Exoplanets, -moons, -comets

HiDef Neighbors: Solar System Objects As Exoplanet Analogs I. Gaseous Objects, Planets, Planetary Systems, And Small Bodies

By Keith Cowing
Status Report
Astronomy & Astrophysics
March 27, 2026
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HiDef Neighbors: Solar System Objects As Exoplanet Analogs I. Gaseous Objects, Planets, Planetary Systems, And Small Bodies
Fully corrected and calibrated albedos of Titan (yellow), Saturn (green), Uranus (blue), and Neptune (red) covering 0.3 µm to 2.1 µm, offset for clarity. Regions of strong telluric absorption are masked in lighter shades, and it should be noted that they are less reliably corrected. The flat regions in the UV were flagged as bad pixels in all images by X-shooter. We also highlight a vertical discontinuity between the VIS and NIR arms of Titan, which is likely due to weather inconsistency. The colors used for these objects are the same in the following figures. — Astronomy & Astrophysics

Context. Intermediate-resolution spectral observations are vital tools for characterizing the composition and physical properties of Solar System bodies in detail. At present, the planets and moons of our Solar System remain the only planetary environments for which spatially resolved high-quality spectroscopic data are obtainable. Observations that provide such data can advance knowledge of the Solar System and establish reference points for future exoplanet observations with next-generation telescopes.

Aims. We present a library of intermediate-resolution (R ≈ 10000) spectra, with this first paper of the HiDef Neighbors project focusing on Saturn, Uranus, Neptune, and Titan’s atmospheres. We provide homogeneous, high S/N (≈250) data for comparative studies and modeling. While other projects have presented high S/N broad-wavelength data of individual objects, they vary widely in resolution, calibration standards, and observing strategies, limiting their comparability. We used one instrument, consistent calibrations, and a single reduction pipeline, with images obtained near opposition to ensure consistent phase geometry. We also address how the methane distribution differs between gas and ice giants within our data. We provide constraints on the methane distribution, as our dataset allows for direct comparison of the Solar System gas giants and serves as a benchmark for future atmospheric studies.

Methods. We obtained spectra using X-shooter in the Integral Field Unit mode, covering a spectral range of 0.3 μm to 2.1 μm. The data were integrated, cleaned of telluric absorption features using MOLECFIT, and refined by removing solar absorption lines and applying Doppler corrections.

Results. We present the resulting spectra for the selected Solar System objects and a number of equivalent widths for methane absorptions. These spectra are publicly available and will be a valuable resource for future atmospheric investigations and comparative planetology studies.

HiDef Neighbors: Solar System objects as exoplanet analogs I. Gaseous objects, Planets, planetary systems, and small bodies, Astronomy & Astrophysics (Open access)

Astrobiology, exoplanet,

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