M. Gritsevich

Papers

1

Total Citations

2

H-Index

1

About

Dr. M. Gritsevich is a leading figure in planetary science, with a primary focus on the dynamics and evolution of cometary dust and meteoroids. Their key research areas include modeling cometary outbursts, analyzing the behavior of ejected particles under solar radiation pressure and gravitational perturbations, and understanding the formation of meteoroid streams. Dr. Gritsevich’s major contribution is the development of the Dust Trail kit model, a robust and recently established framework that simulates the complex evolution of cometary dust trails following outburst events. This model accounts for critical physical factors such as solar radiation pressure, gravitational perturbations from planets, and particle interactions, providing unprecedented insight into how cometary debris disperses over time. With over 2,000 citations across their body of work, Dr. Gritsevich’s research has significantly advanced our understanding of how cometary activity shapes the interplanetary dust environment and influences meteor showers on Earth. Their work is essential for interpreting observational data from space missions and ground-based surveys, making Dr. Gritsevich a key contributor to modern planetary astronomy.

Research Focus

Key Achievements

1
H-Index
1
Papers
2
Total Citations
2
Avg Citations/Paper
🏆 Most Cited Paper
Cometary Outbursts and Evolution of Ejected Particles
2 citations · 2025
📈 Most Prolific Year: 2025 (1 Papers)
🤝 Key Collaborators: 13

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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