NASA’s IMAP spacecraft has completed a mission-critical design review that moves it closer to its planned 2025 launch
NASA’s Interstellar Mapping and Acceleration Probe (IMAP) spacecraft has completed the Mission Critical Design Review and is on track to meet its scheduled 2025 launch.
Southwest Research Institute (SwRI) leads the payload management of the mission to study the boundary of the solar system. The organisation is also providing the scientific instrument Compact Dual Ion Composition Experiment (CoDICE) and is participating on other instrument teams for the mission, which will study the interaction between the solar wind and the interstellar medium as well as the fundamental processes of particle acceleration in space.
Susan Pope, director of SwRI’s Department of Space Instrumentation and IMAP’s payload manager, said: “IMAP will help us gain a greater understanding of how our sun interacts with the rest of the solar system.
“IMAP will give us a more complete picture of the interaction between the interstellar medium and the solar wind, providing a better understanding of our place in the universe.”
IMAP is designed to help researchers better understand the boundary of the heliosphere, the magnetic bubble created by the solar wind, and the constant flow of particles from the sun.
The bubble surrounds and protects our solar system, limiting the amount of harmful cosmic radiation entering the heliosphere. IMAP instruments will collect and analyse particles that make it through the barrier.
Additionally, the mission will examine the fundamental processes that accelerate particles throughout the heliosphere and beyond. The resulting energetic particles and cosmic rays can harm astronauts and space-based technologies.
The institute is providing the CoDICE instrument, which combines the capabilities of multiple instruments into one patented sensor.
Initially developed through SwRI internal funding, CoDICE will measure the distribution and composition of interstellar pickup ions, particles that make it through the ‘heliospheric’ filter.
It will also characterise solar wind ions as well as the mass and composition of highly energised solar particles associated with flares and coronal mass ejections.
SwRI is a key member of the teams for the IMAP-Hi and IMAP-Lo instruments, responsible for the detector on the IMAP-Hi and the conversion subsystem on the IMAP-Lo.
SwRI is also building high-voltage power supplies for the Solar Wind Electron (SWE) instrument, which measures the distribution of thermal electrons in the solar wind, and the Global Solar Wind Structure (GLOWS) instrument, a non-imaging photometer that will observe the structure of the solar wind.
Additionally, SwRI is providing digital electronics for four IMAP instruments.
Pope said: “Most of the instruments have completed their engineering model testing and have started fabricating their flight hardware.
Princeton University professor David J McComas leads the mission with an international team of 24 partner institutions. The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland builds the spacecraft and operates the mission.
IMAP is the fifth mission in NASA’s Solar Terrestrial Probes (STP) Program portfolio. The Explorers and Heliophysics Project Division at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the STP Program for the agency’s Heliophysics Division of NASA’s Science Mission Directorate.
Image: NASA’s Interstellar Mapping and Acceleration Probe (IMAP) spacecraft has completed a critical design review and is on track for its scheduled 2025 launch. Southwest Research Institute is managing the payload office, providing a scientific instrument as well as contributing other technology for the mission. © NASA/ Johns Hopkins APL/ Princeton University. Public domain.