Hemolithin
| Hemolithin | ||
|---|---|---|
| (iron and lithium-containing protein, possibly extraterrestrial[1][2][3]) | ||
 | ||
| Function | unknown, although possibly able to split water to hydroxyl and hydrogen moieties[1] | |
|
| ||
Hemolithin (sometimes confused with the similar space polymer Hemoglycin) is a proposed protein containing iron and lithium, of extraterrestrial origin, according to an unpublished preprint.[1][6][7][8] The result has not been published in any peer-reviewed scientific journal. The protein was purportedly found inside two CV3 meteorites, Allende and Acfer-086,[1][2][4] by a team of scientists led by Harvard University biochemist Julie McGeoch.[1][2] The report of the discovery was met with some skepticism and suggestions that the researchers had extrapolated too far from incomplete data.[9][10]
Sources
[edit]The detected hemolithin protein was reported to have been found inside two CV3 meteorites Allende and Acfer 086.[4] Acfer-086, where the complete molecule was detected rather than fragments (Allende), was discovered in Agemour, Algeria in 1990.[2][5]
Structure
[edit]According to the researchers' mass spectrometry, hemolithin is largely composed of glycine and hydroxyglycine amino acids.[10] The researchers noted that the protein was related to "very high extraterrestrial" ratios of Deuterium/Hydrogen (D/H);[2] such high D/H ratios are not found anywhere on Earth, but are "consistent with long-period comets"[3] and suggest, as reported, "that the protein was formed in the proto-solar disc or perhaps even earlier, in interstellar molecular clouds that existed long before the Sun’s birth".[2]
A natural development of hemolithin may have started with glycine forming first, and then later linking with other glycine molecules into polymer chains, and later still, combining with iron and oxygen atoms. The iron and oxygen atoms reside at the end of the newly found molecule. The researchers speculate that the iron oxide grouping formed at the end of the molecule may be able to absorb photons, thereby enabling the molecule to split water (H2O) into hydrogen and oxygen and, as a result, produce a source of energy that might be useful to the development of life.[2]
Exobiologist and chemist Jeffrey Bada expressed concerns about the possible protein discovery commenting, "The main problem is the occurrence of hydroxyglycine, which, to my knowledge, has never before been reported in meteorites or in prebiotic experiments. Nor is it found in any proteins. ... Thus, this amino acid is a strange one to find in a meteorite, and I am highly suspicious of the results."[10] Likewise, Lee Cronin of the University of Glasgow stated, "The structure makes no sense."[9]
History
[edit]Hemolithin is the name given to a protein molecule isolated from two CV3 meteorites, Allende and Acfer-086. Its deuterium to hydrogen ratio is 26 times terrestrial which is consistent with it having formed in an interstellar molecular cloud, or later in the protoplanetary disk at the start of the Solar System 4.567 billion years ago. The elements hydrogen, lithium, carbon, oxygen, nitrogen and iron that it is composed of, were all available for the first time 13 billion years ago after the first generation of massive stars ended in nucleosynthetic events.
The research leading to the discovery of Hemolithin started in 2007 when another protein, one of the first to form on Earth, was observed to entrap water.[11] That property being useful to chemistry before biochemistry on earth developed, theoretical enthalpy calculations on the condensation of amino acids were performed in gas phase space asking: "whether amino acids could polymerize to protein in space?" - they could, and their water of condensation aided their polymerization.[12] This led to several manuscripts of isotope and mass information on Hemolithin.[1][13][14][15]
See also
[edit]- Earliest known life forms
- Evolutionary history of life
- Extraterrestrial: The First Sign of Intelligent Life Beyond Earth
- List of interstellar and circumstellar molecules
- Panspermia
References
[edit]- ^ a b c d e f McGeoch, Malcolm. W.; Dikler, Sergei; McGeoch, Julie E. M. (22 February 2020). "Hemolithin: a Meteoritic Protein containing Iron and Lithium". arXiv:2002.11688 [astro-ph.EP].
- ^ a b c d e f g Ferreira, Becky (28 February 2020). "A Key Ingredient for Life Has Been Found on an 'Extraterrestrial Source,' Scientists Report in this unpublished report". Vice. Retrieved 2 March 2020.
- ^ a b Starr, Michelle (2 March 2020). "Scientists Claim to Have Found The First Known Extraterrestrial Protein in a Meteorite". ScienceAlert.com. Retrieved 2 March 2020.
- ^ a b c Staff (3 March 2020). "Acfer 086". The Meteoritical Society. Retrieved 3 March 2020.
- ^ a b Wlotza, Frank (1 September 1991). "Meteoritical Bulletin, No. 71". Meteoritical Bulletin. 26 (71): 255–262. Bibcode:1991Metic..26..255W. doi:10.1111/j.1945-5100.1991.tb01047.x. Retrieved 7 March 2020.
- ^ Prostak, Sergio (26 March 2020). "Researchers Find Extraterrestrial Protein in Meteorite Acfer 086". Science News. Retrieved 14 July 2021.
- ^ Yirka, Bob (3 March 2020). "Protein discovered inside a meteorite". Phys.org. Retrieved 14 July 2021.
- ^ Anderson, Paul (17 March 2020). "Have The First Proteins Been Found In Meteorites?". Earth & Sky. Retrieved 14 July 2021.
- ^ a b Crane, Leah (3 March 2020). "Have we really found an alien protein inside a meteorite?". New Scientist. Retrieved 3 March 2020.
- ^ a b c Wall, Mike (3 March 2020). "First known extraterrestrial protein possibly spotted in meteorite". Space.com. Retrieved 3 March 2020.
- ^ McGeoch, J.E.M.; McGeoch, M.W. (11 September 2007). "Entrapment of water by subunit c of ATP synthase". Journal of the Royal Society Interface. 5 (20): 311–318. doi:10.1098/rsif.2007.1146. PMC 2500151. PMID 17848362.
- ^ McGeoch, J.E.M.; McGeoch, M.W. (21 July 2014). "Polymer Amide as an Early Topology". PLOS One. 9 (7): e103036. Bibcode:2014PLoSO...9j3036M. doi:10.1371/journal.pone.0103036. PMC 4105422. PMID 25048204.
- ^ McGeoch, J.E.M.; McGeoch, M.W. (2015). "Polymer amide in the Allende and Murchison meteorites". Meteoritics & Planetary Science. 50 (12): 1971–1983. Bibcode:2015M&PS...50.1971M. doi:10.1111/maps.12558. S2CID 97089690.
- ^ McGeoch, Julie E. M.; McGeoch, Malcolm W. (28 July 2017). "A 4641Da polymer of amino acids in Acfer-086 and Allende meteorites". arXiv:1707.09080 [astro-ph.EP].
- ^ McGeoch, Malcolm. W.; Samoril, Tomas; Zapotok, David; McGeoch, Julie E. M. (28 July 2017). "Polymer amide as a carrier of 15N in Allende and Acfer 086 meteorites". arXiv:1811.06578 [astro-ph.EP].
