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.
Moon rocks on Earth come from four sources: those collected by six United States Apollo program crewed lunar landings from 1969 to 1972; those collected by three Soviet uncrewed Luna probes in the 1970s; those collected by the Chinese Lunar Exploration Program's uncrewed probes; and rocks that were ejected naturally from the lunar surface before falling to Earth as lunar meteorites.
Six Apollo missions collected 2,200 samples of material weighing 381 kilograms (840 lb),[1] processed into more than 110,000 individually cataloged samples.[2]
Mission | Site | Sample mass returned[1] |
Year |
---|---|---|---|
Apollo 11 | Mare Tranquillitatis |
21.55 kg (47.51 lb) |
1969 |
Apollo 12 | Ocean of Storms |
34.30 kg (75.62 lb) |
1969 |
Apollo 14 | Fra Mauro formation |
42.80 kg (94.35 lb) |
1971 |
Apollo 15 | Hadley-Apennine |
76.70 kg (169.10 lb) |
1971 |
Apollo 16 | Descartes Highlands |
95.20 kg (209.89 lb) |
1972 |
Apollo 17 | Taurus-Littrow |
110.40 kg (243.40 lb) |
1972 |
Three Luna spacecraft returned with 301 grams (10.6 oz) of samples.[3][4][5]
Mission | Site | Sample mass returned |
Year |
---|---|---|---|
Luna 16 | Mare Fecunditatis | 101 g (3.6 oz)[6] | 1970 |
Luna 20 | Mare Fecunditatis | 30 g (1.1 oz)[7] | 1972 |
Luna 24 | Mare Crisium | 170 g (6.0 oz)[8] | 1976 |
The Soviet Union abandoned its attempts at a crewed lunar program in the 1970s, but succeeded in landing three robotic Luna spacecraft with the capability to collect and return small samples to Earth. A combined total of less than half a kilogram of material was returned.
In 1993, three small rock fragments from Luna 16, weighing 200 mg, were sold for United States dollar 442,500 at Sotheby's (equivalent to $783,167 in 2019).[9] In 2018, the same three Luna 16 rock fragments sold for United States dollar 855,000 at Sotheby's.[10]
Chang'e 5, the fifth lunar exploration mission of the Chinese Lunar Exploration Program, returned with ~1,731 g (61.1 oz) of samples.
Mission | Site | Sample mass returned |
Year |
---|---|---|---|
Chang'e 5 | Mons Rümker | 1,731 g (3.8 lb)[11] | 2020 |
More than 370 lunar meteorites have been collected on Earth,[12] representing more than 30 different meteorite finds (no falls), with a total mass of over 1,090 kilograms (2,400 lb).[13] Some were discovered by scientific teams (such as ANSMET) searching for meteorites in Antarctica, with most of the remainder discovered by collectors in the desert regions of northern Africa and Oman. A Moon rock known as "NWA 12691", which weighs 13.5 kilograms (30 lb), was found in the Sahara Desert at the Algerian and Mauritanian borders in January 2017,[14] and went on sale for $2.5 million in 2020.[15]
Rocks from the Moon have been measured by radiometric dating techniques. They range in age from about 3.16 billion years old for the basaltic samples derived from the lunar maria, up to about 4.44 billion years old for rocks derived from the highlands.[16] Based on the age-dating technique of "crater counting," the youngest basaltic eruptions are believed to have occurred about 1.2 billion years ago,[17] but scientists do not possess samples of these lavas. In contrast, the oldest ages of rocks from the Earth are between 3.8 and 4.28 billion years.
Mineral | Elements | Lunar rock appearance |
---|---|---|
Plagioclase feldspar | Calcium (Ca) Aluminium (Al) Silicon (Si) Oxygen (O) |
White to transparent gray; usually as elongated grains. |
Pyroxene | Iron (Fe), Magnesium (Mg) Calcium (Ca) Silicon (Si) Oxygen (O) |
Maroon to black; the grains appear more elongated in the maria and more square in the highlands. |
Olivine | Iron (Fe) Magnesium (Mg) Silicon (Si) Oxygen (O) |
Greenish color; generally, it appears in a rounded shape. |
Ilmenite | Iron (Fe), Titanium (Ti) Oxygen (O) |
Black, elongated square crystals. |
Moon rocks fall into two main categories: those found in the lunar highlands (terrae), and those in the maria. The terrae consist dominantly of mafic plutonic rocks. Regolith breccias with similar protoliths are also common. Mare basalts come in three distinct series in direct relation to their titanium content: high-Ti basalts, low-Ti basalts, and Very Low-Ti (VLT) basalts.
