NASA’s DAVINCI — Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging — mission embodies the spirit of innovation and exploration that its namesake, Leonardo da Vinci, was famous for.
Scheduled to launch in the early 2030s, DAVINCI will explore Venus with both a spacecraft and a descent probe.
DAVINCI’s probe will be the first in the 21st century to brave Venus’
atmosphere as it descends from above the planet’s clouds down to its surface.
Two other missions, NASA’s
VERITAS and ESA's (European Space
Agency) Envision, will also explore Venus in the 2030s from the planet’s orbit.
The DAVINCI spacecraft will study Venus’ clouds and highlands during two
flybys. It also will release a spherical probe, about 3 feet wide, that will
plunge through the planet’s thick atmosphere and corrosive clouds, taking
measurements and capturing high-resolution images of the Venusian surface as it
descends below the clouds.
Here are some of DAVINCI’s coming “firsts” in Venus exploration:
Exploring Solar System’s One-of-a-Kind Terrain
The DAVINCI mission will be the
first to closely explore Alpha Regio, a region known as a “tessera.” So far
found only on Venus, where they make up about 8% of the surface, tesserae are
highland regions similar in appearance to rugged mountains on Earth. Previous
missions discovered these features using radar instruments, but of the many
international spacecraft that dove through Venus’ atmosphere between 1966 and
1985, none studied or photographed tesserae.
Thought to be ancient continents,
tesserae like Alpha Regio may be among the oldest surfaces on the planet,
offering scientists access to rocks that are billions of years old.
By studying these rocks from above
Alpha Regio, DAVINCI scientists may learn whether ancient Venus had continents
and oceans, and how water may have influenced the surface.
Photographing One of the Oldest Surfaces on Venus
The DAVINCI probe will capture the
first close-up views of Alpha Regio with its infrared and optical cameras;
these will also be the first photos of the planet’s surface taken in more than
40 years.
With surface temperatures reaching
900° F and air pressure 90 times that of Earth’s, Venus’ harsh environment
makes exploration challenging, while its opaque atmosphere obscures direct
views. Typically, scientists rely on radar instruments from Earth or Venus-orbiting
spacecraft to study its terrain.
But DAVINCI’s probe will descend
through the atmosphere and below the clouds for a clear view of the mountains
and plains. It will capture images comparable to an airplane’s landing view of
Earth’s surface. Scientists will use the photos to compile 3D maps of Alpha
Regio that will provide more detail than ever of Venus' terrain, helping them
look for rocks that are usually only made in association with water.
An artist's visualization of DAVINCI's descent probe
lying on the surface of Venus.
NASA's Scientific Visualization Studio
Unveiling Secrets of Venus’ Mysterious Lower Atmosphere
The DAVINCI mission will be the
first to analyze the chemical composition of Venus’ lower atmosphere through
measurements taken at regular intervals, starting from approximately 90,000
feet above the surface and continuing until just before impact.
This region is critical because it
contains gases and chemical compounds that may originate from Venus’ lower
clouds, surface, or even subsurface.
For example, sulfur compounds
detected here could indicate whether Venusian volcanoes are currently active or
were active in the recent past. Noble gases (like helium or xenon), on the
other hand, remain chemically inert and maintain stable concentrations,
offering invaluable clues about Venus’ ancient history, such as the planet’s
past water inventory.
By comparing Venus’ noble gas
composition with that of Earth and Mars, scientists can better understand why
these planets — despite forming from similar starting materials — evolved into
dramatically different worlds.
Moreover, DAVINCI’s measurements of
isotopes and trace gases in the lower atmosphere will shed light on Venus’
water history, from ancient times to the present, and the processes that
triggered the planet’s extreme greenhouse effect.
State-of-the-Art Technology to Study Venus in Detail
Thanks to modern technology, the
DAVINCI probe will be able to do things 1980s-era spacecraft couldn’t.
The descent probe will be better
equipped than previous probes to protect the sensitive electronics inside of
it, as it will be lined on the inside with high-temperature, multi-layer
insulation — layers of advanced ceramic and silica fabrics separated by
aluminum sheets.
Venus’ super thick atmosphere will
slow the probe’s descent, but a parachute will also be released to slow it down
further. Most Earth-friendly parachute fabrics, like nylon, would dissolve in
Venus’ sulfuric acid clouds, so DAVINCI will have to use a different type of
material than previous Venus missions did: one that’s resistant to acids and
five times stronger than steel.
By Lauren
Colvin, with Lonnie Shekhtman
NASA’s
Goddard Space Flight Center, Greenbelt, Md.
Source: NASA DAVINCI Mission’s Many ‘Firsts’ to Unlock Venus’ Hidden Secrets - NASA Science
No comments:
Post a Comment