Shelf Life 18: Under the Volcanoes
SHELF LIFE 18 - Under the Volcanoes
[HAUNTING STRINGS FROM TCHAIKOVSKY’S NUTCRACKER]
[An animated sequence combining paintings and mosaics from ancient Roman Pompeii—people stand in a city as the volcano, Mt. Vesuvius erupts in the background.]
JIM WEBSTER (Curator, Division of Physical Sciences): Probably one of the most classic eruptions in human history was the eruption of Mt. Vesuvius in 79 A.D.
[VOLCANIC RUMBLE AND EXPLOSION]
[Painting of a Roman family talking, surrounded by fragments of ancient Roman letters. Text reads, “From the letters of Pliny the Younger.”]
VOICE OF PLINY THE YOUNGER: We had scarcely sat down to rest when darkness fell—
[The scene darkens and paintings of people running in fear and pleading for assistance dissolve before a smoldering volcano in the background.
VOICE OF PLINY THE YOUNGER: —not the dark of a moonless or cloudy night, but as if the lamp had been put out in a closed room.
[EXHALED BREATH, AS IF BLOWING OUT A CANDLE]
[The scene darkens further. Only Vesuvius and wisps of smoke can be seen.]
VOICE OF PLINY THE YOUNGER: It grew lighter, though that seemed not a return of day, but a sign that the fire was approaching.
[The scene grows brighter, and buildings in ruins appear. Flames burn low amid the rubble.]
VOICE OF PLINY THE YOUNGER: At last, the cloud thinned out.
[WIND BLOWS, ASH SETTLES]
[Clouds of ash swirl around, revealing the twisted forms of unfortunate victims trapped beneath the lava and ash from Vesuvius’s eruption.]
VOICE OF PLINY THE YOUNGER: The sight that met our still terrified eyes was a changed world, buried in ash like snow.
[Ash cloud blows away, transitioning from the animated sequence to a shot of Curator Jim Webster holding a volcanic sample in the collections at the American Museum of Natural History.]
WEBSTER: My name is Jim Webster and I’m a curator here at the American Museum. I’m the curator of mineral deposits, but it also bridges into volcanology.
[TWINKLING MUSIC PLAYS]
[Shelf Life animated title sequence. Specimens and artifacts from the Museum’s collections fade in and out.]
[CELLO MUSIC PLAYS]
[A montage of photos featuring Webster and volcanic sites around the world.]
WEBSTER: Since I’ve been at the Museum, about 28 years now, I’ve been fortunate. I’ve visited at least several dozen volcanoes around the Earth. But I’ve focused most of my research attention on two particular volcanoes—
[Webster looks out over the crater of Mt. Vesuvius.]
WEBSTER: Mt. Vesuvius, Italy and…
[Smoke comes out the top of a snow covered volcanic island.]
WEBSTER: …Augustine volcano in Alaska.
[WAVES CRASH, GULLS CRY, CHURCH BELLS RING]
[Aerial view of Naples and the surrounding area. Mt. Vesuvius looms over the bay in the background.]
WEBSTER: Mt. Vesuvius is along the Bay of Naples.
[Old newspaper front page showing Vesuvius, with headline reading, “Vesuvius Grows More Violent After a Brief Lull.”]
[SOUNDS OF VOLCANIC ERUPTIONS]
WEBSTER: It has erupted roughly 20 times…
[Various historical images of Mt. Vesuvius.]
WEBSTER: …since the last huge eruption in 79 AD.
[Curator Jim Webster sits in Experimental Petrology Lab.]
WEBSTER: The last eruption of Mt. Vesuvius was at the end of World War II.
[Archival black and white film newsreel features a smoking Mt. Vesuvius.]
NEWSREEL NARRATOR: Up from the crater of 4,000-foot-high Mount Vesuvius rise towering clouds of smoke and volcanic ash.
[American soldiers shield their faces from the smoke and ash in the archival footage.]
[Modern-day scene of people and motorcycles in a crowded Naples street.]
WEBSTER: Now, Naples and the surrounding areas have two to three million inhabitants.
[Time lapse over the Bay of Naples as the sun sets, and street lights turn on.]
WEBSTER: Probably 600,000 live within what’s called the Red Zone, the danger zone.
[The scene transitions to a helicopter flying towards an isolated volcanic island.]
[WHIR OF HELICOPTER ROTORS]
WEBSTER: Augustine volcano is actually a volcanic island.
[Wildflowers bloom at the base of Augustine volcano.]
WEBSTER: It’s located up away from populations, in Alaska.
[Wide shot of Anchorage airport with snowy mountains in the background.]
WEBSTER: It is about 200 or so kilometers from Anchorage…
[Clouds of smoke pour out of Mt. Augustine.]
