Caroline Smith (geologist)

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Caroline Smith
Alma mater University of St Andrews
The Open University
Scientific career
FieldsMeteoritics
Geochemistry
Institutions Natural History Museum, London

Caroline Smith is the Head of Earth Sciences Collections and Principal Curator of Meteorites at the Natural History Museum in London, UK. [1] [2] She specializes in geochemistry, meteorites, microscopy, mineralogy, and public outreach.

Contents

Career

Smith earned her BSc (Hons) in Geology from the University of St Andrews, United Kingdom (1998) and her PhD from The Open University, United Kingdom, in 2002. In 2012, she was named an Honorary Research Fellow of The University of Glasgow, School of Geographical and Earth Sciences, United Kingdom.

Smith has participated in numerous international science working groups. In 2014, she was chosen to be the UK representative to the International Mars Exploration Working Group and the co-chair of the International Mars Architecture for the Return of Samples (iMARS) Working Group Science Team, which assessed programmatic considerations relating to Mars Sample Return. [3]

In addition to science investigations, Smith is responsible for acquiring meteorites and samples for the Natural History Museum's scientific and public collections. In 2012, she carried the museum's largest Martian meteorite sample—a piece of the Tissint meteorite—in her carry-on luggage. [4] She provided a small piece of Zagami, a Martian meteorite, for calibration and testing of the Mars 2020 SHERLOC instrument. Part of the meteorite will be mounted on the rover and sent back to Mars. [5]

Smith has appeared in numerous television documentaries discussing the importance of meteorites. [6] She is the co-author of Meteorites, [7] a Natural History Museum publication, which provides a detailed introduction to these space objects.

Selected publications

Related Research Articles

<span class="mw-page-title-main">Meteorite</span> Solid debris from outer space that hits a planetary surface

A meteorite is a solid piece of debris from an object, such as a comet, asteroid, or meteoroid, that originates in outer space and survives its passage through the atmosphere to reach the surface of a planet or moon. When the original object enters the atmosphere, various factors such as friction, pressure, and chemical interactions with the atmospheric gases cause it to heat up and radiate energy. It then becomes a meteor and forms a fireball, also known as a shooting star; astronomers call the brightest examples "bolides". Once it settles on the larger body's surface, the meteor becomes a meteorite. Meteorites vary greatly in size. For geologists, a bolide is a meteorite large enough to create an impact crater.

<span class="mw-page-title-main">Martian meteorite</span> Meteorite made of rock originating from Mars

A Martian meteorite is a rock that formed on Mars, was ejected from the planet by an impact event, and traversed interplanetary space before landing on Earth as a meteorite. As of September 2020, 277 meteorites had been classified as Martian, less than half a percent of the 72,000 meteorites that have been classified. The largest complete, uncut Martian meteorite, Taoudenni 002, was recovered in Mali in early 2021. It weighs 14.5 kilograms and is on display at the Maine Mineral & Gem Museum.

<span class="mw-page-title-main">Allan Hills 84001</span> Martian meteorite discovered in Antarctica in 1984

Allan Hills 84001 (ALH84001) is a fragment of a Martian meteorite that was found in the Allan Hills in Antarctica on December 27, 1984, by a team of American meteorite hunters from the ANSMET project. Like other members of the shergottite–nakhlite–chassignite (SNC) group of meteorites, ALH84001 is thought to have originated on Mars. However, it does not fit into any of the previously discovered SNC groups. Its mass upon discovery was 1.93 kilograms (4.3 lb).

<span class="mw-page-title-main">Achondrite</span> Stony meteorite that does not contain chondrules

An achondrite is a stony meteorite that does not contain chondrules. It consists of material similar to terrestrial basalts or plutonic rocks and has been differentiated and reprocessed to a lesser or greater degree due to melting and recrystallization on or within meteorite parent bodies. As a result, achondrites have distinct textures and mineralogies indicative of igneous processes.

<span class="mw-page-title-main">Moon rock</span> Rock from the Moon

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.

