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    ESA > Our Activities > Operations

    Space Surveillance and Tracking - SST

    ESA's SSA programme: watching for hazards from space
    A purpose-built radar system will scan low Earth orbit for dangerous debris objects

    The central aim of SST is to provide an independent ability to acquire prompt and precise information regarding objects orbiting the Earth. Using this data, a wide range of services will be provided – such as warning of potential collisions between these objects or alerting when and where debris re-enters the Earth's atmosphere. This data will be stored in a catalogue and made available to SSA customers across Europe.

    During the 2009-12 Preparatory Phase, there are two main roles for the SST: To define the future full SST system and to launch precursor services that serve as a test-bed and demonstrator for future development.

    About SST

    The infrastructure required to provide these capabilities is referred to as the 'SST segment'. It comprises surveillance and tracking sensors – which could be radar or optical – to acquire the raw data, which is then processed to correlate (or link) each object with ones already seen, or to indicate a new object if this has not been seen before.

    Between 2009 and 2012, the SST Segment will obtain data by using currently existing sensors. When the full SSA programme is initiated, dedicated systems, with capabilities matching the needs of the service, will be developed and deployed.

    The SSA-SST Space Surveillance Test and Validation Centre (SSTC) is located at ESA/ESAC, Spain.

    ROLE Detect, catalogue and predict the movement of objects orbiting the Earth
    PRECURSOR
    SERVICE START
    2012
    SERVICE CENTRE Space Surveillance Test and Validation Centre (SSTC), ESA/ESAC, Spain
    SENSORS
    • Now: Mix of radars, telescopes & other assets
    • Future: Dedicated radar & optical systems
    ++ Prediction of potential collisions between orbiting satellites and debris; reentry analysis; detect on-orbit explosions;
    assist missions at launch, deployment and end-of-life; help reduce cost of space access ++

    SST Segment

    Three main elements are required to ensure that the SST Segment can meet critical customer requirements and provide reliable operational services.

    Zimmerwald SMall Aperture Robotic Telescope (ZimSMART)

    A data catalogue

    The core of the SST Segment is the catalogue; this contains information on everything that has been detected in orbit. In order to produce this catalogue, it is necessary to: reconstruct an orbit from the data that is produced by the sensors (orbit determination); check to see if this object has already been seen and is already in the catalogue (correlation); and monitor the data in the catalogue so that sensors can be tasked to update the information when needed.

    A network of sensors to accurately detect objects orbiting the Earth

    These sensors are usually either optical or radar systems. They are divided into two groups: surveillance or tracking.

    1. Surveillance sensors perform the routine task of ensuring that data in the tracking catalogue is accurate and up-to-date. They typically 'stare' across an area of the sky and register objects passing through their field of view. They can observe multiple objects simultaneously and continually add to the quality of the data in the catalogue.
    2. Tracking sensors are used when very high-precision data are needed about a specific object. This happens, for example, if it is predicted that this object will collide with an operational satellite. The highest quality of data is then needed to improve these predictions and assist the satellite operators to plan any necessary avoidance manoeuvres - or confirm that no manoeuvre is necessary. Some sensors can perform just one of these tasks, while others are able to have dual roles within the full system.

    A system of governance and data management

    This will ensure that the right people receive correct information in a timely fashion. Good data management also means that warnings are given as quickly as possible.

    SST team

    We have a very motivated team and invaluable support from colleagues across the Agency and across Europe.

    The SST team is based at ESA's Space Surveillance Test and Validation Centre (SSTC) and comprises experts dedicated to the creation of the initial precursor services as well as the definition of the full SST system.

    In addition, the SST team is supported by specialists and industrial support personnel working at ESA establishments and industry across Europe.

    The team is managed by Emmet Fletcher, from the UK, an engineer experienced in the space surveillance field. "The creation of an independent space surveillance and tracking capability is crucial to helping secure Europe's spaceborne assets. Even though it is a challenging project, we have a very motivated team and invaluable support from colleagues across the Agency and across Europe," says Fletcher.

    Precursor services overview

    Even before the full SST Segment is built, ESA's Space Surveillance Test and Validation Centre will deliver a valuable range of 'precursor' surveillance services to satellite operators/customers, utilising data from a number of existing European and international sources.

    TIRA will work as part of ESA's SSA Programme
    TIRA radardome at FGAN, Wachtberg, Germany

    From 2009, these precursor services will comprise:

    • The creation of a prototype catalogue of orbiting objects
    • Critical collision avoidance services for satellite operators
    • Tracking campaigns, both routine and on-demand in case of an identified collision risk
    • The prediction and warning of uncontrolled re-entry events

    Contributions from ESA Member States

    The SST precursor services will take advantage of the numerous resources that exist across Europe. For data acquisition, data from radar and optical systems will be tasked to obtain both routine and ad-hoc data of both satellites and debris. These sensors are provided by national space agencies, European defence ministries, academia and private entities.

    Control room at ESA's Optical Ground Station, Tenerife

    On the engineering and scientific side, the SST precursor services will make use of contributions from European centres of expertise to ensure that the current store of knowledge is drawn upon where possible.

    Since Space Surveillance is a global concern, the SSTC also works closely with our international partners. ESA has a long history of technical cooperation with agencies outside of Europe, The availability of international channels – such as the data provided by the US Air Force – greatly adds to the SSTC capabilities.

    SSA also includes an upgrade to ESA's Space Debris Telescope at the Optical Ground Station, Tenerife, Spain. This upgrade will enhance the acquisition of data on objects in the geostationary ring and at Medium Earth Orbit (MEO) altitudes.

    Facilities and infrastructure

    Space Surveillance Test and Validation Centre (SSTC), ESA/ESAC

    Starting in 2009, the SSTC became the focal point for all developments regarding the initial set of SST services to be offered in the precursor programme. The centre's activities include the prototyping of analytical software and operational tools and ensuring the development of data management procedure.

    Technology

    The development of SST services entails the development of specific technologies to ensure that performance meets the operational requirements.

    Type

    Details

    Radar systems

    In order to detect fast-moving objects in Low Earth Orbit (LEO), advanced radar systems that can perform both surveillance and tracking are being developed. For this, research and development is being carried out on phased array radar systems, power control, low-noise amplifiers, beam forming and detection algorithms.

    Optical systems

    For higher orbits, the use of optical sensors is most efficient. The development of accurate telescopes, pointing systems, digital detectors and image processing technologies are helping to reduce the cost and increase the performance of the overall system.

    Cataloguing

    The heart of the SSTC is the catalogue. In order to ensure the highest quality for the data, techniques to rapidly process the many thousands of data entries and calculate when each of these should be refreshed are being developed. This is not a trivial task, as it requires the continual processing of the orbital data to define when the next observation should take place.

    Orbit determination

    When a sensor detects an object, it produces a series of data points as the object moves across the sky. Converting these sample points into an accurate description of an orbit is called 'orbit determination'. The SST Segment requires rapid, precise determination under a wide range of viewing conditions.

    Correlation

    When an object has been detected, we need to know if this is something we have already seen, or something new. The process of correlation compares the orbit of a detected object against the whole catalogue to see if there is a match. As the rate of object detection can be very high, it is important to find algorithms that are both efficient and precise in order to process a large amount of data as quick as possible.

    Last update: 9 December 2012

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    • More information
      • Why monitor objects in orbit?
        • Europe flies unprotected
          • Orbital debris mean danger on the ground
          • Space Surveillance and Tracking - background paper May 2010 (PDF)

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