WEBSTER: …and Augustine is the most active volcano in the eastern Aleutian chain.
[Montage of archival images of Augustine erupting in different decades.]
WEBSTER: It’s erupted seven times in the last 200 years. Most recently in 2005, 2006.
[FAR-OFF EXPLOSION]
[Archival images animated with subtle movement—a seaplane lands on Augustine’s island. Webster and colleagues deplane and sample the volcanic slopes for specimens.]
WEBSTER: And fortunately, I and a colleague here were able to go and do sampling in the summer after that eruption settled down.
[Webster stands in front of collections cabinet and indicates the specimens in drawers.]
WEBSTER: All of these drawers are full of Augustine samples.
[Close up of volcanic samples in drawer. Webster’s hand opens drawer, and looks at specimen label. Label reads, “Vessicular olive green porphyritic andesite from Windy Pyroclastic Flow…Location: Augustine Island.”]
WEBSTER: What we want to do to actually understand nature is to begin, really, with natural materials.
[Close up of Webster’s hands holding a large rock sample.]
WEBSTER: So, this is a volcanic rock from Augustine.
[Wider shot of Webster holding the rock in his Experimental Petrology Lab.]
WEBSTER: There are dark and light crystals. So, these are minerals that crystallize out of the liquid rock.
[Animated sequence—crystal-like shapes grow larger in size.]
WEBSTER: Sometimes, as these crystals grow, they may trap some of the molten rock inside of them.
[Camera zooms into one of the crystal-like shapes to show a microscopic image of a “bubble” trapped inside. Text reads, “Molten rock,” and a line is drawn to the bubble.]
SHUO DING (Postdoctoral Fellow, Division of Physical Sciences): The good part is it can preserve the information exactly when that melt was trapped.
[The camera zooms in even further and animated text appears, indicating various temperatures, pressures, and compositions, e.g., “2.2 wt% F” and “200 MPa.”]
[Animated circles appear, representing composition pressure, and temperature. The circles appear in various combinations and are labeled with different temperature, pressure, and composition information.]
DING: So, we can know what kind of compositions and combinations of pressure and temperature relate to certain types of eruptions.
[The animated circles form into the shape of an erupting volcano.]
[Researcher Shuo Ding stands in the Experimental Petrology Lab, holding a gold capsule used in her experiments.]
DING: My name is Shuo Ding. I’m a postdoc in the Museum, and my research is to investigate the pre-eruption stage of a volcano.
[Ding sits in the Experimental Petrology Lab.]
DING: By conducting experiments…
[Ding adjusts various levers and dials, as she runs an experimental trial in the Petrology Lab.]
DING: …we can compare our experimental results to the samples produced from historic eruptions.
[A hand pulls open a drawer of volcanic samples.]
DING: And if we know something about the composition and the conditions,
[An image of Mt. Augustine transitions into animated sequence where temperature, pressure, and composition circles combine with text (e.g., “785° C” and “180 MPa”).]
DING: …we can connect our study to what happens inside the Earth.
[Animated lava flows out over the frame, and then becomes the background for a world map. Dots on the map indicate possible volcanic eruption sites.]
DING: That might be able to help predicting eruptions.
[Archival footage—cross-section of a cylinder in a car engine, showing pumping piston.]
WEBSTER: We use expanding gases in an internally heated combustion engine to drive pistons…
[TIRES SQUEAL ON PAVEMENT]
[Archival footage of an old car driving out of frame.]
WEBSTER: …and move cars.
[Steam cloud.]
[STEAM HISS]
WEBSTER: We use expanding steam…
[Collage of steam cloud, churning turbine, and electrical power plant.]
WEBSTER: …in turbines to drive electricity.
[Archival footage of Mt. St. Helens volcanic eruption. Roiling clouds of ash.]
WEBSTER: And in volcanos, expanding gases drive explosive behavior. So, highly explosive magmas have higher gas content.
ARCHIVAL FILM NARRATOR: It seemed to happen in an instant. The whole top of the mountain—tons of ash, rock, and ice rocket into the stratosphere.
[Hand pops off the top of a seltzer bottle and bubbles rush to the top.]
WEBSTER: Just like when you pop the top on a bottle of seltzer water and the bubbles form.
[Webster sits in Experimental Petrology Lab.]
WEBSTER: But there’s another factor and this gets into the chemistry.
[Bright lava gushes in waves. The chemical symbol for oxygen animates on-screen.]
WEBSTER: The most abundant element in all magmas is oxygen.
[The chemical symbol for silicon animates on-screen.]
WEBSTER: The second most abundant is silicon.
[Webster sits in Experimental Petrology Lab. He is surrounded by animated chemical symbols for oxygen and silicon, which bounce around as if moving through something sticky.]