<span class="mw-page-title-main">Elysium Mons</span> Martian volcano

Elysium Mons is a volcano on Mars located in the volcanic province Elysium, at 25.02°N 147.21°E, in the Martian eastern hemisphere. It stands about 12.6 km (41,000 ft) above its base, and about 14.1 km (46,000 ft) above the Martian datum, making it the third tallest Martian mountain in terms of relief and the fourth highest in elevation. Its diameter is about 240 km (150 mi), with a summit caldera about 14 km (8.7 mi) across. It is flanked by the smaller volcanoes Hecates Tholus to the northeast, and Albor Tholus to the southeast.

<span class="mw-page-title-main">Nakhla meteorite</span> Martian meteorite which landed in Egypt in 1911

Nakhla is a Martian meteorite which fell in Egypt in 1911. It was the first meteorite reported from Egypt, the first one to suggest signs of aqueous processes on Mars, and the prototype for Nakhlite type of meteorites.

<span class="mw-page-title-main">Shergotty meteorite</span> Martian meteorite discovered in India

The Shergotty meteorite is the first example of the shergottite Martian meteorite family. It was a 5-kilogram (11 lb) meteorite which fell to Earth at Sherghati, in the Gaya district, Bihar, India on 25 August 1865, and was retrieved by witnesses almost immediately. Radiometric dating indicates that it solidified from a volcanic magma about 4.1 billion years ago. It is composed mostly of pyroxene and is thought to have undergone preterrestrial aqueous alteration for several centuries. Certain features within its interior are suggestive of being remnants of biofilm and their associated microbial communities.

<span class="mw-page-title-main">Martian dichotomy</span> Geomorphological feature of Mars

The most conspicuous feature of Mars is a sharp contrast, known as the Martian dichotomy, between the Southern and the Northern hemispheres. The two hemispheres' geography differ in elevation by 1 to 3 km. The average thickness of the Martian crust is 45 km, with 32 km in the northern lowlands region, and 58 km in the southern highlands.

<span class="mw-page-title-main">Huo Hsing Vallis</span> Vallis on Mars

Huo Hsing Vallis is an ancient river valley in the Syrtis Major quadrangle of Mars at 30.5° north latitude and 293.4° west longitude. It is about 318 km long and was named after the word for "Mars" in Chinese.

Mars may contain ores that would be very useful to potential colonists. The abundance of volcanic features together with widespread cratering are strong evidence for a variety of ores. While nothing may be found on Mars that would justify the high cost of transport to Earth, the more ores that future colonists can obtain from Mars, the easier it would be to build colonies there.

<span class="mw-page-title-main">Nakhlite</span> Group of Martian meteorites

Nakhlites are a group of Martian meteorites, named after the first one, Nakhla meteorite.

<span class="mw-page-title-main">Tissint meteorite</span>

The Tissint meteorite is a Martian meteorite that fell in Tata Province in the Guelmim-Es Semara region of Morocco on July 18, 2011. Tissint is the fifth Martian meteorite that people have witnessed falling to Earth, and the first since 1962. Pieces of the meteorite are on display at several museums, including the Museum of Natural History of Vienna and the Natural History Museum in London.

This is a glossary of terms used in meteoritics, the science of meteorites.

<span class="mw-page-title-main">Northwest Africa 7034</span> Martian meteorite

Northwest Africa 7034 is a Martian meteorite believed to be the second oldest yet discovered. It is estimated to be two billion years old and contains the most water of any Martian meteorite found on Earth. Although it is from Mars it does not fit into any of the three SNC meteorite categories, and forms a new Martian meteorite group named "Martian ". Nicknamed "Black Beauty", it was purchased in Morocco and a slice of it was donated to the University of New Mexico by its American owner. The image of the original NWA 7034 was photographed in 2012 by Carl Agee, University of New Mexico.

