Visible Analysis of NASA Lucy Mission Targets Eurybates, Polymele, Orus and Donaldjohanson
arXiv:1907.11451 · doi:10.1016/j.icarus.2019.113463
Abstract
Jupiter Trojan asteroids are minor bodies that share Jupiter's orbit around the Sun. Although not yet well understood in origin and composition, they have surface properties that, besides being comparable with other populations of small bodies in the Solar System, hold information that may restrict models of planetary formation. Due their importance, there has been a significant increase in an interest in studying this population. In this context arises the NASA Lucy Mission, with a planned launch of 2021. The Lucy Mission will be the first one to address a group of 6 objects with the aim of investigating, in detail, their nature. In order to provide valuable information for mission planning and maximize the scientific return, we carried out ground based observations of four targets of the mission. Aimed at looking for variabilities on the spectra of (3548) Eurybates, (15094) Polymele and (21900) Orus, we performed rotationally resolved visible spectroscopy of them at SOAR Telescope. We also analyzed the first visible spectrum obtained for the main belt asteroid (52246) Donaldjohanson at Gran Telescopio Canarias. The spectra of Orus and Polymele present rather homogeneous characteristics along the surfaces, and their taxa correspond with those of the two dominant populations in the Trojan population, the P- and the D-type group of objects. Spectroscopy of Eurybates, on the other side, suggests that some variation on the characteristics of the reflectance of this body could be related with its collisional history. Donaldjohanson, the only main belt object in the group of targets, shows, according to our visible spectrum, hints of the presence of hydrated materials. Lucy mission will investigate the surface composition of these targets and will shed light on their connections with other minor bodies populations and in their role on the evolution of the Solar System.
10 pages, 5 figures
References in corpus (18)
- Main Belt Asteroids with WISE/NEOWISE I: Preliminary Albedos and Diameters
- Phase reddening on near-Earth asteroids: Implications for mineralogical analysis, space weathering and taxonomic classification
- Identification and Dynamical Properties of Asteroid Families
- Near-Infrared Spectroscopy of Trojan Asteroids: Evidence for Two Compositional Groups
- WISE/NEOWISE Observations of the Jovian Trojans: Preliminary Results
- WISE/NEOWISE Observations of the Jovian Trojan Population: Taxonomy
- Visible spectroscopic and photometric survey of Jupiter Trojans: final results on dynamical families
- A hypothesis for the color bimodality of Jupiter Trojans
- High Precision Photometry of Extreme KBO 2003 EL61
- The differing magnitude distributions of the two Jupiter Trojan color populations
- Compositional study of asteroids in the Erigone collisional family using visible spectroscopy at the 10.4 m GTC
- Eurybates - the only asteroid family among Trojans?
- The 3-4 m Spectra of Jupiter Trojan Asteroids
- A Near-Infrared Search for Silicates in Jovian Trojan Asteroids
- PRIMASS visits Hilda and Cybele groups
- Time-Resolved Near-Infrared Photometry of Extreme Kuiper Belt Object Haumea
- Asteroids and the James Webb Space Telescope
- A Peculiar Family of Jupiter Trojans: the Eurybates
Cited by in corpus (5)
- The Distribution of Highly Red-sloped Asteroids in the Middle and Outer Main Belt
- Characterisation of the new target of the NASA Lucy mission: asteroid 152830 Dinkinesh (1999 VD57)
- JWST Near Infrared Spectroscopy of High Albedo Jupiter Trojans: A New Surface Type in the Trojan Belt
- Astrocladistics of the Jovian Trojan Swarms
- Ultraviolet Spectroscopy of Lucy Mission Targets with the Hubble Space Telescope