Minor orbital drifts in binary near-Earth asteroids (175706) 1996 FG3 and (385186) 1994 AW1: Implications for their orbital dynamics
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F25%3A00640482" target="_blank" >RIV/67985815:_____/25:00640482 - isvavai.cz</a>
Result on the web
<a href="https://meetingorganizer.copernicus.org/EPSC-DPS2025/EPSC-DPS2025-69.html" target="_blank" >https://meetingorganizer.copernicus.org/EPSC-DPS2025/EPSC-DPS2025-69.html</a>
DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Minor orbital drifts in binary near-Earth asteroids (175706) 1996 FG3 and (385186) 1994 AW1: Implications for their orbital dynamics
Original language description
This study analyzes the orbital evolution of two binary near-Earth asteroids, (175706) 1996 FG3 and (385186) 1994 AW1, using photometric data collected between 1994 and 2024. The authors found that 1996 FG3 shows no significant orbital drift, suggesting a stable equilibrium between BYORP, binary Yarkovsky effects, and mutual tides. In contrast, 1994 AW1 exhibits a small inward drift, indicating active BYORP or Yarkovsky forces. These findings provide insights into the long-term dynamics and stability of binary asteroid systems
Czech name
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Czech description
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Classification
Type
O - Miscellaneous
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA23-04946S" target="_blank" >GA23-04946S: Study of evolutionary paths of asteroids driven by non-gravitational forces with photometric observations</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2025
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů