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    HRE Exploration Science AO - Parabolic Flight (PF)

    ESA is soliciting for experimental proposals for the spaceflight analogue Parabolic Flight
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    Fall 2027 Campaign Announcement:

    The Fall 2027 Parabolic Flight campaign will be performed in microgravity conditions

    1. INTRODUCTION

     

    ESA's Human and Robotic Exploration Directorate and its Exploration Science, a cornerstone of its Explore2040 strategy, invites scientists, researchers, and innovators to join us in pushing the boundaries of human knowledge and technological capabilities. Our programme uniquely balances exploration-focused science, essential for enabling future human missions beyond Earth, with exploration-enabled science that leverages our capabilities for groundbreaking research across disciplines. 

    Guided by core European values of collaboration, scientific excellence, and responsible exploration, we seek proposals that not only advance our understanding of the universe but also contribute to solving global challenges here on Earth. Developing countermeasures for long-duration spaceflight, investigating fundamental physics in microgravity, prospecting for lunar resources, or searching for signs of past life on Mars, the ESA Exploration Science activities offer opportunities to turn your scientific vision into reality and promote open science, international cooperation and the inspiration of future generations.

    This document provides an overview of the research opportunity offered within this Continuously Open Research Announcement for Parabolic Flights. We seek projects that correspond to the rigour and excellence of exploration-enabled science and/or the grand challenges of exploration-focused science. 

    Evaluation planning

    Evaluation sessions are organised typically 8 months prior the campaign. Authors will get the feedback from the idea evaluation sessions typically 4 weeks after evaluation closure. The next evaluation sessions will occur on the following dates:

    • 04 January 2027 for the Fall Campaign 2027 - Microgravity

    Tentative date for the Fall 2027 PFC92 Microgravity Campaign is October 2027.

    (Please note that by default all ideas saved will enter the respective next evaluation round. Authors can edit their ideas until the evaluation round starts, but not once it has already started.)

     

    2. DESCRIPTION OF THIS OPPORTUNITY

     

    Parabolic flights are the only sub-orbital carriers allowing scientists to carry out, in person, biological, biomedical and physiological as well as physical and material science experiments under conditions of microgravity or other (reduced) gravity levels as self-standing experiments.

    This Announcement of Opportunity for the Spaceflight Analogue “Parabolic Flight” in Bordeaux, France, aims to solicit research proposals in Life and Physical Sciences that align with the ESA Explore 2040 Strategy (Annex 2). 

    The ESA Explore2040 strategy implements two streams of science:

    1. Exploration-focused science addresses the needs of ESA in order to meet its exploration objectives. Any research generating knowledge or achieving outcomes required to inform decisions relating to ESA exploration missions, studies, technology developments, operations and strategy fits into this category.
    2. Exploration-enabled science leverages the capabilities of the existing ESA platforms to conduct excellent science. 

    Proposals submitted in the framework of this AO can present research related to Exploration-Focused Science Themes, Exploration-Enabled Science Themes, or both.

     

     A screenshot of a computerDescription automatically generated 

     

    Exploration-focused Science themes (F)

