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DAVINCI: NASA’s Deep Atmosphere Venus Investigation of Noble Gases, Chemistry and Imaging

DAVINCI+ will send a meter-diameter probe to brave the high temperatures and pressures near Venus’ surface to explore the atmosphere from above the clouds to near the surface of a terrain that may have been a past a continent. During its final kilometers of free-fall descent (shown here), the probe will capture spectacular images and chemistry measurements of the deepest atmosphere on Venus for the first time. Credit: NASA GSFC visualization by CI Labs Michael Lentz and others

Launching in 2029, NASAEstablished in 1958, the National Aeronautics and Space Administration (NASA) is an independent agency of the United States Federal Government that succeeded the National Advisory Committee for Aeronautics (NACA). It is responsible for the civilian space program, as well as aeronautics and aerospace research. It’s vision is “To discover and expand knowledge for the benefit of humanity.””>NASA’s Deep Atmosphere VenusVenus, the second planet from the sun, is named after the Roman goddess of love and beauty. After the moon, it is the second-brightest natural object in the night sky. Its rotation (243 Earth days) takes longer than its orbit of the Sun (224.7 Earth days). It is sometimes called Earth’s “sister planet” because of their similar composition, size, mass, and proximity to the Sun. It has no natural satellites.”>Venus Investigation of Noble gases, Chemistry and Imaging (DAVINCI) mission will bring a rich suite of instruments to Venus to address long standing questions about Earth’s sister planet. Some scientists think Venus may once have been more Earth-like in the past, with oceans and pleasant surface temperatures — DAVINCI data will help us determine if this intriguing possibility is true.

Clues to Venus’ mysterious past may be hidden in atmospheric gases or in surface rocks formed in association with ancient water in the planet’s mountainous highlands. During two flybys, the DAVINCI carrier, relay, and imaging spacecraft will collect data on the planet’s day side of unknown compounds that absorb ultraviolet light in the Venus upper atmosphere with an instrument called the Compact Ultraviolet to Visible Imaging Spectrometer (CUVIS); on the planet’s night side, the Venus Imaging System for Observational Reconnaissance (VISOR) will sense heat from Venus’ surface emerging from beneath the clouds to help us better understand the composition of diverse geological highlands regions across Venus. VISOR will also study clouds on the Venus day side in the ultraviolet, producing cloud motion movies.

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Venus has a scorching surface hotter than your home oven, and a complex atmosphere 90 times thicker than Earth’s made mostly of carbon dioxide and with sulfuric acidAny substance that when dissolved in water, gives a pH less than 7.0, or donates a hydrogen ion.”>acid clouds.

Two years after launch, the DAVINCI descent sphere will be dropped by the carrier spacecraft into this extreme environment to provide new direct measurements of the Venus atmosphere, and to reveal a bird’s eye view of the surface below the clouds. The descent location, the Alpha Regio “tessera,” is a mountainous highland region whose rocks may hold clues to the planet’s mysterious past. The titanium sphere is designed to withstand the harsh conditions of the Venus environment while protecting the instruments nestled inside.

The Venus Tunable Laser Spectrometer (VTLS) will measure key gases that offer clues to the planet’s past, including compounds that may hint at the possible history of past water. The Venus Mass Spectrometer (VMS) will study the atmosphere in detail, including noble gases and trace gases from 67 km to the near surface. The Venus Atmospheric Structure Investigation (VASI) will measure pressure, temperature, and winds throughout the descent.

Peering through a transparent sapphire window at the bottom of the descent sphere, the Venus Descent Imager (VenDI) will map the 3-D topography and composition of Alpha Regio, with topographic resolution at up to sub-meter scales. Lastly, a student collaboration experiment called the Venus Oxygen Fugacity experiment (VfOx) will be mounted to the probe to measure oxygen in the deep atmosphere. Together, this set of data will help rewrite the textbooks on Venus and may even help us better understand Venus-like planets in other solar systems.

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NASA has selected the DAVINCI+ (Deep Atmosphere Venus Investigation of Noble-gases, Chemistry and Imaging +) mission as part of its Discovery program, and it will be the first probe to enter the Venus atmosphere since NASA’s Pioneer Venus in 1978 and USSR’s Vega in 1985. Named for visionary Renaissance artist and scientist, Leonardo da Vinci, the DAVINCI+ mission will bring 21st-century technologies to the world next door. DAVINCI+ may reveal whether Earth’s sister planet looked more like Earth’s twin planet in a distant, possibly hospitable past with oceans and continents. Credits: NASA’s Goddard Space Flight Center

DAVINCI is a partnership between NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and Lockheed Martin in Denver, Colorado, with instruments from NASA Goddard, Jet Propulsion Laboratory, Malin Space Science Systems, and key supporting hardware from Johns Hopkins Applied Physics Laboratory and the University of Michigan.

Source: SciTechDaily