Operator | European Space Agency |
---|---|
Manufacturer | TASiCH |
Instrument type | Visible light camera |
Function | Close-up HD imaging ≥ 7 months [1] |
Began operations | Planned: 2030 |
Website | ExoMars Rover Instrument Suite |
Properties | |
Mass | 932 g |
Dimensions | 170 × 80 × 100 mm |
Power consumption | 15 W |
Host spacecraft | |
Spacecraft | Rosalind Frankling rover |
Operator | ESA |
Launch date | NET 2028 |
CLUPI (Close-Up Imager) is a miniaturized camera system on board the planned European Space Agency Rosalind Franklin rover. CLUPI has been designed to acquire high-resolution close-up images in colour of soils, outcrops, rocks, drill fines and drill core samples, [2] as well as and the search for potential biosignature structures and patterns. [3] This camera assembly is part of the science payload on board the European Space Agency 's Rosalind Franklin rover, [4] tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched not earlier than 2028 and land on Mars in 2029.
The CLUPI instrument is being developed by a Swiss–French consortium supported by the Swiss Space Office and the French Space Agency (CNES). Its Principal Investigator is Jean-Luc Josset, from the Space Exploration Institute, Neuchatel in Switzerland. Frances Westall and Beda Hofmann are Co-PIs. [3] The science team includes scientists from Canada, Europe and Russia, especially for biosignature recognition. [3] Instrument field tests started in 2009 with preliminary CLUPI systems tested during several Arctic winters. [3]
CLUPI will be mounted on the movable rover's drill box and it will acquire high-resolution, close-up images in colour of the texture, structure and morphology of rocks and soil. [2] The resolution will be similar to what geologists would obtain by using a hand-held magnifying lens: [3] at a distance of 10 cm from the target, the maximum resolution is 7 μm/pixel. [2] Its field of view can be changed by the use of two fixed, flat mirrors (FOV2 and FOV3). The CLUPI visual images will complement those provided by PanCam to provide the context necessary for interpretation of mineralogy and potential visible biosignatures. [3]
CLUPI will observe the drilling area very closely from different angles to help characterise rock structures such as embedded crystals and fractures. After the drill has been used and retracted, CLUPI will be used to image the amount and appearance of dislodged fines. From the high position, the camera will be able to observe the borehole to a depth of approximately 10 cm, depending on the local illumination conditions. [2] Then, CLUPI will be used to image the collected core prior to delivery to the rovers' internal analytical instruments for further processing and analyses. [2]
CLUPI | Performance/units [2] [3] |
---|---|
Detector | Full colour Active Pixel Sensor (APS) 3 colours |
Image dimension | 2652 × 1768 pixels |
Field of view | 14° |
Image resolution | 7 μm/pixel at 10 cm distance, viewed area 1.9 cm × 1.3 cm 39 μm/pixel at 50 cm distance, viewed area 10 cm × 7 cm 79 μm/pixel at 100 cm distance, viewed area 21 cm × 14 cm |
Focal length | Variable: 10 cm to infinity Autofocus |
Exposure time | ≤ 1024 seconds Automatic exposure time. |
Spectral range | 400 – 700 nm |
Mass | 932 g |
Data storage | 4 Gb |
Max power consumption | 15 W |
Astrobiology is a scientific field within the life and environmental sciences that studies the origins, early evolution, distribution, and future of life in the universe by investigating its deterministic conditions and contingent events. As a discipline, astrobiology is founded on the premise that life may exist beyond Earth.
The possibility of life on Mars is a subject of interest in astrobiology due to the planet's proximity and similarities to Earth. To date, no proof of past or present life has been found on Mars. Cumulative evidence suggests that during the ancient Noachian time period, the surface environment of Mars had liquid water and may have been habitable for microorganisms, but habitable conditions do not necessarily indicate life.
A biosignature is any substance – such as an element, isotope, molecule, or phenomenon – that provides scientific evidence of past or present life on a planet. Measurable attributes of life include its complex physical or chemical structures, its use of free energy, and the production of biomass and wastes.
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Icebreaker Life is a Mars lander mission concept proposed to NASA's Discovery Program. The mission involves a stationary lander that would be a near copy of the successful 2008 Phoenix and InSight spacecraft, but would carry an astrobiology scientific payload, including a drill to sample ice-cemented ground in the northern plains to conduct a search for biosignatures of current or past life on Mars.
Oxia Planum is a 200 km-wide clay-bearing plain located on the planet of Mars inside the Oxia Palus quadrangle on the eastern border of Chryse Planitia. The plain lies between the Mawrth Vallis outflow channel to the north-east and the Ares Vallis outflow channel to the south-west. In 2019, the International Astronomical Union Working Group for Planetary System Nomenclature officially approved Oxia Planum as a feature on the surface of Mars.
The Mars Organic Molecule Analyser (MOMA) is a mass spectrometer-based instrument on board the Rosalind Franklin rover to be launched in 2028 to Mars on an astrobiology mission. It will search for organic compounds in the collected soil samples. By characterizing the molecular structures of detected organics, MOMA can provide insights into potential molecular biosignatures. MOMA will be able to detect organic molecules at concentrations as low as 10 parts-per-billion by weight (ppbw). MOMA examines solid crushed samples exclusively; it does not perform atmospheric analyses.
Mars Multispectral Imager for Subsurface Studies (Ma_MISS) is a miniaturized imaging spectrometer designed to provide imaging and spectra by reflectance in the near-infrared (NIR) wavelength region and determine the mineral composition and stratigraphy. The instrument is part of the science payload on board the European Rosalind Franklin rover, tasked to search for biosignatures, and scheduled to launch not earlier than 2028. Ma_MISS is essentially inside a drill on the Rover, and will take measurements of the sub-surface directly.
MicrOmega-IR is an infrared hyperspectral microscope that is part of the science payload on board the European Rosalind Franklin rover, tasked to search for biosignatures on Mars. The rover is planned to be launched not earlier than 2028. MicrOmega-IR will analyse in situ the powder material derived from crushed samples collected by the rover's core drill.
Raman Laser Spectrometer (RLS) is a miniature Raman spectrometer that is part of the science payload on board the European Space Agency'sRosalind Franklin rover, tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched not earlier than 2028 and land on Mars in 2029.
Infrared Spectrometer for ExoMars (ISEM) is an infrared spectrometer for remote sensing that is part of the science payload on board the European Space Agency'sRosalind Franklin rover, tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched not earlier than 2028 and land on Mars in 2029.
ADRON-RM is a neutron spectrometer to search for subsurface water ice and hydrated minerals. This analyser is part of the science payload on board the European Space Agency'sRosalind Franklin rover, tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched not earlier than 2028 and land on Mars in 2029.
WISDOM is a ground-penetrating radar that is part of the science payload on board the European Space Agency'sRosalind Franklin rover, tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched not earlier than 2028 and land on Mars in 2029.
Signs Of LIfe Detector (SOLID) is an analytical instrument under development to detect extraterrestrial life in the form of organic biosignatures obtained from a core drill during planetary exploration.
The UK Centre for Astrobiology was set up at the University of Edinburgh in 2011 by Charles Cockell. It was set up as a UK node, formally affiliated as an international partner with the NASA Astrobiology Institute (NAI) alongside other national nodes until the NAI's dissolution in 2019. It was established as a virtual centre to sit at the interdisciplinary boundary of planetary sciences/astronomy and biological/earth sciences investigating numerous aspects of life in the universe, specifically 'how habitable worlds form in the Universe and how life emerges, proliferates and leaves traces on these worlds' as well as engaging in work on the robotic and human exploration of space and in space ethics, philosophy and governance.