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Allan Hills 84001 (commonly abbreviated ALH 84001) is a meteorite that was found in Allan Hills, Antarcticamarker on December 27, 1984 by a team of US 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.


This rock is theorized to be one of the oldest pieces of the solar system, proposed to have crystallized from molten rock 4.5 billion years ago. 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 Manoamarker 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 Chasmamarker in the Valles Marinerismarker canyon appears to be the source of the meteorite. 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, 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.

It is hypothesized that ALH 84001 originated from a time period during which water may have existed on Mars. 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.

Possible lifeforms

On August 6, 1996 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 NASAmarker.

The electron microscope revealed chain structures in meteorite fragment ALH84001

Under the scanning electron microscope structures were revealed what 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, they would be the first solid evidence of the existence of extraterrestrial life, aside from the chance of their origin being terrestrial contamination.

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.

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.

Early on, Ralph Harvey of Case Western Reserve Universitymarker and Harry McSween of University of Tennesseemarker 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. 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.

Evidence continues to grow that nanobacteria do exist in nature, in spite of the initial skepticism based on the idea that the particles were too small to contain RNA. Futhermore, microbiologists have succesfully cultured nanobacteria in the lab, with sizes within the range of at least some of the purported microfossils in ALH 84001.

As of 2006, some experts still argue that the biomorphs found in the meteorite are not indicative of life on Mars, but instead are caused by contamination by earthly biofilms. But McKay argues 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 look intergrown or embedded in the indigenous material, while likely contamination do not.

It has not yet conclusively been shown how the features were formed, but similar features have been recreated in labs without biological inputs.

In November 2009, scientists at Johnson Space Centermarker, 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, as well as the objections that had been made since the biogenic hypothesis for the biomorphs first had been put forward.

Student participation

The analysis of ALH84001 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. This technique is known as a single blind. Taunton reported the morphology of biomorpgs in ALH84001 to be very similar to terrestrial samples without knowing that she was describing a Martian meteorite.

See also


  1. Birthplace of famous Mars meteorite pinpointed. New Scientist article. URL accessed March 18, 2006.
  2. 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).
  6. Taylor, Michael Ray, 1999. Dark Life. 0684841916, p. 90.

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