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Hera and CubeSats in Maxwell chamber
Space Safety

Deep space CubeSats

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ESA / Space Safety / Hera

While in the vicinity of the Didymos system, Hera will deploy ESA’s first deep-space CubeSats, in order to gather additional data on the Dimorphos asteroid, its parent and their surrounding environment while testing new intersatellite link technology for future mission architectures, based on distributed systems.

Each companion spacecraft will be small enough to fit inside a briefcase, as compared to the desk-sized Hera. CubeSats are nanosatellites based on standardised 10 cm-sized units. Hera will deliver two ‘six-unit’ CubeSat missions to the Didymos asteroid system.

Milani CubeSat mission patch
Milani CubeSat mission patch

The first CubeSat companion is called Milani, and was developed by a Italian/Czech/Finnish consortium.

It will perform detailed spectral measurements of both asteroids’ surfaces – measuring the sunlight they reflect and breaking down their various colours to discover how these asteroids have interacted with the space environment, pinpointing any differences in composition between the two. In addition, Milani will sample the dust surrounding these bodies, to detect volatiles such as water, characterise light organics and to monitor any molecular contamination of the CubeSat.

Juventas CubeSat mission patch
Juventas CubeSat mission patch

The other CubeSat is called Juventas, developed by Danish company GomSpace and GMV in Romania, and perform the first radar sounding of an asteroid's interior.

Juventas will peer up to 100 m deep within the 160-m-diameter Dimorphos body.

In close orbit around Dimorphos, Juventas will line up with Hera to perform satellite-to-satellite radio-science experiments and carry out a low-frequency radar survey of the asteroid interior, similar to performing a detailed ‘X-ray scan’ of Dimorphos to unveil its interior.

Juventas with radar deployed
Juventas with radar deployed

The adventure will end with a landing, using the dynamics of any likely bouncing to capture details of the asteroid’s surface material – followed by several days of surface operations.

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