Dust Grain Orbital Behavior Around Ceres

@article{Nazzario2002DustGO,
  title={Dust Grain Orbital Behavior Around Ceres},
  author={Raymond Charles Nazzario and Truell W. Hyde and Laura Bringol Barge},
  journal={Advances in Space Research},
  year={2002},
  volume={31},
  pages={2591-2597}
}

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References

SHOWING 1-10 OF 18 REFERENCES

The Electric Charging of Interstellar Dust in the Solar System and Consequences for Its Dynamics

The motion of the solar system relative to the local interstellar medium causes a flux of neutral gas and dust into the solar system. When interstellar dust particles penetrate into the solar system,

DUST LEVITATION ON ASTEROIDS

Abstract In comparison to the lunar regolith, asteroidal regoliths appear to be deficient in dust and in agglutinates, i.e., in particles ≤100 μm across. On asteroid surfaces of high electrical

The Collisional History of Asteroid 253 Mathilde

Abstract Asteroid 253 Mathilde is found to have a collisional lifetime of approximately 4 billion years, essentially indistinguishable from the age of the Solar System. However, uncertainties in our

Radiation forces on small particles in the solar system

Imaging of asteroid 433 eros during NEAR's flyby reconnaissance

During the 23 December 1998 flyby of asteroid 433 Eros, the Near-Earth Asteroid Rendezvous (NEAR) spacecraft obtained 222 images of Eros and reveal an elongated, cratered body with a linear feature extending for at least 20 kilometers.

Astrophysical Data : Planets and Stars

This volume collects reference information for astronomers and astrophysicists, ranging from fundamental physical constants to orbital data for selected asteroids. For the Earth and planets, it