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    9 months left
    Evaluation
    Starts Dec 31
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    Celeste In-Orbit Demonstrator – Call for LEO-PNT experimentation opportunities

    Do you want to be among the first to test the future of satellite-based positioning? Join the experiments of the ESA’s Celeste In-Orbit Demonstration! Between 2026 and 2027, we will launch more than 11 LEO satellites to trial new navigation concepts, and we invite organisations from ESA Participating States to collaborate in shaping the future of satellite navigation in Europe.

    Whether you’re a receiver manufacturer, application developer, public-safety organisation, or research center, this is your chance to evaluate LEO-PNT positioning concepts and technologies under real-world conditions.

    🔍 Why join?
    - Early access to Celeste IOD satellite signals
    - Opportunity to validate LEO-PNT user technology and concepts
    - Collaborate with ESA and innovators across the New Space ecosystem
    - Contribute to shaping the future of satellite navigation in Europe
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    SCOPE
    ESA is offering interested third parties from ESA Participating States to participate in the experimentation phase of the Celeste In-Orbit Demonstrator (IOD). This is a unique opportunity to test and validate innovative positioning, navigation, and timing (PNT) concepts in real-world conditions using ESA's LEO-PNT demonstrator infrastructure.

    We are looking for organisations—industry, research, and academia—who are eager to explore, evaluate, and shape the future of space-based PNT services. Whether you are developing cutting-edge user equipment, testing new use cases, or contributing to service demonstrations, your involvement can help drive the evolution of resilient high-performance PNT solutions.

    The ESA Participant States to Celeste (ESA's FutureNAV Programme - Component 1 LEO-PNT) are: Austria, Belgium, Czech Republic, Finland, France, Germany, Hungary, Italy, Luxembourg, Netherlands, Norway, Poland, Portugal, Romania, Spain, Sweden, Switzerland, United Kingdom.

    INTRODUCTION

    Global Navigation Satellite Systems (GNSS) have enabled a wide range of PNT capabilities, supporting society and the global economy. More than five billion Galileo receivers exist and the number of GNSS receiver shipments is expected to grow significantly. Growth is mainly driven by two areas: consumer solutions – such as smartphones, fitness devices, and tablets – as well as road and automotive technologies, including in-vehicle systems and on-board units.

    However, jamming and spoofing increasingly disrupt services; the current MEO-based GNSS backbone may not meet future performance and resilience needs. This prompts a “multi-layer system of systems” approach combining MEO and LEO satellites, terrestrial systems, and integrated sensors. 

    LEO-PNT can enhance MEO GNSS through spectral and geometrical diversity, enabling new navigation techniques. The European Radionavigation Plan (2023) identifies LEO-PNT as a key emerging technology, envisioning an EU “System of PNT Systems” for resilience.

    Most GNSS systems use L-band signals for performance and size efficiency, but congestion is driving exploration of alternative bands. LEO constellations can use higher frequencies for performance and resilience in advanced applications, and lower frequencies for better indoor and denied-environment coverage, vital for consumer and public safety.

    Adopting open standards, like 5G Non-Terrestrial Networks (5G NTN), presents an opportunity to promote interoperability standards for PNT. It could also accelerate user adoption and enable Fused PNT integrated with SatCom constellations.

    Globally, LEO-PNT is a major trend with multiple commercial and institutional initiatives underway. This makes it one of the most closely followed topics in satellite navigation.

    The Celeste LEO-PNT IOD Component of the ESA FutureNAV Programme, approved at the ESA Council Meeting at Ministerial level CM22, aims to demonstrate the potential of PNT in low Earth orbit. Its first mission will feature a small constellation of demonstrator satellites to showcase the potential of LEO satellites for enhancing resilience, accuracy, and agility in navigation, to enable a long list of new applications and services. Development of two parallel demonstrators began in March 2024, with the first pair of satellites planned for launch by early 2026; these are called Pathfinder A (Pf-A). The full demonstration is expected by 2027 with the launch of eight Pathfinder B satellites (Pf-B).

    More details about Celeste LEO-PNT In-Orbit demonstration (IOD) can be found in ESA's website and Enhancing GNSS with a Low Earth Orbit layer: Celeste In-Orbit Demonstration Mission 

    OBJECTIVES OF THE IOD THIRD PARTY EXPERIMENTATION PHASE

    The primary objective of the experimentation phase is to demonstrate PNT services provided by the LEO satellites, as a standalone system and in conjunction with Galileo and MEO systems. Secondly, this phase aims to enable technologies through a broad range of field-testing carried under realistic operational conditions and involving user segment communities.

