{"id":479128,"date":"2026-03-16T20:11:09","date_gmt":"2026-03-16T20:11:09","guid":{"rendered":"https:\/\/www.newsbeep.com\/uk\/479128\/"},"modified":"2026-03-16T20:11:09","modified_gmt":"2026-03-16T20:11:09","slug":"a-complete-set-of-canonical-nucleobases-in-the-carbonaceous-asteroid-162173-ryugu","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/uk\/479128\/","title":{"rendered":"A complete set of canonical nucleobases in the carbonaceous asteroid (162173) Ryugu"},"content":{"rendered":"<p>Extraction and purification of organic molecules from samples<\/p>\n<p>The Ryugu A0480 (11.9\u2009mg) and C0370 (8.3\u2009mg) aggregate samples were allocated through the Third Announcement of Opportunity (AO3) by the Japan Aerospace Exploration Agency (JAXA) (Supplementary Fig. <a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">1a<\/a>). Further descriptions of the Ryugu samples are available in the Ryugu AO database (\u2018Data availability\u2019). Microscope images and near-infrared reflectance spectra (2.0\u20134.0\u2009\u03bcm) (Supplementary Fig. <a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>) were obtained using the MicrOmega hyperspectral microscope in the clean chamber of the JAXA curation facility before AO3 sample selection, which captured the freshest state of the materials<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 14\" title=\"Yada, T. et al. Preliminary analysis of the Hayabusa2 samples returned from C-type asteroid Ryugu. Nat. Astron. 6, 214&#x2013;220 (2022).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR14\" id=\"ref-link-section-d35076784e2710\" rel=\"nofollow noopener\" target=\"_blank\">14<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 15\" title=\"Pilorget, C. et al. First compositional analysis of Ryugu samples by the MicrOmega hyperspectral microscope. Nat. Astron. 6, 221&#x2013;225 (2022).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR15\" id=\"ref-link-section-d35076784e2713\" rel=\"nofollow noopener\" target=\"_blank\">15<\/a>. These Ryugu aggregate samples are rich in organic matter<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 14\" title=\"Yada, T. et al. Preliminary analysis of the Hayabusa2 samples returned from C-type asteroid Ryugu. Nat. Astron. 6, 214&#x2013;220 (2022).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR14\" id=\"ref-link-section-d35076784e2717\" rel=\"nofollow noopener\" target=\"_blank\">14<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 15\" title=\"Pilorget, C. et al. First compositional analysis of Ryugu samples by the MicrOmega hyperspectral microscope. Nat. Astron. 6, 221&#x2013;225 (2022).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR15\" id=\"ref-link-section-d35076784e2720\" rel=\"nofollow noopener\" target=\"_blank\">15<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 17\" title=\"Naraoka, H. et al. Soluble organic molecules in samples of the carbonaceous asteroid (162173) Ryugu. Science 379, eabn9033 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR17\" id=\"ref-link-section-d35076784e2723\" rel=\"nofollow noopener\" target=\"_blank\">17<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 21\" title=\"Takano, Y. et al. Primordial aqueous alteration recorded in water-soluble organic molecules from the carbonaceous asteroid (162173) Ryugu. Nat. Commun. 15, 5708 (2024).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR21\" id=\"ref-link-section-d35076784e2726\" rel=\"nofollow noopener\" target=\"_blank\">21<\/a>, and some relevant functional groups (\u2013OH, \u2013NH and \u2013CH) were observed in a non-destructive spectroscopic analysis (Supplementary Data Fig. <a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#MOESM3\" rel=\"nofollow noopener\" target=\"_blank\">1b,c<\/a>). The data acquisition procedure is available elsewhere<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 48\" title=\"Hatakeda, K. et al. Homogeneity and heterogeneity in near-infrared FTIR spectra of Ryugu returned samples. Earth Planets Space 75, 46 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR48\" id=\"ref-link-section-d35076784e2734\" rel=\"nofollow noopener\" target=\"_blank\">48<\/a>. The CI1 Orgueil meteorite (30.6\u2009mg; from the Natural History Museum of Denmark)<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 21\" title=\"Takano, Y. et al. Primordial aqueous alteration recorded in water-soluble organic molecules from the carbonaceous asteroid (162173) Ryugu. Nat. Commun. 15, 5708 (2024).