Samuel N. Mellon

University of Rochester

Papers

1

Total Citations

12

H-Index

1

About

Samuel N. Mellon is an astrophysicist specializing in stellar pulsations, exoplanetary systems, and debris disk dynamics. His research focuses on the intersection of young stars and planetary system formation, particularly through the detection of variable phenomena in bright, nearby stars. Mellon’s most cited work, the 2019 discovery of δ Scuti pulsations in the young hybrid debris disk star HD 156623, leveraged data from the bRing robotic observatory network—originally built to monitor β Pictoris b’s circumplanetary material. This finding, with 12 citations, revealed that HD 156623 exhibits both a debris disk and rapid stellar oscillations, making it a rare laboratory for studying star-disk interactions. By demonstrating that bRing’s photometric survey could uncover unexpected stellar variability, Mellon expanded the utility of exoplanet-focused instrumentation. His contributions bridge stellar astrophysics and exoplanet science, offering new insights into how young stars’ internal structures influence their surrounding planetary nurseries. Mellon’s work exemplifies how serendipitous discoveries from targeted surveys can advance our understanding of stellar evolution and debris disk systems.

Research Focus

Key Achievements

1
H-Index
1
Papers
12
Total Citations
12
Avg Citations/Paper
🏆 Most Cited Paper
Discovery of δ Scuti Pulsations in the Young Hybrid Debris Disk Star HD 156623
12 citations · 2019
📈 Most Prolific Year: 2019 (1 Papers)
🤝 Key Collaborators: 13
🏛 Institutions: University of Rochester

Top Papers

  1. 1

Key Collaborators

Contact & Links

Available for collaboration
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