Rendering of the EnVision spacecraft around Venus with SRS, VenSAR feeder and reflectarray antennas deployed. Credit ESA / NASA / Paris Observatory / VR2Planets.
EnVisionis an orbital mission toVenusbeing developed by theEuropean Space Agency(ESA) that is planned to perform high-resolutionradar mappingand atmospheric studies.[5][3]EnVision is designed to help scientists understand the relationships between its geological activity and theatmosphere,and it would investigate why Venus and Earth took such different evolutionary paths. The probe was selected as the fifth medium mission (M5) of ESA'sCosmic Visionprogramme in June 2021,[4]with launch planned for 2031.[1]The mission will be conducted in collaboration withNASA,with the potential sharing of responsibilities currently under assessment.
Animation ofEnVision'sproposed trajectory from 15 June 2032 to 01 March 2034 EnVision·Earth·Venus·Sun Animation of EnVision's proposed trajectory during the aerobraking phase around Venus
EnVision will deliver new insights into geological history through complementary imagery, polarimetry, radiometry and spectroscopy of the surface coupled with subsurface sounding and gravity mapping; it will search for thermal, morphological, and gaseous signs of volcanic and other geological activity; and it will trace the fate of key volatile species from their sources and sinks at the surface through the clouds up to the mesosphere. Core science measurements include: high-resolution mapping of specific targets, surface change, geomorphology, topography, subsurface, thermal emission,SO 2,H 2O,D/H ratio, gravity, spin rate, and spin axis. The specific mission's goals are:[3][6]
Determine the level and nature of current activity
Determine the sequence ofgeological eventsthat generated its range of surface features
Understand the organising geodynamic framework that controls the release of internal heat over the history of the planet
A new fleet of Venus missions has been selected, and new mission concepts will continue to be considered for future selections. Missions under development include ESA's EnVision M5 orbiter mission, NASA-JPL’s VERITAS orbiter mission, NASA-GSFC’s DAVINCI entry probe/flyby mission. The data acquired with the VERITAS, DAVINCI, and EnVision from the end of this decade will fundamentally improve our understanding of the planet’s long term history, current activity and evolutionary path.[6]
EnVision is an ESA mission in collaboration with NASA, and contributions from individual ESA member states for the provision of payload elements. NASA is contributing the VenSAR instrument and supplies DSN support. The other payload instruments are contributed by ESA member states, with ASI, DLR, BelSPO, and CNES leading the procurement of SRS, VenSpec-M, VenSpec-H and VenSpec-U instruments respectively.[2][3][6]
Venus Synthetic Aperture Radar(VenSAR), which will operate at 3.2GHzin theS-band(9.4 cm wavelength). VenSAR will provide several imaging and ranging techniques from a polar orbit: (1) regional and targeted surface mapping, (2) global topography and altimetry, (3) stereo imaging, (4) surfaceradiometryandscatterometry,(5) surfacepolarimetry,(6) repeat passinterferometryopportunities. TheJet Propulsion Laboratory's S-bandsynthetic-aperture radar(VenSAR) selected by NASA is currently undergoing scientific, technical and mission assessment. A SAR is a versatile remote sensing technology that has unique capabilities for determining geophysical information often not available by other remote sensing methods. VenSAR will characterise structural, and geomorphic evidence of multi-scale processes that shaped the geological history of Venus, as well as characterise current volcanic, tectonic, and sedimentary activity. The principal investigator of the Venus Synthetic Aperture Radar isScott Hensley,Jet Propulsion LaboratoryNASA/California Institute of Technology.
Venus Subsurface Radar Sounder(SRS), which will be a fixed dipole antenna operating in the range 9–30 MHz. SRS will search for subsurface material boundaries in various geological terrains that include impact craters and their infilling, buried craters, tesserae and their edges, plains, lava flows and their edges, and tectonic features in order to provide stratigraphic relationships at various depth ranges and horizontal scales. The principal investigator of the Subsurface Radar Sounder isLorenzo Bruzzone,Università di Trento,Italy.[2]
Venus Spectroscopy Suite(VenSpec), which will consist of three channels:VenSpec-M,VenSpec-H and VenSpec-U. VenSpec-M will provide compositional data on rock types, VenSpec-H will perform extremely high resolution atmospheric measurements, and VenSpec-U will monitor sulphured minor species (mainlySOandSO2), as well as the mysterious UV absorber in the Venusian upper clouds. This suite will search for temporal variations in surface temperatures and tropospheric concentrations of volcanic gases, indicative ofvolcanic eruptions.The principal investigator of the Venus Spectroscopy suite and PI of VenSpec-M isJörn Helbert,DLRInstitute of Planetary Research,Berlin, Germany. The PI of VenSpec-H is Ann Carine Vandaele, RoyalBelgian Institute for Space Aeronomy(BIRA/IASB), Belgium. The PI of VenSpec-U isEmmanuel Marcq,LATMOS, IPSL, France.[2]
Radio Science ExperimentAny orbiting spacecraft is sensitive to the local gravity field, plus the gravity field of the Sun and, to a minor extent, other planets. These gravitational perturbations generate spacecraft orbital velocity perturbations, from which the gravity field of a planet can be determined. EnVision's low-eccentricity, near-polar and relatively low altitude orbit offers the opportunity to obtain a high-resolution gravity field at each longitude and latitude of the Venusian globe.[2]
The analysis of the gravity field together with the topography gives insights on the lithospheric and crustal structure, allowing to better understand Venus's geological evolution. In the absence of seismic data, the measurements of the tidal deformation and proper motion of the planet provide the way to probe its deep internal structure (size and state of the core). The tidal deformation can be measured in theEnVisionorbital velocity perturbations through the gravitational potential variations it generates (k2 tidal Love number).
The co-Principal Investigators ofEnVisionRadio Science and Gravity experiment areCaroline Dumoulin,LPG, Université de Nantes, France, andPascal Rosenblatt,LPG, Université de Nantes, France.[2]