<span class="mw-page-title-main">Yamato 000593</span>

Yamato 000593 is the second largest meteorite from Mars found on Earth. Studies suggest the Martian meteorite was formed about 1.3 billion years ago from a lava flow on Mars. An impact occurred on Mars about 11 million years ago and ejected the meteorite from the Martian surface into space. The meteorite landed on Earth in Antarctica about 50,000 years ago. The mass of the meteorite is 13.7 kg (30 lb) and has been found to contain evidence of past water alteration.

Catherine Margaret Corrigan, often known as Cari Corrigan, is an American scientist best known as a curator of the meteorite collection at the Smithsonian Institution. She is a scientist in the Department of Mineral Science at the National Museum of Natural History.

<span class="mw-page-title-main">Sara Russell</span> Professor of planetary sciences

Sara Samantha Russell is a professor of planetary sciences and leader of the Planetary Materials Group at the Natural History Museum, London. She is a Fellow of the Meteoritical Society and of the Royal Astronomical Society.

<span class="mw-page-title-main">Magnetic field of Mars</span>

The magnetic field of Mars is the magnetic field generated from Mars' interior. Today, Mars does not have a global magnetic field. However, Mars did power an early dynamo that produced a strong magnetic field 4 billion years ago, comparable to Earth's present surface field. After the early dynamo ceased, a weak late dynamo was reactivated ~3.8 billion years ago. The distribution of Martian crustal magnetization is similar to the Martian dichotomy. Whereas the Martian northern lowlands are largely unmagnetized, the southern hemisphere possesses strong remanent magnetization, showing alternating stripes. Our understanding of the evolution of the magnetic field of Mars is based on the combination of satellite measurements and Martian ground-based magnetic data.

References

  1. "Dr Caroline Smith | Natural History Museum". www.nhm.ac.uk. Retrieved 13 October 2018.
  2. "European Space Agency: exploration sample analogue collection and curation facility | Natural History Museum". www.nhm.ac.uk. Retrieved 13 October 2018.
  3. Haltigin, Timothy; Lange, Christian; Mugnuolo, Raffaele; Smith, Caroline; Haltigin, T; Lange, C; Mugnolo, R; Smith, C; Amundsen, H (April 2018). "iMARS Phase 2". Astrobiology. 18 (S1): S–1–S–131. doi:10.1089/ast.2018.29027.mars. ISSN   1531-1074. PMC   5926204 . PMID   29683336.
  4. "I carried Mars rock in hand luggage". BBC News. Retrieved 13 October 2018.
  5. "NASA's Mars 2020 rover is sending back an ancient slab of a Martian meteorite to use as target practice". Newsweek. 13 February 2018. Retrieved 13 October 2018.
  6. "Caroline Smith". IMDb. Retrieved 13 October 2018.
  7. Smith, Caroline; Russell, Sara Samantha; Benedix, Gretchen (December 2010). Meteorites. Firefly Books. ISBN   9781554078332.
  8. "The Potential Science and Engineering Value of Samples Delivered to Earth by Mars Sample Return" (PDF).
  9. Cassata, William S.; Cohen, Benjamin E.; Mark, Darren F.; Trappitsch, Reto; Crow, Carolyn A.; Wimpenny, Joshua; Lee, Martin R.; Smith, Caroline L. (1 May 2018). "Chronology of martian breccia NWA 7034 and the formation of the martian crustal dichotomy". Science Advances. 4 (5): eaap8306. Bibcode:2018SciA....4.8306C. doi:10.1126/sciadv.aap8306. ISSN   2375-2548. PMC   5966191 . PMID   29806017.
  10. Cohen, Benjamin E.; Mark, Darren F.; Cassata, William S.; Lee, Martin R.; Tomkinson, Tim; Smith, Caroline L. (3 October 2017). "Taking the pulse of Mars via dating of a plume-fed volcano". Nature Communications. 8 (1): 640. Bibcode:2017NatCo...8..640C. doi:10.1038/s41467-017-00513-8. ISSN   2041-1723. PMC   5626741 . PMID   28974682.