DAVINCI

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DAVINCI (Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging) is a planned mission for an orbiter and atmospheric probe to the planet Venus. Together with the separate VERITAS mission, which will also study Venus, it was selected by NASA on June 2, 2021, to be part of their Discovery Program. Its acronym is inspired by Leonardo da Vinci in honor of his scientific innovations, aerial sketches and constructions. DAVINCI will send both an orbiter and a descent probe to Venus. The orbiter will image Venus in multiple wavelengths from above, while the descent probe will study the chemical composition of Venus's atmosphere and take photographs during descent. The DAVINCI probe will travel through the Venusian atmosphere, sampling the atmosphere, and returning measurements down to the surface. These measurements are important to understanding the origin of the atmosphere, how it has evolved, and how and why it is different from the atmosphere of Earth and Mars. The measurements taken by DAVINCI will investigate the possible history of water on Venus and the chemical processes at work in the unexplored lower atmosphere. Before it reaches the surface, the DAVINCI probe will capture high-resolution images of the planet's ridged terrain ("tesserae"), returning the first images of the planet's surface since the Soviet Venera 14 lander in 1982.…

DAVINCI (Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging) is a planned mission for an orbiter and atmospheric probe to the planet Venus. Together with the separate VERITAS mission, which will also study Venus, it was selected by NASA on June 2, 2021, to be part of their Discovery Program. Its acronym is inspired by Leonardo da Vinci in honor of his scientific innovations, aerial sketches and constructions. DAVINCI will send both an orbiter and a descent probe to Venus. The orbiter will image Venus in multiple wavelengths from above, while the descent probe will study the chemical composition of Venus's atmosphere and take photographs during descent. The DAVINCI probe will travel through the Venusian atmosphere, sampling the atmosphere, and returning measurements down to the surface. These measurements are important to understanding the origin of the atmosphere, how it has evolved, and how and why it is different from the atmosphere of Earth and Mars. The measurements taken by DAVINCI will investigate the possible history of water on Venus and the chemical processes at work in the unexplored lower atmosphere. Before it reaches the surface, the DAVINCI probe will capture high-resolution images of the planet's ridged terrain ("tesserae"), returning the first images of the planet's surface since the Soviet Venera 14 lander in 1982. It will also collect data for studying the planet's origin, and its tectonic and weathering history.

Descent probe instruments

On the descent probe, DAVINCI Venus Analytic Laboratory (VAL) instruments will provide high-fidelity synergistic measurements throughout the probe's descent, particularly in the upper clouds and the unexplored near-surface environment. VAL design is based on the Sample Analysis at Mars (SAM) instrument on the Curiosity rover, which measured the chemical and isotopic composition of the Martian atmosphere, and found the first definitive evidence of organics on Mars. DAVINCI four science instruments are:

Orbiter instruments

On the orbiter, a multi-spectral camera with narrow and wide-angle modes will image the planet in the UV and the 1-micron near-infrared band. The imaging will be done during two Venus flybys before the probe deployment, followed by an orbital remote sensing phase to complement the descent probe.

See also

EnVision, a Venus orbiter selected by ESA with NASA participation Galileo orbiter's Jupiter atmospheric probe Venera, a series of Soviet probes and landers Pioneer Venus Multiprobe

References

External links

Mission website

Text derived from https://en.wikipedia.org/w/index.php?oldid=1353146566 under CC BY-SA 4.0; modifications have been made.

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