Touching an asteroid and coming back: OSIRIS-REx and Bennu
This Tuesday October 20th at around 23.12 hr (Canary time) the NASA space probe OSIRIS-REx will make its first attempt to collect samples from the asteroid...
V-type candidates and Vesta family asteroids in the Moving Objects VISTA (MOVIS) catalogue
Context. Basaltic asteroids (spectrally classified as V-types) are believed to be fragments of large differentiated bodies. The majority of them are found in...
Visible and near-infrared observations of asteroid 2012 DA14 during its closest approach of February 15, 2013
Context. Near-Earth asteroid 2012 DA14 made its closest approach on February 15, 2013, when it passed at a distance of 27 700 km from the Earth's surface. It...
Visible spectra of (474640) 2004 VN112-2013 RF98 with OSIRIS at the 10.4 m GTC: evidence for binary dissociation near aphelion among the extreme trans-Neptunian objects
The existence of significant anisotropies in the distributions of the directions of perihelia and orbital poles of the known extreme trans-Neptunian objects...
Visible spectroscopy of the Polana-Eulalia family complex: Spectral homogeneity
The Polana-Eulalia family complex is located in the inner part of the asteroid belt, bounded by the ν6 and the 3:1 resonances, where we can find another three...
Visible spectroscopy of the Sulamitis and Clarissa primitive families: a possible link to Erigone and Polana
The low-inclination (i 8∘) primitive asteroid families in the inner main belt, that is, Polana-Eulalia, Erigone, Sulamitis, and Clarissa, are considered to be...
Water in Ryugu as a property of processes in its parent body
Context. Samples from the asteroid Ryugu provide key information on the initial composition and evolutionary processes of primitive bodies. Aims. This study...
Water-ice-driven Activity on Main-Belt Comet P/2010 A2 (LINEAR)?
The dust ejecta of Main-Belt Comet P/2010 A2 (LINEAR) have been observed with several telescopes at the Observatorio del Roque de los Muchachos on La Palma...
When the horseshoe fits: Characterizing 2023 FY<SUB>3</SUB> with the 10.4 m Gran Telescopio Canarias and the Two-meter Twin Telescope
Context. The Arjuna asteroid belt is loosely defined as a diverse group of small asteroids that follow dynamically cold, Earth-like orbits. Most of them are not...