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It’s no big secret that volcanoes can build new lands.
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Let’s take the Hawaiian Islands for example.
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They were a result of underwater volcanic eruptions that pumped out molten rock.
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It reached the surface of the sea and formed landmasses.
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But, did you know that the Earth isn’t the only body in our solar system with volcanoes?
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With technological advancements, we were able to explore (from afar) parts of the universe
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and discover volcanic activity on both planets and moons.
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Granted, some of them have been inactive for millions of years.
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But others are spewing all sorts of things into their atmospheres.
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Most volcanic eruptions found on both moons and planets formed millions of years ago,
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when our solar system was still a baby and all cosmic bodies had higher internal temperatures.
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When we think of the term “active volcano”, we usually associate it with the ones on Earth
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that are currently erupting.
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It’s easy, because we can observe them closely.
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Beyond our planet, the luxury of studying volcanic eruptions wasn’t available until
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the invention of powerful telescopes.
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Some were even transported closer to other planets and moons to get a better look.
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The most direct way to get evidence of volcanic eruptions is to see or capture them in action.
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The other way is to observe the body’s surfaces.
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An outburst can cover the ground with debris, or it can cause a resurface.
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Without such studies, it’s almost impossible to know if the volcanic activity is recent,
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or millions of years old.
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Volcanos, as we know them, are mostly mountainous openings in the Earth’s surface that emit
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volcanic ash, lava, and gases.
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Celestial bodies that are closer to the sun have a more solid composition and produce
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silicate rock lavas, just like Earth.
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However, planets and moons beyond Mars are filled with gas and silicate rocks.
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These have cryovolcanoes.
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Instead of hot molten rock; they spew cold liquid or frozen gasses such as ammonia, methane,
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and water.
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Based on studies, only 4 bodies of our solar system have been proven to have active volcanoes,
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and only one of them is a planet.
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The planet is the Earth.
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The rest of them are moons.
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We have Triton – Neptune’s largest natural satellite.
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Then there’s Enceladus, which is Saturn’s 6th largest moon.
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And, the most troubling one: Io, which belongs to the Jupiter Gang.
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It holds the title for the 4th largest moon in our solar system.
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Let’s start with Ioc, which recently made some news.
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Io managed to scare everyone by making them believe there was a black hole on Jupiter.
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NASA’s Juno spacecraft snapped a series of detailed images of the planet back in 2012.
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During the latest approach, which took place this year, it pictured a huge black spot on
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the ringed planet.
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At first, everyone was shocked.
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But as it turned out, it was Io’s shadow being cast on the surface.
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The spacecraft was approximately 5,000 miles away from the planet’s surface, but it just
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so happened to capture an eclipse.
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Due to Io’s distance from the sun, it’s hard to imagine that it has active volcanos.
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But, because of its small volume, it’s influenced by the planet’s gravity.
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This gravitational attraction causes powerful pulls which result in strong internal tides.
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These are followed by inner friction; the moon heats up, and volcanic eruptions occur.
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Io has hundreds of volcanic openings.
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Some of them blast frozen vapor, lava, and so-called volcanic snow.
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It was also hit by asteroids, just like other bodies in our solar system.
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But the impact craters keep disappearing because of the eruptions.
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The volcanic material spills onto the surface of the moon, covering and resurfacing different
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parts.
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That’s the evidence of volcanic activity.
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In august of 2014, NASA showed some images of volcanic eruptions that occurred on Io
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between the 15th and 29th of August in 2013.
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They were gigantic eruptions, projecting hundreds of miles above the surface.
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Oddly, only Earth and Io can spew hot lava in our solar system.
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Now let’s get to the king – Triton.
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This is the largest natural satellite of Neptune, and the first place where cryovolcanoes were
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observed.
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In 1977, space probe Voyager 2 detected a long cloud of smoke filled with nitrogen gas
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and dust.
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It erupted from the moon and traveled 5 miles up in the air.
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These eruptions happened quite often, and Triton’s surface became soft.
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Here’s how it goes: The cryovolcano eruptions fall back onto the surface, creating a soft
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layer similar to snow.
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Researchers believe that radiation from the sun goes through the surface of the moon and
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heats up the underground layer.
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Then, heat gets trapped and vaporizes the nitrogen that lies below the surface.
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That results in the expansion of nitrogen, which then erupts through the icy layers.
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The third active cryovolcano is on – one of the natural satellites of Saturn.
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In fact, this is the best documented active volcano.
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The first activity recorded was in 2005, by the Cassini spacecraft.
