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Impact of eruptio V o l c a n o e s Prediction Part II Supervolcanoe Volcanoes in spac

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V. o. s. l. c. e. a. o. n. Part II. Prediction. Impact of eruptions. Supervolcanoes. Volcanoes in space. Prediction of Volcanic Eruptions. Long Term Prediction. Identify volcanoes and the frequency and style of their eruptions (a geological problem). - PowerPoint PPT Presentation

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Page 1: Impact of eruptions

Impact of eruptions

Vo l c a noes

Prediction

Part II

Supervolcanoes

Volcanoes in space

Page 2: Impact of eruptions

Prediction of Volcanic Eruptions

Identify volcanoes and the frequency and style of their eruptions (a geological problem).

Long Term Prediction

Establish the level of risk based on historic and geologic record.

Establish probabilities of eruption, style and location for individual volcanoes.

E.g., for individual volcanoes: determine most likely routes for lahars, nuees ardentes, lava flows, etc., and avoid construction in those areas.

Page 3: Impact of eruptions

Hazard zones have been distinguished around Mt. Shasta based on topography and past experience with eruptions.

Zone 1: areas likely to be affected most frequently. Most future flows from summit eruptions probably would stay within this zone.

Zone 1

Page 4: Impact of eruptions

Hazard zones have been distinguished around Mt. Shasta based on topography and past experience with eruptions.

Zone 1: areas likely to be affected most frequently. Most future flows from summit eruptions probably would stay within this zone.

Zone 2: areas likely to be affected by lava flows erupted from vents on the flank of the volcano or that move into zone 2 from zone 1.

Zone 2

Page 5: Impact of eruptions

Hazard zones have been distinguished around Mt. Shasta based on topography and past experience with eruptions.

Zone 2: areas likely to be affected by lava flows erupted from vents on the flank of the volcano or that move into zone 2 from zone 1.

Zone 1: areas likely to be affected most frequently. Most future flows from summit eruptions probably would stay within this zone.

Zone 3: areas likely to be affected infrequently and then only by long lava flows that originate at vents in zones 1 and 2

Zone 3

Page 6: Impact of eruptions

Short-term prediction

Based on the recognition of a pattern of events prior to previous eruptions.

Gas emissions: rates of emission and type of gas changes in some volcanoes.

Important gases include sulfur dioxide (SO2) and carbon dioxide (CO2)

Changes in concentration may reflect movement of the magma up the vent.

Page 7: Impact of eruptions

Surface tilting: recognition of changes in the land surface due to building pressure in the conduit.

A surface bulge appeared on Mt. St. Helens prior to its eruption.

April 26 May 2

April 8, 1980

Page 8: Impact of eruptions

Earthquakes: generated as the magma moves up the feeder conduit to the vent.

When viscous magma becomes stuck in the conduit strain energy builds as more magma tries to push out.

Movement takes place in a series of “jerks” as the rock material breaks. Each “jerk” produces an earthquake.

Magnitudes generally less than 5 M.

The more earthquakes the further the magma has moved.

Page 9: Impact of eruptions

Mount Spurr, Alaska:The 1992 Eruption of Crater Peak Vent

USGS

Black bars: earthquake frequency.

Red lines: volcanic eruptions.

Page 10: Impact of eruptions

A combination of approaches is likely the key to short-term prediction.

Page 11: Impact of eruptions

The impact of volcanic eruptions

Page 12: Impact of eruptions

Volcanic Hazards

Damage limited to the vicinity in the immediate area of the volcano.

Lava flows 

Commonly destroy property in Hawaii and Iceland.

Fatalities rare due to slow speed of advancing lava flow.

Page 13: Impact of eruptions

Ash fall

Extensive property damage and fatalities can result from heavy ash falls.

Significant ash in the upper atmosphere can circle the globe in a matter of weeks.

Mt. St. Helens’ ash cloud

More than 80 commercial jets have been damaged by flying through volcanic ash clouds.

Page 14: Impact of eruptions

An ashfall 10 million years ago killed these rhinos that are preserved at Ashfall Fossil Beds State Historic Park, Nebraska.

Death was not by burial but by lung failure due to inhaling the ash.

Page 15: Impact of eruptions

Pyroclastic flows

Lahars can also dam rivers and which can lead to extensive flooding.

Lahars are fast moving mudflows that can inundate urban areas that are nearby the eruption.

Page 16: Impact of eruptions

Lahars can be the most devastating outcome of many volcanoes.

