Established | 1979 |
---|---|
Field of research | Geology |
Address | Lyndon B. Johnson Space Center |
Location | Houston, Texas, U.S. 29°33′34″N95°05′00″W / 29.5594°N 95.0833°W |
77058 | |
Operating agency | NASA |
Website | curator |
The Lunar Sample Laboratory Facility (LSLF) is a repository and laboratory facility at NASA's Lyndon B. Johnson Space Center in Houston, Texas, opened in 1979 to house geologic samples returned from the Moon by the Apollo program missions to the lunar surface between 1969 and 1972. The facility preserves most of the 382 kilograms (842 lb) of lunar material returned over the course of Apollo program and other extraterrestrial samples, along with associated data records. It also contains laboratories for processing and studying the samples without contamination.
Planning for handling returned lunar samples began early in the Apollo program. In 1964, a proposal was made for a small (10 square meters (110 sq ft)) sample receiving laboratory equipped with remote-controlled manipulators operating in a sterile, high-vacuum chamber to prepare samples for distribution to scientists, and this proposal was subsequently expanded to include a clean room with analytical instruments for performing preliminary analyses on the samples. [1]
A committee of the Space Science Board reviewed the idea of a lunar sample receiving laboratory and sought to address multiple concerns. One was the fear that creating a facility with too great a capacity to analyze the samples would discourage distribution of samples to outside researchers and effectively exclude them. [1] In addition, space biologists and the United States Public Health Service expressed concern about "back contamination" of Earth by extraterrestrial microorganisms brought back via returning spacecraft, [2] (although many of the astronauts and scientists involved in the program were skeptical that non-terrestrial microorganisms could survive lunar conditions). To address these issues, the committee in 1965 recommended a laboratory with limited analytical capacity and an ability to quarantine the returning astronauts and samples. [1]
The result of this planning was the Lunar Receiving Laboratory (LRL) in Building 37 at the Johnson Space Center, built to process and conduct basic analysis on lunar materials and to quarantine the materials and astronauts. [1] (The requirement that astronauts be quarantined following their missions was dropped beginning with Apollo 15.) The 8,000-square-meter (86,000 sq ft) LRL was completed in 1967 at a cost of $7.8 million. [1] The LRL was used for study, distribution and safe storage of the samples, but although the LRL had adequate facilities to process samples for the current mission, the facility was not ideal, and it lacked facilities to process or store samples from previous missions. [3] To address some of these concerns, NASA dropped the requirement after Apollo 12 that samples be processed in vacuum (in favor of a simpler-to-work-in nitrogen atmosphere). An additional vault and, subsequently, a new laboratory – the Sample Storage and Processing Laboratory (SSPL) – were built in Building 31 of the Johnson Space Center. All lunar samples were moved from the LRL to Building 31 after the last Apollo mission [1]
Nonetheless, there were still concerns about the adequacy of the facility and about the wisdom of maintaining the entire collection of lunar samples in a single facility that might be vulnerable to natural disasters (especially the hurricanes to which Houston is vulnerable) and military actions. The collection was divided among multiple vaults at the Johnson Space Center while a vault was built in an empty ammunition bunker at Brooks Air Force Base in San Antonio, Texas, as second-site storage. Fourteen percent of the lunar sample collection was moved to this bunker in 1976, transported secretly at night with a police escort in a specially modified passenger bus. [1] This smaller collection of materials remained at Brooks until 2002, when the base was transitioned from military control as part of the Base Realignment and Closure process. The second-site lunar materials were then moved to the White Sands Test Facility, where a new, smaller facility was built inside an existing secure building to house the samples. [3] Of the 382 kilograms (842 lb) of lunar samples returned by the Apollo program, 52 kilograms (115 lb) are currently stored at White Sands. [4]
With a selection of the lunar samples secured offsite, construction began on the LSLF, with state-of-the-art facilities for handling the samples and better protection against natural disasters. The LSLF was constructed in a new annex of Building 31 (Building 31N at the Johnson Space Center) beginning in 1977. [1] Built for a cost of $2.5 million, the building was dedicated on July 20, 1979, the tenth anniversary of the first human Moon landing. [3]
The two-story, 1,300-square-meter (14,000 sq ft) facility consists of storage vaults for the samples, laboratories for sample preparation and study, a vault for sample data and records, and machinery to supply nitrogen to the cabinets in which the samples are stored and processed. [3] [5]
The facility's storage vaults are elevated above anticipated storm-surge sea level heights to protect the samples from threats posed by hurricanes and tornadoes. [6] During hurricane threats, a water-tight door is bolted into the frame of the door to the pristine sample vault in order to protect the samples. [5] The facility takes extensive measures to prevent contamination of the lunar samples. For example:
The facility has room to store many more lunar samples. NASA anticipates that more samples from the Moon will be brought back and processed and curated in the lab. [3]
