[go: nahoru, domu]
Jump to content

Allan Hills 84001: Difference between revisions

Coordinates: 76°55′13″S 156°46′25″E / 76.92028°S 156.77361°E / -76.92028; 156.77361
From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
Hersfold (talk | contribs)
33,142 edits
m Reverted edits by Prathfig (talk) to last version by 67.98.206.2
link jargon to Martian meteorite
Line 21: Line 21:
|Image2_caption=
|Image2_caption=
}}
}}
'''Allan Hills 84001''' (commonly abbreviated '''ALH 84001'''<ref name=database>{{cite web|url=http://www.lpi.usra.edu/meteor/metbull.php?sea=alh+84001&sfor=names&ants=&falls=&stype=contains&lrec=50&map=ge&browse=&country=All&srt=name&categ=All&mblist=All&phot=&snew=0&pnt=no&code=604|title=Meteoritical Bulletin Database: Allan Hills 84001}}</ref>) is a [[meteorite]] that was found in [[Allan Hills]], [[Antarctica]] on December 27, 1984 by a team of U.S. meteorite hunters from the [[ANSMET]] project. Like other members of the group of SNCs (shergottite, nakhlite, chassignite), ALH 84001 is thought to be from [[Mars]]. On discovery, its [[mass]] was 1.93&nbsp;[[kilogram|kg]]. It made its way into headlines worldwide in 1996 when scientists announced that it might contain evidence for microscopic fossils of Martian bacteria based on carbonate globules observed.
'''Allan Hills 84001''' (commonly abbreviated '''ALH 84001'''<ref name=database>{{cite web|url=http://www.lpi.usra.edu/meteor/metbull.php?sea=alh+84001&sfor=names&ants=&falls=&stype=contains&lrec=50&map=ge&browse=&country=All&srt=name&categ=All&mblist=All&phot=&snew=0&pnt=no&code=604|title=Meteoritical Bulletin Database: Allan Hills 84001}}</ref>) is a [[meteorite]] that was found in [[Allan Hills]], [[Antarctica]] on December 27, 1984 by a team of U.S. meteorite hunters from the [[ANSMET]] project. Like other members of the group of [[Martian meteorite|SNC]]s (shergottite, nakhlite, chassignite), ALH 84001 is thought to be from [[Mars]]. On discovery, its [[mass]] was 1.93&nbsp;[[kilogram|kg]]. It made its way into headlines worldwide in 1996 when scientists announced that it might contain evidence for microscopic fossils of Martian bacteria based on carbonate globules observed.


==History==
==History==

Revision as of 23:38, 11 December 2010

Allan Hills 84001
Meteorite fragment ALH 84001
TypeAchondrite
ClassMartian meteorite
GroupALH 84001
Shock stageB
Weathering gradeA/B
CountryAntarctica
RegionAllan Hills, Far Western Icefield
Coordinates76°55′13″S 156°46′25″E / 76.92028°S 156.77361°E / -76.92028; 156.77361[1]
Observed fallNo
Found date1984
TKW1930.9 g
Related media on Wikimedia Commons

Allan Hills 84001 (commonly abbreviated ALH 84001[1]) is a meteorite that was found in Allan Hills, Antarctica on December 27, 1984 by a team of U.S. meteorite hunters from the ANSMET project. Like other members of the group of SNCs (shergottite, nakhlite, chassignite), ALH 84001 is thought to be from Mars. On discovery, its mass was 1.93 kg. It made its way into headlines worldwide in 1996 when scientists announced that it might contain evidence for microscopic fossils of Martian bacteria based on carbonate globules observed.

History

This rock is theorized to be one of the oldest pieces of the solar system, proposed to have crystallized from molten rock 4.091 billion years ago.[2] Based on hypotheses surrounding attempts to identify where extraterrestrial rocks come from, it is supposed to have originated on Mars and is related to other Martian meteorites.

In September 2005, Vicky Hamilton of the University of Hawaii at Manoa presented an analysis of the origin of ALH 84001 using data from the Mars Global Surveyor and Mars Odyssey spacecraft orbiting Mars. According to the analysis, Eos Chasma in the Valles Marineris canyon appears to be the source of the meteorite.[3] The analysis was not conclusive, in part because it was limited to parts of Mars not obscured by dust.

