Proposals for the masses of the three largest asteroids, the Moon-Earth mass ratio and the astronomical unit
From MaRDI portal
Publication:642272
DOI10.1007/S10569-009-9203-8zbMath1223.70050OpenAlexW2063277795WikidataQ55871749 ScholiaQ55871749MaRDI QIDQ642272
Publication date: 26 October 2011
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://zenodo.org/record/1000691
Related Items (5)
The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for fundamental astronomy ⋮ Validated numerics for period-tupling and touch-and-go bifurcations of symmetric periodic orbits in reversible systems ⋮ Constraining the electric charges of some astronomical bodies in Reissner-Nordström spacetimes and generic \(r ^{ - 2}\)-type power-law potentials from orbital motions ⋮ EFFECTS OF STANDARD AND MODIFIED GRAVITY ON INTERPLANETARY RANGES ⋮ Dynamical portrait of the Lixiaohua asteroid family
This page was built for publication: Proposals for the masses of the three largest asteroids, the Moon-Earth mass ratio and the astronomical unit