César León Jr.🌋👋

César León Jr.🌋👋

César León Jr.🌋👋

César León is a PhD Student of Planetary Geology at Washington University in St. Louis. His current research focuses on understanding the surface of rocky planets in our solar system, like Venus and the Moon. He aims to better understand Earth's tectonic evolution (structure of a planet's crust) and volcanism (volcanic and magmatic processes).


César strives to make science accessible through writing and scientific translation. He continues to mentor other first-generation and underrepresented students in higher education.

César León is a PhD Student of Planetary Geology at Washington University in St. Louis. His current research focuses on understanding the surface of rocky planets in our solar system, like Venus and the Moon. He aims to better understand Earth's tectonic evolution (structure of a planet's crust) and volcanism (volcanic and magmatic processes).


César strives to make science accessible through writing and scientific translation. He continues to mentor other first-generation and underrepresented students in higher education.

Curriculum Vitae 🔬

Curriculum Vitae 🔬

Curriculum Vitae 🔬

Education

Education

Ph.D. Planetary Geology

Ph.D. Planetary Geology

College of Arts & Sciences, Washington University

College of Arts & Sciences, Washington University

St. Louis, Missouri

St. Louis, Missouri

expected 2029

exp. 2029

B.A. Earth Science

B.A. Earth Science

Columbia College, Columbia University

Columbia College, Columbia University

New York, New York

New York, New York

2024

2024

Study abroad

Study abroad

Queen Mary University of London

Queen Mary University of London

2023

2023

Education

Ph.D. Planetary Geology

College of Arts & Sciences, Washington University

St. Louis, Missouri

exp. 2029

B.A. Earth Science

Columbia College, Columbia University

New York, New York

2024

Study abroad

Queen Mary University of London

2023

Appointments

Appointments

Appointments

Graduate Research Fellow

Graduate Research Fellow

Dept. of Earth, Environmental, and Planetary Sciences

Dept. of Earth, Environmental, and Planetary Sciences

Washington University in St. Louis

Washington University in St. Louis

08/2024 - present

Aug 2024 to present

Undergraduate Research Assistant

Undergraduate Research Assistant

Lamont-Doherty Earth Observatory, Geophysics

Lamont-Doherty Earth Observatory, Geophysics

Columbia University in the City of New York

Columbia University in the City of New York

08/2023 - 12/2023

Aug 2023 to

Dec 2023

Graduate Research Fellow

Department of Earth, Environmental, and Planetary Sciences

Washington University in St. Louis

08/2024 - present

Undergraduate Research Assistant (Senior Thesis)

Lamont-Doherty Earth Observatory, Geochemistry Division

Columbia University

11/2021 - 05/2024

Undergraduate Research Assistant

Lamont-Doherty Earth Observatory, Marine Geology and Geophysics Division

Columbia University

08/2023 - 12/2023

Undergraduate Research Fellow

Division of Geologic and Planetary Sciences, Planetary Science Option

California Institute of Technology

06/2023 - 08/2023

Undergraduate Research Assistant (Senior Thesis)

Undergraduate Research Assistant (Senior Thesis)

Lamont-Doherty Earth Observatory, Geochemistry

Lamont-Doherty Earth Observatory, Geochemistry

Columbia University in the City of New York

Columbia University in the City of New York

11/2021 - 05/2024

Nov 2021 to

May 2024

Undergraduate Research Fellow

Undergraduate Research Fellow

Division of Geologic and Planetary Sciences, Planetary

Division of Geologic and Planetary Sciences, Planetary

California Institute of Technology

California Institute of Technology

06/2023 - 08/2023

June 2023 to Aug 2023

Teaching

Teaching

Teaching

Graduate Teaching Assistant

Graduate Teaching Assistant

Department of Earth, Environmental and Planetary Sciences, Washington University

Department of Earth, Environmental and Planetary Sciences, Washington University

EEPS 171 The Solar System

EEPS 171 The Solar System

01/2025 - 05/2025

Aug 2022 to

May 2024

Undergraduate Teaching Assistant

Undergraduate Teaching Assistant

Department of Earth and Environmental Sciences, Columbia University

Department of Earth and Environmental Sciences, Columbia University

EESC 2200 Solid Earth Systems (Fall 2022, Spring 2024)

EESC 2200 Solid Earth Systems

EESC 2100 Climate Systems (Fall 2023)

