#AceNewsReport – June.04: NASA has selected two new missions to Venus, Earthβs nearest planetary neighbor. Part of NASAβs Discovery Program, the missions aim to understand how Venus became an inferno-like world when it has so many other characteristics similar to ours β and may have been the first habitable world in the solar system, complete with an ocean and Earth-like climate:
NASA: These investigations are the final selections from four mission conceptsNASA picked in February 2020 as part of the agencyβs Discovery 2019 competition. Following a competitive, peer-review process, the two missions were chosen based on their potential scientific value and the feasibility of their development plans. The project teams will now work to finalize their requirements, designs, and development plans.
NASA is awarding approximately $500 million per mission for development. Each is expected to launch in the 2028-2030 time-frame:
The selected missions are:
DAVINCI+ (Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging)
DAVINCI+ will measure the composition of Venusβ atmosphere to understand how it formed and evolved, as well as determine whether the planet ever had an ocean. The mission consists of a descent sphere that will plunge through the planetβs thick atmosphere, making precise measurements of noble gases and other elements to understand why Venusβ atmosphere is a runaway hothouse compared the Earthβs.
In addition, DAVINCI+ will return the first high resolution pictures of the unique geological features on Venus known as βtesserae,β which may be comparable to Earthβs continents, suggesting that Venus has plate tectonics. This would be the first U.S.-led mission to Venusβ atmosphere since 1978, and the results from DAVINCI+ could reshape our understanding of terrestrial planet formation in our solar system and beyond. James Garvin of Goddard Space Flight Center in Greenbelt, Maryland, is the principal investigator. Goddard provides project management.
VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy)
VERITAS will map Venusβ surface to determine the planetβs geologic history and understand why it developed so differently than Earth. Orbiting Venus with a synthetic aperture radar, VERITAS will chart surface elevations over nearly the entire planet to create 3D reconstructions of topography and confirm whether processes such as plate tectonics and volcanism are still active on Venus.
VERITAS also will map infrared emissions from Venusβ surface to map its rock type, which is largely unknown, and determine whether active volcanoes are releasing water vapor into the atmosphere. Suzanne Smrekar of NASAβs Jet Propulsion Laboratory in Southern California, is the principal investigator. JPL provides project management. The German Aerospace Center will provide the infrared mapper with the Italian Space Agency and Franceβs Centre National d’Etudes Spatiales contributing to the radar and other parts of the mission.
βWeβre revving up our planetary science program with intense exploration of a world that NASA hasnβt visited in over 30 years,β said Thomas Zurbuchen, NASAβs associate administrator for science. βUsing cutting-edge technologies that NASA has developed and refined over many years of missions and technology programs, weβre ushering in a new decade of Venus to understand how an Earth-like planet can become a hothouse. Our goals are profound. It is not just understanding the evolution of planets and habitability in our own solar system, but extending beyond these boundaries to exoplanets, an exciting and emerging area of research for NASA.β
Zurbuchen added that he expects powerful synergies across NASAβs science programs, including the James Webb Space Telescope. He anticipates data from these missions will be used by the broadest possible cross section of the scientific community.
βIt is astounding how little we know about Venus, but the combined results of these missions will tell us about the planet from the clouds in its sky through the volcanoes on its surface all the way down to its very core,β said Tom Wagner, NASAβs Discovery Program scientist. βIt will be as if we have rediscovered the planet.β
In addition to the two missions, NASA selected a pair of technology demonstrations to fly along with them. VERITAS will host the Deep Space Atomic Clock-2, built by JPL and funded by NASAβs Space Technology Mission Directorate. The ultra-precise clock signal generated with this technology will ultimately help enable autonomous spacecraft maneuvers and enhance radio science observations.
DAVINCI+ will host the Compact Ultraviolet to Visible Imaging Spectrometer (CUVIS) built by Goddard. CUVIS will make high resolution measurements of ultraviolet light using a new instrument based on freeform optics. These observations will be used to determine the nature of the unknown ultraviolet absorber in Venusβ atmosphere that absorbs up to half the incoming solar energy.
Established in 1992, NASAβs Discovery Program has supported the development and implementation of over 20 missions and instruments. These selections are part of the ninth Discovery Program competition.
The concepts were chosen from proposals submitted in 2019 under NASA Announcement of Opportunity NNH19ZDA010O. The selected investigations will be managed by the Planetary Missions Program Office at NASAβs Marshall Space Flight Center in Huntsville, Alabama, as part of the Discovery Program. The Discovery Program conducts space science investigations in the Planetary Science Division of NASAβs Science Mission Directorate. The goals of the program are to provide frequent opportunities for principal investigator-led investigations in planetary sciences that can be accomplished under a not-to-exceed cost cap.
For more information about NASAβs planetary science, visit:
https://www.nasa.gov/solarsystem
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Last Updated: Jun 2, 2021
Editor: Sean Potter
#AceNewsDesk report β¦β¦Published: Jun.04: 2021:
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