Program Description
The Earth and Planetary Science Interdisciplinary Internships (EPIIC) program at the Carnegie Science Earth and Planets Laboratory (EPL) offers a unique opportunity for undergraduate students to gain hands-on experience in the fields of Earth, planetary, and astronomical sciences. We are particularly interested in applications from students attending institutions with limited local research opportunities (e.g., community and liberal arts colleges) and/or those who have not conducted research before.
During the 10-week program (June 2, 2025 - August 8, 2025), interns will work under the supervision of experienced researchers in the fields of astronomy, astrobiology, biogeochemistry, cosmochemistry, data science, experimental geochemistry/petrology, geophysics, isotope geochemistry, high-pressure mineral physics, mineralogy, organic geochemistry, and petrology.
Interns will work with their Carnegie mentor on an assigned research project with the ultimate goal of developing an original research finding that is suitable for presentation at a national scientific meeting during the following academic year. Interns are full members of their mentors’ research groups, participate in regular group meetings, and attend weekly seminars and social events at the EPL aimed at establishing a collegial cohort. EPIIC’s intensity and training will prepare its participants for graduate student life.
Program Dates: June 2, 2025 - August 8, 2025
Move-in: May 31, 2025 | Move-out: August 9, 2025
Applications Due: January 31, 2025
Decisions will be made by March 3, 2025. Replies will be requested by March 10, 2025.
- This is a paid, full-time position with a stipend of $6000 dispersed at the beginning, middle, and end of the program.
- Apartment-style housing will be provided at American University. This includes full linen sets, Wi-Fi and cable access, shuttle service to/from the nearest metro stop, and complimentary access to the university’s fitness facilities. Pets are not allowed. Move-in/out days will be May 31st and Aug. 9th.
- Interns will also have access to the Earth and Planets Laboratory facilities including the library and research facilities necessary for carrying out their research.
- Interns will be provided with necessary computing resources (e.g., a laptop, project-specific software).
- Interns can receive support for relocation expenses up to $300.
- Funds are available for the interns to attend and present their work at professional meetings following the conclusion of the internship and in consultation with their research mentor(s).
Please contact program manager Dr. Dionysis Foustoukos at dfoustoukos@carnegiescience.edu and/or Dr. Johanna Teske at jteske@carnegiescience.edu with any questions or concerns.
Participants in the EPIIC internship are expected to:
- Work on a research project under the guidance of a mentor.
Mentor(s) and mentee(s) sign a document after discussion that sets expectations and goals for their summer collaboration. The student carries out a research project crafted by the mentor(s), with the opportunity for modifications and/or additions based on the student’s skills and motivation.
- Acquire expertise in research methods while carrying out a research project.
Acquiring expertise in the research methods starts the first week the student is at EPL, and within several weeks, students can carry out independent work.
- Participate in professional development workshops.
The student participates in several research and science communication skills workshops that supplement the more topic-specific skills they gain from the research project and meets weekly as a group with the coordinator to provide research updates.
- Prepare an AAS- or AGU-style abstract of the work presented before the end of July
The oral presentations are styled after national meetings (AGU, GSA, or AAS), and questions by the audience are encouraged. An abstract for the presentation is required, which will, if the student chooses, form the basis for an abstract to be submitted for a presentation at a national meeting during the following academic year.
- Participate in evaluations
Students and mentors participate in a series of beginning, mid-, and end-of-program evaluations to assess the mentor-mentee interactions, the progress of the students in gaining research skills, and overall experience in the full program.
- Meet weekly with the program coordinator to provide research updates.
- Must be an undergraduate student enrolled (part-time or full-time) in a degree program leading to a baccalaureate or associate degree.
- Students who are transferred from one college/university to another and are enrolled at neither institution during the intervening summer may participate.
- Must be able to commit to the full 10-week program in person (June 2, 2025 - August 8, 2025)
- Research projects will be conducted on campus and in person.
- Strong interest in Earth, planetary, and/or astronomical sciences
- No minimum GPA is required
The online application form asks for information about you, your previous research experience, and your motivation for pursuing this internship. There are several short prompts (< 250 words.) We also ask for the contact information of one reference (but they do not need to submit letters).
Please read over the application first, and draft your response in a separate document before filling out the online form for submission.
Application Materials to Prepare:
- Curriculum Vitae
- Unofficial Transcript
- Reference Contact Information
- Short Essay Question Responses
Note: We believe academic environments should be places where diverse groups of people with a variety of viewpoints and ideas can thrive and work together. As such, we encourage applicants from underrepresented groups and backgrounds to apply. The Carnegie Institution is an equal-opportunity employer. All qualified applicants will receive consideration for employment and will not be discriminated against on the basis of gender, race/ethnicity, protected veteran status, disability, or another protected group status.
Use of AI algorithms in preparing your responses to short questions is strictly prohibited.
