Monday Geology Picture: Glass House Mountains, Australia

A shot of part of the stunning Glass House Mountains in Queensland, Australia. Photo taken April 2019.

I have been terribly neglecting my blog this year. However, I have a good excuse: over the past few months I have accepted a new job working as a geologist for Anglo American… and  I have moved my family to beautiful Brisbane, Australia. On top of that, I am mother to a young son (18 months old now) and I’m also studying part-time… so, I have my hands very full!

However, now that the chaos of moving is over, I thought I would revive my blog… once again! There is much new geology to see here in our new home country, so I’ll try to share some georneys (geology journeys!) here more regularly!

As a start, here is a picture of the majestic, magical Glass House Mountains in Queensland. These mountains are young (26-27 million year old) volcanic plugs. I’ll blog more about their geology soon! For now, enjoy this teaser shot.

Monday Geology Picture: Another View of Formica Leo Volcanic Crater

A closer view of the volcanic crater. Note the person for scale.

Last week I shared a picture of the beautiful and impressive Formica Leo, a volcanic crater located at the Piton de la Fournaise volcano on Réunion Island in the Indian Ocean. Last week’s picture showed the crater from a distance. You can just barely make out some small people in last week’s picture, to give you some sense of scale. However, I thought I would share a closer view of the crater this week. This picture, which was taken as we hiked around the rim of the crater, shows a person and gives you a sense that this crater is actually pretty large, if small compared to the overall volcano. The background also gives you a glimpse of the edge of the larger volcanic feature in which this small crater sits. You can see some lava flows on the cliffs in the background.

Stay tuned for more pictures and information from Réunion — there’s much interesting geology to share!

Monday Geology Picture: Formica Leo Volcanic Crater

A gorgeous volcanic crater known as “Formica Leo”. Note the people for scale – click to enlarge image.

Today I’m sharing a picture of the stunning Formica Leo (foreground), a volcanic crater located at the Piton de la Fournaise volcano on Réunion Island in the Indian Ocean. My husband and I hiked up this crater when we visited the island for a holiday last year. We also hiked up to the top of the volcanic hill in the distance — crossing over a number of lava flows of various ages. If you ever have the chance, I highly recommend a visit to Piton de la Fournaise — and to Réunion in general. We certainly plan to go back within the next couple of years.

Monday Geology Picture: Pahoehoe Lava Flow

Pahoehoe lava flow on Piton de la Fournaise volcano. Photo taken March 2017.

For this week’s “Monday Geology Picture” here’s a stunning example of a pahoehoe lava flow. I took this picture back in March when I visited Piton de la Fournaise volcano on Réunion Island. I’ll be sharing more pictures from Réunion soon – stay tuned!

Monday Geology Picture(s): Stunning Shots of Santorini

Santorini #1.
Santorini #1.

Last week I shared a lovely view of Santorini taken by my friends Patrick and Nia during their vacation back in June. This week I thought I’d share several more of their Santorini shots. Some of them are quite stunning. Enjoy!

When Patrick and Nia sent through these pictures to me, my husband commented:

Ah, a geologist’s nightmare. Photographs without scale! Except for the one with the boat… and the one with Nia…

Despite the lack of scale in some of them, these photographs are still pretty neat! If you are familiar with Santorini geology, please feel free to point out notable features. There are some great volcanic rocks in these pictures!

Santorini #2.
Santorini #2, with sailboat for scale.
Santorini #3.
Santorini #3.
Santorini #4.
Santorini #4, with some houses for scale.
Santorini #5.
Santorini #5, with Nia for scale.
Santorini #6.
Santorini #6.
Santorini #7.
Santorini #7.
Santorini #9.
Santorini #8, with some beach visitors for scale.
Santorini #9.
Santorini #9, with flag and a building for scale.

Monday Geology Picture: Scenic Santorini

Beautiful Santorini.
Beautiful Santorini. The boats are travelling across an enormous, water-filled volcanic caldera.

Courtesy of my friends Patrick and Nia, here is a lovely picture of Santorini, a Greek island that is a the remnant of a volcanic caldera. Patrick and Nia were on vacation in Greece back in June. I’ll share a few more of their Santorini pictures for next week’s “Monday Geology Picture” post.

A Geology Song: Pompeii by Bastille

One of my favorite new songs is “Pompeii” by the UK band Bastille. I’m not sure how popular this song is in the USA, but in the UK and also here in South Africa it’s quite popular at the moment. If you haven’t heard the song yet, please take a listen.

