SUMMARY
LEDA 074886, or PGC 74886, is a dwarf galaxy located approximately 70 million light-years away, characterized by its unusual rectangular shape. The prevailing hypothesis suggests that this unique morphology results from the collision of two disk galaxies. This phenomenon highlights the complex interactions in galactic formations and raises questions about the evolutionary processes of dwarf galaxies.
PREREQUISITES
- Understanding of galactic morphology and classifications
- Familiarity with astronomical distance measurements (light-years and parsecs)
- Knowledge of galaxy collision dynamics
- Basic concepts of dwarf galaxies and their characteristics
NEXT STEPS
- Research the dynamics of galaxy collisions and their effects on morphology
- Explore the classification of dwarf galaxies in astronomical studies
- Investigate the implications of galactic interactions on star formation
- Learn about observational techniques used in studying distant galaxies
USEFUL FOR
Astronomers, astrophysicists, and students of cosmology interested in galactic structures and the effects of galactic collisions on morphology.