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR21\" id=\"ref-link-section-d35076784e2738\" rel=\"nofollow noopener\" target=\"_blank\">21<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 26\" title=\"Oba, Y. et al. Uracil in the carbonaceous asteroid (162173) Ryugu. Nat. Commun. 14, 1292 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR26\" id=\"ref-link-section-d35076784e2741\" rel=\"nofollow noopener\" target=\"_blank\">26<\/a> was also analysed as a suitable reference due to its mineralogical and elemental similarities to the Ryugu samples<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 29\" title=\"Yokoyama, T. et al. Samples returned from the asteroid Ryugu are similar to Ivuna-type carbonaceous meteorites. Science 379, eabn7850 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR29\" id=\"ref-link-section-d35076784e2745\" rel=\"nofollow noopener\" target=\"_blank\">29<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 30\" title=\"Nakamura, T. et al. Formation and evolution of carbonaceous asteroid Ryugu: direct evidence from returned samples. Science 379, eabn8671 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR30\" id=\"ref-link-section-d35076784e2748\" rel=\"nofollow noopener\" target=\"_blank\">30<\/a>. Procedural blanks using baked sea sand (14.4\u2009mg, FUJIFILM Wako Pure Chemical Corporation; 30\u201350 mesh) and baked serpentine (8.8\u2009mg; 500\u2009\u00b0C for 3\u2009h) were prepared following the same protocol as the Ryugu samples and used to assess background signals.<\/p>\n<p>All extraction and purification procedures were conducted on an ISO Class 5 clean bench within an ISO Class 6 clean room at Kyushu University. Each sample was suspended in ultrapure water and transferred to a 1.5\u2009ml polytetrafluoroethylene (PTFE) tube using a glass Pasteur pipette. A total of 550\u2009\u03bcl of ultrapure water was used to complete the transfer from the sapphire dish to the PTFE tube. Organic molecules were extracted at 25\u2009\u00b0C with 15\u2009min of ultrasonication. After centrifugation for 10\u2009min at 10,000\u2009rpm (equivalent to 14,093g), the supernatant was collected in a glass ampoule. The residue was rinsed with 200\u2009\u03bcl of ultrapure water, and the rinse was combined with the supernatant to yield approximately ~640\u2009\u03bcl in total, designated as the \u2018H2O extract\u2019. Altogether, 80% of the combined H2O extracts from the A0480 and C0370 samples were freeze-dried under reduced pressure for subsequent analysis.<\/p>\n<p>The residues extracted from the Ryugu samples were suspended in 600\u2009\u03bcl of 6\u2009M HCl and then transferred to glass ampoules using glass Pasteur pipettes. After purging the headspace with dry N2 gas, the ampoules were flame-sealed and heated at 110\u2009\u00b0C for 12\u2009h. The HCl extraction procedure (temperature and duration) was identical to that previously applied to the Bennu sample<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 27\" title=\"Glavin, D. P. et al. Abundant ammonia and nitrogen-rich soluble organic matter in samples from asteroid (101955) Bennu. Nat. Astron. 9, 199&#x2013;210 (2025).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR27\" id=\"ref-link-section-d35076784e2767\" rel=\"nofollow noopener\" target=\"_blank\">27<\/a>; however, in the present study, a preliminary water-based ultrasonic extraction at room temperature was performed to selectively isolate molecules that might otherwise be decomposed during acid treatment. Following the acid extraction, the supernatant and sample residues were transferred back into the same PTFE tubes used for the initial water extraction, using glass Pasteur pipettes. After centrifugation for 10\u2009min at 10,000\u2009rpm, the supernatant was collected into a glass ampoule. The residues were washed twice with 200\u2009\u03bcl of ultrapure water, and the rinses were combined with the supernatant, designated as the \u2018HCl extract\u2019. Secondary minerals (for example, carbonates and phyllosilicates)<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 22\" title=\"Yoshimura, T. et al. Chemical evolution of primordial salts and organic sulfur molecules in the asteroid (162173) Ryugu. Nat. Commun. 