Passion for understanding
Neutron Stars and Pulsars
The dense, rapidly rotating remnants left after some supernova events, emitting beams of radiation When massive stars reach the end of their lives in a core-collapse supernova, their cores can...
Neutron Stars and Pulsars
The dense, rapidly rotating remnants left after some supernova events, emitting beams of radiation When massive stars reach the end of their lives in a core-collapse supernova, their cores can...
High-Mass Stars: Supergiants and Core-Collapse ...
How massive stars rapidly burn through nuclear fuels and explode, influencing their surroundings Whereas lower-mass stars evolve relatively gently into red giants and white dwarfs, massive stars (≥8 M⊙) follow...
High-Mass Stars: Supergiants and Core-Collapse ...
How massive stars rapidly burn through nuclear fuels and explode, influencing their surroundings Whereas lower-mass stars evolve relatively gently into red giants and white dwarfs, massive stars (≥8 M⊙) follow...
Low-Mass Stars: Red Giants and White Dwarfs
The evolutionary path of Sun-like stars after core hydrogen depletion, ending as compact white dwarfs When a Sun-like star or other low-mass star (roughly ≤8 M⊙) finishes its main sequence...
Low-Mass Stars: Red Giants and White Dwarfs
The evolutionary path of Sun-like stars after core hydrogen depletion, ending as compact white dwarfs When a Sun-like star or other low-mass star (roughly ≤8 M⊙) finishes its main sequence...
Nuclear Fusion Pathways
Proton-proton chain vs. CNO cycle, and how core temperature and mass determine fusion processes At the heart of every shining main sequence star lies a fusion engine, where light nuclei...
Nuclear Fusion Pathways
Proton-proton chain vs. CNO cycle, and how core temperature and mass determine fusion processes At the heart of every shining main sequence star lies a fusion engine, where light nuclei...
Main Sequence Stars: Hydrogen Fusion
The long, stable phase where stars fuse hydrogen in their cores, balancing gravitational collapse with radiation pressure At the heart of nearly every star’s life story lies the main sequence—a...
Main Sequence Stars: Hydrogen Fusion
The long, stable phase where stars fuse hydrogen in their cores, balancing gravitational collapse with radiation pressure At the heart of nearly every star’s life story lies the main sequence—a...
Molecular Clouds and Protostars
How cold, dense clouds of gas and dust collapse to form new stars in stellar nurseries Amid the seemingly empty vastness between the stars, enormous clouds of molecular gas and...
Molecular Clouds and Protostars
How cold, dense clouds of gas and dust collapse to form new stars in stellar nurseries Amid the seemingly empty vastness between the stars, enormous clouds of molecular gas and...