activity
20142022
most citedVolumes and bulk densities of forty asteroids from ADAM shape modeling

103 citations · 577 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.EP2022★ 5 cited

The equilibrium shape of (65) Cybele: primordial or relic of a large impact?

M. Marsset, M. Brož, J. Vermersch +24

Cybele asteroids constitute an appealing reservoir of primitive material genetically linked to the outer Solar System, and the physical properties of the largest members can be rea…

astro-ph.EP2021★ 29 cited

(216) Kleopatra, a low density critically rotating M-type asteroid

F. Marchis, L. Jorda, P. Vernazza +36

Context. The recent estimates of the 3D shape of the M/Xe-type triple asteroid system (216) Kleopatra indicated a density of 5 g.cm. Such a high density implies a high metal…

astro-ph.EP2021★ 23 cited

An advanced multipole model for (216) Kleopatra triple system

M. Brož, F. Marchis, L. Jorda +37

To interpret adaptive-optics observations of (216) Kleopatra, we need to describe an evolution of multiple moons, orbiting an extremely irregular body and including their mutual in…

astro-ph.EP2021★ 29 cited

Evidence for differentiation of the most primitive small bodies

B. Carry, P. Vernazza, F. Vachier +40

Dynamical models of Solar System evolution have suggested that P-/D-type volatile-rich asteroids formed in the outer Solar System and may be genetically related to the Jupiter Troj…

astro-ph.EP2020★ 25 cited

Binary asteroid (31) Euphrosyne: Ice-rich and nearly spherical

B. Yang, J. Hanus, B. Carry +38

Asteroid (31) Euphrosyne is one of the biggest objects in the asteroid main belt and the Euphrosyne family occupies a highly inclined region in the outer main belt and contains a r…

astro-ph.EP2019★ 18 cited

(704) Interamnia: A transitional object between a dwarf planet and a typical irregular-shaped minor body

J. Hanuš, P. Vernazza, M. Viikinkoski +56

With an estimated diameter in the 320 to 350 km range, (704) Interamnia is the fifth largest main belt asteroid and one of the few bodies that fills the gap in size between the fou…

astro-ph.EP2019★ 17 cited

The shape of (7) Iris as evidence of an ancient large impact?

J. Hanuš, M. Marsset, P. Vernazza +35

Asteroid (7) Iris is an ideal target for disk-resolved imaging owing to its brightness (V7-8) and large angular size of 0.33 arcsec during its apparitions. Iris is believed t…

astro-ph.EP2019★ 26 cited

Closing the gap between Earth-based and interplanetary mission observations: Vesta seen by VLT/SPHERE

R. JL. Fétick, L. Jorda, P. Vernazza +34

Context. Over the past decades, several interplanetary missions have studied small bodies in situ, leading to major advances in our understanding of their geological and geophysica…

astro-ph.EP2018★ 66 cited

(16) Psyche: A mesosiderite-like asteroid?

M. Viikinkoski, P. Vernazza, J. Hanus +35

Asteroid (16) Psyche is the target of the NASA Psyche mission. It is considered one of the few main-belt bodies that could be an exposed proto-planetary metallic core and that woul…

astro-ph.EP2017★ 39 cited

Adaptive optics and lightcurve data of asteroids: twenty shape models and information content analysis

Matti Viikinkoski, Josef Hanus, Mikko Kaasalainen +2

We present shape models and volume estimates of twenty asteroids based on relative photometry and adaptive optics images. We discuss error estimation and the effects of myopic deco…

astro-ph.EP2017★ 46 cited

3D shape of asteroid (6)~Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondrites

M. Marsset, B. Carry, C. Dumas +15

Context. The high-angular-resolution capability of the new-generation ground-based adaptive-optics camera SPHERE at ESO VLT allows us to assess, for the very first time, the crater…

astro-ph.EP2017★ 103 cited

Volumes and bulk densities of forty asteroids from ADAM shape modeling

Josef Hanus, Matti Viikinkoski, Franck Marchis +11

Disk-integrated photometric data of asteroids do not contain accurate information on shape details or size scale. Additional data such as disk-resolved images or stellar occultatio…

astro-ph.EP2016★ 22 cited

Shape model of asteroid (130) Elektra from optical photometry and disk-resolved images from VLT/SPHERE and Nirc2/Keck

Josef Hanus, Franck Marchis, Matti Viikinkoski +2

Asteroid (130) Elektra belongs to one of the six known triple asteroids in the main belt, so its mass has been reliably determined. We aim to use all available disk-resolved images…

astro-ph.EP2015★ 67 cited

ADAM: a general method for using various data types in asteroid reconstruction

Matti Viikinkoski, Mikko Kaasalainen, Josef Durech

We introduce ADAM, the All-Data Asteroid Modelling algorithm. ADAM is simple and universal since it handles all disk-resolved data types (adaptive optics or other images, interfero…

astro-ph.EP2014★ 62 cited

The Puzzling Mutual Orbit of the Binary Trojan Asteroid (624) Hektor

F. Marchis, J. Durech, J. Castillo-Rogez +9

Asteroids with satellites are natural laboratories to constrain the formation and evolution of our solar system. The binary Trojan asteroid (624) Hektor is the only known Trojan as…