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Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe

P. C. BrandtThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAElena ProvornikovaThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAS. D. BaleUniversity of California Berkeley, Berkeley, CA USAAlice CocorosThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAR. DemajistreThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAK. DialynasOffice of Space Research and Technology, Academy of Athens, Athens, 10679 GreeceH. A. ElliottSouthwest Research Institute, San Antonio, TX USAS. ErikssonLaboratory for Atmospheric and Space Physics, University of Colorado at Boulder, Boulder, CO USABrian D. FieldsUniversity of Illinois Urbana-Champaign, Urbana, IL USAAndré GalliUniversity of Bern, Bern, SwitzerlandM. E. HillThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAM. HorányiLaboratory for Atmospheric and Space Physics, University of Colorado at Boulder, Boulder, CO USAT. S. HorburyImperial College London, London, UKS. HunzikerETH, Zurich, SwitzerlandP. KollmannThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAJ.D. KinnisonThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAGlen H. FountainThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAS. M. KrimigisOffice of Space Research and Technology, Academy of Athens, Athens, 10679 GreeceW. S. KŭrthUniversity of Iowa, Iowa City, IA USAJeffrey L. LinskyUniversity of Colorado Boulder, Boulder, CO USAC. M. LisseThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAKathleen MandtThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAW. MagnesSpace Research Institute, Austrian Academy of Sciences, Graz, AustriaR. L. McNuttThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAJesse MillerBoston University, Boston, MA USAE. MoebiusUniversity of New Hampshire, Durham, NH USAParisa MostafaviThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAM. OpherBoston University, Boston, MA USAL. J. PaxtonThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAFerdinand PlaschkeTechnical University Braunschweig, Braunschweig, GermanyA. R. PoppeUniversity of California Berkeley, Berkeley, CA USAE. C. RoelofThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAKirby RunyonPlanetary Science Institute, Tucson, AZ USASeth RedfieldWeslayan University, Middeltown, CT USAN. A. SchwadronUniversity of New Hampshire, Durham, NH USAVeerle SterkenETH, Zurich, SwitzerlandP. SwaczynaPrinceton University, Princeton, NJ USAJ. R. SzalayPrinceton University, Princeton, NJ USAD. L. TurnerThe Johns Hopkins University Applied Physics Laboratory, Laurel, MD USAHunter VannierWeslayan University, Middeltown, CT USAR. F. Wimmer‐SchweingruberUniversity of Kiel, Kiel, GermanyP. WurzUniversity of Bern, Bern, SwitzerlandE. J. ZirnsteinPrinceton University, Princeton, NJ USA

2023en

ABI

Annotatsiya

A detailed overview of the knowledge gaps in our understanding of the heliospheric interaction with the largely unexplored Very Local Interstellar Medium (VLISM) are provided along with predictions of with the scientific discoveries that await. The new measurements required to make progress in this expanding frontier of space physics are discussed and include in-situ plasma and pick-up ion measurements throughout the heliosheath, direct sampling of the VLISM properties such as elemental and isotopic composition, densities, flows, and temperatures of neutral gas, dust and plasma, and remote energetic neutral atom (ENA) and Lyman-alpha (LYA) imaging from vantage points that can uniquely discern the heliospheric shape and bring new information on the interaction with interstellar hydrogen. The implementation of a pragmatic Interstellar Probe mission with a nominal design life to reach 375 Astronomical Units (au) with likely operation out to 550 au are reported as a result of a 4-year NASA funded mission study.

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DOI: 10.1007/s11214-022-00943-x

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