IMAP Mission

NASA’s Interstellar Mapping and Acceleration Probe (IMAP) mission held a critical design review (CDR) last week with a NASA Standing Review Board (SRB). This mission-level review was the culmination of individual CDRs conducted for all the instruments and subsystems. While there are still challenges ahead to face as a team, the review board is confident that IMAP has a plan to succeed.

Although CDR is often a gate to spacecraft construction, IMAP has already begun building important components such as instrument engineering and flight models as well as parts of the structure. With 10 instruments designed and built globally, the complicated dance of testing, cross-calibrating, and integrating these pieces is carefully choreographed so that the completed observatory will be ready for launch in 2025.

IMAP will explore our solar neighborhood, known as the heliosphere, and decode the messages in particles from the Sun and beyond. Three of the instrument suites will work together to build detailed maps of the boundaries of the solar system using energetic neutral atoms, which travel from the edge to Lagrange point 1 (L1), the point between the Sun and Earth where gravitational forces balance. IMAP’s other instruments collect information from the Sun’s solar wind and provide timely updates about space weather conditions.

The SRB chair noted that IMAP was “good to go” and had a lot of work to do.

Princeton University professor and IMAP Principal Investigator David J. McComas expressed his gratitude to the board for the good questions and said, “New challenges will surely emerge between now and launch, but I have every confidence in the awesome, committed, and resilient team that we have assembled to carry out this challenging mission.”

“We’re finally starting to see the integration of all these efforts, which is absolutely remarkable for me,” said Deputy Principal Investigator Nathan Schwadron. “We started with an idea. We proposed the concept, and then there’s this shift of momentum into actually making the hardware, building the spacecraft, getting them to work together. It really is our commitment to discovery as a team that helps make the transition from concept to reality.”

McComas leads the mission with an international team of 24 partner institutions. The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, is building the spacecraft and will operate 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.

To learn more about the IMAP mission visit the website: https://imap.princeton.edu

By Lindsay Bartolone
IMAP Communications Lead for Princeton University

NASA and the UK Space Agency have agreed to cooperate on NASA’s heliophysics mission, the Interstellar Mapping and Acceleration Probe (IMAP). The agreement, signed Sept. 22, 2021, will allow Imperial College London (ICL) to design and build one of IMAP’s 10 instruments – a magnetometer called MAG – as well as provide ground support and personnel necessary to support the instrument and the IMAP science team.

Scheduled to launch in 2025, IMAP will observe and map the Sun’s heliosphere – the volume of space filled with particles streaming out from the Sun, known as the solar wind – and study how it interacts with the local galactic neighborhood beyond. The boundary zone at the edge of the heliosphere offers protection from the harsher radiation of interstellar space; it may have played a role in creating a habitable solar system and is critical in NASA’s plans for safe human exploration of the Moon and Mars.

MAG will contribute to our understanding of the acceleration and transportation of charged particles in the heliosphere. It will do this by measuring the interplanetary magnetic field around the spacecraft. From these measurements, MAG will identify interplanetary shocks and measure the waves and turbulences that scatter particles.

MAG will also provide measurements for the IMAP Active Link for Real-Time (I-ALiRT) space weather monitoring service. With I-ALiRT, IMAP will enable new ways of forecasting space weather by streaming real-time observations of conditions headed towards Earth to operators on the ground.

MAG is a dual sensor fluxgate magnetometer and includes electronics, a power supply system, and an on-board computer. The two sensors are located on a boom to reduce the effects of magnetic interference from the spacecraft.

“The UK and the United States are working together on some of the most exciting space missions of our time, from the Mars Perseverance rover to the James Webb Space Telescope,” said Dr Paul Bate, Chief Executive of the UK Space Agency. “There is still so much we don’t know about the Sun and the behaviour of phenomena like the solar wind. This new partnership will help NASA answer some of these questions, using the expertise of scientists at Imperial College London. It is an excellent example of the importance of international collaboration in the study and exploration of our solar system.”

“IMAP will be doing some really exciting science that neatly fits with expertise we have at Imperial, both for understanding how particles get accelerated to the highest energies, and how our Sun interacts with our neighbourhood in the galaxy,” said Science Lead for MAG, Professor Tim Horbury from the Department of Physics at Imperial College London.

“The rest of the IMAP team and I are so pleased to have this partnership with the UK Space Agency and Imperial College London” said Professor David McComas, the IMAP principal investigator. “International collaboration such as this makes our mission even stronger.”