    • Local Resources (F-RES): Characterising surface and near-surface resources including water, chemicals, and materials, including those for functional and structural use. Determining processes for resource extraction.
      • Resources exploration: Abundance, distribution, geological context and extractability of water ice, volatiles, and mineral resources.
      • Resource extraction processes: Chemical and physical processes that can be applied for the extraction and purification of lunar resources.
      • Regolith physical properties: Physical and geotechnical properties of lunar regolith.  
      • Regolith handling and processing: Processes for the extraction, handling, distribution and beneficiation of regolith.
    • Environments & Effects (F-ENV): Determining environmental characteristics and dynamic processes in space, exospheres, atmospheres, and surfaces. Investigating effects on exploration systems and monitoring environmental impacts of human activity.
      • Regolith physical properties: Physical and geotechnical properties of lunar regolith. 
      • The integrated environment: Properties and dynamics of dust, plasma, radiation, electric field and magnetic fields on the Moon and the effects of this environment on technologies, materials and equipment. 
      • Environmental impacts of human activity: The effects of human activity on the pristine lunar environment, landing sites and surface assets.
      • Technologies and operations: How the design and operations of technologies and equipment are affected by the characteristics of the lunar environment. 
      • Biomedical models as a research tool: Use of human-like biomedical models (tissue-on-chip, organoids)
      • Space Materials: Design of new materials tailored to withstand the harsh conditions of space or atmosphere re-entry, including extreme temperatures, radiation, and aggressive chemical environments.
      • Fluid and Thermal Management: Development of technologies to store, pump and dispense fluids, to exchange heat or mass under varying gravity fields. 
      • Fire Safety and Combustion: Research on flame propagation and detection in various gravity and chemical environments.
      • Navigation & Communication: Development of precision instruments (atomic clocks, interferometers, ...) improving navigation precision and communication. 
    • Crew health & performance (F-CREW): Investigating physiological adaptations, addressing behavioural and radiation-related health risks, and developing countermeasures and medical capabilities for long-duration missions.
      • Radiation: Investigate health risks associated to space radiation, and develop, test and implement countermeasures (CMs) to counteract the unwanted effects, including cosmic ray detectors and shielding technologies.
      • Biomedical models as a research tool: Use of human-like biomedical models (tissue-on-chip, organoids).
      • Biomedical countermeasures: Developing tools for acute damage repair and the production of pharmaceutical countermeasures. 
    • Habitation (F-HAB): Investigating innovative approaches for the creation of solutions to sustain life in space, maximise crew comfort, and provide life support. 
      • Nutrition: Understanding the impact of space stressors on food production processes and development of adequate nutritional supply solutions, including countermeasures against space stressors and contamination. 
      • Life support systems: and safe habitable environments including countermeasures against space stressors and contamination. 

    Exploration-enabled science themes (E)

    • Fundamental Physics and Astrophysics (E-FPA): Validity of the Einstein's Equivalence Principle; Origin and nature of dark matter and dark energy; Decoherence and collapse models in quantum mechanics; Quantum many-body physics; Astrophysics and cosmological history of the universe.
    • Materials Science (E-MAT): Solidification physics; Thermophysical properties of metallic (and other) materials; Structural evolution in materials during solidification.
    • Fluids Science, Soft Matter, Biophysics (E-FSB): Mass, momentum and energy transport during liquid and gas motion (including biological systems e.g., protein crystals and biochemicals); Physical chemistry of polymers, gels, colloids and foams; Dusty plasmas; Combustion.
    • Deep Space and Planetary Environments (E-SPACE): Characterising and understanding planetary and deep space and expanding our understanding of their properties and dynamics. Includes heliophysical, radiation and solar observations, magnetometry, atmospheric phenomena, lightning and interaction with climate and the atmosphere chemistry.
    • Biology (E-BIO):
      • Fundamental (E-BIO-FUN): Research into the physiological, genetic, molecular and behavioural responses of biological systems to altered gravity and radiation, aiming to uncover fundamental principles of biology.
      • Space Biotechnology and Agriculture (E-BIO-TECH): Research aiming to utilise the space environment for spin-down applications on Earth (e.g., drug screening, biomedical production, vertical farming).
      • Astrobiology (E-BIO-AST): Research into fundamental questions regarding the origin and limit of life and biosignatures for life detection.
    • Human Physiology (E-PHYSIO): Research using the space environment to better understand fundamental physiological processes that might be relevant for terrestrial medicine (e.g., insight into ageing, osteoporosis, etc.).
    • Planetary Science (E-PLANET): Origin and evolution of terrestrial planets, with a focus on the dynamic aspects affecting climate and habitability; comparative planetology and search for extraterrestrial life. 

    In your proposal, please mention the different elements in this section corresponding to your research themes. They can span both exploration-focused and exploration-enabled science. If you believe your project falls into other areas that are of particular interest to ESA, you can also mention it in your proposal by selecting the "OTHER" category. 

     

    3. DETAILS ABOUT ESA'S PARABOLIC FLIGHT CAMPAIGN

     

    The ESA Parabolic Flight Campaigns take place with the Airbus A310 ZERO-G operated out of the Bordeaux-Mérignac airport by the company Novespace. Novespace’s A310 ZERO-G aircraft has been certified for flying parabolas that can provide reduced gravity levels between 0g and 1g (1g being Earth’s gravity).

    ESA Parabolic flight campaigns are typically conducted twice per year in Spring and Autumn. Each flight campaign normally consists of three individual flights, each of which has 31 parabolas, i.e. a campaign has 93 parabolas in total. During each parabola, there is a period of increased gravity (1.8g), immediately prior to and following a period of reduced gravity.

    Interested science teams are invited to specify in their proposal which g-level campaign (if 0g and/or between 0g and 1g) they are applying for.