The theory holds that ALH 84001 was shocked and broken by one or more meteorite impacts on the surface of Mars some 3.9 to 4.0 billion years ago,[need quotation to verify] but remained on the planet. It was later blasted off from the surface in a separate impact about 15 million years ago and impacted Earth roughly 13,000 years ago. These dates were established by a variety of radiometric dating techniques, including samarium-neodymium (Sm-Nd), rubidium-strontium (Rb-Sr), potassium-argon (K-Ar), and carbon-14.[4][5]

It is hypothesized that ALH 84001 originated from a time period during which liquid water may have existed on Mars.[6] Other meteorites that have potential biological markings have generated less interest because they do not originate from a "wet" Mars. ALH 84001 is the only meteorite collected from such a time period.[6]

Possible biogenic features

On August 6, 1996[6] ALH 84001 became newsworthy when it was announced that the meteorite may contain evidence for traces of life from Mars, as published in an article in Science by David McKay of NASA.[7]

The electron microscope revealed chain structures in meteorite fragment ALH84001

Under the scanning electron microscope structures were revealed that may be the remains—in the form of fossils—of bacteria-like lifeforms. The structures found on ALH 84001 are 20-100 nanometres in diameter, similar in size to the theoretical nanobacteria, but smaller than any known cellular life at the time of their discovery. If the structures are in fact fossilized lifeforms, as proposed by the so-called biogenic hypothesis of their formation, they would be the first solid evidence of the existence of extraterrestrial life, aside from the chance of their origin being terrestrial contamination.[8]

The announcement of possible extraterrestrial life caused considerable controversy at the time and opened up interest in Martian exploration. When the discovery was announced, many immediately conjectured that the fossils were the first true evidence of extraterrestrial life—making headlines around the world, and even prompting U.S. President Bill Clinton to make a formal televised announcement to mark the event.[9]

Several tests for organic material have been performed on the meteorite and amino acids and polycyclic aromatic hydrocarbons (PAH) have been found. The debate over whether the organic molecules in the meteorite are in fact of exobiologic origin or are due to abiotic processes on Mars or contamination from the contact with Antarctic ice on Earth is still ongoing.[10][11]

Early on, Ralph Harvey of Case Western Reserve University and Harry McSween of University of Tennessee reported evidence that the carbonate globules found in the meteorite were formed at high temperature (above 650°C) by volcanic or impact processes on Mars.[12] At such high temperatures, it would be very unlikely that the morphology of the globules could have had any kind of biological origin. Later, however, the same authors published papers supporting a hypothesis in which the globules formed at low temperature from an aqueous solution. Most scientific papers published in the past 10 years now accept that carbonates on Mars formed this way.[13]

Other initial skepticism towards the biogenic hypothesis focused on the idea that the nanometer-sized filaments were too small to contain RNA, but evidence continues to grow that nanobacteria do exist in nature.[14] Furthermore, microbiologists have successfully cultured nanobacteria in the lab, with sizes within the range of at least some of the purported microfossils in ALH 84001.[15]

Some[who?] experts argue that the biomorphs found in the meteorite are not indicative of life on Mars, but instead are caused by contamination by earthly biofilms. However, scientists at NASA argue that likely microbial terrestrial contamination found in other Martian meteorites do not resemble the texture of the biomorphs in ALH 84001. In particular, the biomorphs in ALH 84001 look intergrown or embedded in the indigenous material, while likely contamination do not.[13]

While it has not yet conclusively been shown how the features in the meteorite were formed, similar features have been recreated in the lab without biological inputs by a team led by D.C. Golden of Hernandez Engineering Inc. in Houston.[16] David McKay says these results were obtained using unrealistically pure raw materials as a starting point[6], and "will not explain many of the features described by us in ALH84001." According to McKay, a plausible inorganic model "must explain simultaneously all of the properties that we and others have suggested as possible biogenic properties of this meteorite."[16]

In November 2009, a team of scientists at Johnson Space Center, including David McKay, reasserted that there is "strong evidence that life may have existed on ancient Mars", after having reexamined the meteorite using more advanced analytical instruments now available, in light of the objections that had been made since the biogenic hypothesis for the biomorphs first had been put forward.[17][18] Overall, the team concluded that:

None of the original features supporting our hypothesis for ALH84001 has either been discredited or has been positively ascribed to non-biologic explanations.[13]

In addition, they argued that since the original paper was published, the biogenic hypothesis has been "further strengthened by the presence of abundant biomorphs in other Martian meteorites."[13]

Student participation

The initial analysis of ALH 84001 was unusual in that an undergraduate student, Anne Taunton of the University of Arkansas, performed much of the SEM work used to correlate the suspected nanobacterial fossils with known terrestrial nanobacterial fossils. NASA's David McKay hired Anne Taunton for a 10-week student internship to perform the SEM analysis, but did not inform her about the nature of what she was investigating.[19] This technique is known as a single blind. Taunton reported the morphology of the biomorphs in ALH 84001 to be very similar to terrestrial samples without knowing that she was describing a Martian meteorite.

