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\t\t\t\t\t\t14\/03\/2024<\/span> The shoebox-sized Milani CubeSat, which will perform close-up mineral prospecting of the Dimorphos asteroid, is ready for delivery to ESA\u2019s Hera asteroid mission for planetary defence. The spacecraft will carry Milani and a second CubeSat, the Juventas radar imaging spacecraft for probing into the target asteroid, which together will be ESA\u2019s first CubeSats to operate in deep space.<\/p>\n<\/div>\n Funded through the Italian Space Agency, ASI, the Milani CubeSat was shown to the press at the premises of its prime contractor Tyvak International\u00a0in Turin. It will now be flown to ESA\u2019s ESTEC Test Centre in the Netherlands, where Hera is currently undergoing pre-flight testing, for integration with its mothership and subsequent validation of the inter-satellite link system that will connect Hera, Milani and Juventas as they fly around the Didymos system.<\/p>\n \u201cThis is a paramount achievement for Tyvak International,\u201d explains Margherita Cardi, VP Programmes for Tyvak International and Milani Programme Manager. \u201cMilani is now ready to be delivered to ESA and undergo the system tests with Hera, to ensure the validation of the interfaces and the end-to-end communication prior to the launch. The journey is not over, but we are a step closer to Didymos, and it was a real honour to host here at Tyvak all the persons who contributed to this amazing project and celebrate together this achievement.\u201d\u00a0<\/p>\n<\/p><\/div>\n Origin of Hera mission<\/b><\/p>\n Also present at Milani\u2019s delivery event was Alice Milani, daughter of the man the CubeSat was named for. Andrea Milani, professor of mathematics at the University of Pisa, was a planetary defence pioneer\u00a0who first devised what became ESA\u2019s Near Earth Object Coordination Centre, based at the Agency\u2019s ESRIN centre in Frascati, Italy. Then in 2004 he proposed the idea of a double spacecraft planetary defence mission called Don Quijote. One spacecraft \u2013 called Hidalgo\u00a0\u2013 would impact a non-threatening asteroid while another spacecraft \u2013 called Sancho\u00a0\u2013 would gather data to validate asteroid impact models.<\/p>\n His proposal evolved into the NASA\u2019s DART mission (formerly Hidalgo) \u2013 which in 2022 diverted the orbit of Dimorphos around Didymos \u2013 and the follow-up Hera mission (formerly Sancho) to gather close-up data on the mass and makeup of the asteroid and DART\u2019s impact site. Sadly, Andrea never lived to see the implementation of his idea, passing away unexpectedly in 2018.<\/p>\n<\/p><\/div>\n Milani to stay linked with its mothership<\/b><\/p>\n Milani will survey Dimorphos as well as the larger Didymos object that the asteroid orbits around in a wider range of colours than the human eye can see, to identify the mineral makeup of the asteroids and even individual boulders resting on them. It will also survey the dust environment surrounding these bodies. And the inter-satellite link system between the Hera mothership and its smaller companions will track small tugs in their relative positions due to the gravitational pulls of the asteroids, helping to assess their mass.<\/p>\n<\/p><\/div>\n But the miniature Milani is also a full-fledged spacecraft in its own right, incorporating a visible light camera, laser altimeter and star trackers for navigation, plus a cold gas propulsion system. While Hera will orbit about 20 \u2013 10 km from the asteroids, Milani will risk lower altitudes, starting at 10 km and coming as close as 2 km. Going into a traditional orbit around the Didymos system is impractical because of its extremely low gravity. Instead Milani will fly a series of \u2018hyberbolic arcs\u2019 in its vicinity, like repeated flybys involving its thrusters regularly changing direction to remain as close as required.<\/p>\n Finally, Milani will attempt a landing on Dimorphos. Its onboard gyros and accelerometers will gather valuable data on the landing and any subsequent low-gravity bounces, to give insight into the surface properties of the asteroid.<\/p>\n<\/p><\/div>\n First ESA CubeSats in deep space<\/b><\/p>\n CubeSats are small, low-cost satellites built up from 10 cm boxes, traditionally employed for educational purposes but increasingly finding operational uses in Earth orbit. Milani and Juventas will be the first ESA CubeSats to remain several months in deep space, operating in close proximity to a small Solar System body.<\/p>\n They will spend Hera\u2019s two-year cruise phase to Didymos inside a pair of \u2018Deep Space Deployers\u2019 which will keep them alive and healthy. The pair will be deployed one at a time, starting with a partial deployment to check each CubeSat\u2019s functionality. Finally, they will be deployed at just a few centimetres per second \u2013 any faster and they would risk being lost in space within the prevailing low gravity.<\/p>\n<\/p><\/div>\n Milani instruments<\/b><\/p>\n Milani is a \u20186-unitXL\u2019 CubeSat measuring just 13 x 24.6 x 36.6 cm in size. On one side of Milani are the four sensors of its main ASPECT, Asteroid Spectral Imager, instrument developed by the\u00a0VTT Technical Research Centre of Finland, which will image the asteroids in visible, near and shortwave infrared bands.<\/p>\n \u201cASPECT is a hyperspectral imager whose heritage goes back to a series of instruments flown on drones, variously used for agricultural, forestry and pollution monitoring,\u201d explains Antti N\u00e4sil\u00e4, Principal Scientist and ASPECT project manager at VTT.\u00a0<\/p>\n<\/p><\/div>\n \u201cSo the miniaturisation involved meant that switching to CubeSats was a straightforward transition, and a predecessor version of the instrument flew on Finland\u2019s first CubeSat,\u00a0Aalto-1\u00a0in 2017. But despite ASPECT\u2019s small size it is extremely complex, with each of the four channels requiring roughly 50 control signals each, criss-crossing through the instrument.\u201d<\/p>\n MILANI\u2019s second instrument is VISTA, Volatile In-Situ Thermogravimetre Analyser, an Italian-built dust detector. This is based on quartz microcrystals whose piezoelectric responses are altered slightly by the adhesion of tiny dust particles.<\/p>\n<\/p><\/div>\n Ernesto Palomba of Italy\u2019s\u00a0Istituto di Astrofisica e Planetologia Spaziali, VISTA\u2019s principal investigator, explains: “On Earth this same precision technology is used in analytical laboratories and checking thin film deposition processes. VISTA will use it to identify water and other volatile species around the asteroids, as well as the presence of dust. We hope our instrument will be able to keep operating even on the surface of Dimorphos.\u201d<\/p>\n Hera\u2019s ESA system engineer Franco Perez Lissi Comments: \u201dESA\u2019s first deep-space CubeSat was developed in record time by an incredible team. ESA is extremely impressed by the skills, motivation and commitment of Tyvak International. We are eager to see the spacecraft in action, helping us to unveil the many mysteries of the Didymos asteroid system.\u201d<\/p>\n<\/p><\/div>\n
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