1
|
Chen K, Yang D. Tandem MS Elucidation of the Late-Stage Degradation Mechanism of Nitroplasticizer. ACS OMEGA 2024; 9:36600-36608. [PMID: 39220529 PMCID: PMC11359627 DOI: 10.1021/acsomega.4c04923] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 05/24/2024] [Revised: 07/20/2024] [Accepted: 08/06/2024] [Indexed: 09/04/2024]
Abstract
Understanding the degradation behavior of nitroplasticizer (NP) and the subsequent production of nitro-organics is crucial for both environmental monitoring and material development. A nontargeted approach via LC-QTOF-MS was employed to thoroughly study the degradation mechanism of NP in its late aging stage. Both positive and negative modes of ESI were performed to increase the compound coverage. To shed light on the fragmentation behavior of NP degradants (e.g., compounds containing a high density of NO2 moieties and oxygen sites) in the positive mode, which is rarely reported, the high-resolution tandem MS information on precursor ions at m/z 251(+), 254(+), 266(+), and 270(+) and a pair of isomeric ions at m/z 284(+) was investigated to extract their common diagnostic ions and dissociation channels, including the neutral loss of 2,2-dinitropropanol, nitro-nitrite rearrangement, homolytic cleavage of NO2, and simple inductive cleavage. Additionally, leveraging the sensitivity for nitroaromatics in the negative polarity, negative ions m/z 182(-) and 233(-) are identified as dinitroaniline and dinitronaphthol, respectively, which confirm the secondary hydrolysis pathway of the antioxidant (e.g., N-phenyl-2-naphthylamine) postulated in our previous work. In addition to earlier findings, the detection of these eight degradants further supports the evidence of increased acid concentration and aging temperatures in the late-stage NP environment, which contribute to intricate degradation behaviors in different aging environments.
Collapse
Affiliation(s)
- Kitmin Chen
- MST-7: Engineered Materials,
Material Sciences and Technology Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, United States
| | - Dali Yang
- MST-7: Engineered Materials,
Material Sciences and Technology Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, United States
| |
Collapse
|
2
|
Poch O, Istiqomah I, Quirico E, Beck P, Schmitt B, Theulé P, Faure A, Hily-Blant P, Bonal L, Raponi A, Ciarniello M, Rousseau B, Potin S, Brissaud O, Flandinet L, Filacchione G, Pommerol A, Thomas N, Kappel D, Mennella V, Moroz L, Vinogradoff V, Arnold G, Erard S, Bockelée-Morvan D, Leyrat C, Capaccioni F, De Sanctis MC, Longobardo A, Mancarella F, Palomba E, Tosi F. Ammonium salts are a reservoir of nitrogen on a cometary nucleus and possibly on some asteroids. Science 2020; 367:367/6483/eaaw7462. [PMID: 32165559 DOI: 10.1126/science.aaw7462] [Citation(s) in RCA: 17] [Impact Index Per Article: 4.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/21/2019] [Revised: 10/11/2019] [Accepted: 02/14/2020] [Indexed: 11/02/2022]
Abstract
The measured nitrogen-to-carbon ratio in comets is lower than for the Sun, a discrepancy which could be alleviated if there is an unknown reservoir of nitrogen in comets. The nucleus of comet 67P/Churyumov-Gerasimenko exhibits an unidentified broad spectral reflectance feature around 3.2 micrometers, which is ubiquitous across its surface. On the basis of laboratory experiments, we attribute this absorption band to ammonium salts mixed with dust on the surface. The depth of the band indicates that semivolatile ammonium salts are a substantial reservoir of nitrogen in the comet, potentially dominating over refractory organic matter and more volatile species. Similar absorption features appear in the spectra of some asteroids, implying a compositional link between asteroids, comets, and the parent interstellar cloud.
Collapse
Affiliation(s)
- Olivier Poch
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France.
