PDS_VERSION_ID = PDS3 /* File Characteristics */ RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 32 FILE_RECORDS = 315 /* Data Object Pointers */ ^TABLE = "smasspc.tab" /* Identification Keywords */ DATA_SET_ID = "EAR-A-M3SPEC-3-RDR-SMASS-V1.0" PRODUCT_NAME = "SMASS Principal Components Table" PRODUCT_ID = "SMASS-SMASSPC-199604" INSTRUMENT_HOST_NAME = "MICHIGAN-DARTMOUTH-MIT OBSERVATORY" INSTRUMENT_NAME = "MARK III SPECTROGRAPH" TARGET_NAME = ASTEROID START_TIME = 1990 STOP_TIME = 1994 PRODUCT_CREATION_TIME = 1996-03-29 /* Peer Review Date */ RECORD_FORMAT = "(i5,1x,a8,1x,f7.3,1x,f6.3)" /* Data Object Descriptions */ OBJECT = TABLE ROWS = 315 ROW_BYTES = 32 INTERCHANGE_FORMAT = ASCII COLUMNS = 4 DESCRIPTION = "Principal component analysis (PCA) is a multivariate analysis technique that transforms a set of correlated variables into a new set of uncorrelated variables called principal components. PCA requires no underlying assumptions. The principal components are linear combinations of the original variables and are derived in decreasing order of importance, so that the first principal component accounts for the largest possible amount of variance within the dataset. The second principal component will account for the second largest amount of the original variance. For this dataset, polynomial fits to the scaled reflectances formed the original variable set from which the principal components were derived. The first and second principal components, containing 870f the variance distribution information, are included here. The first principal component appears to be correlated to the ultraviolet absorption band and the second to the near-infrared absorption band. Prior to performing the PCA, the spectra were fitted with high (7th to 9th) order polynomials as a means of smoothing the data. From this smoothing, 50 points were chosen from the polynomial with wavelength coverage ranging from 4800 to 9700 A, with a point for every 100 A. The spectrum of asteroid 5145 Pholus is so different from that of the other asteroids surveyed that it would fall far away from the others in principal component space. Asteroid 5154 Pholus was omitted from the analysis for that reason. See Xu et al. 1995 (Icarus 115, 1-35) for further information and discussion." OBJECT = COLUMN COLUMN_NUMBER = 1 NAME = "ASTEROID CATALOG NUMBER" DESCRIPTION = "For unnumbered asteroids, this field will be blank. For these asteroids, see the next field, ASTEROID PROVISIONAL DESIGNATION, for the identification of the asteroid." DATA_TYPE = ASCII_INTEGER START_BYTE = 1 BYTES = 5 FORMAT = I5 END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 2 NAME = "ASTEROID PROVISIONAL DESIGNATION" DESCRIPTION = "For numbered asteroids, this field will be blank. For these asteroids, see the previous field, ASTEROID CATALOG NUMBER, for the asteroid identification." DATA_TYPE = CHARACTER START_BYTE = 7 BYTES = 8 FORMAT = A8 END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 3 NAME = "FIRST PRINCIPAL COMPONENT" DATA_TYPE = ASCII_REAL START_BYTE = 16 BYTES = 7 FORMAT = "F7.3" END_OBJECT = COLUMN OBJECT = COLUMN COLUMN_NUMBER = 4 NAME = "SECOND PRINCIPAL COMPONENT" DATA_TYPE = ASCII_REAL START_BYTE = 24 BYTES = 6 FORMAT = "F6.3" END_OBJECT = COLUMN END_OBJECT = TABLE END