Journal Article

A basin-free spherical shape as an outcome of a giant impact on asteroid Hygiea

Jorda, L., Dumas, C., Durech, J., Lamy, P., Vigan, A., Michalowski, T., Witasse, O., Rambaux, N., Gillon, M., Brož, M., Podlewska-Gaca, E., Tanga, P., Benkhaldoun, Z., Birlan, M., Vernazza, P., Santana-Ros, T., Ferrais, M., Le Coroller, H., Szakats, R., Carry, B., DeMeo, F., Ševeček, P., Maestre, J. L., Marchis, F., Bartczak, P., Drouard, A., Dudzinski, G., Kryszczynska, A., Viikinkoski, M., Kaasalainen, M., Hanuš, J., Berthier, J., Fusco, T., Duffard, R., Colas, F., Chapman, A., Cipriani, F., Marsset, M., Jehin, E., Vachier, F., Castillo-Rogez, J., Grice, J., Yang, B., Marciniak, A., Michel, P., Hirsch, R., Fetick, R.

2020

Overview

(10) Hygiea is the fourth largest main belt asteroid and the only known asteroid whose surface composition appears similar to that of the dwarf planet (1) Ceres 1 , 2 , suggesting a similar origin for these two objects. Hygiea suffered a giant impact more than 2 Gyr ago 3 that is at the origin of one of the largest asteroid families. However, Hygeia has never been observed with sufficiently high resolution to resolve the details of its surface or to constrain its size and shape. Here, we report high-angular-resolution imaging observations of Hygiea with the VLT/SPHERE instrument (~20 mas at 600 nm) that reveal a basin-free nearly spherical shape with a volume-equivalent radius of 217 ± 7 km, implying a density of 1,944 ± 250 kg m − 3 to 1 σ . In addition, we have determined a new rotation period for Hygiea of ~13.8 h, which is half the currently accepted value. Numerical simulations of the family-forming event show that Hygiea’s spherical shape and family can be explained by a collision with a large projectile (diameter ~75–150 km). By comparing Hygiea’s sphericity with that of other Solar System objects, it appears that Hygiea is nearly as spherical as Ceres, opening up the possibility for this object to be reclassified as a dwarf planet. SPHERE at the VLT observed Hygiea, the fourth largest body in the main belt and the parent body of a big asteroid family, at unprecedented spatial resolution. Its unexpected spherical shape without any impact crater is explained by numerical simulations with a big impact that fluidized the body, reassembling it in a rotational equilibrium regime.

• Publisher: Nature Publishing Group UK,Nature Publishing Group,Springer Nature
• Subject: 704/445 / 704/445/848 / Asteroids / Astronomy / Astrophysics / Astrophysics and Cosmology / Aérospatiale, astronomie & astrophysique / Earth and Planetary Astrophysics / hygiea / Letter / Physical, chemical, mathematical & earth Sciences / Physics / Physics and Astronomy / Physique, chimie, mathématiques & sciences de la terre / Sciences of the Universe / Space science, astronomy & astrophysics