     

    Micro-gravity campaigns

    Typically ESA Parabolic Flight campaigns focus on 0g, of which the Airbus A310 ZERO- G can produce about 20 seconds per parabola, giving a total of about 10 minutes of microgravity per flight, and 30 minutes per campaign.

     

    Partial-gravity campaigns

    In contrast to the 0-g campaigns, the campaigns focusing on intermediate gravity levels are less frequent and depend on demand.

    For these campaigns, the durations of the parabolas may vary depending on the g-level and the partial-g levels provided will reflect the prevalent scientific interest from both ESA and the science teams of that campaign (usually Moon and Mars). Selected proposals may therefore be asked about the possibility of adjusting to the chosen levels for a given campaign and thus be in better alignment with ESA's scientific strategy, provided that such modifications do not compromise the scientific objectives of their experiments.

    Detailed description of the ESA Parabolic Flight and campaign organisation can be found in Annex 1.

    Please find additional information here:

    4. APPLICATION PROCESS

     

    You can submit your proposal by clicking on the "Submit Your Idea" button.

    Complete all sections of the submission form according to the guidelines outlined in the call, respective attachments, and the provided proposal template. Additionally, upload any required supplementary information.

    Please note that, in parallel to submission, it is mandatory that all submitting proposers contact their national representatives to inform them about their submission and to investigate possible national funding procedures and timelines, as well as probability of funding in order to identify alternative funding sources if necessary. Points of Contacts for each country are provided in the attachments lower down (Annex 3).

    If you have further technical questions during submission, feel free to contact the Campaign Manager (contact details at the end of the page). 

     

    5. IMPLEMENTATION OF THE SELECTED PROPOSALS

     

    After positive peer and technical review, the scientific coordinator of the experiment will be informed that the proposal has been accepted and added to the pool of activities awaiting the next flight campaign. It will then be the responsibility of the scientific coordinator to communicate this preliminary selection to the rest of the science team.

    Please note that the acceptance of a proposal does not guarantee a flight opportunity, as the selection outcome may still change if feasibility issues arise during experiment preparation for flight. 

    It's important to emphasize that through this Announcement of Opportunity, only the research opportunity aboard the parabolic flight aircraft is provided. The science team is accountable for funding their expenses, including their work, necessary equipment for supporting their activities, travel, etc. Hence, it is necessary for the experimenter to request funding in parallel to their application, enabling them to initiate the process of applying for national funding as early as possible or to explore alternative funding sources if necessary  (refer to "Who can apply?" section, below).

     

    6. DATA MANAGEMENT PLAN

     

    Please see Annex 4.

    Publications and Acknowledgement
    Any publication of the results generated in the context of this research announcement of opportunity shall be provided to ESA and must acknowledge the sponsorship of the study by the European Space Agency.
     
    Support of Education and Outreach
    The activities covered in this research announcement provide an opportunity for the European Space Agency to engage the public and offer opportunities for education and outreach. Science Teams are encouraged to promote and communicate their investigations to a wide audience (general public, colleagues, involvement of students, social media) and to support the European Space Agency in the event of organized press conferences, social media events, educational activities, publications, etc.

     

    CONTRIBUTION TO ESA'S HRE Archiving 

    Calibrated data shall be provided by the Science Team to ESA. Please note that this does not refer to processed analyses/statistics/conclusions (for these, the science team retains full ownership from an Intellectual Property Right standpoint), only to the calibrated observations, imagery, measurements, etc. The aim is to allow for the archival of a complete and meaningful investigation dataset at ESA. The data deliverables from the Science Team to ESA shall be provided in open and readable formats (not requiring special or proprietary tools to read them), unless otherwise is agreed with the HRE Science Data Centre. HRE Data Archive 

     

    Who can apply?

    The scientific institution for which the coordinator of a proposal is working must be located in one of the ESA member or associated member states that contribute to the Exploration Science Programme: Austria, Belgium, Canada, Czech Republic, Denmark, Estonia, Finland, France, Germany, Greece, Hungary, Ireland, Italy, Latvia, Luxemburg, Netherlands, Norway, Poland, Portugal, Romania, Slovenia, Spain, Sweden, Switzerland, United Kingdom.

    Scientists from other ESA Member States that do not contribute to the Exploration Programme and scientists from other European countries having a cooperation agreement with ESA are encouraged to enquire with their national space organisation about the conditions for their participation in proposals to ESA. Furthermore, applicants will need to confirm that they have informed their national agency/delegation before submitting their proposal. The Points of Contacts can be found in the Attachments section of this page.