Water and debris rushed down the slopes, picking up more debris along the way.

A relatively small eruption of Nevada del Ruiz, Columbia, in 1985, generated a lahar when the volcano melted a 2.5 km2 area of snow and ice.

Page 17: Impact of eruptions

A 5 metre wall of water and debris slammed into the town of Amero, 72 km from the volcano.

The lahar killed 28,700 people and destroyed over 5,000 structures in the city.

Page 18: Impact of eruptions

Nuée ardentes destroy life and property in their paths.

60 people, thousands of animals and fish, and hundreds of acres of lumber were destroyed by ash flows from Mt. St. Helens.

A Nuée Ardent killed 20,000 people when Mt. Vesuvius exploded and shed a pyroclastic flow across the village of Pompeii in 79 AD.

Page 19: Impact of eruptions

People and animals died instantly from the rushing cloud of hot gas and ash.

Page 20: Impact of eruptions

Landslides

Landslides can be generated when a volcano collapses during an eruption.

During the Mt. St. Helens eruption 2.3 km3 of debris slid down the mountain at speeds up to 240 km/hr.

The slide traveled over 24 km and left a 45 m deep deposit.

350,000 years ago Mt. Shasta experienced a similar eruption and landslide that was 20 times greater than that of Mt. St. Helens.

Page 21: Impact of eruptions

Volcanic Gases

In addition to making magma more explosive, volcanic eruptions also include gases that can be deadly to all life.

CO2, SO2 and CO are the most abundant of harmful gases.

Page 22: Impact of eruptions

Volcanoes release more than 130 to 230 million tonnes of CO2 into the atmosphere every year

Humans add CO2 at the rate of approximately 22 billion tonnes per year (150 times the rate of volcanic production)

Human CO2 production is equal to that if 17,000 volcanoes like Kilauea were erupting every year.

SO2 emissions can have direct effects on life in the vicinity of a volcano.

An eruption in 1783 of Laki Crater (Iceland) produced a sulfurous haze that lasted for 9 months and killed 75% of all livestock and 24% of the Icelandic population.

Page 23: Impact of eruptions

Mammoth Mountain is a relatively young volcano that is emitting large volumes of CO2.

Gas concentrations in the soil in some areas near the mountain are high enough to kill trees and small animals.

Page 24: Impact of eruptions

If the air that we breath has more than 10% CO2 it becomes deadly because it displaces the Oxygen that we need for respiration.

Lake Nios, Cameroon, is a very deep lake within a volcanic crater.

The lake is so deep that hydrostatic pressure forces CO2 to remain at the lake bottom.

When the pressure of the CO2 exceeds a certain limit the gas rapidly bubbles up out of the lake and flows as an invisible gas cloud down the adjacent slopes.

On August 61, 1986 such a gas release flowed 19 km suffocating 1,700 people along its route.

Page 25: Impact of eruptions

The fountain in the background lifts CO2 up to the surface so that it no longer accumulates.

Lake Nyos 10 days after the 1986 eruption

Page 26: Impact of eruptions

Tsunamis

Caused by the displacement of seawater by eruptions of volcanic islands and submarine volcanoes.

Krakatoa (1883 eruption) killed 36,000 people by the tsunami, alone (the most deadly outcome of the eruption).

This is the newly forming summit of Krakatoa, growing where the 1883 eruption blew the top off of the original volcano.

Page 27: Impact of eruptions

Global Climate Change

Due to ash and gas that may spend years in the upper atmosphere; reduces incoming solar radiation.

SO2 from an eruption forms tiny droplets of sulfuric acid

in the upper atmosphere.

The droplets significantly increase global albedo…..a negative radiative forcing that leads to cooling.

Mt. Pinatubo (1991) released 22 million metric tons of SO2 and reduced the Earth’s average temperature by 0.5 degrees Celsius in the year following the eruption.

Page 28: Impact of eruptions

Tambora (1815 eruption) was followed in 1816 by the “year without a summer”.

Average global temperature is estimated to have been reduced by 3 degrees Celsius.

A series of eruptions of Tambora (Indonesia) extruded up to 150 km3 of magma (solid equivalent), much of it into the atmosphere.

Page 29: Impact of eruptions

Food shortages and starvation are attributed to the deaths of 80,000 people.

In June of 1816 there was widespread snowfall throughout the eastern United States.

