Non-detection of CH4 and CO fluorescence in JWST spectra sets upper limits on their surface partial pressures at (3-10)×10^{-6} and (50-300)×10^{-6} nbar, well below the 100-200 nbar total pressure from occultation data.
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High-speed imaging of four lunar impact flashes reveals lower variance in initial intensity than total energy and no correlation between them, suggesting decoupled vapor and ejecta phases.
The paper assesses the feasibility of using SKA-AA4 for thermal detections and characterization of TNOs and Centaurs at cm wavelengths.
citing papers explorer
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Constraints on the Atmospheric Composition of 2002 XV$_{93}$ from JWST Spectroscopy
Non-detection of CH4 and CO fluorescence in JWST spectra sets upper limits on their surface partial pressures at (3-10)×10^{-6} and (50-300)×10^{-6} nbar, well below the 100-200 nbar total pressure from occultation data.
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High-Speed Observations of Lunar Impact Flashes
High-speed imaging of four lunar impact flashes reveals lower variance in initial intensity than total energy and no correlation between them, suggesting decoupled vapor and ejecta phases.
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Unveiling the Trans-Neptunian Region with the SKA
The paper assesses the feasibility of using SKA-AA4 for thermal detections and characterization of TNOs and Centaurs at cm wavelengths.