Hexapods / Stewart Platforms in Astronomy

Commercial Stewart-Gough platform and parallel-kinematic hexapod systems for telescope alignment, active optics, image stabilization, radio telescope instrumentation, and precision observatory applications.

Active OpticsMirror Alignment6-Axis MotionParallel KinematicsTip/TiltObservatory Instrumentation
Stewart Platforms for Telescope Alignment

The resolution of large ground-based telescopes is often limited by atmospheric turbulence, structural vibrations, and thermal disturbances. Over the past three decades, PI has developed numerous large-aperture fast steering mirrors (FSMs), tip/tilt systems, and hexapod alignment platforms for astronomical image stabilization and optical alignment. Piezo-driven active secondary mirrors can dramatically improve image quality by correcting wavefront distortions and image motion in real time. In many applications, these adaptive optics systems can increase effective resolution by up to an order of magnitude, particularly during long-exposure observations of faint celestial objects. Today, fast steering mirrors are also widely used in free-space optical communications, where they provide high-speed beam stabilization and tracking for satellite-to-satellite and ground-to-satellite links.

More information on FSMs, hexapods and other precision motion systems for Astronomy.

PI's hexapod 6-axis stewart platforms are key components for the precise alignment of active mirrors.

PI precision actuators provide superior performance and lifetime and have been used in large telescopes such as the ALMA Telescope in Chile consisting of 60+ Antennas spread across distances of up to 16 kilometers.

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Serial kinematics versus parallel kinematics hexapod positioner
A custom Stewart platform was developed to align the large segmented mirrors of the James Webb Space Telescope during assembly and testing. Combining sub-micron positioning resolution with a payload capacity of up to 100 kg, the six-axis motion system provided the precision, stability, and load-handling capability required for accurate mirror segment alignment, one of the most critical steps in achieving the telescope's unprecedented optical performance. Image Courtesy: NASA, Chris Gunn. More information on the custom PI Stewart platform for JWST.
Examples of Custom Hexapods for Astronomy

PI has designed a number of Stewart platforms (hexapods) and fast tip/tilt systems for the alignment of mirrors in astronomical telescopes. Talk to a PI engineer for more information.

Tip/Tilt secondary hexapod

Active Secondary Hexapod with Tip/Tilt Mirror — NASA IRTF

Active secondary mirror for NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawaii, with a hexapod 6D alignment system.

  • Mirror diameter: 244 mm
  • Tip/tilt range: ±250 µrad
  • Resonant frequency: 490 Hz

More Information on Stewart platforms and Tip/Tilt Steering Mirror Platforms for Astronomy

UKIRT active tip tilt mirror hexapod

Active Secondary Stewart platform with Tip/Tilt Mirror — UKIRT

Active tip/tilt mirror for the United Kingdom Infrared Telescope (UKIRT) on Mauna Kea, Hawaii, with a secondary hexapod 6D alignment system.

  • Mirror diameter: 314 mm
  • Tip/tilt range: ±500 µrad
  • Resonant frequency: 280 Hz

More Information on 6-Axis Stewart platforms and Fast Steering Mirrors for Astronomy

Custom secondary mirror hexapod

Miniature Stewart platform for WFIRST Telescope

Custom compact hexapod for prism alignment of the slitless spectrometer for the WFIRST Telescope

More Information

Weatherproof Hexapod for Outdoor Telescope Operation
Weatherproof hexapod

Custom Ultra-High-Precision Stewart Platform for Telescopes / Outdoor Operation

Custom secondary 6-axis hexapod for APEX radio telescopy in Chile.

  • Load capacity to 750 N
  • Unidirectional repeatability to 5 µm
  • Clear aperture Ø420 mm
  • Long lifetime: 2 million cycles
  • Drive: brushless motors
  • Protection class IP64
  • Corrosion protection

Video on ALMA (Atacama Large Millimeter Array) radio telescope. PI Stewart platform is shown at 0:38.

More Information on the ALMA Telescope Hexapods

Why Parallel Kinematics Is Useful in Astronomy

Compact 6-Axis Motion

Stewart platforms provide X, Y, Z, pitch, roll, and yaw motion from one compact mechanism instead of a stack of individual linear and rotary stages.

High Stiffness

The payload is supported by six parallel struts, helping provide stiffness and stability for optics, mirrors, sensors, and telescope instrumentation.

Reduced Moving Mass

A common moving platform reduces the cumulative moving mass associated with serial stage stacks, improving dynamic behavior and settling.

