Mio is an octagonal spin-stabilized satellite designed to measure in-situ plasma and electromagnetic fields from the orbit of Mercury.
Schematic view of the Mio spacecraft identifying the science instruments. The location of each instrument and sensor is indicated from top view [Murakami et al., 2020].
[Murakami et al., 2020].
Shape | Octagonal shape within a 1.8 m diameter circle with two 5 m extendable mast and four 15 m (from tip to root) electric field antenna |
Height |
1.52 m (launch configuration)
2.66 m (observational configuration) |
Mass | 255 kg (including 3.7 kg N2 gas) excluding 20 kg separation mechanism which remains on MMO sunshield interface (MOSIF) |
Power (spin averaged) |
≧271 W (periapsis at aphelion)
≧368 W (average at aphelion) ≧530 W (average at perihelion) |
Designed mission life | One Earth year observation at the Mercury orbit and an extension of one Earth year (or more) |
Thruster | 6 × 0.4 N N2 cold gas jet |
spin rate | 15 rpm (4 s/spin) |