NEAR Radio Science Subsystem Gravity and Landmark Files ======================================================= The following information was included in the data set catalog file of the original data submission. The "Parameters" section has been edited to reflect the current state of the files in this collection. Data Set Overview ================= This data set includes a 15x15 gravity model for Eros derived from radio and landmark tracking of the NEAR spacecraft, several images/maps, and a file of surface landmarks. The gravity model and images/maps were produced by Alex Konopliv of the NEAR Radio Science Team at the NASA Jet Propulsion Laboratory. The landmark file was compiled by the NEAR Navigation Team and was used in the solution for the gravity field. Parameters ========== The gravity model is defined by a set of spherical harmonic coefficients -- GM, Cmn, and Smn. These can be evaluated to give the gravitational potential of Eros. The coefficients and their individual uncertainties are provided in one ASCII table file. The covariance table is supplied in a separate ASCII file. General model parameters (GM, pole position, etc.) are included in the labels of both these files. Several image files contain digital maps of Bouguer anomaly and radial gravity acceleration where the gravity field has been evaluated to degree and order less than the full 15x15 range in the model. The truncation reduces noise in the maps resulting from uncertainty in the higher degree and order coefficients. Three maps are provided, truncated to orders 5, 6 and 7. The landmark file contains rotation information for Eros and X, Y, and Z coordinates for the centers of craters identified on its surface. Processing ========== Spherical harmonic models and maps were derived from raw radio tracking data in several steps. The gravity field coefficients were obtained by solving systems of equations with about 5000 unknowns. Radio tracking data in long arcs were delimited mostly by propulsive maneuvers and were used in solutions which were obtained iteratively and by least squares. Maps of vertical gravity acceleration and Bouguer anomaly were generated from the spherical harmonic model(s) evaluated at regular grid points. Coordinate System ================= The gravity model, maps, and landmark file use the IAU 1994 right ascension and declination system [DAVIESETAL1996A]. The Eros prime meridian is fixed at 326.08 degrees. Overview ======== Data in this archive have been reduced as part of mission data analysis activities of the NEAR Radio Science Team. Data of questionable validity have been omitted from the solutions. Data Coverage and Quality ========================= The data included in this archive were collected during the NEAR orbital phase from 2000-02-14 to 2001-02-12.