EESC 2100 Climate Systems

08/2022 - 05/2024

Aug 2022 to

May 2024

Graduate Teaching Assistant

Department of Earth, Environmental and Planetary Sciences, Washington University

EEPS 171 The Solar System

Aug 2022 to

May 2024

Undergraduate Teaching Assistant

Department of Earth and Environmental Sciences, Columbia University

EESC 2200 Solid Earth Systems

EESC 2100 Climate Systems

Aug 2022 to

May 2024

Leadership & Service

Leadership & Service

04/2024 - 08/2024

April 2024 to Aug 2024

Volunteer Staff Lead (YLI Program)

Volunteer Staff Lead (YLI Program)

Hispanic Scholarship Fund

Hispanic Scholarship Fund

04/2021 - 04/2024

April 2021 to April 2024

Volunteer Mentor (YLI Program)

Volunteer Mentor (YLI Program)

Hispanic Scholarship Fund

Hispanic Scholarship Fund

08/2023 - 05/2024

Aug 2023 to

May 2024

Residential Advisor (Student Leader)

Residential Advisor (Student Leader)

Columbia University, Student Life

Columbia University, Student Life

06/2021 - 08/2021

June 2021 to Aug 2021

Peer Counselor (Student Leader)

Peer Counselor (Student Leader)

Columbia University, Academic Success Program

Columbia University, Academic Success Program

10/2021 - 05/2022

Oct 2021 to

May 2022

Vice President of Sustainability (Student Leader)

Vice President of Sustainability (Student Leader)

Columbia University, Residence Hall Council

Columbia University, Residence Hall Council

August 2021

August 2021

Orientation Leader (Student Leader)

Orientation Leader (Student Leader)

Columbia University, Student Life

Columbia University, Student Life

Volunteer Staff Lead (YLI Program)

Hispanic Scholarship Fund

04/2024 - 08/2024

Volunteer Mentor (YLI Program)

Hispanic Scholarship Fund

04/2021 - 04/2024

Residential Advisor (Student Leader)

Columbia University, Student Life

08/2023 - 05/2024

Peer Counsel (Student Leader)

Columbia University, Academic Success Programs

06/2021 - 08/2021

Vice President of Sustainability (Student Leader)

Columbia University, Residence Hall Council

10/2021 - 05/2022

Orientation Leader (Student Leader)

Columbia University, Student Life

August 2021

Membership

Membership

08/2024 - present

Nov 2022 to

present

Washington University in St. Louis

Washington University in St. Louis

08/2024 - present

Aug 2024 to present

Washington University in St. Louis

Washington University in St. Louis

11/2022 - present

Nov 2022 to

present

03/2022 - 05/2024

Mar 2022 to

May 2024

Columbia University

Columbia University

07/2020 - 05/2024

July 2020 to May 2024

08/2020 - 05/2024

Aug 2020 to May 2024

07/2020 - 05/2024

July 2020 to May 2024

Academic Success Programs

Academic Success Programs

Columbia University

Columbia University

Latino Graduate Student Association

Washington University in St. Louis

08/2024- present

American Geophysical Union

National, USA

11/2022 - present

Blueshift Club (Astronomy)

Columbia University

03/2022 - 05/2024

Marie Thorp Society (Geology)

Columbia University

07/2020 - 05/2024

Questbridge Network (First-Generation, Low-Income)

Columbia University

08/2020 - 05/2024

Academic Success Programs

Columbia University

07/2020 - 05/2024

Presentations

Presentations

Presentations

Senior Thesis, Columbia University

Senior Thesis, Columbia University

April 2024

April 2024

Senior Thesis, Columbia University

September 2023

September

2022

April 2024

Undergraduate Research Symposium (Poster), Columbia University

Undergraduate Research Symposium (Poster), Columbia University

September 2022

Undergraduate Research Symposium (Talk), California Institute of Technology

Undergraduate Research Symposium (Talk), California Institute of Technology

August

2023

Undergraduate Research Symposium (Talk),
California Institute of Technology

Undergraduate Research Symposium (Talk),
California Institute of Technology

August 2023

August

2023

Undergraduate Research Symposium,
Lamont-Doherty Earth Observatory

Undergraduate Research Symposium,
Lamont-Doherty Earth Observatory

August 2022

August

2023

American Geophysical Union Fall Conference (Poster), Chicago, IL

December 2022

Undergraduate Research Symposium, Lamont-Doherty Earth Observatory

August

2022

Skills

Labratory

Labratory

Labratory

Fourier Transform Infrared (FTIR) Spectroscopy, Electron Microprobe, Scanning Electron Microscopy (SEM), Mass Spectroscopy (ICP-MS), Piston-Cylinder Apparatus

