25 June Interview

motivation and qualification for the Master's Program.
32 selection points


Background

  • Mexico
  • Computer science
    • embedded systems
  • Nature
  • Organic Agriculture
  • GIS
  • 3D game engine, planets

Motivation

I'm particularly fascinated by how we can use technology to study Earth's geological processes, such as volcanism, and apply this knowledge to other planets.

I'm keen to explore how studying volcanic processes and water cycles on other planets can enhance our understanding of similar phenomena on Earth.

  • geology
  • ecology
  • sensing
  • simulations
  • planetary geology
  • isotopic signals
    • Climate science: Stable isotopes are used as climate proxies for temperature reconstruction.
    • Solar System research: Isotopic fingerprints help study the origin of materials in the Solar System, such as comparing the Moon's composition to Earth's.
  • plate tectonics
  • volcanism
  • atmospheres/climate
  • laboratory work and excursions

I'm fascinated by the concept of terraforming
terraformation ("Earth-shaping") is the hypothetical process of deliberately modifying the atmosphere, temperature, surface topography or ecology of a planet, moon, or other body to be similar to the environment of Earth to make it habitable for humans to live on.

Create habitable conditions and how geological processes contribute to Earth's life-supporting systems

I'm especially interested in studying how Earth's geological processes, such as plate tectonics and volcanism, work together with other factors like the water cycle and atmosphere to create and maintain habitable conditions. Understanding these interactions on Earth could provide insights into the potential habitability of other planets.

Skills

  • creative
  • problem solver
  • analytical and critical thinker
  • navigation, sense of orientation

Know about the program

  • Planetary Climate and Atmospheres

  • Remote Sensing of Atmosphere and Ocean

  • Late Accretion Onto Terrestrial Planets

  • Formation and evolution of crust on early earth

  • Global volatile cycles on early Earth


Summary of Projects

1. DIVERSE (DIVerse Exoplanet Redox State Estimations)

The DIVERSE project focuses on understanding the redox states of exoplanets, particularly those with strongly reduced interior chemistry. These planets, termed "Class X planets," are expected to have atmospheres formed by volcanic outgassing, differing significantly from Earth-like planets and resembling ice giants like Neptune. The project aims to explore the relationship between a planet's interior chemistry and its atmospheric composition, providing insights into diverse planetary formation and evolution processes.

2. SPP1883: Building a Habitable Earth

The SPP1883 project addresses the question of how Earth became the only known habitable planet. It focuses on three critical aspects: the compositions and sources of Earth's building materials, the early internal processing into crust, mantle, and core, and the evolution of the ocean-atmosphere system. The project employs an interdisciplinary Earth Science approach, utilizing novel analytical techniques and experimental and modeling approaches to study early geological and extraterrestrial samples. The initiative aims to understand the unique conditions that made Earth habitable and involves various Earth Science disciplines, including geology, geochemistry, planetology, cosmochemistry, geobiology, and geophysical modeling.

3. Habitat-OASIS – Habitability of Oceans and Aqueous Systems on Icy Satellites

The Habitat-OASIS project investigates the habitability of oceans and aqueous systems on icy satellites. It focuses on understanding the conditions that could support life in these extreme environments, examining the chemical and physical processes that influence habitability. The project aims to provide insights into the potential for life on icy moons, such as Europa and Enceladus, by studying their subsurface oceans and the interactions between the ice shell and the underlying water.

Comments to Mention

  1. DIVERSE Project:

    • "The DIVERSE project is fascinating as it explores a unique class of exoplanets with strongly reduced interior chemistry, providing new insights into planetary formation and evolution."
    • "I am particularly interested in how the project investigates the relationship between a planet's interior chemistry and its atmospheric composition, which could have significant implications for identifying potential biosignatures."
  2. SPP1883: Building a Habitable Earth:

    • "The SPP1883 project is crucial for understanding the unique combination of processes that made Earth habitable, focusing on early geological and extraterrestrial samples."
    • "I appreciate the interdisciplinary approach of the project, combining geology, geochemistry, and geophysical modeling to reconstruct Earth's early evolution and its habitability."
  3. Habitat-OASIS Project:

    • "The Habitat-OASIS project is exciting as it delves into the habitability of oceans on icy satellites, which could expand our understanding of potential life beyond Earth."
    • "I am intrigued by the project's focus on the chemical and physical processes that influence habitability in extreme environments, such as those found on Europa and Enceladus."

These comments highlight your interest in the specific aspects of each project and demonstrate your enthusiasm for the research being conducted in the FU Berlin Planetary Sciences Master's program.

Questions

  • Does the program offer any courses or research opportunities specifically focused on terraforming concepts or technologies?

  • Are there modules or research projects that deal with planetary volcanism, both on Earth and other celestial bodies?

  • What kind of water analysis techniques are taught in the program, especially in relation to planetary exploration?

  • How much emphasis is placed on comparative planetology and geological processes across different planets and moons?

  • Are there opportunities to participate in field trips or excursions to study geological formations relevant to planetary science?

  • What kind of laboratory facilities are available for students to conduct experiments in planetary sciences?

  • Are there any ongoing research projects at FU Berlin related to the search for water or habitable environments on other planets?

  • Are there opportunities to study the potential geological and environmental impacts of terraforming on other planets?

  • Does the curriculum cover the study of extremophiles and their implications for potential life on other planets?

Articulating complex ideas

the role of geology in Earth's habitability, I would explain: Geological processes play a crucial role in maintaining Earth's habitability. Plate tectonics, for instance, regulates the carbon cycle and helps maintain a stable climate over geological timescales. Volcanism contributes to atmospheric composition and can influence climate. The interaction between the solid Earth and the hydrosphere creates a diverse range of environments suitable for life.

Current Developments

I'm particularly interested in recent research on how Earth's magnetic field, generated by its molten core, protects our atmosphere from solar wind erosion, thus contributing to long-term habitability. This showcases how deep Earth processes can have far-reaching effects on surface conditions.

Interdisciplinary thinking

My background in computer science, combined with my interests in geology, biology, and planetary science, allows me to approach the study of Earth's habitability from a systems perspective. I'm interested in developing models that integrate geological, atmospheric, and biological data to better understand how these systems interact to create and maintain habitable conditions.

Showcase

Plate tectonics is crucial for Earth's long-term habitability. It regulates the carbon cycle by subducting carbon-rich sediments and releasing CO2 through volcanism, helps create diverse environments through mountain building and basin formation, and may play a role in generating Earth's magnetic field, which protects our atmosphere.