The normal growing season experienced repeated frosts as cold air extended much more southerly than normal.

The global population was about 1 billion people in 1816.

Our current population is a little over 6 billion.

The 1816 fatality rate would have resulted in a death toll of nearly 500,000 people due to starvation.

Page 30: Impact of eruptions

Approximately 260,000 people have been killed by volcanoes in historic times…most by a handful of individual eruptions.

Page 31: Impact of eruptions

Volcanic Explosivity Index

Page 32: Impact of eruptions

http://pubs.usgs.gov/publications/msh/comparisons.html

Page 33: Impact of eruptions

Deadly Historic Volcanic Eruptions

A stratovolcano along the Caribbean trench.

Mt. Pelée(West Indes)

VEI = 4

Page 34: Impact of eruptions

Lava domes are constructed of viscous lava and are prone to collapse, unleashing a violent pyroclastic flow.

An eruption in 1902 following the growth of a lava dome on the side of the mountain.

Page 35: Impact of eruptions
Page 36: Impact of eruptions

The nuée ardente that was generated when Mt. Pelée erupted swept 6 km downslope through the town of St. Vincent.

Page 37: Impact of eruptions

Almost the entire population of 30,000 people were killed within minutes of inhaling the hot gases and ash.

There were only two survivors; one was in a dungeon!

Page 38: Impact of eruptions

Tambora (1815) VEI = 7

The largest eruption of historic time.

Greatest impacts from pyroclastic flows and ash and gas eruptions.

Approximately 150 km3 of ash was erupted with the explosions.

10,000 people were killed by bomb impacts, tephra falls and pyroclastic flows.

By far the largest impact was on the Earth’s atmosphere.

The eruption plume reached 44 km above the earth, loading the stratosphere with ashes and gases.

Page 39: Impact of eruptions

The concentration mercury in ice cores from glaciers in Wyoming record a peak in atmospheric mercury that corresponds to the Tambora eruption.

The atmospheric impact caused the “year without a summer” along with 80,000 deaths due to famine and disease.

Page 40: Impact of eruptions

Krakatoa (1883)

On the Island of Rakata, Krakatoa was one of 130 active volcanoes in Indonesia (the country with the most active volcanoes in the world).

The volcano had been inactive for almost 200 years prior to a series of small eruptions that began in 1883.

VEI = 6

Page 41: Impact of eruptions

The volcanoes of Indonesia are due to the northeastward subduction of the Indo-Australian plate beneath the Eurasian plate.

Stratovolcanoes with a high probability of violent eruption.

Page 42: Impact of eruptions

Krakatoa began its eruptive stage on May 20, 1883 immediately following a strong earthquake (no sensors were there to measure it).

The first explosions were heard 160 km away and sent steam and ash upwards to a height of 11 km.

By August 11 three vents were active on the volcano.

On August 26 several loud eruptions took place over the course of the day sending dust and ash to over 25 km elevation into the atmosphere.

Page 43: Impact of eruptions

On August 27, four very large eruptions began at 5:30 am.

The last of the four was the largest and could be heard from Sri Lanka to Australia, up to 4,600 km from the volcano.

A 23 km2 area of the island was gone following the fourth eruption.

Page 44: Impact of eruptions

The caldera collapsed with the explosion, from an original height of 450m above sea level to 250m below sea level.

The pyroclastic flow was experienced at sea as far as 80 km away.

Ships experienced hurricane force winds loaded with tephra and smelling strongly of Sulfur.

An estimated 4,500 people died from the direct effects of the blast.

The blast itself is thought to have ejected 20 km3 of tephra.

Burn-related fatalities were recorded up to 40 km away from the blast.

Page 45: Impact of eruptions

The collapse of the caldera, combined with the explosion, generated a massive tsunami with a maximum height at landfall of 45 m.

Coral blocks up to 600 tons were washed ashore.

The impact was greatest on the nearby islands.

This steamship was carried almost 2 km onto the land and dropped 10 m above sea level.

Page 46: Impact of eruptions

Along low lying coasts of Java the waves washed 8 km onshore, dragging people along with them as they washed back to sea.

An estimated 36,417 people were killed by the tsunami alone.

The tsunami was recorded as a small rise in sea level as far away as the California coast (20 hours after the fourth blast).

Ash from the volcano fell to Earth as far away as 2,500 km downwind over the days following the eruption.

Ash and gases in the upper atmosphere led to a lowering of global temperature by several degrees.

