New Metals, Optics, Tools, and Processes Focus on Satellite Imaging
- Created: Sunday, 01 October 2006
Lightweight, aspheric, reflective optical designs commonly are designed and built for demanding space-based remote sensing, targeting systems, and aerial reconnaissance. Traditional designs utilizing low expansion optical glasses steadily are giving way to metals such as aluminum, beryllium, and AlBeMet, and ceramics such as silicon carbide. These materials can be produced in extremely lightweight, yet robust and athermalized, designs by virtue of their superior tensile strength, fracture toughness, and the ability to compose support structures and mirrors from identical materials.
In addition, these materials can often best exploit advancing freeform generating and computer polishing technologies. This discussion focuses on the performance tradeoffs among aluminum, AlBeMet, beryllium, and silicon carbide in the context of modern substrate manufacturing, optical generating, and computer polishing technologies. The goal is to provide the opto-mechanical engineer an overview of the confluence of material science and the state of the art in manufacturing technologies as they relate to ever more demanding optical performance objectives.
Reflective optical systems typically are chosen over refractive systems to achieve wavelength independence and/or lighter, more robust, and shorter packaging for a given aperture and effective focal length (EFL). Reflective designs become attractive for apertures greater than approximately 100-200 mm and where comparatively large fields of view are not required. Because surface figure irregularities of reflecting surfaces cause four times as much transmitted wavefront error (WFE) compared to refractive surfaces, and non-circular apertures and aspheric prescriptions are common, reflective surface manufacturing tolerances and corroborating metrology can be very challenging.
Types of reflecting surfaces range in difficulty from simple round and spherical progressing to irregular shaped flats, symmetric and off-axis aspheric, and finally “free form” surfaces that lack an axis of symmetry. These types of surfaces are commonly combined into symmetric and off-axis assemblies having two or more elements, as shown in Figure 1.
Reflective Optics Materials
A quick reference to the relative properties of various materials suited for manufacture of reflecting optical systems is included in the table on page 6a.
Beryllium exhibits low density, high stiffness, has attractive thermal properties, and can be machined into very thin sections. It is also very expensive, both as bulk material and post-processing. Most typically, beryllium is plated with electroless nickel plating to enable the manufacture of a high-quality optical surface. Beryllium may be bare polished, although at considerable added effort and cost. Aggressively light-weighted, bare polished beryllium was selected for the 18 mirror segments that will comprise the 8.0-meter aperture James Webb Space Telescope (JWST). Beryllium structures also may be brazed with aluminum alloy to create optical bench structures.
Aluminum beryllium such as Brush Wellman (Warren, MI) AlBeMet 162H is lower in bulk material and manufacturing cost, less hazardous, and has advantages in ductility and fracture toughness over beryllium. Laser and electron beam welding of AlBeMet recently has been introduced to form intricate lightweight structures to integrate AlBeMet mirrors, thus minimizing material utilization costs while achieving an athermalized, stiff, strong, and very lightweight design.
There is currently considerable interest in silicon carbide as a challenger to beryllium in many contexts. Many producers of SiC recently have emerged, reducing SiC costs compared to beryllium. Formulations of SiC, such as those produced by Poco Graphite (Decatur, TX), are listed in Table 1. The Poco process consists of manufacturing very intricate mirrors and matching structural elements from inexpensive and easily machined graphite prior to conversion to SiC.