processing
C2004,1,44,0,0 This is the largest impact feature in the cometary tray. The impact feature is large because the cometary particle struck the edge of the tray frame and then bounced into the adjacent aerogel. The cel ... Processing
C2004,1,44,0,0 This is the largest impact feature in the cometary tray. The impact feature is large because the cometary particle struck the edge of the tray frame and then bounced into the adjacent aerogel. The cel ... Processing
C2004,1,44,1,0 [SXRD]: Seussite (Fe3Si), probably formed during capture. Analysis
C2004,1,44,1,0 removed by zolensky 2/14/06; 44,1-4 removed from piece 004,1 by TNakamura
C2004,1,44,2,0 [SXRD]: Seussite (Fe3Si), probably formed during capture. Analysis
C2004,1,44,3,0 [CT tomography]: Small grains of heavy minerals (kamacite?: the size must be less than the CT spatial resolution) are embedded in a porous material, whichmay be aerogel with or without very fine comet ... Analysis
C2004,1,44,3,0 [CT Tomo]: Small grains of heavy minerals (kamacite?: the size must be less than the CT spatial resolution) are embedded in a porous material, which may be aerogel with or without very fine cometary d ... Analysis
C2004,1,44,4,0 Rietmeijer (TEM): Particle contains extremely rare pyrrhotite, extremely raregrains that are a regular mixture (crystallographic controlled intergrowth?) of pyrrhotite and kamacite, round kamacite inc ... Analysis
C2004,1,44,4,0 T. Stephan (Tof-SIMS): Most analyzed elements have essentially chondritic abundances;but K Co, Cu enriched up to 5 x CI. Analysis
C2004,1,44,4,0 Tomeoka (TEM): Fe-Ni metal (incl. kamacite) within Si-rich amorphous material. Analysis
C2004,1,44,4,0 PI note: Grain on glass fiber, then potted butt 12-29-2014 Allocation
C2004,1,44,4,0 From Brownlee files - Fe,Mg,S,Si by EDX, but only iron silicide phase by XRD; so mostly melted? Inventory
C2004,1,44,4,0 From Brownlee files - Grain was mounted in apoxy and cut 3/31/06 Inventory
C2004,1,44,4,0 Grain was mounted in apoxy and cut 3/31/06
C2004,1,44,4,1 slices 1-15
C2004,1,44,4,2 slices 17-26
C2004,1,44,4,3 slices 27-36
C2004,1,44,4,4 slices 37-46
C2004,1,44,4,5 slices 47-56

Track Photos


 
 
 

 
 

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