Page 47: Impact of eruptions

But, there’s a little more to this story…..

Anak Krakatoa (child of Krakatoa) has grown through ongoing volcanism where Krakatoa had existed.

It’s undergoing a constructive phase of mild strombolian and vulcanian eruptions.

Page 48: Impact of eruptions

Catastrophe: An Investigation into the Origins of the Modern World, by David Keys, investigates the role of extreme climate change in a series of events in human history over the 6th and 7th centuries AD.

Could Krakatoa have been the cause of humanity’s descent into the Dark Ages?

The fall of ancient super cities.

The sharp decline of ancient civilizations: Persia, Indonesia, the Nasca culture of South America, and southern Arabian civilizations.

The breakup of the Roman Empire and the formation of many nation states.

Restructuring that led to a new united China.

Page 49: Impact of eruptions

These events all appear to be linked to a major climatic change that took place in 535 AD.

This was also the first time that the Bubonic Plague spread through much of the known world.

This epidemic had hit Alexandria in 541 AD after spreading from east Africa.

The disease is believed to have killed 900,000 people over a 100 year period.

A written description of the time describes a major atmospheric event:

“The Sun became dark, and its darkness lasted for about 18 months. Each day, it shawn for about four hours and still this light was only a feeble shadow.”…. John of Ephesis

Page 50: Impact of eruptions

Keys suggested that a major impact of an asteroid or comet or a major volcanic eruption might have accounted for the global climate change that led to the onset of the dark ages.

No major impact structures are known to have formed over the required time so investigations focused on a volcanic eruption.

Ken Wohletz of the Los Alamos National Laboratory took on a collaboration to try to find a volcanic source of such a major eruption.

He summarizes some of his ideas at:

http://www.ees1.lanl.gov/Wohletz/Krakatau.htm

Historical evidence of calamity in both the northern and southern hemispheres suggested a near-equator eruption and his search focused on Indonesia, a major volcanic hot-spot.

Page 51: Impact of eruptions

Wohletz’s work identified thick pyroclastic deposits in Indonesia, near Krakatoa, that were dated to be about 1500 years old.

Further investigation showed a possible volcanic caldera where Krakatoa now resides.

Page 52: Impact of eruptions

Wohletz describes in some detail a hypothetical eruption of Krakatoa that would have produced such a caldera.

Page 53: Impact of eruptions

As the volcano begins to erupt the Sunda Straits do not exist as the land had been built up by volcanic activity over thousands of years.

Page 54: Impact of eruptions

The onset of eruption was only of steam due to water entering the vent(s), blowing rocks and ash upward with it.

Phreatic eruptions are due to the boiling of groundwater by heat due to the magma chamber as magma slowly rose towards the surface.

Page 55: Impact of eruptions

Once at the surface the 900 degree Celcius magma, charged with gas and water vapor would cause an ultraplinean (very explosive) eruption.

Material would be ejected at a rate of 100 to 1000 million kg/second, much of it falling in the vicinity, the remainder rising into the stratosphere where it would travel around the world.

Page 56: Impact of eruptions

With the ultra plinean eruption the caldera would form as it collapsed and seawater would rush into the magma vent.

Water would flash into vapor causing a giant phreatic eruption to eject debris and vapor upwards and cause pyroclastic flows across the ground.

Page 57: Impact of eruptions
Page 58: Impact of eruptions

The collapse of such a caldera would involve the eruption of 200 km3 of magma; about 75 km3 of ash would be injected into the atmosphere.

The model suggests that the Earth would have cooled by 5 to 10 degrees Celsius for a period of 10 to 20 years.

In addition, another 150 km3 of water would be ejected as 200,000 km3 of water vapor, much of which would remain for some time in the upper atmosphere as ice crystals (increasing global albedo).

Page 59: Impact of eruptions

Such an event would:

Cause crop-failure world-wide.

Modify weather patterns extensively.

Result in poor nutrition that would increase risk to disease.

Decrease populations and lead to political stress that would result in extensive social change.

Possibly leading to the Dark Ages.

Page 60: Impact of eruptions

Super Volcanoes

While not defined officially, lets say any eruption that ejects 1000 km3 or more of pyroclastic material (i.e., VEI 8 or more).

According to M.R. Rampino super eruptions take place, on average, every 50,000 years. Three of the best known eruptions are compared below.

Page 61: Impact of eruptions

Toba: the world’s largest Quaternary caldera.

