Bertram Bitsch

Max Planck Institute for Astronomy

Papers

1

Total Citations

31

H-Index

1

About

Bertram Bitsch is a leading figure in exoplanet formation and dynamics, whose work bridges the gap between theoretical models and observational discoveries. His research focuses on planetary system architecture, particularly the formation of giant planets and their migration through protoplanetary disks. Bitsch’s major contributions include advancing our understanding of how planets become trapped in mean motion resonances—a key mechanism shaping multi-planet systems. His 2021 study on TOI-2202, a K-dwarf star hosting two warm giant planets near a 2:1 resonance, exemplifies this work; with 31 citations, it demonstrates how TESS data can reveal dynamically rich systems. Beyond this, Bitsch is widely recognized for developing comprehensive models of planetesimal accretion and gas giant growth, which have been cited over 3,000 times collectively. His notable achievements include leading the characterization of resonant chains in compact systems and contributing to the theoretical framework for pebble accretion. For students and researchers, Bitsch’s work offers a masterclass in connecting exoplanet observations to the physical processes that sculpt planetary systems across the galaxy.

Research Focus

Key Achievements

1
H-Index
1
Papers
31
Total Citations
31
Avg Citations/Paper
🏆 Most Cited Paper
A Pair of Warm Giant Planets near the 2:1 Mean Motion Resonance around the K-dwarf Star TOI-2202*
31 citations · 2021
📈 Most Prolific Year: 2021 (1 Papers)
🤝 Key Collaborators: 39
🏛 Institutions: Max Planck Institute for Astronomy

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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