This computer-generated 3D model of
Venus’ surface shows the summit of Maat Mons, the volcano that is exhibiting
signs of activity. A new study found one of Maat Mons’ vents became enlarged
and changed shape over an eight-month period in 1991, indicating an eruptive
event occurred. Credits: NASA/JPL-Caltech
In a first, scientists have seen
direct evidence of active volcanism on Earth’s twin, setting the stage for the
agency’s VERITAS mission to investigate.
Direct geological evidence of
recent volcanic activity has been observed on the surface of Venus for the
first time. Scientists made the discovery after poring over archival radar
images of Venus taken more than 30 years ago, in the 1990s, by NASA’s Magellan mission. The images revealed
a volcanic vent changing shape and increasing significantly in size in less
than a year.
Scientists study active volcanoes
to understand how a planet’s interior can shape its crust, drive its evolution,
and affect its habitability. One of NASA’s new missions to Venus will do just
that. Led by the agency’s Jet Propulsion Laboratory in Southern
California, VERITAS – short for Venus Emissivity,
Radio science, InSAR, Topography, And Spectroscopy – will launch within a
decade. The orbiter will study Venus from surface to core to understand how a
rocky planet about the same size as Earth took a very different path,
developing into a world covered in volcanic plains and deformed terrain hidden
beneath a thick, hot, toxic atmosphere.
“NASA’s selection of the VERITAS
mission inspired me to look for recent volcanic activity in Magellan data,”
said Robert Herrick, a research professor at the University of Alaska Fairbanks
and member of the VERITAS science team, who led the search of the archival
data. “I didn’t really expect to be successful, but after about 200 hours of
manually comparing the images of different Magellan orbits, I saw two images of
the same region taken eight months apart exhibiting telltale geological changes
caused by an eruption.”
The search and its conclusions are described in a new study published in the journal Science. Herrick also presented the findings at the 54th Lunar and Planetary Science Conference in the Woodlands, Texas, on March 15.
This computer-generated 3D model of Venus’ surface shows the summit of Maat Mons, the volcano that is exhibiting signs of activity. A new study found one of Maat Mons’ vents became enlarged and changed shape over an eight-month period in 1991, indicating an eruptive event occurred. Credits: NASA/JPL-Caltech
In a first, scientists have seen
direct evidence of active volcanism on Earth’s twin, setting the stage for the
agency’s VERITAS mission to investigate.
Direct geological evidence of
recent volcanic activity has been observed on the surface of Venus for the
first time. Scientists made the discovery after poring over archival radar
images of Venus taken more than 30 years ago, in the 1990s, by NASA’s Magellan mission. The images revealed
a volcanic vent changing shape and increasing significantly in size in less
than a year.
Scientists study active volcanoes
to understand how a planet’s interior can shape its crust, drive its evolution,
and affect its habitability. One of NASA’s new missions to Venus will do just
that. Led by the agency’s Jet Propulsion Laboratory in Southern
California, VERITAS – short for Venus Emissivity,
Radio science, InSAR, Topography, And Spectroscopy – will launch within a
decade. The orbiter will study Venus from surface to core to understand how a
rocky planet about the same size as Earth took a very different path,
developing into a world covered in volcanic plains and deformed terrain hidden
beneath a thick, hot, toxic atmosphere.
“NASA’s selection of the VERITAS
mission inspired me to look for recent volcanic activity in Magellan data,”
said Robert Herrick, a research professor at the University of Alaska Fairbanks
and member of the VERITAS science team, who led the search of the archival
data. “I didn’t really expect to be successful, but after about 200 hours of
manually comparing the images of different Magellan orbits, I saw two images of
the same region taken eight months apart exhibiting telltale geological changes
caused by an eruption.”
The search and its conclusions are
described in a new study published in the journal
Science. Herrick also presented the findings at the 54th Lunar and Planetary Science
Conference in
the Woodlands, Texas, on March 15.
This annotated, computer-simulated global map of Venus’ surface is assembled from data from NASA’s Magellan and Pioneer Venus Orbiter missions. Maat Mons, the volcano that has exhibited signs of a recent eruption, is within the black square near the planet’s equator. Credits: NASA/JPL-Caltech
Magellan’s Legacy
Herrick, Hensley, and the rest of
the VERITAS team are eager to see how the mission’s suite of advanced science
instruments and high-resolution data will complement Magellan’s remarkable
trove of radar imagery, which transformed humanity’s knowledge of Venus.
“Venus is an enigmatic world, and
Magellan teased so many possibilities,” said Jennifer Whitten, associate deputy
principal investigator of VERITAS at Tulane University in New Orleans. “Now
that we’re very sure the planet experienced a volcanic eruption only 30 years
ago, this is a small preview for the incredible discoveries VERITAS will make.”
VERITAS will use state-of-the-art
synthetic aperture radar to create 3D global maps and a near-infrared
spectrometer to figure out what the surface is made of. The spacecraft will
also measure the planet’s gravitational field to determine the structure of
Venus’ interior. Together, the instruments will offer clues about the planet’s
past and present geologic processes.
And whereas Magellan’s data was
originally cumbersome to study – Herrick said that in the 1990s they relied on
boxes of CDs of Venus data that were compiled by NASA and delivered in the mail
– VERITAS’ data will be available online to the science community. That will
enable researchers to apply cutting-edge techniques, such as machine learning,
to analyze the planet and help reveal its innermost secrets.
Those studies will be complemented
by EnVision, an ESA (European Space Agency) mission to Venus slated for launch in the
early 2030s. The spacecraft will carry its own synthetic aperture radar (called
VenSAR), which is being developed at JPL, as well as a spectrometer similar to
the one VERITAS will carry. Both Hensley and Herrick are key members of the
VenSAR science team.
More About the Mission
VERITAS and NASA’s Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging (DAVINCI) mission were selected in 2021 under NASA’s Discovery Program as the agency’s next missions to Venus. VERITAS partners include Lockheed Martin Space, the Italian Space Agency, the German Aerospace Center, and Centre National d’Études Spatiales in France. The Discovery Program is managed by the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the Planetary Science Division of NASA’s Science Mission Directorate in Washington.
Source: NASA’s Magellan Data Reveals Volcanic Activity on Venus | NASA
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