The Australian Plate is subducting beneath the Eurasian plate at a rate of 6.7 cm/yr.

Page 62: Impact of eruptions

Today Toba is a caldera or depression that is occupied by Lake Toba.

It is 100 km long and 30 km wide.

Toba last erupted about 75,000 years ago with the largest eruption of the last 2 million years.

Page 63: Impact of eruptions

840,000 years ago

500,000 years ago

Three eruptive events have been recognized.

74,000 years ago

Each producing a caldera.

Samosir Island, rising 750 m above the lake, is a dome built from lava following the last eruption.

Page 64: Impact of eruptions

The eruption ejected 2,800 cubic km of material and the pyroclastic flows covered an area of at least 20,000 square km.

In the immediate vicinity of the volcano ash deposits reach 600 metres in thickness

Ash fall from the eruption covers an area of at least 4 million square km; half the area of the continental United States.

Global cooling is estimated at between 3 and 5 degrees Celsius with regional cooling of 15 degrees C.

Tropical plant life would have been all but eliminated

Temperate forests would loose 50% of all trees.

Page 65: Impact of eruptions

It is estimated that the growing population of homo sapiens (i.e., us) was reduced from 100,000 individuals to as few as 3,000 individuals (97% of all humans were lost!).

This reduction had been estimated for approximately the time of Toba’s eruption on the basis of genetic studies and is termed the “human population bottleneck”.

Page 66: Impact of eruptions

Yellowstone Caldera

Known for its hot springs and geysers, Yellowstone National Park, is likely the most popular super volcano in the world.

The park sits on an active caldera that rises and sinks in response to magma movement and pressure fluctuations within the Earth.

Over recent years the surface has risen by as much as a metre and sunk back by 1/3 of a metre.

Thousands of small earthquakes are produced as earth surface moves.

Page 67: Impact of eruptions

The magma chamber is only 5 to 13 km below the land surface.

The caldera is 80 km long and 50 km wide.

Page 68: Impact of eruptions

The caldera and its magma chamber are due to a hot spot in the mantle that has moved several hundred kilometres over the past 12.5 million years.

The movement is due to the drift of the north American continent over the hot spot.

Ancient, inactive calderas mark the path of the hot spot.

Page 69: Impact of eruptions

The current caldera was formed with an eruption 640,000 years ago (the Lava Creek Eruption).

This eruption ejected 1,000 km3 of pyroclastic debris.

An earlier eruption (the Huckleberry Ridge Eruption, 2 million years ago) ejected 2,500 km3

of pyroclastic debris.

A smaller eruption happened 1.3 million years ago, releasing 280 km3 of debris.

Page 70: Impact of eruptions

Eruptions appear to have a 600,000 year period (that long between eruptions) so we’re overdue for another one.

Previous eruptions spread ash over thousands of km2 across the US.

Page 71: Impact of eruptions

Heightened monitoring of the Yellowstone Caldera in recent years has led to media concern of an impending eruption.

Government officials and geologists indicate that there have been no clear indicators of high risk at this time.

If such an eruption were to take place, North America and the rest of the world could experience another “Dark Ages”.

Page 72: Impact of eruptions

Volcanoes in Space

NASA

Page 73: Impact of eruptions

Venus has over 100,000 shield volcanoes.

Anemone 1

40 kmhttp://volcano.und.edu/vwdocs/planet_volcano/venus

Sapas Mons

120 km

Page 74: Impact of eruptions

Volcanoes on mars: giant volcanoes are present, far larger than anything on Earth.

Mars

Page 75: Impact of eruptions

Ceraunius Tholus and Uranius Tholus

Page 76: Impact of eruptions

Craters on the volcanoes suggest that they may not have been active for millions of years.

Page 77: Impact of eruptions

Olympus Mons: 24 km high, 500 km across, with a 6 km high cliff at its base.

Page 78: Impact of eruptions

Not erupting at present but it may still erupt in future.

Page 79: Impact of eruptions
Page 80: Impact of eruptions

Olympus Mons is thought to be located over a hot spot but the crust is stationary so that it grew to greater size than any Earth volcano.

Page 81: Impact of eruptions

Volcanoes on Io (a moon of Jupiter)

Page 82: Impact of eruptions
Page 83: Impact of eruptions
Page 84: Impact of eruptions

Volcano Prometheus

Volcano Pele

Page 85: Impact of eruptions

Babbar Patera Volcano (300 km across)