| | - Istiqomah Istiqomah
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Eric Quirico
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Pierre Beck
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France.,Institut Universitaire de France (IUF), Paris, France
| | - Bernard Schmitt
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Patrice Theulé
- Aix-Marseille Université, CNRS, Centre National d'Etudes Spatiales (CNES), Laboratoire d'Astrophysique de Marseille (LAM), Marseille, France
| | - Alexandre Faure
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Pierre Hily-Blant
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Lydie Bonal
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Andrea Raponi
- Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), 00133 Rome, Italy
| | - Mauro Ciarniello
- Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), 00133 Rome, Italy
| | - Batiste Rousseau
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Sandra Potin
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Olivier Brissaud
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Laurène Flandinet
- Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France
| | - Gianrico Filacchione
- Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), 00133 Rome, Italy
| | - Antoine Pommerol
- Physikalisches Institut, Sidlerstrasse 5, University of Bern, CH-3012 Bern, Switzerland
| | - Nicolas Thomas
- Physikalisches Institut, Sidlerstrasse 5, University of Bern, CH-3012 Bern, Switzerland
| | - David Kappel
- Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam, Germany.,Institute for Planetary Research, German Aerospace Center (DLR), 12489 Berlin, Germany
| | - Vito Mennella
- Istituto Nazionale di Astrofisica (INAF)-Osservatorio Astronomico di Capodimonte, Napoli, Italy
| | - Lyuba Moroz
- Institute for Planetary Research, German Aerospace Center (DLR), 12489 Berlin, Germany
| | - Vassilissa Vinogradoff
- CNRS, Aix-Marseille Université, Laboratoire Physique des Interactions Ioniques et Moléculaires (PIIM), Unité Mixte de Recherche (UMR) CNRS 7345, 13397 Marseille, France
| | - Gabriele Arnold
- Institute for Planetary Research, German Aerospace Center (DLR), 12489 Berlin, Germany
| | - Stéphane Erard
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (LESIA), Observatoire de Paris, Université Paris Sciences et Lettres (PSL), CNRS, Sorbonne Université, Université de Paris, 92195 Meudon, France
| | - Dominique Bockelée-Morvan
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (LESIA), Observatoire de Paris, Université Paris Sciences et Lettres (PSL), CNRS, Sorbonne Université, Université de Paris, 92195 Meudon, France
| | - Cédric Leyrat
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique (LESIA), Observatoire de Paris, Université Paris Sciences et Lettres (PSL), CNRS, Sorbonne Université, Université de Paris, 92195 Meudon, France
| | - Fabrizio Capaccioni
- Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), 00133 Rome, Italy
| | - Maria Cristina De Sanctis
- Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), 00133 Rome, Italy
| | - Andrea Longobardo
- Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), 00133 Rome, Italy.,Dipartimento di Scienze e Tecnologie (DIST), Università Parthenope, 80143 Napoli, Italy
| | - Francesca Mancarella
- Dipartimento di Matematica e Fisica "E. De Giorgi," Università del Salento, Lecce, Italy
| | - Ernesto Palomba
- Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), 00133 Rome, Italy
| | - Federico Tosi
- Istituto di Astrofisica e Planetologia Spaziali (IAPS), Istituto Nazionale di Astrofisica (INAF), 00133 Rome, Italy
| |
Collapse
|
3
|
Scrape PG, Chang CH, Nesbitt DJ. Suppressed-Doppler slit jet infrared spectroscopy of astrochemically relevant cations: ν1 and ν4 NH stretching modes in NH 3D +. J Chem Phys 2019; 151:084302. [DOI: 10.1063/1.5113962] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Affiliation(s)
- Preston G. Scrape
- JILA, National Institute of Standards and Technology and University of Colorado, Boulder, Colorado 80309, USA
| | - Chih-Hsuan Chang
- SpectraSensors, 4333 West Sam Houston Pkwy N., Houston, Texas 77043, USA
| | - David J. Nesbitt
- JILA, National Institute of Standards and Technology and University of Colorado, Boulder, Colorado 80309, USA
- Department of Physics, University of Colorado, Boulder, Colorado 80309, USA
- Department of Chemistry, University of Colorado, Boulder, Colorado 80309, USA
| |
Collapse
|
5
|
Jiménez-Redondo M, Carrasco E, Herrero VJ, Tanarro I. Chemistry in glow discharges of H 2 / O 2 mixtures. Diagnostics and modelling. PLASMA SOURCES SCIENCE & TECHNOLOGY 2015; 24:015029. [PMID: 26702195 PMCID: PMC4685741 DOI: 10.1088/0963-0252/24/1/015029] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/05/2023]
Abstract
The chemistry of low pressure H2 + O2 discharges with different mixture ratios has been studied in a hollow cathode DC reactor. Neutral and positive ion distributions have been measured by mass spectrometry, and Langmuir probes have been used to provide charge densities and electron temperatures. A simple zero order kinetic model including neutral species and positive and negative ions, which takes into account gas-phase and heterogeneous chemistry, has been used to reproduce the global composition of the plasmas over the whole range of mixtures experimentally studied, and allows for the identification of the main physicochemical mechanisms that may explain the experimental results. To our knowledge, no combined experimental and modelling studies of the heavy species kinetics of low pressure H2 + O2 plasmas including ions has been reported before. As expected, apart from the precursors, H2O is detected in considerable amounts. The model also predicts appreciable concentrations of H and O atoms and the OH radical. The relevance of the metastable species O(1D) and O2(a1Δg) is analysed. Concerning the charged species, positive ion distributions are dominated by H3O+ for a wide range of intermediate mixtures, while H3+ and O2+ are the major ions for the higher and lower H2/O2 ratios, respectively. The mixed ions OH+, H2O+ and HO2+ are also observed in small amounts. Negative ions are shown to have a limited relevance in the global chemistry; their main contribution is the reduction of the electron density available for electron impact processes.
Collapse
Affiliation(s)
- M Jiménez-Redondo
- Instituto de Estructura de la Materia (IEM-CSIC), Serrano 123, 28006 Madrid, Spain
| | - E Carrasco
- Instituto de Estructura de la Materia (IEM-CSIC), Serrano 123, 28006 Madrid, Spain
| | - V J Herrero
- Instituto de Estructura de la Materia (IEM-CSIC), Serrano 123, 28006 Madrid, Spain
| | - I Tanarro
- Instituto de Estructura de la Materia (IEM-CSIC), Serrano 123, 28006 Madrid, Spain
| |
Collapse
|