The song has a geological theme and makes reference to the famous eruption of Mt. Vesuvius in AD 79, which destroyed and buried the Roman cities of Pompeii and Herculaneum. Here are the lyrics:

I was left to my own devices
Many days fell away with nothing to show

And the walls kept tumbling down
In the city that we love
Great clouds roll over the hills
Bringing darkness from above

But if you close your eyes,
Does it almost feel like
Nothing changed at all?
And if you close your eyes,
Does it almost feel like
You’ve been here before?
How am I gonna be an optimist about this?
How am I gonna be an optimist about this?

We were caught up and lost in all of our vices
In your pose as the dust settles around us

And the walls kept tumbling down
In the city that we love
Great clouds roll over the hills
Bringing darkness from above

But if you close your eyes,
Does it almost feel like
Nothing changed at all?
And if you close your eyes,
Does it almost feel like
You’ve been here before?
How am I gonna be an optimist about this?
How am I gonna be an optimist about this?
If you close your eyes

Oh where do we begin?
The rubble or our sins?
Oh where do we begin?
The rubble or our sins?

And the walls kept tumbling down
In the city that we love
Great clouds roll over the hills
Bringing darkness from above

But if you close your eyes,
Does it almost feel like
Nothing changed at all?
And if you close your eyes,
Does it almost feel like
You’ve been here before?
How am I gonna be an optimist about this?
How am I gonna be an optimist about this?

I really like this song. The music is nice, and I also appreciate the lyrics. I am sure that there is metaphor and that there are many ways to interpret the lyrics, but for me the lyrics of “Pompeii” express what it must feel like to be suddenly caught up in a devastating volcanic eruption– or any sudden natural disaster. The environment around you changes so quickly and so shockingly that you are left in a state of disbelief. Your mind can’t keep up. You feel, almost, that if you closed your eyes and opened them again everything would return to normal.

What do you think of the song? Does anyone else have geology-themed songs they enjoy? Perhaps we can start a geoblogging meme!

Here’s the music video for “Pompeii”:

http://www.youtube.com/watch?v=F90Cw4l-8NY

Plane Views: Amsterdam to Cape Town– Part II

Algeria #1.

Here is Part II of the views that I observed during a flight from Amsterdam to Cape Town back in September 2012. Part I is here. I believe that all of these shots were taken over Algeria. There are some stunning desert views. Although I grew up in relatively lush New England, I have always liked deserts. I think I first became enchanted by deserts when I was an exchange student and lived in Jordan for 5 months when I was 15 years old. My school in Jordan took me on visits to places such as Wadi Rum and Petra, and I quickly fell in love with the sands, rocks, animals, people, and historical ruins of the deserts there. Visiting the Jordanian deserts certainly helped inspire me to study geology.

I’ve never been to Algeria, but the desert views I observed while flying over Algeria are certainly enchanting. The young, volcanic Hoggar Mountains look particularly enticing. I hope that I can one day visit the deserts of Algeria. Has anyone been there?

Enjoy the desert views below. And, as always, feel free to point out interesting locations and geological features.

I still have some more views to share from this flight, so stay tuned for Part III!

Algeria #2.
Algeria #3.
Algeria #4.
Algeria #5.
Algeria #6.
Algeria #7. Sand ripples.
Algeria #8. Sings of man.
Algeria #9. A lone fire.
Algeria #10. Another view of the fire.
Algeria #11. Sand, sand, sand.
Algeria #12.
Algeria #13.
Algeria #14. Signs of salt.
Algeria #15.
Algeria #16.
Algeria #17. Red, white, and blue desert hues.
Algeria #18.
Algeria #19. A winding wadi leading into the Hoggar Mountains.
Algeria #20.
Algeria #21.
Algeria #22.
Algeria #23.
Algeria #24.
Algeria #25.
Algeria #26. Volcanic mountain tops.
Algeria #27.
Algeria #28.
Algeria #29.
Algeria #30.
Algeria #31.
Algeria #32.
Algeria #33.
Algeria #34.
Algeria #35.
Algeria #36.

LASI V: Silica Flour Crust and Vegetable Oil Magma– Using Laboratory Experiments to Better Understand Ground Deformation, Magma Movement, and Volcanic Eruptions

Note: Dr. Olivier Galland, a senior researcher at the Physics of Geological Processes Center of Excellence at the University of Oslo, presented a talk, “Ground deformation associated with shallow magma intrusions” at the LASI V conference in Port Elizabeth, South Africa in October 2012. The article below is based on this talk and also an interview with Dr. Galland. Over a few weeks, I am highlighting some of the research that was presented at the LASI V workshop. This is the fourth post in that series.

