My research interests focus on early Solar System processes. I aim to understand the evolution of the first solid bodies that formed around our Sun. These bodies, called planetesimals, were the building blocks of planets; those that remain in the Solar System today are known as asteroids. In my research, I use numerical models to quantify the collateral effects of hypervelocity collisions between planetesimals on their thermal and compaction histories.

Experience

  • –present
    Research Fellow, Imperial College London

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