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Millimetric thermal emission from the two faces of Iapetus

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Abstract

We observed the two faces of Iapetus at 1.2and2.0mm using the New IRAM (Institut de RadioAstronomie Millimétrique) Kids Array (NIKA2)mounted on the IRAM-30 m telescope. On Iapetus’ trailing side, we confirm thepredictionof Ries (2012). On the leading side, however, we find that thebrightnesstemperatureis much lower at 1.2 and 2.0 mm than observed at 3 mm by Ries (2012).
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Dates and versions

insu-02264965 , version 1 (08-08-2019)

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  • HAL Id : insu-02264965 , version 1

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Léa Bonnefoy, Jean-Francois Lestrade, Alice Le Gall, Emmanuel Lellouch, Cédric Leyrat, et al.. Millimetric thermal emission from the two faces of Iapetus. EPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-574-1. ⟨insu-02264965⟩
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