Backward simulation based on nominal orbital parameters (updated by Sam Deen ):
Backward simulation based on nominal orbital parameters available on 15-October-2022
Backward simulation based on nominal orbital parameters (updated by Sam Deen ):
Backward simulation based on nominal orbital parameters available on 15-October-2022
See this MPML message and related thread about this probable asteroid cluster.
Using Sam Deen's updated orbital elements, we get this result from a backward simulation performed with Mercury6 software:
2022 QB59 and 2022 RM50 are likely to have separated from a common parent body.
Best wishes,
Alessandro Odasso