Anton Ermakov
Assistant Professor of Aeronautics and Astronautics and, by courtesy, of Geophysics and of Earth and Planetary Sciences
Web page: http://web.stanford.edu/people/aie
Bio
Dr. Ermakov's research lies at the intersection of planetary science and planetary exploration by robotic means and focuses on studying the internal structure and evolution of the Solar System bodies ranging from asteroids to gas giants. In his research, Dr. Ermakov combines a diverse range of spacecraft data (e.g., spacecraft radiometric tracking, stereo-imaging, magnetometry, microwave radiometry and geologic mapping) with geophysical and orbital dynamics modeling to probe the interiors and histories of Solar System bodies.
Dr. Ermakov has been a member of the NASA Dawn mission team. Dawn was the first mission to orbit two small bodies in the Solar System: asteroid Vesta and dwarf Ceres. Small bodies are a time machine that lets us explore the environment in which planets formed. Combining gravity and topography data sets is one of the most powerful tool to study deep planetary interiors from orbit. Dr. Ermakov used gravity and shape data for detailed studies of asteroid Vesta's and dwarf planet Ceres's internal structures. The Dawn data have established a framework for future geophysical investigations of water-rich worlds in the outer Solar System such as Europa and Enceladus.
Currently, Dr. Ermakov is a participating scientist in the NASA’s Juno mission. Juno is currently orbiting Jupiter and has performed several flybys of the Jovian moons. Dr. Ermakov uses the data from the Juno’s instrument suite to study the interior of Jupiter and its satellites in context of their formation and evolution models.
He received an Engineer Degree in Space Geodesy from the Moscow State University of Geodesy and Cartography in 2010 and a Ph.D. in Planetary Sciences from the Massachusetts Institute of Technology in 2017. After receiving his doctorate degree, Dr. Ermakov was a post-doctoral scholar at the Jet Propulsion Laboratory and at the Earth and Planetary Science Department of the University of California, Berkeley. From 2021 to 2023, Dr. Ermakov was a research scientist at UC Berkeley's Space Sciences Lab.
Academic Appointments
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Assistant Professor, Aeronautics and Astronautics
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Assistant Professor (By courtesy), Geophysics
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Assistant Professor (By courtesy), Earth & Planetary Sciences
Honors & Awards
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Robert N. Noyce Faculty Fellow, School of Engineering, Stanford University (2024)
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Team Award for the development the Mercury gravity field model, Jet Propulsion Laboratory (2019)
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Asteroid 10680 Ermakov, Minor Planet Center (2017)
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NASA Group Achievement Award to the Dawn Gravity Team, NASA (2016)
Professional Education
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Ph.D., Massachusetts Institute of Technology, Planetary Science (2017)
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Engineer, Moscow State University of Geodesy and Cartography, Space Geodesy (2010)
Current Research and Scholarly Interests
I am interested in the formation and evolution of the Solar System bodies and the ways we can constrain planetary interiors by geophysical measurements.
2024-25 Courses
- How to Design a Space Mission: from Concept to Execution
AA 118N (Aut) - Orbital Mechanics and Attitude Dynamics
AA 179 (Spr) - Planetary Geophysics: Theory, Observational Techniques and Data Analysis
AA 234, EPS 233, GEOPHYS 243 (Win) - Planetary Science and Exploration Seminar
AA 299, EPS 375, GEOPHYS 375 (Aut, Win) -
Independent Studies (3)
- Directed Research and Writing in Aero/Astro
AA 190 (Aut, Sum) - Independent Study in Aero/Astro
AA 199 (Aut, Win, Spr, Sum) - Problems in Aero/Astro
AA 290 (Aut, Win, Spr)
- Directed Research and Writing in Aero/Astro
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Prior Year Courses
2023-24 Courses
- Orbital Mechanics and Attitude Dynamics
AA 179 (Spr)
- Orbital Mechanics and Attitude Dynamics
Stanford Advisees
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Doctoral Dissertation Reader (AC)
Zahra Ahmed -
Master's Program Advisor
Nick Bostock, Luca Castelletto, Santiago Thorup -
Doctoral (Program)
Prachet Jain, Riley Tam
All Publications
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Evaluating the Use of Seasonal Surface Displacements and Time-Variable Gravity to Constrain the Interior of Mars
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
2024; 129 (6)
View details for DOI 10.1029/2023JE008053
View details for Web of Science ID 001253251100001
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Microwave Observations of Ganymede's Sub-Surface Ice: I. Ice Temperature and Structure
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
2023; 128 (6)
View details for DOI 10.1029/2022JE007609
View details for Web of Science ID 001010117100001
- Next Generation Planetary Geodesy Keck Institute for Space Studies. 2023
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Probing the Icy Shell Structure of Ocean Worlds with Gravity-Topography Admittance
PLANETARY SCIENCE JOURNAL
2022; 3 (3)
View details for DOI 10.3847/PSJ/ac4d2b
View details for Web of Science ID 000913042000001
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Geophysics of Vesta and Ceres
Vesta and Ceres: Insights from the Dawn Mission for the Origin of the Solar System
Cambridge University Press. 2022: 173-196
View details for DOI 10.1017/9781108856324.015
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A Recipe for the Geophysical Exploration of Enceladus
PLANETARY SCIENCE JOURNAL
2021; 2 (4)
View details for DOI 10.3847/PSJ/ac06d2
View details for Web of Science ID 000917379800001
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Surface Roughness and Gravitational Slope Distributions of Vesta and Ceres
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
2019; 124 (1): 14-30
View details for DOI 10.1029/2018JE005813
View details for Web of Science ID 000459245700002
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Power Laws of Topography and Gravity Spectra of the Solar System Bodies
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
2018; 123 (8): 2038-2064
View details for DOI 10.1029/2018JE005562
View details for Web of Science ID 000448877500005
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Constraints on Ceres' Internal Structure and Evolution From Its Shape and Gravity Measured by the Dawn Spacecraft
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
2017; 122 (11): 2267-2293
View details for DOI 10.1002/2017JE005302
View details for Web of Science ID 000417851800004
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Ceres's obliquity history and its implications for the permanently shadowed regions
GEOPHYSICAL RESEARCH LETTERS
2017; 44 (6): 2652-2661
View details for DOI 10.1002/2016GL072250
View details for Web of Science ID 000399762700005
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Constraints on Vesta's interior structure using gravity and shape models from the Dawn mission
ICARUS
2014; 240: 146-160
View details for DOI 10.1016/j.icarus.2014.05.015
View details for Web of Science ID 000341171500011