Next Generation Sample Preparation
Next Generation Sample Preparation
The Next Generation Sample Preparation laboratory supports sample characterization
facilities in the Astromaterials Research and Exploration Science Division at NASA
Johnson Space Center. In addition to traditional sample preparation protocols
(e.g., mechanical polishing), the facility utilizes a Hitachi ArBlade 5000C to
achieve high-quality sample surfaces (comparable to a 50 nm colloidal silica
dispersion polishing) without the use of contaminating fluids or mechanical polishing.
Purpose
The purpose of the Next Generation Sample Preparation laboratory is to enhance traditional sample preparation procedures with the use of ion polishing systems. The approach enables the preparation of challenging samples, including:
- Poly-phase materials of differential hardness (e.g., diamond-graphite assemblages in ureilites)
- Friable and/or porous samples, e.g., Ivuna-like carbonaceous chondrites (CI)
- Contamination-sensitive samples, such as returned samples
- Samples with fine-grained matrices
- Bulk preparation of small particles
New Approaches to Sample Preparation
Typical ion polishing systems involve cross-section milling, where a sample is ion polished with the ion beam
normal to a pre-cut and/or polished surface (e.g., Figure 1 A). Cross-section polishing is often used to prepare
microelectronics, where microanalysis of the internal structure is of interest. However, cross-section polishing
is spatially limited to only a few millimeters that can be ion polished. As such, it is not well-suited for
investigation of geologic materials, where sufficient surface area must be prepared to provide the necessary
petrologic context for geochemical investigations of heterogeneous materials. Moreover, sample mounts that are
typical for geologic materials are often circular to accommodate sample mount holders in analytical instruments
(e.g., EPMA, SEM, NanoSIMS, etc.) and larger than can be accommodated in cross-section polishing systems (10 – 25 mm diameter sample mounts).
Recent development of broad area flat milling capabilities has addressed the issues with cross-sectional polishing
(Figure 1 B). Flat milling incorporates three additional variables:
- variation in the ion beam angle relative to the sample surface
- sample rotation
- sample offset relative to the axis of rotation (i.e., eccentricity)
The addition of cryogenic stage cooling with temperature control has also resulted in improvements of the ion milling systems
that minimize sample damage. The cryogenic model of the Hitachi ArBlade 5000 (i.e., ArBlade5000C) provides active cooling of both
the cross-section and flat area milling stages during ion polishing. Liquid nitrogen is supplied to the sample holders to remove heat
from both the sample and the milling mask. Following ion milling, the specimen stage is incrementally warmed to prevent ice formation,
water condensation, and sample fracturing. The addition of cryogenic cooling permits samples that are temperature sensitive to be prepared
damage-free, a common problem for previous attempts to ion polish planetary materials. Finally, cryogenic cooling will be greatly beneficial
to future sample return missions that require sample preparation at low temperatures to preserve important characteristics of delicate samples
(e.g., volatiles and organics) and precious samples (e.g., Apollo 17 frozen basalts)

Ion Polishing System Specifications
The ArBlade 5000C is a broad beam Ar ion polishing system with cryogenic cooling and air protection capabilities and has greatly improved capabilities
over earlier cross-section ion polishing systems, which include:
- A hybrid milling system that incorporates flat milling capabilities to permit preparation of typical SIMS and EPMA mounts
- Cryogenic stage cooling temperature control that minimizes sample damage
- Air protection capabilities for sample preparation without exposure to atmosphere
- Increased ion gun milling rate
- In-situ monitoring of sample polishing
Model 1040 NanoMill® TEM Specimen Preparation System
The NanoMill system uses an ultra-low energy, concentrated ion beam to produce high quality specimens free from amorphous and implanted layers.
Ideal for polishing FIB-milled specimens for transmission electron microscopy (TEM) and transmission Kikuchi diffraction (TKD).
NanoMill Specifications:
NanoMill Specifications:
- Ultra-low-energy, argon gas ion source (50-2000 eV)
- Concentrated ion beam with scanning capabilities
- Secondary electron detector allows for real-time viewing of the specimen
- Removes damaged and implanted layers without redeposition
- Room temperature to cryogenically cooled stage (temperatures down to -170 °C)
- Precise stage angle adjustment (range -10° to +30°)
- Ideal for preparing specimens from heterogeneous materials
- Inert gas/vacuum transfer option

Supporting Instrumentation
- Cressington 208HR (Au, Pt, and Ir coatings)
- Cressington 208C Carbon Coater
- Plasma Cleaner
- Buehler VibroMet2
- Buehler Minimet 1000 Grinder-Polishers
- Buehler IsoMet 1000 Precision Saws
- Buehler EcoMet 30 Semi-Automatic Grinder and Polisher
- Buehler PetroThin Sectioning System
- Zeiss Stemi 508 Stereomicroscope
- Zeiss Axioscope 5 Petrographic Microscope
- 2 Ton ICL Press with In-situ, Heated Platens with Temperature Control
- Vacuum Ovens and Dessicators
Sample Preparation Requests
Sample preparation requests, utilizing the Hitachi ArBlade 5000C and/or the NanoMill, can be submitted in two different ways:
- As a requirement included in a sample request to a NASA curation facility (e.g., Astromaterials Acquisition and Curation Office; AACO)
- As a short proposal solicited three times a year by ARES. User requests are evaluated based on suitability for ion polishing techniques and sample preparation requirements. Priority will be given to user requests submitted through the AACO, following review by the Astromaterials Allocation Review Board. All other requests will be prioritized on a first-come first-serve basis
Supported Laboratories
