Collection Information
|
IDENTIFIER |
urn:nasa:pds:ast.nesvorny.families:data::1.0
|
NAME |
data collection for the "NESVORNY HCM ASTEROID FAMILIES" bundle
|
TYPE |
Data
|
DESCRIPTION |
This is the data collection for the ast.nesvorny.families bundle.
This data set contains asteroid
dynamical family memberships for 122 families calculated from
synthetic proper elements, including high-inclination families. These
families were calculated by David Nesvorny (Nesvorny et al. 2015)
using his code based on the Hierarchical Clustering Method (HCM)
described in Zappala et al. (1990, 1994). The input synthetic proper
elements for 384,337 numbered asteroids were calculated by Knezevic
and Milani.
|
SEARCH/ACCESS DATA |
NESVORNY HCM ASTEROID FAMILIES Online
|
|
|
Citation |
DIGITAL OBJECT IDENTIFIER (DOI) |
10.26033/6cg5-pt13 (from parent bundle)
|
AUTHOR LIST |
Nesvorny, D.
|
EDITOR LIST |
|
PUBLICATION YEAR |
2015
|
DESCRIPTION |
This is the data collection for the ast.nesvorny.families bundle.
This data set contains asteroid
dynamical family memberships for 122 families calculated from
synthetic proper elements, including high-inclination families. These
families were calculated by David Nesvorny (Nesvorny et al. 2015)
using his code based on the Hierarchical Clustering Method (HCM)
described in Zappala et al. (1990, 1994). The input synthetic proper
elements for 384,337 numbered asteroids were calculated by Knezevic
and Milani.
|
|
|
Context |
START DATE TIME |
1965-01-01T12:00:00.000Z
|
STOP DATE TIME |
N/A (ongoing)
|
LOCAL MEAN SOLAR TIME |
|
LOCAL TRUE SOLAR TIME |
|
SOLAR LONGITUDE |
|
PRIMARY RESULT PURPOSE |
SCIENCE
|
PRIMARY RESULT PROCESSING LEVEL |
Derived
|
PRIMARY RESULT DESCRIPTION |
|
PRIMARY RESULT WAVELENGTH RANGE |
|
PRIMARY RESULT DOMAIN |
|
PRIMARY RESULT DISCIPLINE NAME |
Small Bodies
Small Bodies
|
INVESTIGATION |
NO SPECIFIC INVESTIGATION
|
OBSERVING SYSTEM |
|
OBSERVING SYSTEM COMPONENT |
Various Ground-Based Telescopes
Various Ground-Based Detectors
|
TARGET |
MULTIPLE ASTEROIDS
|
REFERENCES |
|