WEBSTER: The more silica and oxygen in the magma, the more viscous, sticky, thick that magma becomes.
[A circle of hot lava contains animated gas bubbles, which shake as they try to “escape.”]
WEBSTER: The more viscous the magma, the more difficult for it to release its gases.
[Hundreds of animated gas bubbles whizz past the camera.]
WEBSTER: So, if it’s gas charged, basically, there are billions and trillions of little tiny gas bubbles. Each one has an explosive force.
[The bubbles gather into one central circle that then explodes. Copies of the bubble dot the screen, and they all explode.]
WEBSTER: But there are so many that during the course of a single eruption,
[On the left of the screen is archival footage of a mushroom cloud from a nuclear explosion. Text reads, “Trinity Nuclear Test, 1945 - .02 megatons.” On the right of the screen is archival footage of an ash cloud erupting from a volcano. Text reads, “Mount St. Helens, 1980 – 24 megatons.”]
WEBSTER: …huge amounts of energy can be released during these eruptions.
[Still image of Augustine erupting.]
WEBSTER: And both Augustine volcano in Alaska…
[Archival image of WWII planes flying near the erupting Mt. Vesuvius.]
WEBSTER: …and Mt. Vesuvius in Italy,
[Webster sits in Experimental Petrology Lab.]
WEBSTER: …they’re both very gas-charged magmas.
[Animated graphic compares Vesuvius and Augustine. Photo on the left shows Vesuvius, and on the right is Augustine. The two volcanoes are silhouetted with an animated line, and text labels each volcano—“Vesuvius” and “Augustine.”]
WEBSTER: But there’s something different between Vesuvius and Mt. Augustine.
[The Vesuvius graphic grows larger in size to take up the screen. The chemical symbols for sodium and potassium animate on.]
WEBSTER: Vesuvius is higher in sodium and potassium.
[The chemical symbols disappear and the volcano’s outline is filled with animated yellow circles, representing magma.]
WEBSTER: The more sodium and potassium that’s inside a magma,
[Small blue and pink circles with the chemical symbols of sodium and potassium, respectively, grow between the yellow magma circles. As they grow they push the yellow circles apart.]
WEBSTER: …it tends to break up that structure. It weakens the magma.
[The silhouette of Vesuvius retreats to the left of the screen, and Augustine’s silhouette re-appears on the right. Both contain boxes containing the chemical symbol for sodium and potassium, but Vesuvius has many more of them.]
WEBSTER: So, more in Vesuvius, less in Augustine and they actually have very different eruptive histories—
[Timelines of Augustine and Vesuvius’s eruptive histories unfold. Text reads: “Augustine – 1812, 1883-1884, 1935, 1963-1964, 1971, 1976, 1986, 2005-2006” and “Vesuvius – 1822, 1872, 1906, 1944.”]
WEBSTER: Augustine, the last 200 years it’s been every 10, 20, 30 years there’s been an eruption. Whereas at Vesuvius, it’s been very different.
[Webster sits in Experimental Petrology Lab.]
WEBSTER: So, for a rock sample from a given eruption,
[Image of Mt. Augustine erupting in 2006.]
WEBSTER: …say the 2006 eruption,
[Microscopic images of volcanic samples.]
WEBSTER: …we can analyze its chemistry,
[Webster sits in Experimental Petrology Lab.]
WEBSTER: …but then we need data to compare that to. And that’s what we do here in the lab.
[Ding sits in Experimental Petrology Lab.]
DING: I cook my rock.
[Ding surveys equipment as she begins an experimental run in the lab. Various gauges and digital readouts are shown.]
[WHOOSH OF AIR FROM COMPRESSOR]
DING: My experiment is mainly to replicate the conditions inside the Earth like 10 kilometers depth at the pre-eruption stage.
[Webster sits in Experimental Petrology Lab.]
WEBSTER: We’ll take a powdered material of some- either natural rock or a synthetic equivalent,
[Close up as gloved hands use a specialized scoop to put powder into a gold capsule.]
WEBSTER: …and we’ll put them in a little capsule of gold.
[Tweezers place a gold capsule onto a scale.]
WEBSTER: We use gold because it’s relatively chemically inert.
[Hands add water to gold capsule with pipette.]
WEBSTER: We’ll add water.
[Close up of bottle with label reading “oxalic acid.”]
WEBSTER: We’ll add carbon dioxide.
[Close up of bottle labeled “NKH-1 + sulfur.”]
WEBSTER: We’ll add sulfur,
[Close up of gloved hands adding solution to gold capsule with pipette.]
WEBSTER: …and we’ll add chlorine or fluorine in some form.
[Close up of gloved hands using pliers to seal gold capsule.]
