Cosmic Penguin

7. Mars energetic particles analyser Limit of Detection: Energy range: 0.1 ~ 12 MeV (Electrons) / 2 ~100 MeV (Protons) / 25 ~ 300 MeV (Alpha Particles/Heavy Ions) delta-E/E: 15% Flux: 0 ~ 10^5 cm^-2 s^-1 Atomic Number: 1 <= Z <= 26 (H - Fe)

delta-m/m: <=25% (Z <= 9, 25 ~ 300 MeV & 10 <= Z <= 26, 100 ~ 300 MeV); <=60% (10 <= Z <= 26, 25 ~ 100 MeV) POV: 60° Time resolution: 4s (Electrons, Protons, Alpha Particles); 60s (Heavy Ions)

And here comes the 6 instruments on the yet-to-be-named @PRCMarsRover which will get a name via a planned public naming contest:

A. Terrain Camera Imaging wavelength: Visible Light Color: Standard RGB Nominal imaging distance: 0.5 m ~ ∞ Pixel Resolution: 2048 x 2048

B. Multi-spectral camera Imaging bands (/nm, Full Width At Half Maximum in brackets): 480 (20), 525 (20), 650 (12), 700 (15), 800 (25), 900 (30), 950 (50), 1000 (50) Color: Multi-spectral Nominal imaging distance: 1.5 m ~ ∞ Pixel Resolution: 2048 x 2048

C. Rover sub-surface radar Channel 1: Median frequency: 55 MHz Working bandwidth: 40 MHz Penetrating depth of Martian ice layers: ~1 m Maximum detection depth: >=10 m for Martian sub-surface soil (εr = 3.0~4.0); >=100 m for Martian polar ice layers (εr = 3.0)

Channel 2: Median frequency: 1300 MHz Working bandwidth: 1000 MHz Precision of layer thickness detection: ~cm Maximum detection depth: >=3 m for Martian sub-surface soil (εr = 3.0~4.0); >=10 m for Martian polar ice layers (εr = 3.0)

D. Mars surface composition analyser LIBS measurements: Detects 10+ elements; optimal working distance from sample 2~5 m (max. 10 m); imaging resolution <= 100 μrad (0.2 mm @ 2 m; 0.5 mm @ 5 m) NIR measurments (850~2400 nm): spectral resolution <=12 nm; 130+ bands; POV >=1 mrad