The International Institute of Space Law (IISL) was founded in 1960.

The purposes and objectives of the Institute include the cooperation with appropriate international organisations and national institutions in the field of space law and the carrying out of tasks for fostering space law development.

Space law is an area of the law that encompasses national and international law governing activities in outer space.

The NASA Orbital Debris Program Office, located at the Johnson Space Center, is the lead NASA center for orbital debris research.

It is conducting measurements of the environment and in developing the technical consensus for adopting mitigation measures to protect users of the orbital environment. Work at the Center continues with developing an improved understanding of the orbital debris environment and measures that can be taken to control debris growth.

The ESA Space Debris Office coordinates ESA's research activities in all major debris disciplines, including measurements, modelling, protection, and mitigation, and coordinates such activities with national research efforts with space agencies in Italy (ASI), the United Kingdom (BNSC), France (CNES) and Germany (DLR). Together with ESA, these national agencies form the European Network of Competences on Space Debris (SD NoC).

ESA's Space Debris Office has also been a forerunner in the definition of a European Space Surveillance System.

ESA's Space Debris Office provides operational services in support of planned and ongoing missions within ESA and to third parties.

ESA's Space Debris Office provides operational services in support of planned and ongoing missions within ESA and to third parties.

MASTER (Meteoroid and Space Debris Terrestrial Environment Reference) is a software that can be used to analyze space debris flux and spatial densities. T

he following sources of debris are considered: launch and mission-related objects, explosion and collision fragments, solid rocket motor slag and dust, NaK droplets, surface degradation products, ejecta, and meteoroids. MASTER can deliver flux and spatial density analysis for all epochs between 1957 and 2060. For all epochs, the lower size threshold is one micron. The analysis of the future debris environment is possible based on three different future scenarios (business as usual, intermediate mitigation, full mitigation). The MASTER-2009 software is delivered on a DVD, together with extensive documentation of the underlying models. The software is available for Windows, Linux, Solaris, and MacOS X.

MASTER is developed and maintained by the ESA Space Debris Office.

PROOF (Program for Radar and Observation Forecasting) is a software for the simulation of radar- and telescope-based space debris observations.

It is delivered together with the MASTER software. It can be applied for the validation of space debris models like MASTER against observation data. Another use is the planning of debris observation campaigns, including the derivation of neccessary sensor parameters.

PROOF-2009 has been applied in the course of the MASTER-2009 validation process to properly interpret debris observations performed by the ESA Space Debris Telescope, the Liquid Mirror Telescope, the Tracking and Imaging Radar, the Goldstone, and the Haystack Radar. With the new version of PROOF, a simulation of multistatic radar observations, and of phased array radars is now possible.

The software is available for Windows, Linux, Solaris, and MacOS X.

PROOF is developed and maintained by the ESA Space Debris Office.

PROOF (Program for Radar and Observation Forecasting) is a software for the simulation of radar- and telescope-based space debris observations.

It is delivered together with the MASTER software. It can be applied for the validation of space debris models like MASTER against observation data. Another use is the planning of debris observation campaigns, including the derivation of neccessary sensor parameters.

PROOF-2009 has been applied in the course of the MASTER-2009 validation process to properly interpret debris observations performed by the ESA Space Debris Telescope, the Liquid Mirror Telescope, the Tracking and Imaging Radar, the Goldstone, and the Haystack Radar. With the new version of PROOF, a simulation of multistatic radar observations, and of phased array radars is now possible.

The software is available for Windows, Linux, Solaris, and MacOS X.

PROOF is developed and maintained by the ESA Space Debris Office.

MASTER (Meteoroid and Space Debris Terrestrial Environment Reference) is a software that can be used to analyze space debris flux and spatial densities. T

he following sources of debris are considered: launch and mission-related objects, explosion and collision fragments, solid rocket motor slag and dust, NaK droplets, surface degradation products, ejecta, and meteoroids. MASTER can deliver flux and spatial density analysis for all epochs between 1957 and 2060. For all epochs, the lower size threshold is one micron. The analysis of the future debris environment is possible based on three different future scenarios (business as usual, intermediate mitigation, full mitigation). The MASTER-2009 software is delivered on a DVD, together with extensive documentation of the underlying models. The software is available for Windows, Linux, Solaris, and MacOS X.

MASTER is developed and maintained by the ESA Space Debris Office.

The Spaceflight Meteorology Group (SMG) is a U.S. weather forecasting unit staffed by the National Weather Service (NWS) for the National Aeronautics and Space Administration (NASA) which provides pertinent information on the current and expected state of the atmosphere during human spaceflight operations. It is located at the Johnson Space Center in Houston, Texas.

Meteorological information for the broader space program is provided by the 45th Space Wing's 45th Weather Squadron of the U.S. Air Force.

The Space Weather Prediction Center (SWPC), formerly the Space Environment Center (SEC), is a laboratory and service center of the National Oceanic and Atmospheric Administration (NOAA) located in Boulder, Colorado. SWPC continually monitors and forecasts Earth's space environment, providing solar-terrestrial information. SWPC is the official source of space weather alerts and warnings for the United States.

The Space Weather Prediction Center is one of the nine National Centers for Environmental Prediction (NCEP) and provides real-time monitoring and forecasting of solar and geophysical events, conducts research in solar-terrestrial physics, and develops techniques for forecasting solar and geophysical disturbances.

The SWPC Forecast Center is jointly operated by NOAA and the U.S. Air Force and is the national and world warning center for disturbances that can affect people and equipment working in the space environment. SWPC works with many national and international partners who contribute with data and observations.

The Institut Supérieur de l'Aéronautique et de l'Espace or ISAE is the name for the French aerospace engineering school.

It is located in Toulouse, France. The "Institut Supérieur de l’Aéronautique et de l’Espace" (ISAE) was created in 2007 from the merger of two prestigious French Engineer School: SUPAERO (founded in 1909) and ENSICA (founded in 1945).

The Institute provides high-level Graduate Programs in engineering for Space and Aerospace domains, Master’s degrees, Postgraduate Specialized Masters, PhD degrees. This opens to the  students a wide range of career opportunities: engineering, research and development, logistics, consulting, finance, etc.

ISAE also develops a very active research policy.