ASTEROID PROPER ELEMENTS V1.0

Proper elements of asteroids are derived from the osculating orbital elements by correcting for the perturbations of the major planets to arrive at elements which are stable over time periods comparable to the age of the solar system. The purpose of computing proper elements is twofold, to detect asteroid 'families', which are dynamically related groupings of asteroids potentially of common origin, and to understand the dynamical structure of the asteroid belt.

Data and Resources

This dataset has no data

Additional Info

Field Value
Maintainer Thomas Morgan
Last Updated March 31, 2025, 12:25 (UTC)
Created March 31, 2025, 12:25 (UTC)
accessLevel public
accrualPeriodicity irregular
bureauCode {026:00}
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catalog_@id https://data.nasa.gov/data.json
catalog_conformsTo https://project-open-data.cio.gov/v1.1/schema
catalog_describedBy https://project-open-data.cio.gov/v1.1/schema/catalog.json
harvest_object_id bd6f9e99-7882-4e6e-997a-3d74c3ff914e
harvest_source_id 61638e72-b36c-4866-9d28-551a3062f158
harvest_source_title DNG Legacy Data
identifier urn:nasa:pds:context_pds3:data_set:data_set.ear-a-5-ddr-proper-elements-v1.0_287k-tc3c
issued 2018-06-26
landingPage https://pds.nasa.gov/ds-view/pds/viewDataset.jsp?dsid=EAR-A-5-DDR-PROPER-ELEMENTS-V1.0
modified 2023-01-26
programCode {026:005}
publisher National Aeronautics and Space Administration
references {https://pds.nasa.gov}
resource-type Dataset
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source_schema_version 1.1
theme {"Earth Science"}