DART/DRACO camera | Angular resolution is 2.48 µrad;aperture is 208 mm; field of view is 0.29°; magnitude detection is 14.5 | New Horizons, Lucy/LORRI | Changed CCD to CMOS; global/rolling shutter dual-mode operation; integrated SMART Nav autonomous navigation algorithm; optimized adaptability to low-temperature conditions [(-85±5) ℃] | Autonomous guidance achieved cm-level impact point positioning for 160 m-class asteroids (1σ error ±68 cm); obtained the size and quantity distribution of boulders on asteroids |
Hera/AFC camera | Spectral band is 370‒1100 nm;angular resolution is 94.1 µrad; field of view is 5.5°×5.5° | Astrohead cameras | Improved close-range imaging resolution (10 cm/pixel); balanced dual-mode functions of navigation and imaging | Supports 3D shape reconstruction and accurate volume calculation of binary systems; determines density and internal structure by combining mass data |
Hera/TIRI thermal infrared imager | 7‒14 μm mid-infrared spectral band; resolution is 5 m@20 km;field of view is 13°×10°;temperature measurement range is 150‒400 K; accuracy is 3 K | Hayabusa 2/ TIR | Resolution increased by 4 times; expanded spectral band width; sensor changed to Lynred Pico 1024 Gen 2 | Retrieves thermal inertia through surface temperature distribution, infers thermophysical properties such as roughness and porosity, and helps understand the Yarkovsky/YORP effect[10] |
Hera/HyperScout H imaging spectrometer | Spectral band is 665‒975 nm; angular resolution is 133 µrad; field of view is 16°×8°; number of spectral bands is 25 | HyperScout-2 | Simplified the infrared spectral band; reduced the number of spectral bands from 45 to 25; lightweight design | Detects post-impact surface mineral changes, impact crater space weathering effects, and ejecta deposition to support impact effect evaluation |
Hera/ASPECT hyperspectral imager | Four-channel independent measurement (visible light, two near-infrared, one short-wave infrared); achieves 20‒40 nm spectral resolution using a tunable Fabry-Perot interferometer (FPI) | CubeSat Aalto-1/ AASI | Expanded the spectral band;optimized the resolution | Explores the surface mineral composition of asteroids, characterizes asteroid volatiles and dust particles, and assists in determining their composition |
LICIACube/LEIA, LUKE | Wide-field and narrow-field cameras respectively; panchromatic, color; resolution is 1.5‒5 m/pixel; field of views are 2.06° and 10° | CubeSat general payload | — | Acquire images of the unimpacted side of the asteroid and videos of the dynamic evolution of ejecta respectively |