RequirementWhy It Matters in AstronomyHexapod Advantage
Mirror AlignmentSecondary mirrors and active optics require precise angular and linear adjustment.Software-controlled six-axis alignment with a virtual pivot point.
Image StabilizationAtmospheric turbulence and vibration can shift images during observation.Fast tip/tilt and multi-axis correction can improve effective imaging performance.
Large PayloadsObservatory components can be heavy and difficult to align manually.Parallel-kinematic designs can position high loads with micron-level precision.
Vacuum / Non-Magnetic NeedsSpace instrumentation and special scientific systems may require low outgassing or non-magnetic operation.Vacuum-compatible and piezomotor-based non-magnetic hexapod designs are available.
Typical Astronomy and Observatory Applications

Active Mirror Positioning

  • Secondary mirror alignment
  • Tip/tilt image stabilization
  • Active optics correction

Radio Telescope Systems

  • Reflector positioning
  • Antenna alignment
  • Sub-micrometer adjustment under harsh conditions

Scientific Instrumentation

  • Spectrograph alignment
  • Sensor positioning
  • Space telescope and satellite receiving antenna systems
Motion Controllers for Stewart Platforms
Hexapod motion controllers
Stewart platform motion controllers provide coordinate transformation, multi-axis trajectory control, and user-defined pivot point control.

All PI Stewart platforms are controlled by a dedicated vector-motion controller specifically developed for six-degree-of-freedom positioning applications. Despite its advanced capabilities, the controller is designed for intuitive operation and seamless integration into laboratory, industrial, and automation environments.

A key feature is the ability to define a virtual pivot point anywhere inside or outside the hexapod workspace through a simple software command. This user-defined center of rotation moves together with the platform, regardless of its position or orientation, providing a powerful advantage in optical alignment, metrology, and precision assembly applications.

Users command motion in familiar Cartesian coordinates, while the controller automatically performs the complex kinematic transformations required to coordinate the individual actuator motions. The latest generation controllers support a wide range of communication interfaces, including TCP/IP for remote, networked, and Industry 4.0 environments, as well as high-speed serial communications for real-time control and system integration.

Stewart Platform Controllers and SoftwareStandard Hexapods

High-Accuracy Hexapod Leadership
Hexapod for telescope secondary reflector alignment
Stewart platforms are ideally suited for the precise alignment of optical systems, telescope mirrors, and radio astronomy antennas. One prominent example is the Atacama Large Millimeter/submillimeter Array (ALMA) in northern Chile, one of the world's largest astronomical observatories. The array consists of more than 60 interconnected radio telescopes that operate together as a single giant antenna, requiring extremely precise alignment of each telescope's secondary reflector.
To meet these demanding requirements, PI developed custom hexapod positioning systems capable of handling payloads of up to 75 kg while providing sub-micrometer positioning resolution and exceptional long-term stability. Designed to operate reliably in the harsh environmental conditions of the high-altitude Atacama Desert, these six-axis alignment systems play a critical role in maintaining the accuracy and performance of the telescope array (Photo: Vertex Antennentechnik GmbH).

PI is a leading manufacturer of high-performance Stewart platform-based positioning systems for precision motion applications ranging from industrial automation and semiconductor manufacturing to aerospace, photonics, and scientific research. Based on parallel-kinematics technology, these six-degree-of-freedom positioning platforms provide exceptional precision, stiffness, and dynamic performance in a compact design.

PI hexapods are used in a wide range of applications, including precision assembly, semiconductor manufacturing, machine tool alignment, medical technology, photonics packaging, telescope mirror positioning, satellite antenna alignment, and aerospace testing. Their ability to simultaneously control motion in all six degrees of freedom makes them ideal for demanding positioning, alignment, and motion simulation tasks.

The parallel-kinematic motion systems are available in a variety of sizes and configurations, with payload capacities ranging from a few kilograms to several hundred kilograms and, in specialized applications, up to one metric ton. Depending on the model, positioning resolution can reach the sub-micrometer and even nanometer range while maintaining high stiffness and dynamic performance.

Most Stewart platforms are based on six high-resolution electromechanical or piezoelectric actuators connected between a fixed base and a common moving platform. While the architecture resembles that of a flight simulator, the precision is orders of magnitude higher. Instead of hydraulic cylinders, PI hexapods employ precision-controlled linear or rotary motor drives optimized for accurate positioning and repeatable motion. Different drive technologies are available to meet specific application requirements. Hexapods based on piezo motor technology, for example, offer vacuum compatibility, self-locking operation, low power consumption at standstill, and completely non-magnetic performance, making them ideal for scientific, semiconductor, cryogenic, and aerospace applications.