Vesta, the second-largest object in the main asteroid belt, is believed to have been on its way to becoming a planet.
New research based on data from NASA's Dawn mission suggests that Vesta may be more uniform than previously thought.
Previous beliefs about Vesta included the presence of a core, mantle, and crust, but this new research challenges that notion.
The research indicates that Vesta's interior may not be as differentiated as previously assumed and may lack a well-defined core.
The lack of a core on Vesta has surprised scientists and led to the proposal of two hypotheses about its nature.
One hypothesis suggests that Vesta's differentiation process stalled, while the other proposes that Vesta is a broken-off chunk of a growing planet.
Further research is needed to determine which hypothesis is accurate and to unravel the mysteries surrounding Vesta's true nature.
The research challenges the established idea that Vesta is a planetary core that never grew very large, introducing doubt into previously held beliefs.
Scientists continue to investigate the origins and nature of Vesta, considering its potential significance in the early formation of the Solar System.
The findings highlight the complex history of Vesta and the unique processes that may have shaped its evolution.