VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy) is an upcoming mission fromNASA'sJet Propulsion Laboratory (JPL) to map the surface of the planetVenus in high resolution. The combination of topography, near-infraredspectroscopy, and radar image data will provide knowledge of Venus's tectonic and impact history, gravity, geochemistry, the timing and mechanisms ofvolcanic resurfacing, and the mantle processes responsible for them.
On 4 November 2022, NASA announced the postponement of the mission launch from 2027 to 2031, citing institutional problems at JPL delaying the launch ofPsyche.[3][4][5][6] The mission's Principal InvestigatorSuzanne Smrekar has counterproposed a November 2029 launch date, which she argued would require only modest "bridge" funding and compared to the 2031 option would offer lower overall cost and fewer conflicts withDAVINCI andEnVision; this position obtained endorsement by a Congressional committee in October 2023.[7] In November 2024, Smrekar stated that the mission was aiming to launch in June 2031.[2]
VERITAS was one of dozens of proposals submitted in 2015 to potentially become the 13th mission ofNASA’sDiscovery Program.Suzanne Smrekar of NASA'sJet Propulsion Laboratory (JPL) would serve as theprincipal investigator, and JPL would be the managing agency. On 30 September 2015, VERITAS was selected as one of five finalists.[8] On 4 January 2017, two other proposals to study small bodies,Lucy andPsyche, were selected as the 13th and 14th Discovery missions, respectively.[9]
VERITAS was again proposed for the Discovery Program in 2019, and was selected for Phase A funding on 13 February 2020.[10] On 2 June 2021, it was selected, along withDAVINCI+, to fly as one of the next Discovery missions.[11][12] Each mission will get approximately US$500 million in funding. VERITAS was originally planned to be launched between the years 2028 and 2030.[10] However, work on the mission was put on hold in November 2022, and the launch was delayed by at least three years (to no earlier than 2031), after an independent review of thePsyche mission found significant institutional issues at NASA and JPL.[13] The FY2024 budget request for VERITAS at $1.5M, released in March 2023, represented a near-complete freeze of the mission attested to be "functionally a soft cancellation".[14] This has been reverted in the FY24 bill released March 3, requesting NASA seek sufficient funding for the VERITAS Venus mission to enable a launch by the end of the decade.[15]
Venus is roughly the same size as Earth, but has a drastically different climate and surface
VERITAS will gather data to help scientists to answer three primary questions about Venus:[16]
How has its geology evolved over time?
What geologic processes are currently operating on it?
Has water been present on or near its surface?
Understanding Venus's geology is of significant scientific interest because of its similarities to Earth. Venus's size, age, and composition are all broadly similar to Earth's, but its environment is significantly different and less hospitable to life. Understanding Venus's geologic evolution therefore will help answer questions about the formation of planets hospitable to life.[16] A key step in developing an understanding of this evolution is an investigation of Venus's current geology. Current data is highly suggestive of recent and active volcanism on Venus, but the extent of this volcanic activity is not completely known.[17][18] Moreover, it is unknown to what degree surface water was historically present on Venus and what role subsurface water plays in Venus's modern geology.[16]
A comparison of past surface-imaging missions to Venus, of whichMagellan is the most recent
VERITAS will collect data to help answer these questions in several ways. High-resolution imagery will be obtained using anX-band radar configured as a single passinterferometric synthetic aperture radar (InSAR).[19] This radar data will be coupled with amultispectralnear-infrared (NIR) emissivity mapping capability. VERITAS will map surface topography with a spatial resolution of 250m and 5m vertical accuracy, and generate radar imagery with 30m spatial resolution.[20][19][21] This high-resolution imaging data will allow scientists to locate active volcanic eruptions, to understand the age and composition of features on the planet's surface, and better understand the planet's overall geology.[22] The spacecraft's communication system will also be used to perform a gravity science experiment to investigate variations in Venus'sgravitational field. The spacecraft's telecom system will be used to map gravity strength at Venus's surface, providing a uniform resolution of better than 160 km.[16][23] The data will provide an estimate of Venus's core size and information about topographic features that lie underneath the planet's surface.[24][25]
VERITAS is designed to produce global, high-resolutiontopography and imaging ofVenus's surface and produce the first maps of deformation and global surface composition, thermal emissivity, and gravity fields. Onboard the spacecraft will be twoscientific instruments, theVenus Emissivity Mapper (VEM) and Venus Interferometric Synthetic Aperture Radar (VISAR).[17][21][20][26]
VISAR (Venus Interferometric Synthetic Aperture Radar) is designed to generate global data sets for topography (250 m horizontal by 5 m vertical accuracy) and SAR imaging at 30 m resolution with targeted resolution at 15 m (compare toMagellan which had 50 km spatial and 100 m vertical resolution). VERITAS will create the first planetary active surface deformation map (1.5 cm vertical).[19][28]
In addition to these two instruments, the spacecraft will also carry the Deep Space Atomic Clock-2 as a secondary payload. The Deep Space Atomic Clock-2 is the successor to theDeep Space Atomic Clock payload flown on theSTP-2 mission in June 2019, and is intended to provide highly precise timing for deep space missions.[29]
^abS. E. Smrekar; L. Elkins-Tanton; S. Hensley; B. A. Campbell (2014).VERITAS: A mission to study the highest priority Decadal Survey questions for Venus. American Geophysical Union - Fall Meeting 2014.NASA.Bibcode:2014AGUFM.P21B3912S. This article incorporates text from this source, which is in thepublic domain.
^abS. Hensley; S. E. Smrekar; B. Pollard (2012). "VERITAS: A Mission Concept for the High Resolution Topographic Mapping and Imaging of Venus".American Geophysical Union, Fall Meeting.Bibcode:2012AGUFM.P33C1950H. P33C-1950.
^J. Helbert (19 September 2013).Observing the surface of Venus after VIRTIS on VEX: new concepts and laboratory work. Infrared Remote Sensing and Instrumentation XXI. San Diego, California, USA.doi:10.1117/12.2025582.
Missions are ordered by launch date.† indicates failure en route or before any data returned.‡ indicates use of the planet as agravity assist en route to another destination.
This article incorporates text from this source, which is in thepublic domain.
