Near-perihelion observations of interstellar comet 3I/ATLAS with JUICE/MAJIS reveal CO2-driven activity, a ~10% CO2/H2O ratio, and tentative evidence for complex organic material in coma dust.
B., Kuesters, D., Shappee, B
4 Pith papers cite this work. Polarity classification is still indexing.
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SCAT DR1 delivers 1810 spectra of 1330 transients with classifications, fitted light curves, new redshifts for many host galaxies, and host properties as a testbed for photometric classification pipelines.
Post-perihelion spectra of 3I/ATLAS show reduced C2 depletion, asymmetric CN/metal outgassing, metal-CO correlation, and an unexplained [O I] residual after standard parent subtraction.
3I/ATLAS lost roughly 1–7 meters of its surface and ~10^9–10^10 kg of mass during its Solar System passage, based on fits to observed gas production rates.
citing papers explorer
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Near-perihelion activity and composition of 3I/ATLAS from JUICE/MAJIS observations
Near-perihelion observations of interstellar comet 3I/ATLAS with JUICE/MAJIS reveal CO2-driven activity, a ~10% CO2/H2O ratio, and tentative evidence for complex organic material in coma dust.
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SCAT Data Release 1: 1810 optical spectra of 1330 transients
SCAT DR1 delivers 1810 spectra of 1330 transients with classifications, fitted light curves, new redshifts for many host galaxies, and host properties as a testbed for photometric classification pipelines.
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Post-perihelion Coma Composition of the Interstellar Comet 3I/ATLAS from Optical Spectroscopy
Post-perihelion spectra of 3I/ATLAS show reduced C2 depletion, asymmetric CN/metal outgassing, metal-CO correlation, and an unexplained [O I] residual after standard parent subtraction.
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Assessment of the Mass Loss and Radius Change of 3I/ATLAS Based on Observed Production Rates
3I/ATLAS lost roughly 1–7 meters of its surface and ~10^9–10^10 kg of mass during its Solar System passage, based on fits to observed gas production rates.