DING: And I seal it to make sure nothing escapes.
[Ding welds the gold capsule shut while viewing it through a microscope.]
[Ding loads the gold capsule into a larger metal cylinder, then inserts the cylinder into a larger, also cylindrical machine—the “bomb.”]
DING: And then I put my capsule in one of these bombs. The bomb is like a pressure pot.
[Hands tighten a fastener on the bomb with a socket wrench.]
DING: You put things inside and…
[Ding makes adjustments to her experiment on a touch pad, and then turns a lever controlling pressure levels.]
DING: …pressurize it and heat it.
[Numbers on a digital readout tick up to 800 degrees Celsius.]
DING: I run all my runs at 800 degrees C. It’s hot enough to…
[Ding sits in Experimental Petrology Lab.]
DING: …melt the rock I’m using, but not hot enough to melt my capsule.
[Webster makes notes in the Experimental Petrology Lab.]
WEBSTER: And then let it sit and cook typically days to weeks, sometimes.
[Webster sits in the Experimental Petrology Lab.]
WEBSTER: It might be a month for a given experiment.
[Ding pulls the metal cylinder containing her gold capsule out of the bomb.]
DING: And then turn off the heat, let it quench to a rock again.
[Ding carefully pulls out the gold capsule from the cylinder on her lab bench.]
DING: I will analyze it, analyze the composition and then…
[Ding examines a sample under a microscope.]
DING: …we can compare the composition of the rocks…
[Close up of volcanic specimens from the Museum’s collection.]
DING: …from historic eruptions…
[Ding flips through the pages of her lab notebook.]
DING: …to my experimental results…
[Ding sits in Experimental Petrology Lab.]
DING: …to see at what condition that natural sample was produced.
[Archival footage of erupting Mt. Vesuvius.]
WEBSTER: Mt Vesuvius was on a 40, 50-year cycle.
[Webster sits in Experimental Petrology Lab.]
WEBSTER: So, the issue now—because it’s been almost 75 years—
[Satellite view of Vesuvius and surrounding city of Naples.]
WEBSTER: —is Vesuvius going into a resting period where potentially the next big eruption might be a huge eruption. Or is it just running a little bit late?
[Webster sits in Experimental Petrology Lab.]
WEBSTER: We’re putting all this together. And I think we’ll have a really good chance, you know, from one explosively erupting volcano to another,
[Painting of Vesuvius from ancient Roman home in Pompeii.]
WEBSTER: …to understand prior eruptions…
[Roman fresco dissolves into image of Vesuvius looming over the Bay of Naples. A satellite map of Italy is ghosted in the background, and animated circles radiate out from the volcano’s area, giving a sense of urgency.]
WEBSTER: …and hopefully forecast future activities.
[PLUCKING STRINGS]
[Production credits roll.]
“If we connect compositions and combinations [of pressure and temperature] to what happens inside the Earth, that might be able to help predict eruptions.”
Shuo Ding, Kalbfleisch Postdoctoral Fellow, Department of Earth and Planetary Sciences
Researchers are trying to uncover the secret “ingredients” behind dangerous eruptions. Expeditions to Mt. Vesuvius—one of the world’s best-known volcanoes—and Alaska’s Mt. Saint Augustine provide specimens that can be compared to materials synthesized in the lab. Understanding what makes one volcano’s magma so much more explosive than another may one day help us avoid volcanic disasters.
Two volcanoes loom large in Jim Webster’s research. Webster, the Museum’s curator of mineral deposits, studies both Mount Vesuvius, Italy—the site of one of the world’s most famous eruptions—and the lesser-known Mount Saint Augustine in Alaska. In 2006, only a few months after an eruption of Augustine, he flew with a small team of geologists to this remote volcanic island in the Aleutian chain. Every morning, they would load into a helicopter and be dropped off at a location on the volcano’s slopes. They’d work their way down, collecting samples along the way. “Hot rocks would occasionally come tumbling down the side of the volcano,” says Webster.
J. Webster/© AMNH
J. Webster/© AMNH
Webster brought some of those rocks back to New York, where he compares them to samples collected at Vesuvius and to artificial materials he synthesizes in his experimental petrology lab. Mt. Saint Augustine and Mt. Vesuvius have several things in common: they’re both young in geologic terms—less than 200,000 years old; they both have magmas rich in volatiles like water, carbon dioxide, sulfur, and chlorine; and both erupt gases that are highly charged with carbon dioxide and water. But, the two volcanoes have very different eruptive cycles. Webster and Kalbfleisch Postdoctoral Fellow Shuo Ding are re-creating pre-eruptive conditions inside the lab and comparing their results to the natural volcanic samples in the hopes that one day we may understand how the different “ingredients” in magma can make one volcano more explosive than another.