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Extreme AO Observations of Two Triple Asteroid Systems with SPHERE

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

We present the discovery of a new satellite of asteroid (130) Elektra - S/2014 (130) 1 - in differential imaging and in integral field spectroscopy data over multiple epochs obtained with SPHERE/VLT. This new (second) moonlet of Elektra is about 2 km across, on an eccentric orbit and about 500 km away from the primary. For a comparative study, we also observed another triple asteroid system (93) Minerva. For both systems, component-resolved reflectance spectra of the satellites and primary were obtained simultaneously. No significant spectral difference was observed between the satellites and the primary for either triple system. We find that the moonlets in both systems are more likely to have been created by sub-disruptive impacts as opposed to having been captured.

years

2026 2

verdicts

UNVERDICTED 2

representative citing papers

Shape, Orientation and Colors Combined approach for Asteroids (SOCCA)

astro-ph.EP · 2026-06-16 · unverdicted · novelty 6.0

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.

citing papers explorer

Showing 2 of 2 citing papers.

  • Shape, Orientation and Colors Combined approach for Asteroids (SOCCA) astro-ph.EP · 2026-06-16 · unverdicted · none · ref 66 · internal anchor

    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.

  • Configuration of the $\xi$ Tau system constrained by multi-technique observations astro-ph.SR · 2026-05-21 · unverdicted · none · ref 223 · internal anchor

    Multi-technique observations constrain the configuration of the ξ Tau system, detecting orbital oscillations on multiple timescales and suggesting component C is itself a binary.