The facility is the chief repository of the samples returned by the Apollo program. [5] The Apollo missions to the lunar surface (Apollo 11, Apollo 12, Apollo 14, Apollo 15, Apollo 16, and Apollo 17) returned a total of 382 kilograms (842 pounds) of lunar rocks, core samples, pebbles, sand and lunar surface dust, comprising 2200 individual specimens. Seventy-five percent of the lunar materials returned by Apollo are housed at the Lunar Sample Laboratory Facility, most in pristine condition. [3] Some of the materials have been processed into smaller samples to meet scientific requirements, resulting in more than 110,000 individually cataloged samples. [6]
Perhaps the most notable of the samples stored at the facility is the Genesis Rock, a sample ultimately determined to be nearly as old as the Moon itself. [7] Also at the facility is the sample known as Big Muley, the largest sample returned from the Moon by Apollo. [5]
In addition to the Apollo materials, the Johnson Space Center also houses other extraterrestrial samples:
52 kilograms (115 lb) of the 382 kilograms (842 lb) of lunar samples returned by the Apollo program are stored at the White Sands Test Facility. [4] Other small samples have been distributed to foreign heads of state, U.S. states, museums, and other institutions. NASA has also made a number of educational packs available for exhibition and educational purposes, each consisting of a disc of six small rock and soil samples in a lucite disc and a pack of thin petrological sections. [9]
In addition to the lunar samples returned by the Apollo missions, an additional 300 grams (11 oz) of lunar samples were returned to Earth by three automated Soviet spacecraft, Luna 16, Luna 20, and Luna 24. [5]
Approximately 100 people visit the facility annually for research or educational purposes, and the facility provides samples to hundreds of others each year for research or educational purposes. [6]
Researchers seeking samples submit proposals, which are evaluated by an independent peer review panel. 40 to 50 such proposals are approved each year and approximately 400 lunar samples (most weighing less than one gram) are sent to these scientists. [7]
The Apollo program, also known as Project Apollo, was the third United States human spaceflight program carried out by the National Aeronautics and Space Administration (NASA), which succeeded in preparing and landing the first humans on the Moon from 1968 to 1972. It was first conceived in 1960 during President Dwight D. Eisenhower's administration as a three-person spacecraft to follow the one-person Project Mercury, which put the first Americans in space. Apollo was later dedicated to President John F. Kennedy's national goal for the 1960s of "landing a man on the Moon and returning him safely to the Earth" in an address to Congress on May 25, 1961. It was the third US human spaceflight program to fly, preceded by the two-person Project Gemini conceived in 1961 to extend spaceflight capability in support of Apollo.
The Surveyor program was a NASA program that, from June 1966 through January 1968, sent seven robotic spacecraft to the surface of the Moon. Its primary goal was to demonstrate the feasibility of soft landings on the Moon. The Surveyor craft were the first American spacecraft to achieve soft landing on an extraterrestrial body. The missions called for the craft to travel directly to the Moon on an impact trajectory, a journey that lasted 63 to 65 hours, and ended with a deceleration of just over three minutes to a soft landing.
Surveyor 3 was the third lander of the American uncrewed Surveyor program sent to explore the surface of the Moon in 1967. It was the first mission to carry a surface-soil sampling-scoop.
The Lyndon B. Johnson Space Center (JSC) is NASA's center for human spaceflight, where human spaceflight training, research, and flight control are conducted. It was renamed in honor of the late US president and Texas native, Lyndon B. Johnson, by an act of the United States Senate on February 19, 1973.
Genesis was a NASA sample-return probe that collected a sample of solar wind particles and returned them to Earth for analysis. It was the first NASA sample-return mission to return material since the Apollo program, and the first to return material from beyond the orbit of the Moon. Genesis was launched on August 8, 2001, and the sample return capsule crash-landed in Utah on September 8, 2004, after a design flaw prevented the deployment of its drogue parachute. The crash contaminated many of the sample collectors. Although most were damaged, some of the collectors were successfully recovered.
Planetary protection is a guiding principle in the design of an interplanetary mission, aiming to prevent biological contamination of both the target celestial body and the Earth in the case of sample-return missions. Planetary protection reflects both the unknown nature of the space environment and the desire of the scientific community to preserve the pristine nature of celestial bodies until they can be studied in detail.
The Lunar Receiving Laboratory (LRL) was a facility at NASA's Lyndon B. Johnson Space Center that was constructed to quarantine astronauts and material brought back from the Moon during the Apollo program to reduce the risk of back-contamination. After recovery at sea, crews from Apollo 11, Apollo 12, and Apollo 14 walked from their helicopter to the Mobile Quarantine Facility on the deck of an aircraft carrier and were brought to the LRL for quarantine. Samples of rock and regolith that the astronauts collected and brought back were flown directly to the LRL and initially analyzed in glovebox vacuum chambers.
