SOCCA extends HG1G2 by modeling the projected surface of a rotating triaxial ellipsoid to jointly retrieve absolute magnitude, phase parameters, spin state, and shape from sparse multi-band photometry, halving residuals and tripling precision on LSST simulations and Eugenia data.
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astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
A Hamiltonian framework maps coupled spin-orbit, spin-spin, and doubly synchronous resonances in ellipsoid binary asteroids and identifies a secondary resonance from nonlinear coupling between primary and secondary synchronous modes.
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Shape, Orientation and Colors Combined approach for Asteroids (SOCCA)
SOCCA extends HG1G2 by modeling the projected surface of a rotating triaxial ellipsoid to jointly retrieve absolute magnitude, phase parameters, spin state, and shape from sparse multi-band photometry, halving residuals and tripling precision on LSST simulations and Eugenia data.
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Resonant Networks of Spin-Orbit Coupling in Ellipsoid-Ellipsoid Binary Asteroid Systems
A Hamiltonian framework maps coupled spin-orbit, spin-spin, and doubly synchronous resonances in ellipsoid binary asteroids and identifies a secondary resonance from nonlinear coupling between primary and secondary synchronous modes.