2025 Internship Projects
Forming exoplanets is similar to baking. If you change the ingredients from which they are made, you can make entirely different types of planets. For example, increasing the heat for a rocky exoplanet can easily turn it into a lava world. Since planets form out of the same material as their host star, we will use stellar elemental abundance data combined with planet masses and radii to understand different planet populations. In this project, you will analyze a population of known exoplanets and determine how composition and location impact planet populations. As you go through this project, you will learn how changing the elemental abundances and location of planets in our galaxy can impact their composition and evolution. Additionally, you will learn valuable skills in programming, statistics, data analysis, and data visualization. Completion of coursework in physics at the 100 and 200 levels is preferred, but not required. No prior programming experience is required.
Recommended prerequisites: 100 and 200-level physics classes.
Debris disks are remnants of planetary system formation, offering a window into the evolution of planetary systems like our own Solar System. By studying debris disks, we can indirectly learn about the presence and properties of planets that may be shaping these structures. In this project, the intern will analyze images of a debris disk from infrared to radio wavelengths. We will aim to understand the disk structure and dust properties using radiation transfer simulations. The intern will learn about the physics of planetary systems and how to interpret astronomical observations to uncover the physical characteristics of the disks. Throughout the process, the intern will gain valuable skills in scientific computing, programming, image processing, and data visualization. The intern is expected to have some basic knowledge of physics. No prior programming experience is required.
Recommended prerequisites: Basic knowledge of physics.
Superconductivity is an emergent phenomenon in which a material exhibits zero electrical resistance and perfect diamagnetism below a critical temperature. Superconducting materials have potential to revolutionize modern technology, yet critical transition temperatures are often too low for wide-spread practical applications. Recent breakthrough research has demonstrated record-high transition temperatures in compounds containing light elements , however the pressures required for stability are very large. This project will focus on the synthesis and characterization of new light-element compounds, including hydrides, which are expected to exhibit remarkably high transition temperatures at near-ambient pressures. Students will learn synthesis and characterization protocols for these novel materials, and learn fundamental physical and chemical concepts related to superconductivity and other physical properties. Students with basic training in physics, chemistry, materials science and/or related fields are encouraged to apply.
Recommended prerequisites: Basic training in physics, chemistry, materials science and/or related fields.
How do planetary systems form and evolve? What new exoplanets are waiting to be discovered? In this project, we will apply machine learning methods to large exoplanet datasets to identify patterns that reveal trends in planetary system architecture, predict the presence of undiscovered planets, and guide future astronomical observations. The intern will learn to curate data from the NASA Exoplanet Archive and utilize machine learning methods to explore exoplanet data. The intern will also develop a deeper understanding of state-of-the-art exoplanetary science, including exoplanet demographics, characterization, and formation. As a result, the intern will gain experience in all aspects of planetary informatics, including data resource management, data visualization, data analysis, the interpretation of machine learning models, and the communication of key scientific findings. The intern is expected to have some degree of experience in coding, preferably in R.
Recommended prerequisites: Experience in coding, preferably in R.
The Earth's record of meteorite / asteroid impacts is key to understanding delivery of volatiles and carbonaceous materials to the early earth. The project would seek to utilize Raman imaging spectroscopy to map the distribution of carbonaceous materials within impacted terrestrial rocks and elucidate the nature of co-occurring minerals in these rocks. From these observations it may be possible to further analyze the minerals using microprobe and electron microscopy to understand the interaction of extraterrestrial carbonaceous materials delivered to the Earth during the impact process. Specific examples of carbonaceous species of interest that would be formed during the impact process are graphite, graphite whiskers, diamonds and other high temperature polymorphs.
Recommended prerequisites: None.
The processes controlling the behavior, budget, and recycling of elements and volatiles in Earth's interior are fundamental to our knowledge of how the solid Earth, its oceans, and atmosphere came to be and have evolved. Understanding how volatile elements dissolve in magma and fluids within Earth's interior is crucial for analyzing mass and energy movement, melting and crystallization, and the formation of rocks. Here, we focus on the partitioning of nitrogen and hydrogen sulfide between silicate (and carbonate) melts with aqueous solutions at pressure and temperature conditions resembling the Earth’s upper mantle. We will employ novel experimental and analytical techniques to study melt/fluid interaction at in-situ conditions. Together, we will explore aspects of experimental geosciences, but no prior knowledge on the subject is required. Students attending Community Colleges are encouraged to apply.
Recommended prerequisites: None.
The origins of Earth’s volatile elements as complex organic molecules come from early Solar System Objects. Research conducted on campus has shown that primitive solar system objects could have been subjected to thermal processes altering their chemical composition. As members of the NASA OSIRIS-Rex Team, we analyze organic solids from the return mission from asteroid Bennu to understand their thermal history. We see evidence that this material evolves through complex chemical kinetics. This project involved a series of hand-on experiments to understand the evolution of organic molecules under conditions of Solar System early evolution. The ultimate goal would be to decipher the processes that might have affected primitive Solar System Objects, such as the asteroid Bennu. The intern student will be trained in experimental organic geochemistry and in advanced spectroscopic analytical methods, such as Nuclear Magnetic Resonance spectroscopy.
