A contact binary satellite of the asteroid (152830) Dinkinesh
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Summary
This summary is machine-generated.Small asteroids like Dinkinesh experience significant changes due to radiative torques (YORP effect). Observations reveal Dinkinesh has a complex structure and a unique satellite, Selam, likely formed from ejected material.
Area Of Science
- Planetary Science
- Asteroid Research
- Spacecraft Observation
Background
- Small asteroids (<5 km) exhibit complex evolutionary histories.
- The Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect significantly influences small asteroid dynamics.
- (152830) Dinkinesh is an S-type asteroid in the inner main belt.
Purpose Of The Study
- To investigate the complex nature of small asteroid (152830) Dinkinesh.
- To characterize the surface features and satellite of Dinkinesh.
- To understand the formation mechanism of Dinkinesh's satellite, Selam.
Main Methods
- Close-proximity flyby observations by the Lucy spacecraft.
- Analysis of geomorphologic features and orbital dynamics.
- Assessment of the system's angular momentum and tidal locking.
Main Results
- Dinkinesh (720 m diameter) displays a prominent longitudinal trough and equatorial ridge.
- Discovery of the first confirmed contact binary asteroid satellite, (152830) Dinkinesh I Selam.
- Selam (210 m and 230 m lobes) orbits Dinkinesh with a 52.7 h period and is tidally locked.
Conclusions
- Dinkinesh's features likely resulted from mass shedding due to YORP spin-up, followed by reaccretion.
- Selam likely formed from material ejected during Dinkinesh's mass-shedding event.
- The YORP effect is a critical factor in the evolution and satellite formation of small asteroids.

