Search

NASA Goddard Space Flight Center has developed a configurable phase mirror system that can address likely obstacles in space optical communications. Through using miniature adjustable mirrors and programmed phase delays to diffract a single communication beam, numerous diffracted beams can be sent to other satellites in various directions for communication and tracking. The initial laser beams wave profile can be dynamically regulated through a fast Fourier transform (FFT) so that when it reaches its desired destination, it forms an intended illuminated spot at the target satellite. Since all the diffracted beams share the same phase mirror, the antenna gain needed to broadcast these beams does not require a multiplied aperture.

Initially developed as a close quarters inspection tool capable of accessing hard to reach, tight, or visibly restricted, areas of satellites, the VIPIR system can be used to remotely inspect inaccessible locations such as behind a sheet of thermal blanketing material, into a satellites plumbing, or perhaps even deep inside the otherwise unreachable crevasses of a spacecraft bus. The VIPIR system incorporates a number of subassemblies for incredible operational freedom and capabilities for imaging and dissemination of componentry. VIPIR’s Video Borescope Assembly (VBA) is a flexible snake-camera capable of multidirectional articulations, making steering and control simple and intuitive for an operator. The VBA also includes at least one imaging sensor and lighting to see in dark, confined spaces. Real-time, high-resolution visual information can be fed back to an operator for live analysis. A reel system extends and retracts the VBA with the use of a spool, and includes position indicators for deployment tracking. The Tendon Management System (TMS), not unlike human tendons, utilizes pulleys and tensioners to articulate the VBA in the confined spaces. A seal system ensures the VBA is free of contamination. VIPIR underwent space-based testing on the ISS during the Robotic Refueling Phase 2 (RRM-2) mission designed to showcase and test several NASA advanced robotic satellite servicing technologies. During this mission, VIPIR demonstrated state-of-the-art near and midrange inspection capabilities. NASA’s VIPIR system is available for licensing to industry, and may be desirable to companies focused on satellite servicing, on-orbit assembly, and other applications requiring detailed inspection of assets in space.

The Client Berthing System (CBS) was originally designed for NASA’s On-orbit Servicing, Assembly, and Manufacturing 1 (OSAM-1) spacecraft, which will grapple and refuel the LandSat 7 satellite. After the OSAM-1 spacecraft has rendezvoused with LandSat 7, a robotic arm equipped with a gripper tool will autonomously grapple the satellite’s Marman ring (launch separation ring) and affix it to the CBS in the appropriate refueling position. The CBS is comprised of three posts protruding from the servicing satellite, each with integrated berthing mechanisms, distributed in a radial pattern of 120° along the client’s Marman ring diameter. Each berthing mechanism includes a rotary clamping jaw with a drawdown and radial contact portion. The clamping jaws are actuated by a motor-driven leadscrew and guided by recirculating linear ball bearings. After the servicing spacecraft’s robotic arm has placed the client satellite Marman ring into the CBS berthing box, the clamping jaws simultaneously move radially inward towards the center of the ring. The lead-in features of the jaws exert downward pressure on the ring, driving it towards the jaw palms as the lead-in portion rises over the surface of the ring flange. Once the flange is drawn down such that it contacts the radial clamp surface of the jaws, force is exerted causing the jaws to pivot, driving the underside of the lead-in surfaces into contact with the upper flange surface. As the jaw mechanisms continue to drive, increased axial load squeezes the ring flange between the lead-in-feature and palm of the jaws, stabilizing the connection. At a predetermined load, brakes are engaged, and system motors shut off. A NASA-developed Marman ring location detection system is employed to guide the berthing process. NASA has developed a suite of cutting-edge technologies that can help your business develop robust satellite servicing offerings. For additional information, please see the NASA Satellite Servicing Technologies Available for Licensing link provided.

Next generation instruments are capable of producing data at rates of 108 to 1011 bits per second, and both their instrument designs and mission operations concepts are severely constrained by data rate/volume. SpaceCube is an enabling technology for these next generation missions. SpaceCube has demonstrated enabling capabilities in Earth Science, Planetary, Satellite Servicing, Astrophysics and Heliophysics prototype applications such as on-board product generation, intelligent data volume reduction, autonomous docking/landing, direct broadcast products, and data driven processing with the ability to autonomously detect and react to events. SpaceCube systems are currently being developed and proposed for platforms from small CubeSats to larger scale experiments on the ISS and standalone free-flyer missions, and are an ideal fit for cost constrained next generation applications due to the tremendous flexibility (both functional and interface compatibility) provided by the SpaceCube system.

