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Meteorites: the inside story Natural History Museum (NHM) meteorite experts Caroline Smith (right), Sara Russell (left) and Gretchen Benedix (middle) talk to Astronomy Now about how to recognise meteorites, what's on display at the NHM, and some of the most interesting meteorite finds. Posted: 20 April 2010
Gretchen Benedix is a researcher in the Meteorites and Cosmic Mineralogy division. Her main area of research is the evolution of the Solar System through study of altered or differentiated meteorite groups. She also studies the geology of Mars. Caroline Smith is the Curator of Meteorites. Her role is to maintain and manage the collection and to facilitate use of the collection by researchers both in the Museum and those from institutes around the world. Her main areas of research are the identification of new meteorites and planning for future space missions designed to return samples from asteroids and the planet Mars.
What are the key diagnostics for identifying a meteorite?
If someone suspects they do have a meteorite, what should they do? Contact our colleagues in the Angela Marmont Centre at the Museum. It will pass through the enquiry service there and if it is promising, will be passed along to the Meteorite team to offer an expert opinion about it. How often do people think they have found a meteorite, but in fact it's just a rock they've picked up in the garden? About 99 percent of samples that come to us as enquiries are "meteorwrongs". The most common meteorwrongs we get sent are industrial slags and pyrite nodules. Typically, the only times when the samples to turn out to be meteorites are the occasions when perhaps the person has purchased the rock as a meteorite or when they have visited an area known for meteorites e.g. the north African deserts and found the rock there. We answer hundreds of enquiries every year and this certainly shows that people are good at recognising rocks that are different from those in the near surroundings. What types of meteorites can people see at the NHM? How common is it that meteorites originate from the same asteroid, or same location on the Moon or Mars? What is the biggest known meteorite that has fallen to Earth? The largest meteorite to fall on Earth is the Hoba meteorite (pictured), which is sitting in the ground where it fell in Namibia. It has an estimated weight of 60,000 kg (60 tonnes). It was not seen to fall, but terrestrial age estimates indicate it may have fallen around 80,000 years ago. This meteorite is unusual in that the total known mass occurs in one stone. Most of the bigger meteorites break up during transit through the atmosphere before hitting the Earth. These next 3 biggest meteorites (also iron meteorites) are Cape York (Greenland - 58.2 tonnes), Campo del Cielo (Argentina – 50 tonnes), and Canyon Diablo (USA - 30 tonnes). But in all these other cases, there are multiple stones associated with the fall. We would also expect large stony meteorites to break up during atmospheric flight. For example in the case of the Allende (Mexico, 1969) over 2 t of material has been recovered and it is estimated that the strewnfield (the area where the meteoritic stones fell) is more than 150km2 in size. Which meteorites do you think are most important to the study of meteorites?
Do you have a favourite sample in the collection? 1) Ivuna – the type specimen of the CI chondrites, which are incredibly rare meteorites – there are only 9 out of ~38,000 known meteorites. We acquired the main mass (the largest piece) of this meteorite in the summer of 2008 and it is certainly one of the ‘star specimens’ in the Collection. We are actively using this sample for our research into the earliest stages of Solar System history. The CI chondrites are particularly interesting as they have some features that suggest they may have originated from comets. 2) Nakhla – a Martian meteorite that contains phyllosilicates (clay minerals) that must have formed in the presence of liquid water. A former colleague at the Museum, Dr Robert Hutchison (who sadly died in 2007), studied Nakhla samples from the Collection and made two seminal discoveries that greatly influenced our thinking about Mars and the Martian meteorites – that this meteorite was ‘young’ and therefore could not be from an asteroid (this led to the idea that meteorites could originate from Mars) and he also studied the phyllosilicate minerals, unequivocally proving that liquid water was once present on Mars. Image, left: Peter Marmet, www.marmet-meteorites.com. 3) Wold Cottage – the first British meteorite, which fell in Yorkshire in 1795. Although it is believed two other meteorites may have fallen in the UK previously (Hatford, 1628 and Stretchleigh, 1623) unfortunately there is no firm evidence in the form of actual samples so Wold Cottage is considered to be the first true British meteorite. It is also important as it is one of the samples that really ‘kick-started’ the scientific study of meteorites. Prior to the early 1800s meteorites were considered to be merely scientific curiosities, the study of which was considered to be unjustified by the scientific elite and intelligentsia of the day. However, the fall of the Wold Cottage, Siena (Italy, 1794) and L’aigle (France, 1803) meteorites proved difficult to dismiss, which led to meteorites being actively investigated to determine their chemical properties, mode of formation and origin. SR: If I had to choose a favourite, I would say the Vigarano meteorite. We have a beautiful slice of this at the Museum. It is a carbonaceous chondrite, and it is easy to see it is made up of chondrules, rounded objects a few millimetres across, and rare calcium-aluminium-rich inclusions (CAIs), which are white or bluish coloured inclusions up to a centimetre across. The CAIs are the oldest solids ever to have their age measured. Chondrules and CAIs formed over four and a half billion years ago, before the planets including our Earth existed. Find out more about the meteorite collection at the NHM at: http://www.nhm.ac.uk/nature-online/space/meteorites-dust/ Read more about meteorites in the May issue of Astronomy Now magazine. |
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