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It captured jets of icy particles coming out from the South Pole Region.
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Cassini even managed to fly over the volcanic cloud and reported that it was composed of
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water vapor, small amounts of methane, nitrogen and carbon dioxide.
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There’s a theory that explains how those specific cryovolcanoes work.
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Below the satellite’s surface, there are pockets of pressurized water.
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It remains in liquid form because it’s warmed up from the interior.
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Occasionally, the pressurized water comes to the surface and produces a cloud of water
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vapor alongside icy particles.
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Cryovolcanoes hadn’t been discovered until 2005, so an extensive search in our solar
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system was limited.
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While not yet proven, there’s a lot of evidence out there hinting at active volcanos elsewhere
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in the solar system.
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Take Venus, for example.
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There’s a lot of action going on there!
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It’s the hottest planet of the group.
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It has over 1,600 large volcanoes, and 100,000 to 1 million smaller ones.
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But what happens on Venus stays on Venus, hidden below it’s thick cloud clover, which
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is mostly composed of sulfuric acid and carbon dioxide.
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That’s a vacation spot!
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There’s no air or water on the surface of the planet – it just boils off.
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Venus has an extreme greenhouse effect.
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Therefore, it’s temperature can soar up to 880F.
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However, it has many layers of different temperatures.
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The atmospheric pressure slows down the winds.
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This stops rain or airstreams from affecting its surface, which is why old volcanic eruptions
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look relatively new.
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The variety of explosions is limited – only lava comes out, without volcanic ash or explosive
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molten rock.
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The tallest feature that resembles a volcano is the Maat Mons.
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It’s 3 miles in height.
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An orbiting probe, called Venus Express, recorded some spikes in temperatures that could indicate
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lava flows.
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However, it hasn’t been confirmed if it’s an active volcano.
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In 2015, scientists working with NASA’s New Horizons mission collected high-resolution
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data of one or two cryovolcanoes on the surface of Pluto.
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They’re 90 miles wide and 2.5 miles in height.
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If scientists are correct, they’ll be the largest cryovolcanoes outside of our solar
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system.
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For the time being, they were given the name Wright Mons to honor the Wright Brothers.
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Another possible volcano was mentioned in a 2019 study.
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Scientists from the European Space Agency, NASA, and the German Aerospace Center might’ve
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solved how the Ahuna Mons was formed.
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This was a mysterious mountain that appeared on the surface of Ceres – the largest object
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in our asteroid belt.
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It’s believed to be a cryovolcano that gushes plumes of saltwater and mud onto its surface.
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Ahuna Montata!
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It’s means no worries, I mean no Lava.
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Mars also had a few volcanic features in the Tharsis Montes region.
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The largest one is the Olympus Mons.
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The mountain was formed because of repeated volcanic eruptions on the planet.
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This was, in fact, the biggest volcano in our solar system.
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It stands 16 miles high and is 374 miles in diameter.
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To put that into perspective, if you were to put Olympus Mons next to Mount Everest,
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well Everest would seem like mole hill.
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The gigantic highland is a slightly sloping shield volcano.
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From the side, it resembles a warrior’s shield laying on the ground.
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That’s how the name was inspired.
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Speaking of inactive volcanoes, Mercury had a ton.
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It’s now filled with craters, and as far as volcanic activity goes, nothing interesting
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happens.
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But, in the distant past, things were more exciting there.
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There were huge stretches of landmasses that formed as a result of liquified rock spreading
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across its surface.
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When the planet began to cool down, those volcanoes went extinct.
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A huge area of the Earth’s moon is also covered in ancient lava flows, but it’s
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no longer volcanically active.
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Those areas are called “Mares” which means “seas” in Latin.
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The somewhat darker-looking areas remained from previous magma streams that spread on
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the surface before they cooled down.
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Mare Tranquilitus (The Sea of tranquility) was where Apollo 11 first landed.
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Lastly, we have the largest moon of Saturn – Titan.
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It’s the only identified moon with a dense atmosphere.
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It’s also the only extra-terrestrial body with lakes, but it doesn’t contain water.
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It’s made up of liquid hydrocarbons.
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One of the famous mountains there is the Doom Mons.
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However, there’s still some debate about whether it has active volcanoes.
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If it does, they’d be cryovolcanoes.
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Astronomers suspect that more volcanic activity will soon be discovered on the moons of icy
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planets in our solar system.
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These include Europa, Dione, Miranda and Ganymede.
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They’ll likely be so excited with the discoveries, they’ll be “over the moon”.
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