The landscape around an active volcano is dynamic: as magma moves about, the ground may change shape, inflating or deflating depending on how the magma is moving (Steps 1-2 of Fig. 1). The deformation may be caused either by the deep movement of magma or by the shallow intrusion of magma as sills or dykes. The movement can be dramatic (hundreds of meters) or it can be barely noticeable (a few millimeters). Big or small, ground deformation at volcanoes is important to monitor as it can provide clues to what is going on under the surface and, importantly, about when and where a volcanic eruption might occur.

At many volcanoes, geologists monitor ground deformation using a variety of techniques, including physical devices such as GPS and tiltometers, remote sensing techniques such as InSAR, and photogrammetry, which is the analysis of photographic images (Step 3 of Fig. 1). From surface measurements of ground movements, geologists can try to model what is going on underneath the surface (Step 4 of Fig. 1). However, linking observations of surface deformation to magma movements is no easy task (Step 5 of Fig. 1). That’s because geologists cannot generally directly observe the insides of a volcano. An analogy might be trying to understand why a kitchen sink is broken—why it is leaking or not flowing, perhaps— without being able to open up the cabinet door and look at the sink’s plumbing. Geologists can observe ancient volcanic plumbing, so to speak, in places where the tops of volcanoes have eroded away. However, observing the plumbing of active volcanoes is very difficult to impossible. Therefore, geologists generally rely on fancy computer models to try to link surface deformation with subsurface magma movement.

Fig. 1. Schematic diagram illustrating the principle of ground deformation analyses on active volcanoes. Numbering gives the succession of the stages of the analyses. 1. Magma intrudes in volcano, feeding magma reservoir or forming a sheet intrusion (dark gray intrusion). 2. Magma intrusion triggers ground deformation at surface, leading to modified topography (dashed line). 3. Topography variation is measured by geodetic techniques (GPS, InSAR, Photogrammetry, etc.). 4. Geodetic data are compared with modelling of ground deformation due to various intrusion shapes. 5. The best fit between models and ground deformation data provides a calculated intrusion shape (light gray dashed intrusion) responsible for the measured ground deformation. Nevertheless, the calculated intrusion shape is not a unique solution, and no direct observation is available to validate the calculation results.

Computer models are extremely helpful in trying to understand the insides of active volcanoes. However, they do have their limitations. This is because the shapes of magma chambers and shallow magma intrusions can be complex. Computer models can easily accommodate simple shapes such as circles or flat bodies. However, they have a harder time simulating more complex shapes, such as cones or saucers. Computer models also have trouble taking into account all environmental factors, such as the various stress fields and the realistic behavior of rocks. Finally, it is difficult to be completely confident in the results of computer models since the results of such models cannot generally be compared with direct observations.

One way to try to bridge the gap between surface observations of ground deformation and subsurface movements of magma inferred through computer models is through laboratory experiments. Dr. Olivier Galland is one scientist who conducts such experiments. Dr. Galland describes his experimental set-up (Fig. 2a) as, “Actually, it’s very simple. It’s just a box filled with silica flour, which is a fine-grained, granular material that is simulating the brittle crust. And into that material I inject a vegetable oil, which represents the magma, and the pressure of that oil is monitored. And then it’s possible to simulate the transport of magma and the formation of dykes and sills in this box.” Although such procedure seems simplistic, robust dimensional analysis of the method shows that the experimental results at the lab scale are valid at the geological scale.

Fig. 2. a. Drawing of the experimental apparatus. b. Representative oblique view photograph of the model surface during an experiment. The surface exhibited a smooth relief, at the rim of which the oil erupted. Dashed white line locates the section in the next image. c. Representative oblique view photograph of the model after the end of the experiment. The oil solidified and the intrusion was excavated, such that its top surface can be observed. The section showed that the intrusion was a thin sheet, resulting from hydraulic fracturing. Thus, the top surface of the intrusion was representative of its whole shape.

In a recent experiment (Galland, 2012) Dr. Galland used this silica flour and vegetable oil set up to simulate three types of shallow magmatic intrusions: a cone sheet, a dyke connected to a cone sheet, and a saucer-shaped sill. The motivation for this experiment was to provide additional data about the deformation that occurs when these shallow magmatic bodies are emplaced and, in addition, the deformation that occurs when they breach the surface and erupt. While the silica flour and vegetable oil set-up can’t simulate everything about a real volcano, it can provide plenty of important information, especially about the shapes of various intrusions and the pressures of the magma which produces these intrusions. This is possible because the oil is solid at room temperature, such that the final intrusion can be excavated out of the silica flour and its 3D shape analyzed (Fig. 2c).

