The Asteroid Spectral Imager (ASPECT) on the Milani CubeSat

Antti Näsilä*, Tomáš Kohout, Maddalena Boselli, Janne Kuhno, Roberts Trops, Christer Holmlund, Rami Mannila, Harri Ojanen, Tahvo Havia, Hans Toivanen, Altti Akujärvi, Leevi Salonen, Timo Ihatsu, Antti Penttilä, Tomáš Kašpárek, Tuomas Tikka, Gábor Kovács, Balázs V. Nagy, David Korda, Margherita CardiMarco Pavoni, Daniele Calvi, Andrea Zanotti, Filippo Corradino, Hannah Goldberg, Michael Kueppers, Mario F. Palos

*Corresponding author for this work

Research output: Contribution to journalArticleScientificpeer-review

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Abstract

Flying on board the Milani CubeSat, The Asteroid Spectral Imager ASPECT is a hyperspectral camera which will measure the spectral characteristics of the Didymos asteroids. This paper describes science objectives of the mission, the operational principle of the camera and primary results of the test campaign. The ASPECT camera operates mainly in the near infrared wavelengths, covering the wavelength range of 650–1600 nm. In addition to the camera, there is a single point spectrometer covering the range of 1650–2500 nm. The instrument was qualified to the Hera environmental specification and the optical properties were cross-calibrated with other optical payloads on the Hera mission.

Original languageEnglish
Article number86
JournalSpace Science Reviews
Volume221
Issue number7
DOIs
Publication statusPublished - Oct 2025
MoE publication typeA1 Journal article-refereed

Funding

The ASPECT instrument was built under ESA contract 0111232456/51/NL/GLC-S-VTT (supported by other smaller ESA contracts), Academy of Finland project No. 335595, and within institutional support RVO 67985831 of the Institute of Geology of the Czech Academy of Sciences, the Czech-German common grant, funded by the Czech Science Foundation under the project 23 07633K and by the Deutsche Forschungsgemeinschaft under the project BE 5771/3-1 (eBer-23 13412).

Keywords

  • Asteroid
  • Hera
  • Hyperspectral
  • Milani

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