Fourier Transform Infrared (FTIR) Spectroscopy, Electron Microprobe, Scanning Electron Microscopy (SEM), Mass Spectroscopy (ICP-MS), Piston-Cylinder Apparatus

Fourier Transform Infrared (FTIR) Spectroscopy, Electron Microprobe, Scanning Electron Microscopy (SEM), Mass Spectroscopy (ICP-MS), Piston-Cylinder Apparatus

Computational

Computational

Computational

Geographic Information Systems (GIS), GeoMapApp, MELTS Software, ENVI, AZtecTEM (for SEM Processing), Python, MatLab

Geographic Information Systems (GIS), GeoMapApp, MELTS Software, ENVI, AZtecTEM (for SEM Processing), Python, MatLab

Geographic Information Systems (GIS), GeoMapApp, MELTS Software, ENVI, AZtecTEM (for SEM Processing), Python, MatLab

Projects & Research 🌎🌍🌏

Projects & Research 🌎🌍🌏

Science Communication

Science Communication

More Communication Project and Articles Upcoming…

More Communication Project and Articles Upcoming…

C.Leon Advising Logo
C.Leon Advising Logo

Mentorship Resources

Mentorship Resources

Documents and Resources for Student Planning and Success Upcoming…
[Instagram Profile]


Documents and Resources for Student Planning and Success Upcoming…
[Instagram Profile]


Understanding CO2-S Degassing from the San Cristóbal Volcano

Understanding CO2-S Degassing from the San Cristóbal Volcano

Understanding CO2-S Degassing from the San Cristóbal Volcano

Abstract
Lab Website
A sudden increase in the CO2/SO2 ratio in high-temperature gas has been observed prior to eruption in many arc volcanoes and can be potentially used as an eruptive precursor. However, this ratio remains tricky to interpret due to the large variability that may be displayed over time and between eruption cycles. San Cristóbal volcano in Nicaragua shows abnormally high CO2/SO2 ratios in its high-temperature gas and has actively degassed and erupted over the past 50 years, making it a useful endmember to study for the factors that control volcanic gas compositions.

Melt Inclusions (MIs), ideally, preserve volatile contents of magma at the time of their entrapment, and can be used to infer the melt and gas composition at different degassing depths. However, shrinkage bubbles in MIs can cause a significant underestimate of the CO2 budget. This study uses olivine-hosted melt inclusions from a primitive, Holocene sample (SC11D) of the San Cristóbal volcano to constrain the CO2 and S contents in the parental magma during ascent and degassing.

To address the shrinkage bubble issue and reconstruct a more accurate MI CO2 concentration, I recreate chamber conditions by conducting piston cylinder experiments at 7 kbar and 1150-1280°C to redissolve bubbles back into their melt. I then use fourier-transform infrared (FTIR) spectroscopy to analyze the H2O and CO2 concentrations, followed by electron probe microanalyzer (EPMA) to measure S and major element concentrations in treated MIs.

Our new rehomogenized MI measurements, with >3600 ppm maximum, increase CO2 measurements for San Cristóbal volcano 50% over previous raman spectroscopy measurements, ~1800 ppm, and ~3x relative to untreated samples, <1000 ppm CO2 (Robidoux et al. 2017, 2018). Our new data increase the estimated depth at which San Cristóbal volcanic gas derives to >20 km and degassing modeling has interpreted the CO2/S ratio’s degassing trend. Constraining CO2/S concentrations by addressing shrinkage bubble formation allows for a more accurate derived depth of degassing to, in turn, better understand dynamics of magma ascension for the San Cristóbal and other arc volcanoes.

Abstract
Lab Website
A sudden increase in the CO2/SO2 ratio in high-temperature gas has been observed prior to eruption in many arc volcanoes and can be potentially used as an eruptive precursor. However, this ratio remains tricky to interpret due to the large variability that may be displayed over time and between eruption cycles. San Cristóbal volcano in Nicaragua shows abnormally high CO2/SO2 ratios in its high-temperature gas and has actively degassed and erupted over the past 50 years, making it a useful endmember to study for the factors that control volcanic gas compositions.

Melt Inclusions (MIs), ideally, preserve volatile contents of magma at the time of their entrapment, and can be used to infer the melt and gas composition at different degassing depths. However, shrinkage bubbles in MIs can cause a significant underestimate of the CO2 budget. This study uses olivine-hosted melt inclusions from a primitive, Holocene sample (SC11D) of the San Cristóbal volcano to constrain the CO2 and S contents in the parental magma during ascent and degassing.

