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2. High Resolution Camera Image resolution: < 2.5 m (< 0.5 m in certain regions) multi-color; < 10 m (< 2.0 m in certain regions) panchromatic Image swath: >= 9 km at 265 km altitude
3. Mars orbiter sub-surface radar Radar frequency: 10-20 & 30-50 MHz Transmitter power: >= 100 W Receiver power: <= -87 dBm Maximum detection depth: ~100 m for Martian sub-surface soil (εr = 3.0~4.0); ~1000 m for Martian polar ice layers (εr = 3.0) Depth resolution: ~ 1 m
4. Mars mineralogy spectrometer Wavelength bands: Visible Light - NIR band 0.45~1.05 μm; NIR-MIR band 1.00~3.40 μm Spectral resolution: < 10 nm for Visible Light - NIR band; < 12 nm for 1.0~2.0 μm; < 25 nm for 2.0~3.4 μm
5. Mars magnetometer Measurement range: +- 2000 nT Noise level <= 0.01 nT/√Hz Resolution: <= 0.01 nT Precision: 0.1 nT
6. Mars ions and neutral particles analyser Limit of Detection of low energy ions: Energy range: 5 eV ~ 25 keV delta-E/E: 15% Mass: 1~ 70 amu delta-m/m: 25% POV: 90° x 360° Angular resolution: 11.2° x 22.5° Time resolution: 8s
Limit of Detection of low energy neutral particles: Energy range: 50 eV ~ 3 keV delta-E/E: 100% Mass: 1 ~ 32 amu POV: 15° x 160° Angular resolution: 10° x 25° Time resolution: 4s
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
E. Mars surface magnetometer Measurement range: +- 2000 nT Noise level <= 0.01 nT/√Hz Resolution: <= 0.01 nT Stability: <= 0.01 nT/°C Sampling rate: 1/16/32/128 Hz Range: +- 65000 nT
F. Mars meteorology instrument Temperature -120~50 °C (precision 0.1 °C); Pressure 1~1500 Pa (precision 0.1 Pa); Windspeed 0~70 m/s (precision 0.1 m/s); Wind Direction 0°~360° (precision 5°); Sound detection 20 Hz~2.5 kHz/2.5~20 kHz (Sensibility >50 mV/Pa; Dynamic Range >=90 dB)
Hopefully this will be useful for interpreting what abilities the orbiter and rover will have and also assists in public data analysis when they come later. 
@elakdawalla @AJ_FI @doug_ellison @NASASpaceflight @plutogno @planet4589 @girlandkat
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