14, 5284 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR22\" id=\"ref-link-section-d35076784e2771\" rel=\"nofollow noopener\" target=\"_blank\">22<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 29\" title=\"Yokoyama, T. et al. Samples returned from the asteroid Ryugu are similar to Ivuna-type carbonaceous meteorites. Science 379, eabn7850 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR29\" id=\"ref-link-section-d35076784e2774\" rel=\"nofollow noopener\" target=\"_blank\">29<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 30\" title=\"Nakamura, T. et al. Formation and evolution of carbonaceous asteroid Ryugu: direct evidence from returned samples. Science 379, eabn8671 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR30\" id=\"ref-link-section-d35076784e2777\" rel=\"nofollow noopener\" target=\"_blank\">30<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 49\" title=\"Yoshimura, T. et al. Breunnerite grain and magnesium isotope chemistry reveal cation partitioning during aqueous alteration of asteroid Ryugu. Nat. Commun. 15, 6809 (2024).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR49\" id=\"ref-link-section-d35076784e2780\" rel=\"nofollow noopener\" target=\"_blank\">49<\/a> also dissolved during the acid extraction and contributed to the composition of the HCl extract. The entirety of the combined HCl extracts from the A0480 and C0370 samples were freeze-dried under reduced pressure.<\/p>\n<p>The freeze-dried H2O and HCl extracts were redissolved in 0.5\u2009ml of 0.1\u2009M HCl for desalting using an improved cation-exchange chromatography method<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 10\" title=\"Koga, T., Takano, Y., Oba, Y., Naraoka, H. &amp; Ohkouchi, N. Abundant extraterrestrial purine nucleobases in the Murchison meteorite: implications for a unified mechanism for purine synthesis in carbonaceous chondrite parent bodies. Geochim. Cosmochim. Acta 365, 253&#x2013;265 (2024).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR10\" id=\"ref-link-section-d35076784e2789\" rel=\"nofollow noopener\" target=\"_blank\">10<\/a>. A 0.5-ml aliquot of AG 50W-X8 cation-exchange resin (Bio-Rad Laboratories; analytical grade, 200\u2013400 mesh, hydrogen form) was packed into a glass Pasteur pipette and preconditioned sequentially with 1.5\u2009ml of 1\u2009M HCl, ultrapure water, 1\u2009M NaOH, ultrapure water, 1\u2009M HCl and ultrapure water. The extract solution was then loaded onto the column. The resins were rinsed with 2.5\u2009ml of ultrapure water to recover acidic, neutral and weakly basic compounds (designated as the \u2018H2O fraction\u2019). Subsequently, 2.5\u2009ml of 10% NH4OH was applied to elute basic compounds, including most nucleobases (designated as the \u2018NH4OH fraction\u2019). As a result, four fractions (H2O\u2013H2O, H2O\u2013NH4OH, HCl\u2013H2O, and HCl\u2013NH4OH) were obtained from the Ryugu A0480 and C0370 samples. Despite the prewashing of the cation-exchange chromatography resin, trace amounts of N-containing molecules were detected in the NH4OH fractions of the procedural blank. These fractions were freeze-dried and reconstituted in 50\u2013100\u2009\u03bcl of ultrapure water for subsequent analyses. A fragment of the Orgueil CI meteorite (30.6\u2009mg, purchased from a meteorite trading company) was extracted using the same protocol with ultrapure water and 6\u2009M HCl. Note that the H2O extract of the Orgueil meteorite was not subjected to cation-exchange chromatography.<\/p>\n<p>Carbon and nitrogen contents and the isotopic compositions of the extracted residues<\/p>\n<p>The elemental abundances of carbon (C, wt%) and nitrogen (N, wt%) and their isotopic compositions (\u03b413C and \u03b415N, \u2030 versus the international standards) in the residues extracted from the A0480, C0370 and the Orgueil meteorite were measured using an ultrasensitive nano-EA\/IRMS system (Flash EA1112 elemental analyser\/Conflo III interface\/Delta Plus XP isotope-ratio mass spectrometer, Thermo Finnigan, Bremen)<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 31\" title=\"Ogawa, N. O. et al. in Earth, Life, and Isotopes (eds Keisuke, K. et al.) 339&#x2013;353 (Kyoto Univ. Press, 2010).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR31\" id=\"ref-link-section-d35076784e2829\" rel=\"nofollow noopener\" target=\"_blank\">31<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 32\" title=\"Koga, T. et al. Compound-specific carbon and nitrogen isotopic analyses of underivatized pyrimidine and purine nucleobases. ACS Earth Space Chem. 9, 424&#x2013;432 (2025).