To address the shrinkage bubble issue and reconstruct a more accurate MI CO2 concentration, I recreate chamber conditions by conducting piston cylinder experiments at 7 kbar and 1150-1280°C to redissolve bubbles back into their melt. I then use fourier-transform infrared (FTIR) spectroscopy to analyze the H2O and CO2 concentrations, followed by electron probe microanalyzer (EPMA) to measure S and major element concentrations in treated MIs.

Our new rehomogenized MI measurements, with >3600 ppm maximum, increase CO2 measurements for San Cristóbal volcano 50% over previous raman spectroscopy measurements, ~1800 ppm, and ~3x relative to untreated samples, <1000 ppm CO2 (Robidoux et al. 2017, 2018). Our new data increase the estimated depth at which San Cristóbal volcanic gas derives to >20 km and degassing modeling has interpreted the CO2/S ratio’s degassing trend. Constraining CO2/S concentrations by addressing shrinkage bubble formation allows for a more accurate derived depth of degassing to, in turn, better understand dynamics of magma ascension for the San Cristóbal and other arc volcanoes.

Abstract
Lab Website
A sudden increase in the CO2/SO2 ratio in high-temperature gas has been observed prior to eruption in many arc volcanoes and can be potentially used as an eruptive precursor. However, this ratio remains tricky to interpret due to the large variability that may be displayed over time and between eruption cycles. San Cristóbal volcano in Nicaragua shows abnormally high CO2/SO2 ratios in its high-temperature gas and has actively degassed and erupted over the past 50 years, making it a useful endmember to study for the factors that control volcanic gas compositions.

Melt Inclusions (MIs), ideally, preserve volatile contents of magma at the time of their entrapment, and can be used to infer the melt and gas composition at different degassing depths. However, shrinkage bubbles in MIs can cause a significant underestimate of the CO2 budget. This study uses olivine-hosted melt inclusions from a primitive, Holocene sample (SC11D) of the San Cristóbal volcano to constrain the CO2 and S contents in the parental magma during ascent and degassing.

To address the shrinkage bubble issue and reconstruct a more accurate MI CO2 concentration, I recreate chamber conditions by conducting piston cylinder experiments at 7 kbar and 1150-1280°C to redissolve bubbles back into their melt. I then use fourier-transform infrared (FTIR) spectroscopy to analyze the H2O and CO2 concentrations, followed by electron probe microanalyzer (EPMA) to measure S and major element concentrations in treated MIs.

Our new rehomogenized MI measurements, with >3600 ppm maximum, increase CO2 measurements for San Cristóbal volcano 50% over previous raman spectroscopy measurements, ~1800 ppm, and ~3x relative to untreated samples, <1000 ppm CO2 (Robidoux et al. 2017, 2018). Our new data increase the estimated depth at which San Cristóbal volcanic gas derives to >20 km and degassing modeling has interpreted the CO2/S ratio’s degassing trend. Constraining CO2/S concentrations by addressing shrinkage bubble formation allows for a more accurate derived depth of degassing to, in turn, better understand dynamics of magma ascension for the San Cristóbal and other arc volcanoes.

Investigation of Hydrothermal Alteration of Prehnite and Epidote from the Oman Ocean Crust and on other Planetary Bodies through Imaging Spectroscopy

Investigation of Hydrothermal Alteration of Prehnite and Epidote from the Oman Ocean Crust and on other Planetary Bodies through Imaging Spectroscopy

Investigation of Hydrothermal Alteration of Prehnite and Epidote from the Oman Ocean Crust and on other Planetary Bodies through Imaging Spectroscopy

Abstract
Lab Website
Earth’s ocean crust covers around 60% of the surface of the planet, and hydrothermal systems are very common on Earth and other planetary bodies. Yet, geochemical interactions which form, cool, and alter oceanic crust are not entirely understood because access to samples is not easy or cheap.

In this project, we are looking at ~1.2 km drill cores (Holes GT1A, GT2A & GT3A) from the Oman ophiolite recovered by the International Continental Scientific Drilling Program’s Oman Drilling Project (Kelemen et al. 2020). This region of oceanic crust is particularly interesting because it is an area where ocean crust and parts of the upper mantle outcropped onto the surface (Searle and Cox 1999) which provides easier access. Surface processes, such as weathering, could have altered the state of the ophiolite, consequently, their effects need to be considered before extrapolating geochemical processes from its suboceanic roots. These cores were scanned with an imaging spectrometer which measures reflected light at many wavelengths (Crotteau, M. A. et al. 2021; Greenberger, et al. 2021).

