論文

査読有り 本文へのリンクあり
2019年4月16日

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

Planetary and Space Science
  • Harald Krüger
  • Peter Strub
  • Ralf Srama
  • Masanori Kobayashi
  • Tomoko Arai
  • Hiroshi Kimura
  • Takayuki Hirai
  • Georg Moragas-Klostermeyer
  • Nicolas Altobelli
  • Veerle J. Sterken
  • Jessica Agarwal
  • Maximilian Sommer
  • Eberhard Grün
  • 全て表示

172
開始ページ
22
終了ページ
42
記述言語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/j.pss.2019.04.005
出版者・発行元
Elsevier BV

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.

リンク情報
DOI
https://doi.org/10.1016/j.pss.2019.04.005
arXiv
http://arxiv.org/abs/arXiv:1904.07384
URL
http://arxiv.org/abs/1904.07384v1
URL
http://arxiv.org/pdf/1904.07384v1 本文へのリンクあり
ID情報
  • DOI : 10.1016/j.pss.2019.04.005
  • ISSN : 0032-0633
  • arXiv ID : arXiv:1904.07384

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