Almost all lunar rocks are depleted in volatiles and are completely lacking in hydrated minerals common in Earth rocks. In some regards, lunar rocks are closely related to Earth's rocks in their isotopic composition of the element oxygen. The Apollo Moon rocks were collected using a variety of tools, including hammers, rakes, scoops, tongs, and core tubes. Most were photographed prior to collection to record the condition in which they were found. They were placed inside sample bags and then a Special Environmental Sample Container for return to the Earth to protect them from contamination. In contrast to the Earth, large portions of the lunar crust appear to be composed of rocks with high concentrations of the mineral anorthite. The mare basalts have relatively high iron values. Furthermore, some of the mare basalts have very high levels of titanium (in the form of ilmenite).[19]
Plagioclase | Pyroxene | Olivine | Ilmenite | |
---|---|---|---|---|
Anorthosite | 90% | 5% | 5% | 0% |
Norite | 60% | 35% | 5% | 0% |
Troctolite | 60% | 5% | 35% | 0% |
Primary igneous rocks in the lunar highlands compose three distinct groups: the ferroan anorthosite suite, the magnesian suite, and the alkali suite.
Lunar breccias, formed largely by the immense basin-forming impacts, are dominantly composed of highland lithologies because most mare basalts post-date basin formation (and largely fill these impact basins).
Plagioclase | Pyroxene | Olivine | Ilmenite | |
---|---|---|---|---|
High titanium content | 30% | 54% | 3% | 18% |
Low titanium content | 30% | 60% | 5% | 5% |
Very low titanium content | 35% | 55% | 8% | 2% |
Mare basalts are named as such because they frequently constitute large portions of the lunar maria. These typically contain 18–21 percent FeO by weight, and 1–13 percent TiO2. They are similar to terrestrial basalts, but have many important differences; for example, mare basalts show a large negative europium anomaly. The type location is Mare Crisium sampled by Luna 24.
The main repository for the Apollo Moon rocks is the Lunar Sample Laboratory Facility at the Lyndon B. Johnson Space Center in Houston, Texas. For safekeeping, there is also a smaller collection stored at White Sands Test Facility in Las Cruces, New Mexico. Most of the rocks are stored in nitrogen to keep them free of moisture. They are handled only indirectly, using special tools.
Some Moon rocks from the Apollo missions are displayed in museums, and a few allow visitors to touch them. One of these, called the Touch Rock, is displayed in the Smithsonian National Air and Space Museum in Washington, D.C.[22] The idea of having touchable Moon rocks at a museum was suggested by Apollo scientist Farouk El-Baz, who was inspired by his childhood pilgrimage to Mecca where he touched the Black Stone (which in Islam is believed to be sent down from the heavens).[23]
Moon rocks collected during the course of lunar exploration are currently considered priceless.[22] In 2002, a safe was stolen from the Lunar Sample Building that contained minute samples of lunar and Martian material. The samples were recovered, and NASA estimated their value during the ensuing court case at about $1 million for 10 oz (280 g) of material.[citation needed]
Naturally transported Moon rocks in the form of lunar meteorites are sold and traded among private collectors.[citation needed]
Apollo 17 astronauts Eugene Cernan and Harrison Schmitt picked up a rock "composed of many fragments, of many sizes, and many shapes, probably from all parts of the Moon". This rock was later labeled sample 70017.[24] President Nixon ordered that fragments of that rock should be distributed in 1973 to all 50 US states and 135 foreign heads of state. The fragments were presented encased in an acrylic sphere, mounted on a wood plaque which included the recipients' flag which had also flown aboard Apollo 17.[25] Many of the presentation Moon rocks are now unaccounted for, having been stolen or lost.
Three minerals were discovered from the Moon: armalcolite, tranquillityite, and pyroxferroite. Armalcolite was named for the three astronauts on the Apollo 11 mission: Armstrong, Aldrin and Collins.
Because of their rarity on Earth, and the difficulty of obtaining more, Moon rocks have been frequent targets of theft and vandalism, and many have gone missing or were stolen.
NASA Lunar sample 15555 on display at Space Center Houston Lunar Samples Vault, at NASA's Johnson Space Center
NASA Lunar sample 15498 on display at Space Center Houston Lunar Samples Vault, at NASA's Johnson Space Center
NASA Lunar sample 60015 on display at Space Center Houston Lunar Samples Vault, at NASA's Johnson Space Center
NASA Lunar sample 60016 on display at Space Center Houston Lunar Samples Vault, at NASA's Johnson Space Center
NASA Lunar Sample Return Container with Lunar soil on display at Space Center Houston Lunar Samples Vault, at NASA's Johnson Space Center
Lunar Ferroan Anorthosite #60025 (Plagioclase Feldspar). Collected by Apollo 16 from the Lunar Highlands near Descartes Crater. This sample is currently on display at the National Museum of Natural History in Washington, DC
A piece of regolith from Apollo 11 presented to the Soviet Union and exhibited in the Memorial Museum of Cosmonautics in Moscow.
Sample 15016, the Seatbelt basalt
Apollo 16's sample 61016, better known as Big Muley, is the largest sample collected during the Apollo program
Big Bertha, collected on Apollo 14, is among the largest rock samples returned from the Moon (nearly 9 kilograms)
Original source: https://en.wikipedia.org/wiki/Moon rock.
Read more |