# Hubble Ultraviolet Spectroscopy of Jupiter Trojans

## TL;DR

This study presents the first ultraviolet spectra of Jupiter Trojans, revealing spectral differences between subpopulations and challenging previous hypotheses about their surface compositions.

## Contribution

It provides novel UV spectral data for Jupiter Trojans and analyzes their spectral features, offering new insights into their surface compositions and origins.

## Key findings

- Spectral differences between less-red and red Trojans in UV range
- Absence of discernible absorption features in UV spectra
- H2S alone unlikely responsible for color bimodality

## Abstract

We present the first ultraviolet spectra of Jupiter Trojans. These observations were carried out using the Space Telescope Imaging Spectrograph on the Hubble Space Telescope and cover the wavelength range 200-550 nm at low resolution. The targets include objects from both of the Trojan color subpopulations (less-red and red). We do not observe any discernible absorption features in these spectra. Comparisons of the averaged UV spectra of less-red and red targets show that the subpopulations are spectrally distinct in the UV. Less-red objects display a steep UV slope and a rollover at around 450 nm to a shallower visible slope, whereas red objects show the opposite trend. Laboratory spectra of irradiated ices with and without H$_{2}$S exhibit distinct UV absorption features; consequently, the featureless spectra observed here suggest H$_{2}$S alone is not responsible for the observed color bimodality of Trojans, as has been previously hypothesized. We propose some possible explanations for the observed UV-visible spectra, including complex organics, space weathering of iron-bearing silicates, and masked features due to previous cometary activity.