Estimating the mass of asteroid 433 eros during the NEAR spacecraft flyby

DK Yeomans; PG Antreasian; A Cheng; DW Dunham; RW Farquhar; RW Gaskell; JD Giorgini; CE Helfrich; AS Konopliv; JV McAdams; JK Miller; WM Owen Jr; PC Thomas; J Veverka; BG Williams

doi:10.1126/science.285.5427.560

Estimating the mass of asteroid 433 eros during the NEAR spacecraft flyby

Science. 1999 Jul 23;285(5427):560-1. doi: 10.1126/science.285.5427.560.

Authors

DK Yeomans¹, PG Antreasian, A Cheng, DW Dunham, RW Farquhar, RW Gaskell, JD Giorgini, CE Helfrich, AS Konopliv, JV McAdams, JK Miller, WM Owen Jr, PC Thomas, J Veverka, BG Williams

Affiliation

¹ Navigation and Flight Mechanics Section at the Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA. Cornell University, Ithaca, NY.

PMID: 10417380
DOI: 10.1126/science.285.5427.560

Abstract

The Near Earth Asteroid Rendezvous (NEAR) spacecraft flew within 3830 kilometers of asteroid 433 Eros on 23 December 1998. The gravitational perturbation on NEAR was evident in the spacecraft tracking data. Ground-based Doppler and range tracking of the spacecraft as well as spacecraft images of the asteroid's center of figure and surface features were used to determine the mass and rotation pole of Eros. The mass of Eros is (7.2 +/- 1.8) x 10(18) grams and, coupled with a volume estimate provided by the NEAR imaging team, this mass suggests a bulk density of 2.5 +/- 0.8 grams per cubic centimeter. The rotation pole position is 15.6 (+/-3.7) degrees in right ascension and 16.4 (+/-1.8) degrees in declination, which is consistent with ground-based and NEAR imaging team observations.