See also

References

  1. ^ a b "Meteoritical Bulletin Database: Allan Hills 84001".
  2. ^ Lapen, T. J. (2010). "A Younger Age for ALH84001 and Its Geochemical Link to Shergottite Sources in Mars". Science. 328 (5976): 347–351. doi:10.1126/science.1185395. {{cite journal}}: Unknown parameter |coauthors= ignored (|author= suggested) (help)
  3. ^ Birthplace of famous Mars meteorite pinpointed. New Scientist article. URL accessed March 18, 2006.
  4. ^ Nyquist, L. E. (1999). "Lunar Meteorites and the Lunar Crustal SR and Nd Isotopic Compositions". Lunar and Planetary Science. 27: 971. Bibcode:1996LPI....27..971N. {{cite journal}}: Cite has empty unknown parameter: |month= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  5. ^ Borg, Lars (1999). "The Age of the Carbonates in Martian Meteorite ALH84001". Science. 286 (5437): 90–94. doi:10.1126/science.286.5437.90. {{cite journal}}: Cite has empty unknown parameter: |month= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  6. ^ a b c d Crenson, Matt (2006-08-06). "After 10 years, few believe life on Mars". Associated Press (on usatoday.com). Retrieved 2009-12-06. {{cite web}}: External link in |publisher= (help)
  7. ^ McKay, David S. (1996). "Search for Past Life on Mars: Possible Relic Biogenic Activity in Martian Meteorite ALH84001". Science. 273 (5277): 924–930. doi:10.1126/science.273.5277.924. PMID 8688069. {{cite journal}}: Cite has empty unknown parameter: |month= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  8. ^ McSween, H. Y. (1997). "Evidence for life in a martian meteorite?". GSA Today. 7 (7): 1–7. PMID 11541665.
  9. ^ Clinton, Bill (1996-08-07). "President Clinton Statement Regarding Mars Meteorite Discovery". NASA. Retrieved 2006-08-07.
  10. ^ Bada, J. L. (1998). "A Search for Endogenous Amino Acids in Martian Meteorite ALH84001". Science. 279 (5349): 362–365. doi:10.1126/science.279.5349.362. PMID 9430583. {{cite journal}}: Cite has empty unknown parameter: |month= (help); Unknown parameter |coauthors= ignored (|author= suggested) (help)
  11. ^ Becker L., Glavin D. P., Bada J. L. (1997). "Polycyclic aromatic hydrocarbons (PAHs) in Antarctic Martian meteorites, carbonaceous chondrites, and polar ice". Geochimica et Cosmochimica Acta. 61 (2): 475–481. doi:10.1016/S0016-7037(96)00400-0. PMID 11541466.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  12. ^ Harvey, R. P., and J. H. Y. McSween, "A possible high-temperature origin for the carbonates in the Martian meteorite ALH84001", Nature, 382(6586), 49-51, (1996).
  13. ^ a b c d http://www.nasa.gov/centers/johnson/pdf/403089main_7441-1.pdf
  14. ^ Cisar J, Xu D, Thompson J, Swaim W, Hu L, Kopecko D (2000). "An alternative interpretation of nanobacteria-induced biomineralization". PNAS. 97 (21): 11511–11515. doi:10.1073/pnas.97.21.11511. PMC 17231. PMID 11027350.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  15. ^ http://www.agu.org/sci_soc/eisromanek.html
  16. ^ a b http://www.nasa.gov/centers/johnson/news/releases/2004/J04-025.html
  17. ^ "New Study Adds to Finding of Ancient Life Signs in Mars Meteorite". NASA. 2009-11-30. Retrieved 2009-12-01.
  18. ^ Thomas-Keprta, K., S. Clemett, D. McKay, E. Gibson and S. Wentworth 2009. Origin of Magnetite Nanocrystals in Martian Meteorite ALH84001 journal Geochimica et Cosmochimica Acta: 73. 6631-6677.
  19. ^ Taylor, Michael Ray, 1999. Dark Life. 0684841916, p. 90.
Retrieved from "https://en.wikipedia.org/w/index.php?title=Allan_Hills_84001&oldid=401858103"