Determination of the mass of Ceres based on the most gravitationally efficient close encounters

ISSN： 0035-8711

Source： Monthly Notices of the Royal Astronomical Society, Vol.419, Iss.3, 2012-01, pp. : 2725-2736

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

A New Determination of the Mass of (1) Ceres

By Kovačević A. Kuzmanoski M.

Earth, Moon, and Planets, Vol. 100, Iss. 1-2, 2007-04 ,pp. : 117-123

Springer Publishing Company

Access to resources Recommend Favorite

Why are most molecular clouds not gravitationally bound?

By Dobbs C. L. Burkert A. Pringle J. E.

Monthly Notices of the Royal Astronomical Society, Vol. 413, Iss. 4, 2011-06 ,pp. : 2935-2942

Oxford University Press

Access to resources Recommend Favorite

Close Encounters of Minor Bodies with the Earth

By Carusi A. Dotto E.

Icarus, Vol. 124, Iss. 2, 1996-12 ,pp. : 392-398

Academic Press

Access to resources Recommend Favorite

Asteroid close encounters characterization using differential algebra: the case of Apophis

By Armellin R. Di Lizia P. Bernelli-Zazzera F. Berz M.

Celestial Mechanics and Dynamical Astronomy, Vol. 107, Iss. 4, 2010-08 ,pp. : 451-470

Springer Publishing Company

Access to resources Recommend Favorite

A revised historical light curve of Eta Carinae and the timing of close periastron encounters

By Smith Nathan Frew David J.

Monthly Notices of the Royal Astronomical Society, Vol. 415, Iss. 3, 2011-08 ,pp. : 2009-2019

Oxford University Press

Access to resources Recommend Favorite