    Minimum Use Case Coverage

    • High-Accuracy Positioning

      • Fast convergence using Precise Point Positioning (PPP) algorithms.

    • PNT Resilience

      • Frequency diversity in L, S, and C-band.
      • Robustness against jamming and interference.
    • 5G/6G NTN Compatibility

      • Signals aligned with 3GPP 5G satellite standards for integration in S-band Mobile Satellite Spectrum (MSS).
    • Low-Energy PNT for User Terminals

      • Optimized signal design to reduce power consumption in mobile and IoT devices.
    • GNSS LEO Science enabler

      • Study of new LEO signals to conduct science experiments (.i.e. Ground GNSS-R, Propagation campaigns)

    • Additional PNT Data Provision

      • Enhanced data services for improved positioning and timing accuracy.
    • Indoor Navigation

      • Broadcast in UHF band to improve signal penetration and availability.

    Targeted End-User Verticals

    The experimentation aims to involve representative users from the following sectors:

    • Autonomous Vehicles (road, UAV)
    • Railway and Maritime
    • Aviation
    • Critical Infrastructure
    • Polar and Arctic Users
    • Wireless Networks (5G/6G)
    • Personal Emergency Services
    • Asset Tracking and IoT

    PLANNED APPROACH FOR EXPERIMENT PARTICIPATION

    ESA opens the experimentation to third parties from ESA Participating States via this OSIP call, after completion of the expression of interest. Through the OSIP platform, ESA will share the signal-in-space characteristics, the timeline for experimentation, and technical information (e.g. identification of Pf-A and Pf-B satellites, allocation of satellite number, type of signals activated in each experiment, frequencies activated in each experiment) in due course prior to the experimentation. More details on the concept of operations for the experiments will be provided in the future via this OSIP page to the registered parties fulfilling the conditions of registration.

    The technical material will be provided after signature of the terms and conditions attached to this page. Signing the terms and conditions does not automatically grant access to the Celeste technical material.

    ESA reserves the right to cancel all or part of the experimentation with third parties participating to this OSIP call and/or modify the approach proposed to conduct the experimentation at any time.

    DUTIES OF THE THIRD PARTY PARTICIPANTS

    The parties that intend to express their interest need to provide, in answer to this OSIP call, a document describing how they intend to participate in the experimentation, which tools they plan to use, and the expected results. The answer shall include the entities involved and the respective ESA Participating States. ESA is particularly interested in knowing which of the use cases and end users might be covered. The document in answer to this call shall be no more than 5 to 7 pages.

    The third-party participants to the experimentation agree to share with ESA the results of the experiments and be available to participate in potential workshops, organised by ESA, to share their results and discuss with the community.

    DISCLAIMER

    All information requested and provided in the frame of this OSIP call will be used for information purposes only. This OSIP call does not bind ESA to any present or future procurement actions, nor does it create any rights for respondents in relation to any present or future ESA procurements, output of evaluation, and/or related contract awards. The Agency reserves the right to issue amendments to the OSIP call.

    PERSONAL DATA PROTECTION

    ESA will use any personal data included in the responses to this OSIP call (e.g. names and contact details) exclusively for contacting the respondents in case it becomes necessary in relation to their submission. ESA will not disclose personal data to third parties without prior agreement of the respondent that had submitted their response, as per “ESA Personal Data Protection Framework”.[1]

    [1] Details of this framework can be found via the link given on ESA STAR Publication (https://esastar-publication-ext.sso.esa.int/ under “Supporting Documentation” à “Reference Documentation” à “Administrative Documents”).

     

    The Campaign/Channel is open for submissions for participants registered in one of ESA Member States, Associate Member States or Cooperating States  (link).

    For general conditions of participation to this campaign, please refer to the above document.

    Please note, that restrictions exist for certain implementation paths, e.g. ESA procurement actions are restricted to entities eligible for doing business with ESA (see also here).

     

    Do you need help?

    Campaign Manager - Florin-Catalin Grec, LEO-PNT Mission & Experimentation Eng.

    Florin Grec is LEO-PNT Mission and Experimentation responsible and will act as interface between external entities and ESA Celeste team.

    Background Information

    Innovation Area

    Positioning, Navigation & Timing

    Since the beginning of time, human beings have looked to the sky to determine their whereabouts. Traditionally, the Sun and the pattern of fixed stars have been their guides. But in the second millennium, constellations of man-made satellites have taken over as beacons to guide the way.

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