日本地球惑星科学連合2015年大会

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インターナショナルセッション(口頭発表)

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS01] Outer Solar System Exploration Today, and Tomorrow

2015年5月26日(火) 16:15 〜 18:00 A03 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*木村 淳(東京工業大学地球生命研究所)、藤本 正樹(宇宙航空研究開発機構・宇宙科学研究本部)、笠羽 康正(東北大学大学院 理学研究科 地球物理学専攻)、佐々木 晶(大阪大学大学院理学研究科宇宙地球科学専攻)、谷川 享行(産業医科大学医学部)、関根 康人(東京大学大学院新領域創成科学研究科複雑理工学専攻)、佐柳 邦男(ハンプトン大学)、Steven Vance(Jet Propulsion Laboratory, Caltech)、座長:佐々木 晶(大阪大学大学院理学研究科宇宙地球科学専攻)、並木 則行(国立天文台 RISE月惑星探査検討室)

17:15 〜 17:30

[PPS01-14] ENERGETIC NEUTRAL ATOM (ENA) IMAGING OF THE EUROPA GAS CLOUD FROM JUICE

*Pontus BRANDT1Donald MITCHELL1Joseph WESTLAKE1Barry MAUK1Todd SMITH1 (1.The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA)

キーワード:Europa, Jupiter, Torus, Magnetosphere

The Jupiter Energetic Neutrals and Ions (JENI) Camera is one out of six sensors of the Particle Environment Package (PEP) suite that was selected for flight on the ESA Jupiter Icy Moon Explorer (JUICE). JENI is a combined imaging energetic ion spectrometer and an ENA camera that operates in the 〜0.5 keV to 1 MeV range for ions and 〜0.5 ? 500 keV for ENAs and is capable of separating H, O, and S. Its angular resolution is ≤2⁰ for ≥10 keV H.

In ENA mode JENI's main objective is to constrain the Europa surface (or subsurface) mechanisms that release material to space by imaging the neutral gas surrounding Europa using ENAs produced when energetic ions of the Jovian magnetosphere charge exchange with the extended neutral gas atoms or molecules.

ENA observations of Jupiter by the Ion and Neutral Camera (INCA) the Cassini spacecraft have revealed ENA emissions surrounding Jupiter at about the orbital distance of Europa. The observations are consistent with a column density peaking around Europa's orbit in the range from 2×1012 cm-2 to 7×1012 cm-2, assuming H2, and are consistent with the upper limits reported from the Cassini/UVIS observations. Detailed analysis shows indications that the neutral gas cloud may be centered on Europa and not symmetric around Jupiter. This would directly imply that the source of the gas is Europa itself. The INCA observations also show indications of magnetospheric dynamics that result in about a factor of two variation in ENA intensity.

We describe the INCA observations and its implications for JUICE, Juno and Europa Clipper, and discuss the neutral-plasma coupling pertinent to the Europa/Io plasma/neutral environment.