David McComas of Princeton University leads the IMAP mission and an international team of 24 partner institutions. The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, will build the IMAP spacecraft and operate the mission for NASA. IMAP is the fifth mission in NASA’s Solar Terrestrial Probes (STP) Program portfolio and newest addition to NASA’s fleet of heliophysics spacecraft. The Heliophysics Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the STP Program for the Heliophysics Division of NASA’s Science Mission Directorate.

NASA’s Interstellar Mapping and Acceleration Probe – IMAP – has completed a key milestone in mission development. After rigorous review, IMAP has passed what is known as Key Decision Point C, or KDP-C, which marks the mission’s progression from formulation to implementation.

As a modern-day celestial cartographer, IMAP will chart the very boundaries of the heliosphere – the bubble surrounding the Sun and planets that is inflated by the solar wind – and study how it interacts with the local galactic neighborhood beyond.

These measurements will help scientists better understand fundamental physics of the heliosphere and our place in the stellar neighborhood at scales both tiny and immense. It will also help scientists understand how the interaction of solar and stellar winds forms a barrier that shields the inner solar system from harmful cosmic rays, which will help protect astronauts.

IMAP will launch into orbit of Earth-Sun Lagrange point 1 – a location towards the Sun about a million miles from Earth ­– no earlier than 2025.

David McComas of Princeton University leads the IMAP mission and an international team of 24 partner institutions. The Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, will build the IMAP spacecraft and operate the mission for NASA. IMAP is the fifth mission in NASA’s Solar Terrestrial Probes (STP) Program portfolio and newest addition to NASA’s fleet of heliophysics spacecraft. The Heliophysics Program Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the STP Program for the Heliophysics Division of NASA’s Science Mission Directorate.

To accommodate schedule changes due to precautions regarding COVID-19, the preliminary design review for NASA’s Interstellar Mapping and Acceleration Probe, or IMAP, has been moved from February to May 2021. Similarly, the launch readiness date is delayed from Oct. 1, 2024, to Feb. 1, 2025.

Over the course of its mission, IMAP will explore and map the boundaries of our heliosphere – the volume of space filled with the wind from the Sun – and study how it interacts with the local galactic neighborhood beyond. These boundaries, which offer protection from the harsher radiation of interstellar space, may have played a role in creating a habitable solar system, and are critical in enabling safe human exploration of the Moon and Mars.

Designed with 10 scientific instruments to measure a large range of particles and fields, IMAP will investigate how particles are accelerated and determine the composition of particles and dust in our local neighborhood. IMAP also will enable and mature new ways of forecasting space weather, including geomagnetic storms and solar energetic particles, through streaming real-time observations to the ground.

IMAP will launch on a  Falcon 9 Full Thrust rocket provided by Space Exploration Technologies (SpaceX) of Hawthorne, California. This launch will include several other Rideshare missions: NASA’s Global Lyman-alpha Imagers of the Dynamic Exosphere, NASA’s Solar Cruiser, NASA’s Lunar Trailblazer, and NOAA’s Space Weather Follow-On L1.

Princeton University professor, David J. McComas leads the mission and 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 Heliophysics Program Office 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.

NASA has selected Space Exploration Technologies (SpaceX) of Hawthorne, California, to provide launch services for the agency’s Interstellar Mapping and Acceleration Probe (IMAP) mission, which includes four secondary payloads. IMAP will help researchers better understand the boundary of the heliosphere, a magnetic barrier surrounding our solar system. This region is where the constant flow of particles from our Sun, called the solar wind, collides with winds from other stars. This collision limits the amount of harmful cosmic radiation entering the heliosphere. IMAP will collect and map neutral particles that make it through, as well as investigate the fundamental processes of how particles are accelerated in space, from its vantage point orbiting the Sun at the Lagrange 1 point directly between the Sun and Earth. . .  [more]

NASA has selected a science mission planned for launch in 2024 that will sample, analyze, and map particles streaming to Earth from the edges of interstellar space.

The Interstellar Mapping and Acceleration Probe (IMAP) mission will help researchers better understand the boundary of the heliosphere, a sort of magnetic bubble surrounding and protecting our solar system. This region is where the constant flow of particles from our Sun, called the solar wind, collides with material from the rest of the galaxy. This collision limits the amount of harmful cosmic radiation entering the heliosphere. IMAP will collect and analyze particles that make it through. . . .[more]