Dr. Galland explains, “When a volcano is about to erupt or as it is erupted it either inflates or deflates, and this movement can be monitored. And then afterwards this movement is analyzed and inverted by geophysicists who try to calculate the geometry of the magma conduits. The problem is that we can never test these modeling results because we don’t see the intrusions because they are buried. The only way to really test these inversion techniques is to have a system where you measure the deformation and also know the shape of the intrusion and the pressure into the intrusion. And this is what we are doing in our experiments. We can quantify the shape of the intrusion and measure the pressure into the intrusion and measure the surface deformation, and then we can use this dataset to help test the inversion tools used by the geophysicists.”

Already, Dr. Galland’s experimental work is providing some interesting clues as to what is going on under the surface at volcanoes. “Recently, we figured out that there is clearly a link between how magma rises towards the surface and the pattern of the deformation at the surface,” Dr. Galland says. “Interestingly, this pattern develops very early during the experiments in the very early stages. So, we can observe some asymmetric development of this pattern which indicates where the magma is rising. So, if we can analyze that in real time, we could theoretically use it to predict where an eruption will occur. Obviously, in terms of volcanic hazard that is very important.” This is illustrated in the Figure 3, which shows the good match between the shape of the intrusion with the resulting ground deformation.

Fig. 3. Correlation between the shape of the ground deformation and the underlying intrusion in a characteristic experiment. a. Topographic map of model surface before the eruption of the oil. b. Plots of the temporal evolution of topographic profiles across the ground deformation pattern. The profiles are located on the map described in a. Each curve of the plots represents a transient stage of the model surfaces during each experiment. One can notice an initial symmetrical ground deformation, evolving to asymmetrical. c. Topographic map of the top surface of the excavated intrusion. The grey scale indicates the depth in mm below the initial surface. The locations of topographic profiles are the same as on the map of model surface in a, such that the profiles of the ground deformation and of the intrusions can be compared. d. Plots of topographic profiles of the model surface (top) and the underlying intrusion (down) parallel to the X-axis (X-profile). e. Plots of topographic profiles of the model surface (top) and the underlying intrusion (down) parallel to the Y-axis (Y-profile). Notice the vertical scale dilation for the profiles of the model surface. The correlation between e and d show that the ground deformation pattern reflects the shape of the underlying intrusion. This suggests that the asymmetrical development of the ground deformation pattern can be analysed to predict where the magma rises towards the surface.

However, Dr. Galland doesn’t spend all of his time in the laboratory. He believes that it is important for him to regularly go into the field to directly observe volcanoes, modern and ancient. He is particularly interested in observing subvolcanic systems, such as the saucer-shaped sills exposed in South Africa’s Karoo region and intrusive complexes formed in compressional settings exposed in the Neuquén Basin in the north Patagonian Andes. Dr. Galland explains, “My approach is to go to the field and really observe and do some detailed work and then out of that comes a question and then these questions can be subsequently addressed with experiments.” After all, that field knowledge is important for turning silica flour into the Earth’s crust and vegetable oil into magma.

Reference:
Galland, O. 2012. Experimental modelling of ground deformation associated with shallow magma intrusions. Earth and Planetary Science Letters, Vol. 317-318: 145-156.

***Note: Thanks very much to Dr. Galland for providing the three figures and captions.***

LASI V: Fire and Ice– Antarctic Glaciovolcanism Provides Clues to Past Climate

Brown and black products of Quaternary glaciovolcanic activity, with Paleozoic granite in the background, northern Victoria Land Antarctica. John Smellie for scale. Photo Credit: National Antarctic Research Program of Italy.

Note: Dr. Sergio Rocchi, an associate professor at the University of Pisa in Italy, presented a talk, “Intravolcanic sills, lava flows, and lava-fed deltas (Victoria Land, Antarctica): Paleoenvironmental Significance” at the LASI V workshop in Port Elizabeth, South Africa in October 2012. The article below is based on this talk and also an interview with Dr. Rocchi. Over a few weeks, I am highlighting some of the research that was presented at the LASI V workshop. This is the third post in that series.

When volcanoes erupt underneath and in the vicinity of glaciers and ice sheets, a unique geological record is created that provides information about both the volcanism and the snow and ice which interacted with the lava as it was being erupted. “Glaciovolcanism” is the term used to describe the interaction of lava with ice, snow (in all its forms, such as “firn” or compacted snow), and meltwater.

Glaciovolcanism includes study of modern examples in places such as Iceland and Antarctica as well as study of ancient examples. For the ancient examples, the ice and snow have generally long since melted away as a result of changing climate over the ages. Furthermore, the sediments and sedimentary rocks—tills and moraines and diamicts— associated with the glaciers and ice sheets have also often long since eroded away. However, volcanic rocks which interacted with the ice and snow are harder and slower to erode, and they often remain long after ice and sediment have disappeared.