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR32\" id=\"ref-link-section-d35076784e2832\" rel=\"nofollow noopener\" target=\"_blank\">32<\/a>. The masses of the analysed samples were 0.063\u2009mg (A0480), 0.097\u2009mg (C0370) and 0.125\u2009mg (Orgueil). Each residue was loaded into precleaned smooth-wall Sn capsules (L\u00fcdi Swiss AG), whose C and N blanks had been previously evaluated<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 32\" title=\"Koga, T. et al. Compound-specific carbon and nitrogen isotopic analyses of underivatized pyrimidine and purine nucleobases. ACS Earth Space Chem. 9, 424&#x2013;432 (2025).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR32\" id=\"ref-link-section-d35076784e2836\" rel=\"nofollow noopener\" target=\"_blank\">32<\/a>. Isotopic compositions are expressed in conventional \u03b4 notation relative to the Vienna Peedee Belemnite for carbon and atmospheric air for nitrogen (denoted as \u2018standard\u2019), defined as:<\/p>\n<p>$${\\rm{\\delta }}\\equiv {10}^{3}({R}_{\\mathrm{sample}}\/{R}_{\\mathrm{standard}}-1)\\,({\\permil }),$$<\/p>\n<p>\n                    (1)\n                <\/p>\n<p>where R represents the 13C\/12C or 15N\/14N ratio of the sample (Rsample) or the standard (Rstandard). Calibration was performed using an international and three inter-laboratory standards\u2014L-glutamic acid (USGS-41), L-tyrosine, L-alanine and nickel octaethylporphyrin\u2014spanning \u03b413C values from \u221234.2\u2030 to +37.4\u2030 and \u03b415N values from +0.86\u2030 to +47.6\u2030. The isotope and elemental analyses were calibrated using standards spanning 1.5\u201327.1\u2009\u00b5g (C) and 0.19\u20133.51\u2009\u00b5g (N). The analytical uncertainties, determined from replicate analyses of the L-tyrosine standard, were \u00b10.27\u2030 (1\u03c3, n\u2009=\u20098) for \u03b413C and \u00b10.50\u2030 (1\u03c3, n\u2009=\u20099) for \u03b415N.<\/p>\n<p>Analysis of nucleobases and other N-containing molecules<\/p>\n<p>The H2O and HCl extracts derived from the Ryugu and Orgueil samples, alongside procedural blanks and authentic reference compounds, were analysed using a high-resolution online HPLC\/ESI-HRMS system<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 9\" title=\"Oba, Y. et al. Identifying the wide diversity of extraterrestrial purine and pyrimidine nucleobases in carbonaceous meteorites. Nat. Commun. 13, 2008 (2022).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR9\" id=\"ref-link-section-d35076784e2999\" rel=\"nofollow noopener\" target=\"_blank\">9<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 10\" title=\"Koga, T., Takano, Y., Oba, Y., Naraoka, H. &amp; Ohkouchi, N. Abundant extraterrestrial purine nucleobases in the Murchison meteorite: implications for a unified mechanism for purine synthesis in carbonaceous chondrite parent bodies. Geochim. Cosmochim. Acta 365, 253&#x2013;265 (2024).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR10\" id=\"ref-link-section-d35076784e3002\" rel=\"nofollow noopener\" target=\"_blank\">10<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 26\" title=\"Oba, Y. et al. Uracil in the carbonaceous asteroid (162173) Ryugu. Nat. Commun. 14, 1292 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR26\" id=\"ref-link-section-d35076784e3005\" rel=\"nofollow noopener\" target=\"_blank\">26<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 27\" title=\"Glavin, D. P. et al. Abundant ammonia and nitrogen-rich soluble organic matter in samples from asteroid (101955) Bennu. Nat. Astron. 9, 199&#x2013;210 (2025).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR27\" id=\"ref-link-section-d35076784e3008\" rel=\"nofollow noopener\" target=\"_blank\">27<\/a>. The instrumentation consisted of an UltiMate 3000 HPLC coupled to a mass spectrometer (Q Exactive Plus Hybrid Quadrupole-Orbitrap, Thermo Fisher Scientific), operated at a mass resolution of 140,000 at m\/z\u2009=\u2009200. A reversed-phase column was maintained at 40\u2009\u00b0C for chromatographic separation.<\/p>\n<p>Purine nucleobases were quantified using an isocratic elution programme with a pentafluorophenyl column (1.0\u2009mm\u2009\u00d7\u2009250\u2009mm, 3-\u03bcm particle size; InertSustain, GL Sciences). The mobile phase consisted of 90% water (solvent A) and 10% acetonitrile containing 0.1% (by volume) formic acid (solvent B), delivered at a flow rate of 50\u2009\u03bcl\u2009min\u22121 for 20\u2009min. For the pyrimidine nucleobase analysis, a column (2.1\u2009mm\u2009\u00d7\u2009150\u2009mm, 3-\u03bcm particle size; HyperCarb, Thermo Fisher Scientific) was used with a linear gradient of solvent A (water plus 0.1% formic acid) and solvent B (acetonitrile plus 0.1% formic acid), progressing from 99:1 at 0\u2009min to 70:30 at 20\u2009min, at a flow rate of 200\u2009\u03bcl\u2009min\u22121.