Recommended prerequisites: None.
Is there life beyond Earth? In 2023, Carnegie scientists pioneered a brand-new technique for searching for life in the cosmos based on machine learning. The accuracy and applicability of this biosignature technique rely on a breadth of data collected by a laboratory method called “pyrolysis–gas chromatography–mass spectrometry” (pyGCMS). In this project, we will explore scores of synthetic carbon-rich samples using pyGCMS. Not only will the student intern help build the training data set for the next-generation machine learning model, but they will also pioneer the analyses of enigmatic specimens from the early Earth that may contain remnants of ancient life. As a result, the intern will become an expert in the pyGCMS analytical technique, gain experience in data processing and data analysis, learn the basics of machine learning, and gain valuable experience in the communication of key scientific findings.
Recommended prerequisites: None.
Are you passionate about Earth sciences and eager to dive into the world of geochemistry? Join us as an intern to explore how micro-materials, such as diamonds and their inclusions, reveal hidden processes deep within our planet. This project addresses big questions, from tracking water’s journey in Earth’s interior to understanding how critical elements accumulate in ore deposits. As an intern, you will gain hands-on experience with state-of-the-art geochemical tools, including electron microscopy and advanced isotope analysis techniques. You’ll learn to characterize and analyze rocks and minerals and develop valuable skills in data management, visualization, and interpretation. By the end of this internship, you’ll have practical experience in cutting-edge geochemistry and have gained a new perspective on how geochemistry can illuminate hidden deep-Earth processes. Students majoring in geology are encouraged to apply.
Recommended prerequisites: Geology major.
To better quantify timescales of how Earth will respond to anthropogenic climate change, we must investigate timing and rates of environmental and ecosystem perturbations in the past. This internship will expose you to multiple aspects of geochronology, the science of applying ages to the rock record. You will gain laboratory experience in pursuit of quantifying the timing and climatic effect of volcanism around the Caribbean during the Cretaceous. You will also perform a literature-based investigation of hiatuses in the Early Miocene deep-sea sedimentary record, to inform our understanding of the timing of changes in oceanographic processes across an interval of biotic transition. By the end of this internship, you will gain experience in mineral separation techniques, extracting information from scientific papers, analyzing and visualizing scientific data, talking with scientific collaborators, and the ways we make sure records from across the Earth system are temporally “on the same page.” The student is expected to have completed at least one geology course, with additional coursework in Earth system science, stratigraphy/sedimentology, and/or oceanography preferred. No prior laboratory or research experience is required.
Recommended prerequisites: None.
The thermal history of the core and mantle and their dynamics is one of the most fundamental topics in geophysics. It is related to the processes of planetary accretion and differentiation, the time evolution of mantle and core temperatures, and the generation of Earth’s magnetic field. The thermal conductivity of materials in the Earth’s and planetary interiors is the key to understanding these phenomena.Thermal conductivity depends on the depth at which the materials reside and their composition and spin state. These dependencies will be explored via investigations of materials of various composition/state and variable pressure-temperature conditions. These questions will be addressed by direct measurements of thermal conductivity of Earth’s minerals and alloys in a laser heated diamond anvil cell at extreme pressure-temperature conditions representative for the Earth’s interior. Students should be expected to have some familiarity with optics and spectroscopy.
Recommended prerequisites: Familiarity with optics and spectroscopy.
Frequently Asked Questions
We are proud to say that the Earth and Planets Laboratory is an REU site!
Undergraduate students supported with NSF funds must be citizens, permanent residents, or nationals of the United States or its territories.
From the National Science Foundation website:
NSF funds a large number of research opportunities for undergraduate students through its REU Sites program. An REU Site consists of a group of ten or so undergraduates who work in the research programs of the host institution. Each student is associated with a specific research project, where he/she works closely with the faculty and other researchers. Students are granted stipends and, in many cases, assistance with housing and travel. Undergraduate students supported with NSF funds must be citizens or permanent residents of the United States or its possessions. An REU Site may be at either a US or foreign location.
Because the project is funded through the National Science Foundation, EPIIC interns must be U.S. citizens, U.S. nationals, or U.S. permanent residents. If you do not meet this requirement, please reach out to the EPL HR representative Lauren Gilmer at gilmer@carnegiescience.edu to discuss other options.
Yes. We consider applications from current seniors, even if you would potentially be attending our program after you graduate. If this applies to you, please include a brief description of your plans in the "other information" part of the application (e.g. I’ve applied to graduate schools, I want to take a year off and work, I have a job lined up at Observatory X / Research Lab Y, etc.). However, preference will be given to students not beyond rising seniors at the beginning of the program.
Our program is primarily intended for students pursuing STEM degrees and careers. We will also consider applications from students pursuing a degree in a related field like engineering or mathematics if there is a clear connection expressed to one of the research subfields on our campus.
Interns are required to stay at our accommodation at AU, which is a few miles from EPL by car, bus, and/or walking. If this presents any issues, please contact the program coordinator.
This program does not accept high school students.
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