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Set of cameras to characterise the landing site environment. IR Fourier spectrometer to study the martian atmosphere. RLS will support the scientific measurements of other instruments such as the MicrOmega, and is capable of measuring a sample at a fast-pace in order to release it for further analysis by other ExoMars instruments. Some of them are used by ESA missions: The WebGeocalc tool (WGC) provides a web-based graphical user interface to many of the observation geometry computations available from the SPICE system.

pck: Kernels that define planetary constants. For information about the mission operations, go to the ExoMarsRSP ESA Robotic Exploration web. WISDOM is a UHF ground penetrating radar, covering the frequency range from 500 MHz to 3 GHz, designed to map the subterranean layers of Mars. If you want to receive updates and notifications for SPICE for ExoMarsRSP you might join the SPICE_EMRSP mailing list, You can also join the #SPICE channel in the OpenPlanetary Group in Slack. This will provide valuable information on the site's stratigraphy, the distribution and state of water-related minerals, and will help to characterise the geophysical Martian environment. In order to obtain the latest operational kernels we recommend you to download the kernels listed in the metakernel. For information about the scientific data, go to the ExoMarsRSP PSA web. You can access using this, root directory (named after the mission: ExoMarsRSP). ExoMars 2020 RSP 3 Carrier S/C: OHB. MicrOmega is a visible and infrared imaging spectrometer that will identify, at grain scale, the mineralogical and the molecular composition of the Martian samples collected by the ExoMars drill. ESA uses cookies to track visits to our website only, no personal information is collected. In addition to the detailed sampling, the Rover will carry a suite of instruments designed to establish the geological and depositional context of each site visited. WISDOM will be used in combination with Adron to provide information on subsurface water content and decide where to collect subsurface samples for analysis. image the walls of the borehole to study Martian mineralogy and rock formation. This is the web home for SPICE data for ExoMars RSP (also known as ExoMars2020). release notes: Includes the Release Notes of the SKD. The Rover is expected to travel several kilometres during its mission.
EXOMARS RSP SPICE KERNELS SET. Once on ground, the ExoMars Rover will establish the physical and chemical properties of Martian samples, mainly from the subsurface where biomarkers are more likely to be present. is a mast-mounted infrared spectrometer, designed to determine the major mineral composition of distant rocks, outcrops, and soils. ExoMars (Exobiology on Mars) is an astrobiology programme by the European Space Agency (ESA) and the Russian space agency Roscosmos.. ESA uses cookies to track visits to our website only, no personal information is collected. ik: Kernels for the instruments on board the Rover and the Surface Platform. fk: Kernels that define reference frames needed for the Mission.

Operational SPICE Kernel Dataset Information.

spk: Orbit kernels, for the Rover, Surface Platform and Carrier Module and other solar system bodies. These images will help determine the sample's depositional environment. Dust particle size, impact, and atmospheric charging instrument suite, IR Fourier spectrometer to study the martian atmosphere, Habitability, brine irradiation and temperature package, Multi-channel Diode-Laser Spectrometer for atmospheric investigations, Spectrometer for atmospheric investigations, Gas chromatography-mass spectrometry for atmospheric analysis, Radio thermometer for measurement of soil temperatures (down to 1-m depth), Set of cameras to characterise the landing site environment.
Notifications from the ESA SPICE Service can also be obtained via twitter. It will also provide textural information on rocks (for example, laminations or pitting) that can be related to the presence of organisms on Mars. In combination with PanCam, ISEM will contribute to the selection of suitable samples for further analysis by the other instruments. CLUPI is a camera system that will  acquire high-resolution colour close-up images of rocks, outcrops, drill fines and drill core samples. You can access using this link.

For information about the scientific data, go to the, (WGC) provides a web-based graphical user interface to many of the observation geometry computations available from the SPICE system. sclk: Spacecraft clock coefficients kernels. cosmo: The SPICE-enchanced configuration for the ExoMarsRSP mission. The ExoMars RSP SPICE kernel dataset (SKD) contains the operational observation geometry and other ancillary data in the form of SPICE System kernel files for the ExoMars Rover, Surface Platform and Carrier Module spacecraft and its instruments and targets. The ExoMars programme comprises two missions: the first – the Trace Gas Orbiter – launched in 2016 while the second, comprising a rover and surface platform, is planned for 2022. This is the web home for SPICE data for ExoMars RSP (also known as ExoMars2020).

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