Volcanic activity lasting hundreds to thousands of centuries and erupting massive amounts of material may have helped transform Venus from a temperate and wet world to the acidic hothouse it is today, a NASA paper suggests.
The paper also discusses these “large
igneous provinces” in Earth’s history which caused several mass extinctions on
our own planet millions of years ago.
Maat Mons is displayed in this computer-generated, three-dimensional
perspective of the surface of Venus. The viewpoint is located 634 kilometers
(393 miles) north of Maat Mons at an elevation of 3 kilometers (2 miles) above
the terrain. Lava flows extend for hundreds of kilometers across the fractured
plains shown in the foreground, to the base of Maat Mons. NASA Magellan mission
synthetic aperture radar data is combined with radar altimetry to develop a
three-dimensional map of the surface. The vertical scale in this perspective
has been exaggerated 10 times. Credits: NASA/JPL Full caption
“By understanding the record of large igneous provinces on Earth and Venus,
we can determine if these events may have caused Venus’ present condition,”
said Dr. Michael J. Way, of NASA’s Goddard Institute for Space Studies in New
York. Way is lead author on the paper, published April 22 in the Planetary Science Journal.
Large igneous provinces are the products of periods of large-scale
volcanism lasting tens of thousands or even hundreds of thousands of years.
They can deposit more than 100,000 cubic miles of volcanic rock onto the
surface. At the upper end, this could be enough molten rock to bury the entire
state of Texas half a mile deep.
Venus today boasts surface temperatures of around 864 F on average, and an
atmosphere 90 times the surface pressure of Earth’s. According to the study,
these massive volcanic outpourings may have initiated these conditions sometime
in Venus’ ancient history. In particular, the occurrence of several such
eruptions in a short span of geologic time (within a million years) could have
led to a runaway greenhouse
effect which kicked off the planet’s transition from
wet and temperate to hot and dry.
Large fields of solidified volcanic rock cover 80% of Venus’ surface in
total, Way said. “While we’re not yet sure how often the events which created
these fields occurred, we should be able to narrow it down by studying Earth’s
own history.”
Life on Earth has endured at least five major mass extinction events since
the origin of multicellular life about 540 million years ago, each of which
wiped out more than 50% of animal life across the planet. According to this
study and others before it, the majority of these extinction events were caused
or exacerbated by the kinds of eruptions that produce large igneous provinces.
In Earth’s case, the climate disruptions from these events were not sufficient
to cause a runaway greenhouse effect as they were on Venus, for reasons that
Way and other scientists are still working to determine.
NASA’s next missions to Venus, scheduled for launch in the late 2020s – the
Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and
Imaging (DAVINCI) mission and the Venus Emissivity, Radio science, InSAR, Topography, And
Spectroscopy (VERITAS) mission – aim to study the origin, history, and present state of Venus in
unprecedented detail.
“A primary goal of DAVINCI is to narrow down the history of water on Venus
and when it may have disappeared, providing more insight into how Venus’
climate has changed over time,” Way said.
The DAVINCI mission will precede VERITAS, an orbiter designed to
investigate the surface and interior of Venus from high above, to better
understand its volcanic and volatile history and thus Venus’ path to its current
state. The data from both missions could help scientists to narrow down the
exact record of how Venus may have transitioned from wet and temperate to dry
and sweltering. It may also help us to better understand how volcanism here on
Earth has affected life in the past, and how it may continue to do so in the
future.
This study was supported by Goddard Space Flight Center’s Sellers Exoplanet Environments Collaboration (SEEC) and was part of NASA’s Nexus for Exoplanet System Science (NExSS) RCN.
By: Nick Oakes NASA Goddard Space Flight Center, Greenbelt, Maryland
Source: NASA
Study: Massive Volcanism May Have Altered Ancient Venus’ Climate
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