Measurement of CHD on Titan at Submillimeter Wavelengths
arXiv:1905.00576 · doi:10.3847/1538-3881/ab19bb
Abstract
We present the first radio/submillimeter detection of monodeuterated methane (CHD) in Titan's atmosphere, using archival data from of the Atacama Large Millimeter/submillimeter Array (ALMA). The and transitions at 465.235 and 465.250 GHz ( mm) were measured at significance levels of and , respectively. These two lines were modeled using the Non-linear optimal Estimator for MultivariatE spectral analySIS (NEMESIS) radiative transfer code to determine the disk-averaged CHD volume mixing ratio = in Titan's stratosphere (at altitudes km). By comparison with the CH vertical abundance profile measured by Cassini-Huygens mass spectrometry, the resulting value for D/H in CH is . This is consistent with previous ground-based and in-situ measurements from the Cassini-Huygens mission, though slightly lower than the average of the previous values. Additional CHD observations at higher spatial resolution will be required to determine a value truly comparable with the Cassini-Huygens CH measurements, by measuring CHD with ALMA close to Titan's equator. In the post-Cassini era, spatially resolved observations of CHD with ALMA will enable the latitudinal distribution of methane to be determined, making this an important molecule for further studies.
arXiv comment9 pages, 4 figures
References in corpus (10)
- ALMA Observations of HCN and its Isotopologues on Titan
- ALMA measurements of the HNC and HCN distributions in Titan's atmosphere
- Isotopic Ratios of Carbon and Oxygen in Titan's CO using ALMA
- Abundance Measurements of Titan's Stratospheric HCN, HCN, CH, and CHCN from ALMA Observations
- A primordial origin for the atmospheric methane of Saturn's moon Titan
- Spatial Variations in Titan's Atmospheric Temperature: ALMA and Cassini Comparisons from 2012 to 2015
- Interferometric imaging of Titan's HCN, HCCCN and HCCCN
- Mapping Vinyl Cyanide and Other Nitriles in Titan's Atmosphere Using ALMA
- Photochemical enrichment of deuterium in Titan's atmosphere: new insights from Cassini-Huygens
- Tentative Detection of Deuterated Methane toward the Low-Mass Protostar IRAS 04368+2557 in L1527
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- Modeling transmission windows in Titan's lower troposphere: Implications for infrared spectrometers aboard future aerial and surface missions
- Measurements of Titan's Stratospheric Winds during the 2009 Equinox with the eSMA