These datasets can be used to obtain mineralogical data of the core at sub-millimeter spatial resolution. Visible-shortwave infrared reflectance micro-imaging spectroscopy (Leask, et al. 2016) has incredible applications for observing planetary surfaces as the technique is highly practical, speedy, and non-destructive. However, mineral quantification studies with empirical data are necessary before deploying this technique for observable, but not physically attainable, measurements (e.g. rocks from Mars).

We completed scanning electron microscopy (SEM) measurements and developed correlations with existing spectroscopic data. We then analyzed and corroborated elemental composition data to quantify minerals. This study aims to develop more accurate methods of quantifying prehnite and epidote, distinguish between different minerals and their relative abundance, and find a holistic understanding of the core in its entirety instead of assumption-based correlations through targeted measurement sites.


Abstract
Lab Website
Earth’s ocean crust covers around 60% of the surface of the planet, and hydrothermal systems are very common on Earth and other planetary bodies. Yet, geochemical interactions which form, cool, and alter oceanic crust are not entirely understood because access to samples is not easy or cheap.

In this project, we are looking at ~1.2 km drill cores (Holes GT1A, GT2A & GT3A) from the Oman ophiolite recovered by the International Continental Scientific Drilling Program’s Oman Drilling Project (Kelemen et al. 2020). This region of oceanic crust is particularly interesting because it is an area where ocean crust and parts of the upper mantle outcropped onto the surface (Searle and Cox 1999) which provides easier access. Surface processes, such as weathering, could have altered the state of the ophiolite, consequently, their effects need to be considered before extrapolating geochemical processes from its suboceanic roots. These cores were scanned with an imaging spectrometer which measures reflected light at many wavelengths (Crotteau, M. A. et al. 2021; Greenberger, et al. 2021).

These datasets can be used to obtain mineralogical data of the core at sub-millimeter spatial resolution. Visible-shortwave infrared reflectance micro-imaging spectroscopy (Leask, et al. 2016) has incredible applications for observing planetary surfaces as the technique is highly practical, speedy, and non-destructive. However, mineral quantification studies with empirical data are necessary before deploying this technique for observable, but not physically attainable, measurements (e.g. rocks from Mars).

We completed scanning electron microscopy (SEM) measurements and developed correlations with existing spectroscopic data. We then analyzed and corroborated elemental composition data to quantify minerals. This study aims to develop more accurate methods of quantifying prehnite and epidote, distinguish between different minerals and their relative abundance, and find a holistic understanding of the core in its entirety instead of assumption-based correlations through targeted measurement sites.


Abstract
Lab Website
Earth’s ocean crust covers around 60% of the surface of the planet, and hydrothermal systems are very common on Earth and other planetary bodies. Yet, geochemical interactions which form, cool, and alter oceanic crust are not entirely understood because access to samples is not easy or cheap.

In this project, we are looking at ~1.2 km drill cores (Holes GT1A, GT2A & GT3A) from the Oman ophiolite recovered by the International Continental Scientific Drilling Program’s Oman Drilling Project (Kelemen et al. 2020). This region of oceanic crust is particularly interesting because it is an area where ocean crust and parts of the upper mantle outcropped onto the surface (Searle and Cox 1999) which provides easier access. Surface processes, such as weathering, could have altered the state of the ophiolite, consequently, their effects need to be considered before extrapolating geochemical processes from its suboceanic roots. These cores were scanned with an imaging spectrometer which measures reflected light at many wavelengths (Crotteau, M. A. et al. 2021; Greenberger, et al. 2021).

These datasets can be used to obtain mineralogical data of the core at sub-millimeter spatial resolution. Visible-shortwave infrared reflectance micro-imaging spectroscopy (Leask, et al. 2016) has incredible applications for observing planetary surfaces as the technique is highly practical, speedy, and non-destructive. However, mineral quantification studies with empirical data are necessary before deploying this technique for observable, but not physically attainable, measurements (e.g. rocks from Mars).

We completed scanning electron microscopy (SEM) measurements and developed correlations with existing spectroscopic data. We then analyzed and corroborated elemental composition data to quantify minerals. This study aims to develop more accurate methods of quantifying prehnite and epidote, distinguish between different minerals and their relative abundance, and find a holistic understanding of the core in its entirety instead of assumption-based correlations through targeted measurement sites.


Let's have a conversation 🪐

Let's have a conversation 🪐

Let's have a conversation 🪐

Get in touch.

Get in touch.

Get in touch.

© César León 2023 | In Collaboration