2003
DOI: 10.1002/mrc.1193
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Solid‐state cross‐polarization magic angle spinning 13C and 15N NMR characterization of Sepia melanin, Sepia melanin free acid and Human hair melanin in comparison with several model compounds

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Cited by 67 publications
(100 citation statements)
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“…4B) and GSM120386 (Fig. S1D) confirm the presence of aliphatic groups 0-90 ppm (CH x , CNH 2 ), aromatic groups 90-160 ppm (CH x , C─O, C 2 NH) and carboxylic acid groups and ketones 160-200 ppm (C═O, COO), consistent with those previously reported for S. officinalis (33). The spectra of the background sediments of GSM 122841 and GSM 120386 lack the aromatic, carboxylic acid, and ketone signals present in the fossil pigment ( Fig.…”
Section: Resultssupporting
confidence: 89%
“…4B) and GSM120386 (Fig. S1D) confirm the presence of aliphatic groups 0-90 ppm (CH x , CNH 2 ), aromatic groups 90-160 ppm (CH x , C─O, C 2 NH) and carboxylic acid groups and ketones 160-200 ppm (C═O, COO), consistent with those previously reported for S. officinalis (33). The spectra of the background sediments of GSM 122841 and GSM 120386 lack the aromatic, carboxylic acid, and ketone signals present in the fossil pigment ( Fig.…”
Section: Resultssupporting
confidence: 89%
“…Figure 5 showed the 13 C CP/MAS NMR spectra for natural squid ink melanin and soluble fraction B. Both of the two samples showed similar peaks among three characteristic spectral regions as described in the previously literature for the NMR of the melanin (Adhyaru et al 2003;Tian et al 2003, Jalmi et al 2012: (1)δ10-95 ppm was assigned to aliphatic carbons, which was due to proteinaceous material; (2)δ95-165 ppm was assigned to aromatic carbons, including indole or pyrrole type carbons within the polymer; (3)δ165-200 ppm, carbonyl carbon atoms in amides, carboxylates and quinones, which came from the carbonyl in the oxidized quinone form of DHI and DHICA. More specifically, the signals near~δ30ppm and~δ50ppm were assigned to aliphatic groups which come from dihydroderivatives of DHICA, DHI (Knicker et al 1995;Adhyaru et al 2003;Tian et al 2003;Jalmi et al 2012); the signals near~δ103ppm was suggestive of C-3 of indole nucleus, which was from the anomeric carbon of carbohydrates; the peak near~δ130ppm was assigned to aromatic group; the signal near~δ174ppm was due to carbonyl group present as carboxylic acid group, which was derived from DHICA, and the degradation products of DHI and DHICA.…”
Section: Nmr Spectrumsupporting
confidence: 65%
“…In comparison with the fraction B, natural melanin exhibited higher intensity of signals in the rangeδ95-165 ppm. This was presumably attributable to the greater percentage of protonated carbon atoms (δ95-130 ppm) and quaternarycarbon atoms in the melanin backbone (δ130-145 ppm) (Adhyaru et al 2003), which indicated that aromatic structure was broken down in some extent through the degradation process.…”
Section: Nmr Spectrummentioning
confidence: 99%
“…Solid State CP-MAS NMR-Based on expected chemical shifts of model compounds and published NMR assignments (26) of Sepia melanin, the 13 C CP-MAS NMR data collected for hydrolyzed Glycera jaw residue fit well (Fig. 4).…”
Section: Resultsmentioning
confidence: 71%