Venus has a volcano that is active. The earth is still alive.
Maat Mons is displayed in this computer generated three-dimensional perspective of the surface of Venus. The viewpoint is located 393 miles (634 kilometers) north of Maat Mons at an elevation of 2 miles (3 km) above the terrain. Lava flows extend for hundreds of kilometers across the fractured plains shown in the foreground, to the base of Maat Mons. (Image credit: NASA/JPL-Caltech)
Volcanic
activity has been detected on Venus, according to researchers looking at data
returned to Earth by NASA's Magellan probe in the early 1990s. The finding was
made public in a paper released on March 15 and is based on modifications to a
vent close to Maat Mons, one of the planet's largest volcanoes.
"Where
we made the discovery is the most likely place that there should have been new
volcanism," Robert Herrick, a researcher at the University of Alaska
Fairbanks Geophysical Institute, said Wednesday (March 15) at the 54th Lunar
and Planetary Science Conference (LPSC) being held in Texas and virtually.
Lava flows
from Venusian volcanoes that exploded a few million years ago have long been
known to scientists. Although nearly a million smaller volcanoes and 1,600 main
ones make up the majority of the planet's surface, it is debatable whether any
of them still erupt.
The most
recent discovery is the first time that researchers have discovered concrete
proof of recent volcanic activity on Venus, Earth's nearest neighbor. They
believe that such eruptions, which are less violent than those on Earth, take
place at least a few times annually, adding to the mounting proof that
volcanoes are a significant factor in forming the planet's young surface.
In the most
recent investigation, researchers examined two Magellan photographs taken in
1991 eight months apart. They observed that during those eight months, a
volcanic vent that had previously been 0.7 square miles (2 square kilometers)
in size had increased "considerably," to approximately 1.5 square
miles. (4 square km).
In the
second picture, the vent was kidney-shaped with a dark interior, as opposed to
the first image's circular form. This is proof that "a volcano has erupted
on the surface of Venus," as Herrick stated during his presentation at
LPSC. According to him, the dark area is probably a lava lake that has filled
the outlet to the rim.
With the
scant information available, the team makes the assumption that Venus' intense
heat and high pressure cause the lava to flow longer on Venus than it does on
Earth.
There are
likely many more active volcanoes yet to be found since Venus is largely
covered with them. After making the find, Herrick said he stopped looking, but
"by no means has all the potential searching for new stuff with the
Magellan data been done."
Only 1.5% of
the planet is covered by the most recent research, but 40% has been imaged
twice by the Magellan spacecraft, providing scientists with a wealth of radar
data to sort through.
There is
still much to be done there, according to Herrick, as there are still a number
of Hawaii-like volcanoes on Venus that I did not have time to explore.
A discovery from 30-year old data
in 1990, the
Magellan probe reached Venus and spent two years taking pictures from orbit.
The spacecraft made eight-monthly returns to the same locations during this
period. The images were taken at varying angles and heights back then because
the goal of each visit was not to detect surface changes like scientists are
doing now, according to Herrick. He added that it's possible to imagine both of
the discovery's pictures as having been taken from windows on various airplane
sides.
Herrick
attributed the timing of this finding to recent advancements in planetary
scientists' software and hardware, despite the fact that the Magellan images
are 30 years old. Scientists can now quickly download huge datasets and zoom in
and out of radar images, which they were unable to do thirty years ago, much
like Google Earth.
Herrick and
his team chose specific locations on the surface of Venus that stayed the same
in both of Magellan's images because the images were taken at different angles,
and they processed the images to make them appear as though they were taken
from above. Scientists use a technique called orthorectification to transform
unprocessed pictures into a modeling-friendly format.
During his
presentation at LPSC, Herrick stated, "We really wanted to nail down that
the difference we saw in the vent could not conceivably, in any way, be a
factor of merely looking at the same feature from different angles.
Herrick
collaborated with Scott Hensley, a project scientist for two future NASA
missions to Venus, to determine whether what they were seeing was actually
volcanic activity.
Hensley
remarked, "I was immediately cautiously optimistic and excited because it
did look real, but it did not look real," adding that earlier attempts to
find comparable changes in the images had not produced fruitful outcomes. In
addition, because of variations in lighting and spacecraft angles, many
characteristics on Venus that did not change appeared different in distinct
Magellan images.
Hensley
stated, "We wanted to be very careful here that we really had something."
None of our
simulations could reproduce the kidney-shaped vent, he claimed, adding that
their simulations also failed to depict the vent's entire dark bottom as
observed by Magellan. We had a real change on the surface of Venus because of
this, we firmly believe.
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