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dc.contributor.authorGlass, Keely
dc.contributor.authorIto, Shosuke
dc.contributor.authorWilby, Philip R.
dc.contributor.authorSota, Takayuki
dc.contributor.authorNakamura, Atsushi
dc.contributor.authorBowers, C. Russell
dc.contributor.authorVinther, Jakob
dc.contributor.authorDutta, Suryendu
dc.contributor.authorBriggs, Derek E. G.
dc.contributor.authorWakamatsu, Kazumasa
dc.contributor.authorSimon, John D.
dc.contributor.authorSummons, Roger E
dc.date.accessioned2012-12-12T14:05:11Z
dc.date.available2012-12-12T14:05:11Z
dc.date.issued2012-06
dc.date.submitted2011-11
dc.identifier.issn0027-8424
dc.identifier.issn1091-6490
dc.identifier.urihttp://hdl.handle.net/1721.1/75399
dc.description.abstractMelanin is a ubiquitous biological pigment found in bacteria, fungi, plants, and animals. It has a diverse range of ecological and biochemical functions, including display, evasion, photoprotection, detoxification, and metal scavenging. To date, evidence of melanin in fossil organisms has relied entirely on indirect morphological and chemical analyses. Here, we apply direct chemical techniques to categorically demonstrate the preservation of eumelanin in two > 160 Ma Jurassic cephalopod ink sacs and to confirm its chemical similarity to the ink of the modern cephalopod, Sepia officinalis. Identification and characterization of degradation-resistant melanin may provide insights into its diverse roles in ancient organisms.en_US
dc.description.sponsorshipNASA Astrobiology Institute (Grant)en_US
dc.language.isoen_US
dc.publisherNational Academy of Sciencesen_US
dc.relation.isversionofhttp://dx.doi.org/10.1073/pnas.1118448109en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourcePNASen_US
dc.titleDirect chemical evidence for eumelanin pigment from the Jurassic perioden_US
dc.typeArticleen_US
dc.identifier.citationGlass, K. et al. “Direct Chemical Evidence for Eumelanin Pigment from the Jurassic Period.” Proceedings of the National Academy of Sciences 109.26 (2012): 10218–10223.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorSummons, Roger Everett
dc.contributor.mitauthorDutta, Suryendu
dc.relation.journalProceedings of the National Academy of Sciencesen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsGlass, K.; Ito, S.; Wilby, P. R.; Sota, T.; Nakamura, A.; Bowers, C. R.; Vinther, J.; Dutta, S.; Summons, R.; Briggs, D. E. G.; Wakamatsu, K.; Simon, J. D.en
dc.identifier.orcidhttps://orcid.org/0000-0002-7144-8537
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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