The TerraROVER’s core functionality is centered around its electric propulsion system, enabling it to traverse various outdoor environments. Its drive system consists of electric motors and gearboxes that provide controlled speed and maneuverability. The remote-control interface allows users to adjust speed and direction, making it an effective platform for training and testing mobility systems. For advanced applications, the TerraROVER can be adapted for pre-programmed or autonomous navigation, expanding its use in robotics and automation research. A key design feature of the TerraROVER is its adaptability for sensor integration. It includes mounting provisions for miniaturized sensors capable of capturing environmental data such as temperature, GPS location, and visual imagery. The platform supports both onboard data logging and real-time transmission, making it suitable for field studies, distributed sensing applications, and educational experiments. Fabrication is streamlined through the use of 3D-printed components, allowing for cost-effective production and easy assembly in classroom or research settings. Currently at Technology Readiness Level (TRL) 7, the system has been successfully demonstrated in an operational environment and is available for patent licensing.

To enable it to acquire GPS signals very quickly and also track weak signals, the radiation-hardened Navigator receiver utilizes a bank of hardware correlators, a ColdFire microprocessor, and a specialized fast acquisition module (see figure 1). The hardware is implemented in VHSIC Hardware Description Language (VHDL) to target radiation-hardened Field Programmable Gate Arrays (FPGA) rather than Application-Specific Integrated Circuits (ASIC), in order to maintain flexibility for growth and design modifications. The Navigator was designed to operate autonomously to enable the use of GPS for onboard navigation in high altitude space missions. With the exception of GPS signals, Navigator requires no external data (e.g., current time estimate, recent GPS almanac, or converged navigation filter estimate of the receiver dynamics). By double buffering data up front in 1ms blocks, data can be processed as it is acquired. A discrete Fourier transform (DFT) is used to calculate the 1ms correlations, significantly reducing computing time. Computational efficiency is optimized and tradeoffs among sampling rate, data format, and data-path bit rate are carefully weighed in order to increase performance of the algorithm. In addition, the Navigators hardware-independent receiver software includes both a hardware interface to perform low-level functions as well as basic navigation. Onboard orbit determination and accurate state estimation/propagation during periods with no GPS access are accomplished by integration with the GPS Enhanced Onboard Navigation System (GEONS). Exploiting the properties of Fourier transform in a massively parallel search for the GSP signal, the Navigator has been tested and proven capable of acquiring signals at 25dB-Hz and below.

The Gripper is located at the end of a robotic system consisting of a robotic arm equipped with a Tool Drive or End Effector comprising the input actuator to the Gripper as well as the structural, power and data link between the Gripper and the robotic arm. In a notional concept of operations, a Servicer would approach the Client in an autonomous rendezvous and capture (AR&C) maneuver. When the Servicers sensor suite confirms that the distance, orientation, and relative translational and angular rates with respect to the Client are within an acceptable range, the Servicer enables the grasping sequence, where the robotic arm, equipped with Gripper, extend forward to the Client. When the Gripper/ Servicer sensors indicate that the Client marman ring is sufficiently within the capture range of the Gripper, a trigger signal is sent to the robot control system that commands the End Effector to drive the mechanism of the Gripper and affect closure around the marman ring. The Gripper consists of a pair of jaws which are driven by an internal transmission. The transmission receives input torque from the End Effector and converts the torque to appropriate motion of the jaws.

The CSV replaces a standard spacecraft Fill and Drain Valve to facilitate cooperative servicing. The CSV offers various advantages over standard service valves: a robotic interface, three individually actuated seals, a self-contained anti-back drive system, and built-in thermal isolation. When mounted to a spacecraft as designed, the CSV transfers all operational and induced robotic loads to the mounting structure. An anti-back drive mechanism prevents the CSV seal mechanism from inadvertent actuation. Alignment marks, thermal isolation, and a mechanical coupling capable of reacting operational and robotic loads optimize the CSV for tele-robotic operations. Unique keying of the mating interface prevents mixing of media where more than one configuration of the CSV is used. Color-coding and labels are also used to prevent operator error. The CSV has four configurations for different working fluids, all with essentially unchanged geometry and mechanics.

The MXS produces electrons by shining UV light from an LED onto a photocathode material such as magnesium. The electrons are then accelerated across several kV and into a chosen target material; deceleration produces X-rays characteristic of the target. The MXS uses an electron multiplier for high X-ray production efficiency. The MXS is more compact, rugged, and power-efficient than standard X-ray sources. It can be manufactured using commercially available components and 3D printed housing, resulting in a low cost to manufacture. Unlike traditional X-ray sources, the MXS does not require a filament or vacuum and cooling systems. Most importantly, enabling rapid and arbitrary modulation allows using X-rays in the time domain, a new dimension to X-ray applications.