(121514) 1999 UJ7: A primitive, slow-rotating Martian Trojan

TL;DR

This study characterizes asteroid 1999 UJ7 as a primitive, slow-rotating Martian Trojan with potential hydrated minerals, suggesting an origin beyond the snow line and complex rotational behavior.

Contribution

It provides the first detailed spectral and photometric analysis of 1999 UJ7, revealing its primitive composition and possible non-principal axis rotation.

Findings

Spectral features suggest a C-complex taxonomy.

Possible presence of hydrated minerals indicated by absorption features.

Complex photometric behavior hints at non-principal axis rotation.

Abstract

Aims. The goal of this investigation is to determine the origin and surface composition of the asteroid (121514) 1999 UJ7, the only currently known L4 Martian Trojan asteroid. Methods. We have obtained visible reflectance spectra and photometry of 1999 UJ7 and compared the spectroscopic results with the spectra of a number of taxonomic classes and subclasses. A light curve was obtained and analysed to determine the asteroid spin state. Results. The visible spectrum of 1999 UJ7 exhibits a negative slope in the blue region and the presence of a wide and deep absorption feature centred around ~0.65 microns. The overall morphology of the spectrum seems to suggest a C-complex taxonomy. The photometric behaviour is fairly complex. The light curve shows a primary period of 1.936 d, but this is derived using only a subset of the photometric data. The asteroid may be in a non-principal axis rotational state, but our observational coverage is insufficient to draw definitive conclusions. Conclusions. Although the observed spectral absorption is wider and deeper, this finding may be compatible with the 0.7 microns spectral feature exhibited by some Ch-type asteroids and could possibly be interpreted as diagnostic of the presence of hydrated minerals. The inferred composition of 1999 UJ7 as a primitive object can be consistent with a volatile-rich object originally accreted beyond the snow line of the solar system and subsequently evolved to reach the inner regions of the solar system.