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      Modelling DESTINY+ interplanetary and interstellar dust measurements en route to the active asteroid (3200) Phaethon

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          Abstract

          The JAXA/ISAS spacecraft DESTINY\(^+\) will be launched to the active asteroid (3200) Phaethon in 2022. Among the proposed core payload is the DESTINY+ Dust Analyzer (DDA) which is an upgrade of the Cosmic Dust Analyzer flown on the Cassini spacecraft to Saturn (Srama et al. 2011). We use two up-to-date computer models, the ESA Interplanetary Meteoroid Engineering Model (IMEM, Dikarev et al. 2005), and the interstellar dust module of the Interplanetary Meteoroid environment for EXploration model (IMEX; Sterken2013 et al., Strub et al. 2019) to study the detection conditions and fluences of interplanetary and interstellar dust with DDA. Our results show that a statistically significant number of interplanetary and interstellar dust particles will be detectable with DDA during the 4-years interplanetary cruise of DESTINY+. The particle impact direction and speed can be used to descriminate between interstellar and interplanetary particles and likely also to distinguish between cometary and asteroidal particles.

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          Most cited references29

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          Discovery of Jovian dust streams and interstellar grains by the Ulysses spacecraft

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            The Interstellar Medium Surrounding the Sun

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              ACTIVITY IN GEMINID PARENT (3200) PHAETHON

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                Author and article information

                Journal
                15 April 2019
                Article
                1904.07384
                0041e8f7-f755-4e24-b6f6-b0ec23fd65bc

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                40 pages, 18 Figures, accepted for Planetary and Space Science
                astro-ph.EP

                Planetary astrophysics
                Planetary astrophysics

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