Dissected late Pliocene volcano, northern Victoria Land Antarctica. John Smellie for scale. Photo Credit: National Antarctic Research Program of Italy.

Glaciovolcanic rocks can provide much valuable information about ancient glaciers and ice sheets. For example, study of glaciovolcanic rocks can help geologists identify if ice was present and, if so, can help geologists learn about the thickness of the ice, the elevation where the ice was present, the temperature conditions at the base of the ice, and the structure of the ice. A limitation is that volcanic eruptions do not occur continuously. Depending on the circumstances, they may occur at intervals of 10s—or even of 100s or 1000s— of years. Also, over time even hard glaciovolcanic rocks can erode away. Nevertheless, study of glaciovolcanic rocks is a powerful tool for reconstructing past ice cover and conditions, which in turn provides much information about past climate that can complement other paleoclimate studies—for example, study of sedimentary and coral records. Volcanic rocks are also fairly easy to date using isotopic techniques, so they can provide clear age constraints to help with paleoclimatic reconstructions.

Dr. Sergio Rocchi is a volcanologist who has studied glaciovolcanic rocks in Antarctica along with his colleague Dr. John Smellie and other co-workers. Dr. Rocchi explains, “Volcanic eruptions in subglacial environments generate some glacial volcanic lithofacies [units of rocks with certain characteristics] which can tell us the thickness and also the type of ice that was present at the time of the eruption. Additionally, the volcanic rocks can be dated by isotopic means, so the combination of the age and thickness of the ice can be a very useful source of paleoenvironmental information.”

Sergio Rocchi flying over Mt Melbourne Volcano, northern Victoria Land Antarctica. Photo credit: National Antarctic Research Program of Italy.
Sergio Rocchi over Campbell Glacier, northern Victoria Land Antarctica. Photo credit: National Antarctic Research Program of Italy.

As an example, Dr. Rocchi and his co-workers have studied Late Miocene glaciovolcanic rocks of Victoria Land, Antarctica. There, hyaloclastite-rich glaciovolcanic rocks, including some “lava-fed deltas” (features which form when lava enters water either in a marine/lacustrine or a glacial meltwater environment), have enabled reconstruction of Late Miocene glacial cover over Victoria Land. The glaciovolcanic rocks indicate that at this time Victoria Land was covered by a thin (<300 m thick) cover of ice. This ice sheet is much thinner than that predicted by some modeling studies and implies a more complex climatic transition in the Miocene than previously thought.

While most work regarding glaciovolcanism to date has been carried out in Antarctica, study of glaciovolcanism can also be done in many other places. “Similar work can obviously been done wherever there are or were volcanoes and ice,” says Dr. Rocchi. “The main places where volcano-ice interaction can be studied are Antarctica, Iceland, and British Columbia in the northern Cascades. A future project for which we are raising funding is making a comparison of the glaciovolcanic record in Antarctica with that in Iceland.”

In the future, study of glaciovolcanism will no doubt continue to help geologists and climate scientists unravel the history and nature of past glaciers and ice sheets. Combined with other paleoclimate records, study of glaciovolcanism will help scientists to better understand how Earth’s climate used to be and how climate changes over time. This information is invaluable in a time when humans are experiencing the effects of anthropogenic climate change and when scientists need as much information as possible in order to evaluate what may happen to Earth’s climate in the coming years.

References:
Prof. John Smellie’s website about Antarctic Glaciovolcanism.

Smellie, J., Wilch, T., and Rocchi, S., 2013. ‘A‘ā lava-fed deltas: A new reference tool in paleoenvironmental studies. Geology. (to be published in the April issue).

Smellie, J., Rocchi, S., and Armienti, P. 2011. Late Miocene volcanic sequences in northern Victoria Land, Antarctica: products of glaciovolcanic eruptions under different thermal regimes. Bulletin of Volcanology, Vol. 73: 1-25.

Smellie, J., Rocchi, S., Gemelli, M., Di Vincenzo, G., and Armienti, P. 2011. A thin predominantly cold-based Late Miocene East Antarctic ice sheet inferred from glaciovolcanic sequences in northern Victoria Land, Antarctica. Palaeogeography, Palaeoclimatology, Palaeoecology, Vol. 307: 129-149.

Smellie, J., Johnson, J., McIntosh, W., Esser, R., Gudmundsson, M., Hambrey, M., van Wyk de Vries, B. 2008. Six million years of glacial history recorded in volcanic lithofacies of the James Ross Island Volcanic Group, Antarctica Peninsula. Palaeogeography, Palaeoclimatology, Palaeoecology, Vol. 260: 122-148.