ThousandWorlds: A Benchmark For Climate Emulation Of Potentially Habitable Exoplanets
Dataset overview. Output fields are defined on a 32 × 64 latitude–longitude grid. There are 53 fields in…
Quantifying Surface Heterogeneity Across Asteroid (101955) Bennu using Candidate Site Remote Sensing Data
Locations of the four candidate sites across a 2D map projection of Bennu’s surface captured by the OSIRIS-REx…
An Unidentified Absorption Feature At 5.11 μm On The Surface Of Titan And Pluto From JWST Spectroscopy
NIRSpec average spectrum of Titan (black) compared with a radiative transfer calculation in which the surface albedo decreases…
An 800-Million-Year-Old Impact Shower on the Terrestrial Planets from the Breakup of the Eulalia Parent Body
Schematic illustrating the evolutionary stages of the Eulalia asteroid family. (a) The Eulalia parent body resides near the…
Transport of Water In A Transient, Impact-Generated Atmosphere On Mercury
Initial structure of the Impact Plume 60 s post impact. The impactor strikes from the left, at a…
HWO Target Stars and Systems: Activity and Rotation Catalog (ARC) of Potential Target Stars for the Habitable Worlds Observatory
Upper panels: Equatorial rotational velocity (veq) vs. projected rotational velocity (v sin i) for stars in Tiers 1,…
Constraints On The Crystallinity Of Water Ice In Planet-forming Disks From Infrared Scattered-Light Spectra
Protoplanetary disk images (top row) and scattered-/transmitted-light spectra (bottom-left and bottom-middle) obtained from the radiative-transfer simulations, together with…
Astrometric Exoplanet Detection Survives Solar-like Stellar Contamination
A demonstration of the limitations of the PSPT data processing pipeline, which did not process the limb uniformly…
Maximum Lifetime Of The Vegetative Biosphere
ExoCAM simulations of Earth from the present up to 2.0 Gyr in the future, assuming CO2 remains fixed…
The Multi-planet System TOI-5624: Four Transiting Sub-Neptunes With An Outer Companion Revealed By Transit-timing Variations
Stability analysis of the TOI-5624 planetary system focusing on planet f. We vary the orbital period Pf and…
Icy Volatile Enhancements in Evolving Protoplanetary Disks
Outer disk regions become increasingly H2O ice poor as compared to dominating N2, CO, and CO2 ices over…
The Identification of CS2 and Evidence for Carbon-Sulfur Chemical Coupling in a Warm Giant Exoplanet Atmosphere
The retrieved transmission spectrum using the results from the free retrieval plotted as a black line, along with…