Direct Samples of Interstellar and Interplanetary Material with IMAP

The Interstellar Mapping and Acceleration (IMAP) mission probes the interaction between our heliosphere and the interstellar medium (ISM) in unprecedented detail. The broad science that IMAP addresses has been organized into three distinct science themes: A) Acceleration and the broader context of the solar wind and space weather; B) Exploring the outer heliosphere through energetic neutral atoms, and C) Sampling of the interstellar and interplanetary material. This paper summarizes the scientific goals of the latter theme and identifies the key scientific opportunities for IMAP available due to its unique ability to directly sample the interstellar and interplanetary material from 1 au. It is organized into three broad scientific questions that directly relate to IMAP's science objectives: 1) What is the state of the pristine upstream LISM and how does it relate to its origins and evolution? 2) How does the VLISM interact with the heliosphere? 3) How does interstellar material, as well as interplanetary dust, affect the near-Sun environment?

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Publication Details

Journal
Space Science Reviews
Published
2026-04-01
DOI
https://doi.org/10.1007/s11214-026-01291-w
Citations
2
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
28.42

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article

Direct Samples of Interstellar and Interplanetary Material with IMAP

F. Rahmanifard, Elena Provornikova, Z. Sternovsky, Ethan Ayari et al.
2 citations
Space Science Reviews
Solar and Space Plasma Dynamics
28.42
article

Direct Samples of Interstellar and Interplanetary Material with IMAP

F. Rahmanifard, Elena Provornikova, Z. Sternovsky, Ethan Ayari, M. Bzowski, P. Swaczyna, E. Möbius, J. S. Rankin, H. O. Funsten, M. Gkioulidou, E. R. Christian, N. A. Schwadron, A. Galli, E. J. Zirnstein, G. P. Zank, D. Turner, S. Livi, J. R. Szalay, K. Ogasawara, D. B. Reisenfeld, D. J. McComas, M. Horányi
article en
2 citations

Abstract

The Interstellar Mapping and Acceleration (IMAP) mission probes the interaction between our heliosphere and the interstellar medium (ISM) in unprecedented detail. The broad science that IMAP addresses has been organized into three distinct science themes: A) Acceleration and the broader context of the solar wind and space weather; B) Exploring the outer heliosphere through energetic neutral atoms, and C) Sampling of the interstellar and interplanetary material. This paper summarizes the scientific goals of the latter theme and identifies the key scientific opportunities for IMAP available due to its unique ability to directly sample the interstellar and interplanetary material from 1 au. It is organized into three broad scientific questions that directly relate to IMAP's science objectives: 1) What is the state of the pristine upstream LISM and how does it relate to its origins and evolution? 2) How does the VLISM interact with the heliosphere? 3) How does interstellar material, as well as interplanetary dust, affect the near-Sun environment?

Space Science ReviewsVol. 222(3)
University of Bern (CH), Centrum Badań Kosmicznych (PL), Southwest Research Institute (US), Goddard Space Flight Center (US), Los Alamos National Laboratory (US), University of New Hampshire (US), University of Colorado Boulder (US), Princeton University (US), Johns Hopkins University Applied Physics Laboratory (US), Heliophysics (US), University of Alabama in Huntsville (US), International Space Science Institute (CH)
National Aeronautics and Space Administration, Narodowym Centrum Nauki, Narodowa Agencja Wymiany Akademickiej
Openalex Percentile: Top 1%
Solar and Space Plasma Dynamics
28.42
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