Proper Elements Catalogs
The catalogs contain proper orbital elements of numbered asteroids and main-belt comets computed numerically by means of a synthetic theory by Knežević & Milani (2000,2003).
There are however some differences between the procedure proposed by aforementioned authors and the one used to produce the catalogs available here:
- Orbits of all asteroids are numerically propagated for 10 Myr
- All numerical integrations are made within the same dynamical model
- All proper elements calculations are performed using the same version of the software
Asteroid proper orbital elements (available for 1,052,382 objects in total, as of October 2022):
Numbered asteroids (596,526 objects):
- afp.num.pro (file size: ~63MB)    
- afp.num.sig (file size: ~50MB)    
Multi-opposition asteroids (455,856 objects):
- afp.mult.pro (file size: ~48MB)      
- afp.mult.sig (file size: ~38MB)      
Proper orbital elements for active main-belt asteroids:
Information on the format of the catalogs:
The format of files containing proper elements:
- Column 1: Asteroid number/designation
- Column 2: Absolute magnitude   (Note: The flag '99.99' is used when the information is not available.)
- Column 3: Proper semi-major axis [au]
- Column 4: Proper eccentricity
- Column 5: Sine of proper inclination
- Column 6: Proper frequency of mean motion [deg/yr]
- Column 7: Proper frequency of perihelion longitude [arcsec/yr]
- Column 8: Proper frequency of nodal longitude [arcsec/yr]
- Column 9: Lyapunov time [kyr]
- Column10: Integration time span [Myr]
The format of files containing standard deviations of proper elements residuals:
- Column 1: Asteroid number/designation
- Column 2: Root-mean-square error of proper semi-major axis
- Column 3: Root-mean-square error of eccentricity
- Column 4: Root-mean-square error of sine of proper inclination
- Column 5: Root-mean-square error of proper of mean motion frequency [deg/yr]
- Column 6: Root-mean-square error of proper perihelion longitude frequency [arcsec/yr]
- Column 7: Root-mean-square error of proper nodal longitude frequency [arcsec/yr]
Referencing the proper elements dataset:
If your publication is based on the asteroid proper elements dataset, please cite the following work as a general reference for the AFP portal:Bojan Novaković, David Vokrouhlický, Federica Spoto and David Nesvorný: Asteroid Families: properties, recent advances and future opportunities 2022, Celest Mech Dyn Astro, 134, id. 34