<\/p>\n<p>The eluent was introduced into a HESI-II ion source (Thermo Fisher Scientific), operated at 280\u2009\u00b0C for desolvation. The spray voltage and capillary temperature were set to 3.5\u2009kV and 295\u2009\u00b0C, respectively. Full-scan mass spectra were collected in positive ion mode across m\/z ranges of 111\u2013155 or 50\u2013500 with mass accuracies better than 5\u2009ppm. Mass calibration was occasionally performed using known ions, including protonated tyrosine (m\/z\u2009=\u2009182.08117), tert-butylamine (m\/z\u2009=\u200974.09643) and its fragment ion (m\/z\u2009=\u200957.06988), with an acetonitrile dimer (m\/z\u2009=\u200983.06037) serving as the lock mass.<\/p>\n<p>For confident identification of guanine and cytosine in the HCl\u2013NH4OH fraction of the Ryugu C0370 sample, tandem mass spectrometry analyses were performed under the same ionization conditions as the full-scan analyses. The target positive ions were isolated using a quadrupole with a 0.4 atomic mass unit for the isolation window and fragmented by high-energy collisions with N2 gas. The resulting product ions were analysed using a mass spectrometer (Orbitrap) at a resolution of 140,000 at m\/z\u2009=\u2009200.<\/p>\n<p>To cross-validate the detailed analysis of organic molecules in the Ryugu extracts, CE-HRMS was employed, as previously described<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 21\" title=\"Takano, Y. et al. Primordial aqueous alteration recorded in water-soluble organic molecules from the carbonaceous asteroid (162173) Ryugu. Nat. Commun. 15, 5708 (2024).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR21\" id=\"ref-link-section-d35076784e3058\" rel=\"nofollow noopener\" target=\"_blank\">21<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 26\" title=\"Oba, Y. et al. Uracil in the carbonaceous asteroid (162173) Ryugu. Nat. Commun. 14, 1292 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR26\" id=\"ref-link-section-d35076784e3061\" rel=\"nofollow noopener\" target=\"_blank\">26<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 50\" title=\"Sasaki, K. et al. Metabolomics platform with capillary electrophoresis coupled with high-resolution mass spectrometry for plasma analysis. Anal. Chem. 91, 1295&#x2013;1301 (2019).\" href=\"http:\/\/www.nature.com\/articles\/s41550-026-02791-z#ref-CR50\" id=\"ref-link-section-d35076784e3064\" rel=\"nofollow noopener\" target=\"_blank\">50<\/a>. Briefly, the CE-HRMS measurements were conducted with a capillary electrophoresis system (Agilent 7100, Agilent Technologies) coupled to a mass spectrometer (Q Exactive Plus, Thermo Fisher Scientific), an isocratic HPLC pump (Agilent 1260, Agilent Technologies), an adapter kit (G1603A CE-MS, Agilent Technologies) and a CE-ESI-MS sprayer kit (G1607A, Agilent Technologies). The CE and MS components were interfaced using a fused silica capillary (80\u2009cm total length\u2009\u00d7\u200950\u2009\u03bcm inner diameter), with a cation buffer solution (H3301-1001, HMT) serving as the electrophoretic electrolyte. Spectral data were acquired in positive ion mode over an m\/z range of 60\u2013900 at a resolution of 140,000 at m\/z\u2009=\u2009200.<\/p>\n","protected":false},"excerpt":{"rendered":"Extraction and purification of organic molecules from samples The Ryugu A0480 (11.9\u2009mg) and C0370 (8.3\u2009mg) aggregate samples were&hellip;\n","protected":false},"author":2,"featured_media":479129,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[23],"tags":[3503,63217,1813,36587,170400,3250,2302,90,416,56,54,55],"class_list":["post-479128","post","type-post","status-publish","format-standard","has-post-thumbnail","category-space","tag-asteroids","tag-astrobiology","tag-astronomy","tag-astrophysics-and-cosmology","tag-comets-and-kuiper-belt","tag-general","tag-physics","tag-science","tag-space","tag-uk","tag-united-kingdom","tag-unitedkingdom"],"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts\/479128","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/comments?post=479128"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/posts\/479128\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/media\/479129"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/media?parent=479128"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/categories?post=479128"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/uk\/wp-json\/wp\/v2\/tags?post=479128"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}