What can an interstellar probe mission at large heliocentric distances achieve with remote imaging and in situ dust measurements ?

Carey M. Lisse (1) , M.B. Zemcov (2) , A.R. Poppe (3) , J.R. Szalay (4) , B.T. Draine (4) , M. Horányi (5) , R.L. Mcnutt (1) , A. Corcoros (1) , P.C. Brandt (1) , M.V. Paul (1) , V. Sterken (6) , Anny Chantal Levasseur-Regourd (7) , Rosine Lallement (8) , C.A. Beichman (9)

1 APL - Johns Hopkins University Applied Physics Laboratory [Laurel, MD]
2 RIT - Rochester Institute of Technology
3 SSL - Space Sciences Laboratory [Berkeley]
4 Princeton University
5 LASP - Laboratory for Atmospheric and Space Physics [Boulder]
6 UNIBE - Universität Bern / University of Bern
7 PLANETO - LATMOS
8 GEPI - Galaxies, Etoiles, Physique, Instrumentation
9 NExScI - NASA ExoPlanet Science Institute

Domaines: Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]

Carey M. Lisse, M.B. Zemcov, A.R. Poppe, J.R. Szalay, B.T. Draine, et al.. What can an interstellar probe mission at large heliocentric distances achieve with remote imaging and in situ dust measurements ?. 52nd Lunar and Planetary Science Conference 2021, Mar 2021, Virtual Meeting, United States. ⟨insu-03133701⟩