<sup>14</sup> NH, <sup>14</sup> ND, and <sup>15</sup> NH cometary fluorescence models and D/H measurement in NH

Context . NH, a product of dissociation of ammonia, NH 3 , produces emission lines in the visible spectral range and its (0–0) band has largely been observed in cometary spectra. An updated fluorescence model of NH allows measurement of the abundance of the NH radical. This fluorescence model can also shed light on the ongoing question of isotopic ratios in comets, particularly the D/H ratio. Aims . The aim of this NH fluorescence model is to have an updated model to access the line positions and intensities in order to identify new lines in the observed cometary spectra, compute new fluorescence efficiencies, and measure the isotopic ratios 14 ND/ 14 NH and 15 NH/ 14 NH. Methods . New laboratory Einstein coefficients from ExoMol enabled new fluorescence models for 14 NH, 14 ND, and 15 NH to be computed. To increase the signal-to-noise ratio, we then coadded selected emission lines to measure the isotopic ratios 14 NH/ 14 ND and 15 NH/ 14 NH in high-resolution spectra of the bright comets C/2002 T7 (LINEAR), C/2006 F6 (Lemmon), and 73P/Schwassmann-Wachmann obtained with UVES at the ESO Very Large Telescope. Results . Comparisons of the modeled spectrum of 14 NH and observed comet spectra taken at various heliocentric distances confirmed the accuracy of our model. New fluorescence efficiencies were calculated for the three isotopologs and found to be about 20% higher than in previous studies. We were able to measure an isotopic ratio 14 ND/ 14 NH of (2.7 ± 1.8) × 10 −3 in comet 73P, while no average ND line was detected in the two other comets. This is the first D/H ratio measured in the NH radical and it is in agreement with the 14 ND/ 14 NH upper limit of 0.006 found in Comet Hyakutake, and with the ratio (D/H) NH 3 = 1.1 × 10 −3 measured in Comet 67P during the Rosetta mission. Our measurement confirms that the D/H ratio is about one order of magnitude larger for cometary nitrogen-bearing molecules compared to water. No measurements could be carried out regarding the 15 NH/ 14 NH ratio, due to the limited shift between the lines of both isotopologs.

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Journal
Astronomy and Astrophysics
Published
2025-10-01
DOI
https://doi.org/10.1051/0004-6361/202555354
Primary Topic
Atmospheric Ozone and Climate
Type
article
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article

14 NH, 14 ND, and 15 NH cometary fluorescence models and D/H measurement in NH

J. Manfroid, E. Jehin, D. Hutsemékers, Pierre Hardy et al.
Astronomy and Astrophysics
Atmospheric Ozone and Climate
article

14 NH, 14 ND, and 15 NH cometary fluorescence models and D/H measurement in NH

J. Manfroid, E. Jehin, D. Hutsemékers, Pierre Hardy, P. Rousselot, Elsa Blond Hanten
article en

Abstract

Context . NH, a product of dissociation of ammonia, NH 3 , produces emission lines in the visible spectral range and its (0–0) band has largely been observed in cometary spectra. An updated fluorescence model of NH allows measurement of the abundance of the NH radical. This fluorescence model can also shed light on the ongoing question of isotopic ratios in comets, particularly the D/H ratio. Aims . The aim of this NH fluorescence model is to have an updated model to access the line positions and intensities in order to identify new lines in the observed cometary spectra, compute new fluorescence efficiencies, and measure the isotopic ratios 14 ND/ 14 NH and 15 NH/ 14 NH. Methods . New laboratory Einstein coefficients from ExoMol enabled new fluorescence models for 14 NH, 14 ND, and 15 NH to be computed. To increase the signal-to-noise ratio, we then coadded selected emission lines to measure the isotopic ratios 14 NH/ 14 ND and 15 NH/ 14 NH in high-resolution spectra of the bright comets C/2002 T7 (LINEAR), C/2006 F6 (Lemmon), and 73P/Schwassmann-Wachmann obtained with UVES at the ESO Very Large Telescope. Results . Comparisons of the modeled spectrum of 14 NH and observed comet spectra taken at various heliocentric distances confirmed the accuracy of our model. New fluorescence efficiencies were calculated for the three isotopologs and found to be about 20% higher than in previous studies. We were able to measure an isotopic ratio 14 ND/ 14 NH of (2.7 ± 1.8) × 10 −3 in comet 73P, while no average ND line was detected in the two other comets. This is the first D/H ratio measured in the NH radical and it is in agreement with the 14 ND/ 14 NH upper limit of 0.006 found in Comet Hyakutake, and with the ratio (D/H) NH 3 = 1.1 × 10 −3 measured in Comet 67P during the Rosetta mission. Our measurement confirms that the D/H ratio is about one order of magnitude larger for cometary nitrogen-bearing molecules compared to water. No measurements could be carried out regarding the 15 NH/ 14 NH ratio, due to the limited shift between the lines of both isotopologs.

Astronomy and AstrophysicsVol. 702
University of Liège (BE), Institut UTINAM (FR), Laboratoire Interdisciplinaire Carnot de Bourgogne (FR), Université Bourgogne Europe (FR), Université Marie et Louis Pasteur (FR)
Openalex Percentile: Top 68%
Atmospheric Ozone and Climate
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