Planetary Sciences Group
University of Central Florida
The UCF Planetary Sciences Group uses spacecraft, telescopes, meteorites, moon rocks, laboratories, and supercomputers to investigate our own Solar System as well as others around the Galaxy.
Our Research
Atmospheric Evolution and Habitability
Our research group develops atmospheric models of varying complexity (1D, 2D, 3D) to simulate the atmospheres and habitability of the rocky worlds in our solar system (i.e., Venus, Earth, Mars, Titan) and assess their atmospheric/climatic evolution through time.
Dust Dynamics
We are studying the dynamics of dust particles in various solar system environments, including near the lunar surface, asteroid surface, ring systems, and in interplanetary space. This can include motion due to impacts and other disturbances or the motion of charged dust particles in plasma and electric fields.
Exoplanets and Brown Dwarfs
The Exoplanets Group uses space telescopes to reveal the sizes, temperatures, atmospheric properties, and orbits of many planets and brown dwarfs outside our solar system. We develop new theory and models to interpret and understand those data. We also lead several open-source software projects that provide tools for exoplanet research to the astronomical community.
Laboratory Astrophysics
We trace the molecular basis for the evolution of interstellar clouds, the formation of Solar Systems, the incorporation of molecular species into planetary bodies, including comets and meteorites and how these systems evolve in time. Astrochemistry is often a culmination of different fields acting synergistically.
Laboratory Surface Science
We study the physical properties and compositions of the Moon, asteroids, and Mars. The surfaces of these bodies are covered with a fine-grained particulate regolith (or soil) that marks the boundary between internal geologic processes, and the space environment. What are these regoliths made of? How did they form and how have they evolved over time? Most important: what can this tell us about the earliest history of the solar system and the formation of planets?
Microgravity and Planet Formation
Simulations of planet formation that begin with planetesimals have reached a state where the main properties of the solar system are reproduced. Formation of planetesimals themselves remains poorly understood, however. The role of gravitational instabilities in the disk is not known. The outcome of interactions of small aggregates and dust in the presence of the protoplanetary nebula is also poorly understood.
Planetary Rings
We are studying the structure, composition, and evolution of Saturn’s rings through a combination of analysis of data from the Cassini Ultraviolet Imaging Spectrograph (UVIS) and numerical modeling of the rings. We combine multiple stellar occultations to understand the three-dimensional structure of the rings in the same way doctors use CT scans to study the structure of the body. These occultations provide exquisitely detailed maps of the finest structures in the rings which we can then compare to N-body simulations to better understand the dynamics of the rings and their origins.
Small Bodies
“Small bodies” are big on science! Small bodies are comets, asteroids, trans-Neptunian objects (TNOs), Trojans, and Centaurs that are all remnants from the planetary formation era 4 ½ billion years ago. Studying these objects’ behavior and evolution allows us to answer some of the most fundamental questions in astronomy and planetary science.
Academic Programs
Our Latest Papers
| Authors | Title | Published Date | Journal |
|---|---|---|---|
| Abarzuza, Fernando; Pinilla-Alonso, Noemí; Serra-Ricart, Miquel; and 2 coauthors | On the rotation of M-type asteroids: Statistical evidence for higher rotation rates | Nov 2026 | Icarus 458, 117187 |
| Cai, Yanqing; Wu, Ziwei; Zhu, Weiwei; and 24 coauthors | Probing Variations in Earth’s Ionosphere Using Pulsars | Sep 2026 | The Astrophysical Journal Letters 1008, L44 |
| Margoti, Giuliano; Braga-Ribas, Felipe; Ortiz, José Luis; and 176 coauthors | Size, Shape, Density, and Atmospheric Limit of (50000) Quaoar Revealed from 14 years of Stellar Occultation | Sep 2026 | The Astrophysical Journal 1008, 159 |
| Roselló Del Valle, Lorraine; Donaldson Hanna, Kerri L.; Chazallon, Bertrand; and 3 coauthors | MicroRaman Spectroscopy of Carbonaceous Chondrites to Constrain Peak Metamorphic Temperature and Mineralogy | Aug 2026 | The Planetary Science Journal 7, 204 |
| Cartwright, Richard J.; Cryan, Sasha; Brunetto, Rosario; and 15 coauthors | Tracing the Source of Carbon Oxides on the Large Moons of Uranus | Aug 2026 | The Planetary Science Journal 7, 199 |
| McClure, Lucas T.; Emery, Joshua P.; Takir, Driss; and 8 coauthors | The Polana-Eulalia Complex with JWST NIRSpec: Connections to Bennu, Ryugu, and Outer Solar System Bodies | Aug 2026 | The Planetary Science Journal 7, 194 |
| Milliken, Ralph E.; Hiroi, Takahiro; Hamilton, Victoria E.; and 8 coauthors | The role of composition in the spectral evolution of carbonaceous asteroids as informed by Bennu sample return | Aug 2026 | Meteoritics and Planetary Science 61, 1875 |
| Hamilton, V. E.; Cloutis, E. A.; Milliken, R. E.; and 30 coauthors | Visible, near-, and thermal infrared spectra of asteroid Bennu samples: Relationship to and implications for remote sensing of carbonaceous asteroids | Aug 2026 | Meteoritics and Planetary Science 61, 1788 |
| de Oliveira Gradovski, Eros; Braga-Ribas, Felipe; Gomes-Junior, Altair R.; and 63 coauthors | Rigorous Use of Light-curve Inversion and Stellar Occultation Techniques for Deriving a Scaled Three-dimensional Shape for the Jupiter Trojan (911) Agamemnon | Aug 2026 | The Astrophysical Journal 1007, 102 |
| Catani, Luan M.; Morgado, Bruno E.; Gradovski, Eros; and 49 coauthors | An Irregular Shape of the Jupiter Trojan (3317) Paris Revealed by Stellar Occultations and Rotational Light Curves | Aug 2026 | The Astronomical Journal 172, 120 |
Query returned 1144 total number of records, 10 are shown.