The geology of the Moon is quite different from that of Earth. The Moon lacks a true atmosphere, and the absence of free oxygen and water eliminates erosion due to weather. Instead, the surface is eroded much more slowly through the bombardment of the lunar surface by micrometeorites. It does not have any known form of plate tectonics, it has a lower gravity, and because of its small size, it cooled faster. In addition to impacts, the geomorphology of the lunar surface has been shaped by volcanism, which is now thought to have ended less than 50 million years ago. The Moon is a differentiated body, with a crust, mantle, and core.
Moon rock or lunar rock is rock originating from Earth's Moon. This includes lunar material collected during the course of human exploration of the Moon, and rock that has been ejected naturally from the Moon's surface and landed on Earth as meteorites.
The Lunar and Planetary Institute (LPI) is a scientific research institute dedicated to study of the solar system, its formation, evolution, and current state. The Institute is part of the Universities Space Research Association (USRA) and is supported by the Science Mission Directorate of the National Aeronautics and Space Administration (NASA). Located at 3600 Bay Area Boulevard in Houston, Texas, the LPI maintains an extensive collection of lunar and planetary data, carries out education and public outreach programs, and offers meeting coordination and publishing services. The LPI sponsors and organizes several workshops and conferences throughout the year, including the Lunar and Planetary Science Conference (LPSC) held in March in the Houston area.
A sample-return mission is a spacecraft mission to collect and return samples from an extraterrestrial location to Earth for analysis. Sample-return missions may bring back merely atoms and molecules or a deposit of complex compounds such as loose material and rocks. These samples may be obtained in a number of ways, such as soil and rock excavation or a collector array used for capturing particles of solar wind or cometary debris. Nonetheless, concerns have been raised that the return of such samples to planet Earth may endanger Earth itself.
David Stewart McKay was chief scientist for astrobiology at the Johnson Space Center. During the Apollo program, McKay provided geology training to the first men to walk on the Moon in the late 1960s. McKay was the first author of a scientific paper postulating past life on Mars on the basis of evidence in Martian meteorite ALH 84001, which had been found in Antarctica. This paper has become one of the most heavily cited papers in planetary science. The NASA Astrobiology Institute was founded partially as a result of community interest in this paper and related topics. He was a native of Titusville, Pennsylvania.
Extraterrestrial material refers to natural objects now on Earth that originated in outer space. Such materials include cosmic dust and meteorites, as well as samples brought to Earth by sample return missions from the Moon, asteroids and comets, as well as solar wind particles.
Interplanetary contamination refers to biological contamination of a planetary body by a space probe or spacecraft, either deliberate or unintentional.
Lunar Sample 61016, better known as "Big Muley", is a lunar sample discovered and collected on the Apollo 16 mission in 1972 in the Descartes Highlands, on the rim of Plum crater, near Flag crater. It is the largest sample returned from the Moon as part of the Apollo program. The rock, an 11.7 kg (26 lb) breccia consisting mainly of shocked anorthosite attached to a fragment of troctolitic "melt rock", is named after Bill Muehlberger, the Apollo 16 field geology team leader.
Lunar Sample 15016, better known as the "Seatbelt Basalt", is a lunar sample discovered and collected on the Apollo 15 mission in 1971 in the Hadley-Apennine region of the Moon. The rock is a 0.923 kg (2.03 lb) vesicular olivine basalt.
CAESAR is a sample-return mission concept to comet 67P/Churyumov–Gerasimenko. The mission was proposed in 2017 to NASA's New Frontiers program mission 4, and on 20 December 2017 it was one of two finalists selected for further concept development. On 27 June 2019, the other finalist, the Dragonfly mission, was chosen instead.
The Planetary Material Sample Curation Facility (PMSCF), commonly known as the Extraterrestrial Sample Curation Center is the facility where Japan Aerospace Exploration Agency (JAXA) conducts the curation works of extraterrestrial materials retrieved by some sample-return missions. They work closely with Japan's Astromaterials Science Research Group. Its objectives include documentation, preservation, preparation, and distribution of samples. All samples collected are made available for international distribution upon request.
The curation of extraterrestrial samples (astromaterials) obtained by sample-return missions take place at facilities specially designed to preserve both the sample integrity and protect the Earth. Astromaterials are classified as either non-restricted or restricted, depending on the nature of the Solar System body. Non-restricted samples include the Moon, asteroids, comets, solar particles and space dust. Restricted bodies include planets or moons suspected to have either past or present habitable environments to microscopic life, and therefore must be treated as extremely biohazardous.
ISOCHRON is a proposed lunar sample-return mission that would retrieve samples of the youngest lunar mare basalt.