     

    ESA will make use of independent experts for the relevance and scientific merit evaluation of proposals. The proposal coordinator will receive information on the outcome of the review, typically within 2 months.

    The evaluation criteria that will be applied for evaluation of the proposals are:

    • Scientific Merit

      • Significance (50%): Does the proposed study address an important problem or challenge indicated within AO? Is there a clear, well- grounded and elaborated scientific justification and motivation provided in the proposal? Does the proposed research lead to an advance which is incremental or paradigm shifting? 
      • Approach (35% and pass/fail*): Are the conceptual framework, design, methods, and analyses adequately developed, well integrated, and appropriate to the aims of the project? *Will the experiment yield statistically robust results and if not, is it justified? *Does the applicant acknowledge scientific risks and suggest mitigation? *Has a data management plan been provided? Is the requested platform mandatory for the proposed study, or can other (laboratory) means be used before using this platform? 

      • Knowledge translation (15%): Will the results of the research provide a benefit to Earth or for space exploration? Will the results (or other aspects related to the experiment) have a sustained impact on research in the future?

      • Personnel and Environment (Pass/fail): Are there sufficient and appropriate personnel dedicated to the project?

    Each proposal will receive a scientific merit score between 0 and 100 points. The proposals will receive one of the following marks:

    • Outstanding (100 - 91 points) ​
    • Excellent (90 - 81 points) ​
    • Very Good (80 - 71 points) ​
    • Good (70 – 61 points) ​
    • Fair (60 - 51 points) ​
    • Inadequate (50 - 0 points) ​

    Only proposals receiving a scientific merit score of “Excellent” or higher (score of 81 or higher) will proceed in the evaluation process. Furthermore, a minimum score of "Very Good" or higher (score of 71 or higher) is needed for each sub-criterion. This is to ensure the selection of proposals that are balanced and scoring well across all sub-criteria composing the science merit score.  

    In addition, the following criteria will also be applied:

      • Relevance (Pass/fail): Can the objectives and protocol be effectively achieved within the capabilities and limitations of the platform? Is there a demonstrated necessity for utilizing the chosen research platform? For calls related to the space station, does the proposal justify why the experiment cannot be conducted on the ground? Will the proposed research significantly benefit from the unique conditions offered by the selected platform? Does the proposed research align with  ESA Explore 2040 Strategy and address the specific questions outlined in the call for proposals? 

      • Programmatic Assessment (Pass/fail): To ensure efficient program implementation within a defined timeline, project selection will be balanced with available resources and program capabilities. ESA will choose projects from each Announcement of Opportunity (AO) based on existing research pools and work plan. Furthermore, to foster inclusivity and equal opportunities, ESA encourages the submission of diverse proposals. This includes promoting balanced collaborations among institutions and scientific communities from all ESA Member States, ensuring representation across early-career and senior scientists, as well as gender diversity.

      • Technical Feasibility Assessment (Pass/fail): Each proposal will undergo a preliminary pass/fail technical and operational feasibility assessment, either prior to or in parallel with the peer review process. This assessment aims to determine the proposal's compatibility with the capabilities of the chosen research platform, evaluate the technical, operational, and development complexity of the required hardware and activities, and identify the resources necessary for successful project implementation.

    Following approval of the proposal, the proposers will be informed of the outcome of the review. This will include the report of the scientific and technical review with overall scoring.

    The results of the selection will be final and not open to appeal. A positive selection may still require adjustments to enhance scientific return and optimize feasibility.

     

    Do you need help?

    Channel Manager - Zuzanna Pasko, National Graduate Trainee

    Thank you for your interest in our AO. My name is Zuzanna, I am the channel manager of this OSIP call. You can ask questions in the discussion section below your idea. We will do our best to respond to your questions as quick as possible.

    Background Information

    Innovation Area

    Human and Robotic Exploration

    ESA’s Terrae Novae exploration programme is leading Europe’s human journey into the Solar System using robots as precursors and scouts. Exploring space is about travelling farther and coming back with new experiences and knowledge to help us on Earth. Humankind will benefit from the new discoveries, ambitions, science, inspiration and challenges. 

    What's your idea?

    We appreciate all input. Even rough ideas can fuel a discussion and help to ideate. Help us to improve by submitting your own ideas to this channel.