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Space rocks

Meteorites, like E.T. and Superman, come from space. If you go outside and look up, you’ll see it, even though it’s very far away. Their arrival here is a happy accident; a violent end to an incredible journey. Meteorites are classified in a number of ways, but mostly by their chemistry. The simplest way to split them up is into three broad groups: stony – known as chondrites and the most common type, iron and stony-iron, a combination of the first two. There are about 60,000 documented finds, with examples of a few millimetres across to the 60-tonne Hoba, in Namibia.

Meteorites fall all the time and everywhere, but they are not all large enough to notice, and a surprisingly small percentage of our planet’s surface is covered in humans that might notice. Most – the vast majority – are chondrites, which can be difficult to distinguish from slightly polished rocks. Easier to actually find and collect, however, are the iron type. Mostly because you can use a metal detector to find them, and – once you have it in your hand – is easier to recognise as something unusual. A larger fall will result in a strewn field – a spread of small pieces across a wide area, as the mass breaks up on entering the atmosphere. Even once you have a good idea where you might find the pieces, finding some can take a bit of careful planning and a lot of physical work.

So – what actually IS it? Most of the material that hits Earth is simply leftover matter from the event that created our solar system. Stuff that didn’t get to be part of a planet, and have been flying around the sun since then, lonely and afraid, and roughly the same age as our planet – about 4.54-4.55 billion years old. The oldest meteorite found so far, Muonionalusta, which fell over Sweden a million years ago, has been dated at 4.5653 billion. The nomenclature can be a little confusing. These leftover lumps take a few different forms. Asteroids are big chunks, determinedly orbiting the sun pretending they are planets. We think they have iron-rich cores surrounded by a thick rocky jacket. That’s where the meteorites come from – iron-nickels are bits of the centre, chondrites from the edges, and so on.

Meteorites have a bit of a bad rep, for killing the dinosaurs and Bruce Willis. But we need to forgive them, because in reality they are amazing things. Space travellers, older than the mountains, that may well be the end of us one day, but also perhaps brought us some of the building blocks of life in the first place. In 1969 near Murchison in Australia, a meteorite fell that contained organic molecules, including amino acids. Perhaps we all came from space, too.

Smaller pieces are meteoroids, which become meteors as they come through our atmosphere, the heat creating a fireball and long, burning tail. Shooting stars. They only become meteorites once they land. Landing is not just what makes them meteorites – it’s the scariest part of the whole phenomenon for us humans. In the long term, provided we avoid killing ourselves, the impact of a huge meteorite may well be what finishes us off. Perhaps only a great many from the initial impact, but then quite possibly the rest of us from the resulting environmental mess.

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Meg – The Monster Shark

We have a fascination with sharks, and we have a fascination with enormous animals. It follows that one of the most popular fossils in the commercial world is the tooth of the biggest ever shark, Otodus megalodon, often known simply as Meg. Sharks, on the other hand, don’t care about us at all.

As shark skeletons are made of cartilage rather than bone, they tend not to fossilize. What do get preserved are the teeth, and it’s these that give Meg its name – megalodon simply means “big tooth”. It’s thought there would have been between 250-280 teeth in its jaw. Sharks grow and shed teeth constantly throughout their life, so over a lifetime a single animal will have produced thousands of teeth. As a result, there are plenty fossilized for us to find and treasure.

Size estimates vary, depending on who you listen to, but most would put the adult shark somewhere between 34 and 60 feet long, with the biggest of these (probably females) weighing as much as 60 tons. The figures vary as there are different ways to calculate the size of the shark from the teeth alone. What we are sure about is that the biggest tooth found – so far – measures over 7” long.

Huge teeth, lots of them, and incredible power in the bite makes for a terrifying predator. So – what did they eat? Megs first appear in the fossil record at 20-23 million years ago, and we think they became extinct at around 3.6 million years ago. Modern humans have never had to worry about exactly what being eaten by a meg would be like. We can speculate, of course. It would almost certainly be an unsettling experience, uncomfortable and painful, if mercifully brief. And we’d probably swallow a lot of seawater, which is never fun. Great Whites, the largest predatory shark living today, have a varied diet, feeding on seals, turtles, large fish, American teenagers*, smaller cetaceans and even birds. Although not closely related, it’s likely meg would have been similar. There are plenty of whale bones – from very large whales – that show predation from megalodon.

Megalodons have shifted around the shark family tree a few times, and were recently moved into the genus Otodus. It had wrongly been thought they were ancestors of the modern Great White, but were then assigned the name Carcharocles. This latest reshuffle means meg has a family history going back about 100 million years. Like many deep water sharks, it was a traveller, and teeth have been found on every continent apart from Antarctica. The main source is South Carolina, where collectors can pick them up at beach and river sites, though the best are found by divers using feeling their way through the soft sediments of the riverbeds, blinded by the mud they stir up. Must be quite a thrill to head to the surface with a giant tooth in your hand.
*This is a Jaws joke. Sharks don’t eat many humans, really, and don’t seem to be fussy when they do.

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Man on the Moon

As you likely noticed, from extensive media coverage, it’s now been fifty years since man first set foot on the moon. An iconic event in human history; the names of those involved, quotes, indelible images firmly planted in the collective consciousness of most of the planet.

Although Armstrong and Aldrin carried with them a selection of crackers and pickles, NASA already suspected the moon was not made of cheese. They were right. The moon is actually a lump of our very own Earth, knocked off in a collision with planet-sized lump of matter (called Theia) when Earth was just a baby, some 4.51 billion years ago. What happened to Theia? It’s now thought the collision was more than a glancing blow and that what remains of Theia was essentially absorbed by Earth and our moon. She may have brought us the bulk of our water, for which we should be eternally grateful. No water, no us… Thanks, Theia.

The Apollo missions around the turn of the 1970s brought back with them some 2,200 samples of moon rock, and no cheese. The un-manned Russian Luna projects also collected specimens, and a lot of pieces of the moon have made it to Earth as meteorites, similarly dislodged from their second home and returned to their roots via an exciting journey through space, unassisted by astronaut or robot. In 1973 NASA made a gift of a mounted piece of the Apollo material, a fragment of sample 70017, to each US state and independent nation – the Goodwill Moonrocks. There’s an on-going project to locate each of these pieces, but perhaps unsurprisingly, a sizeable number (180 of 270) have gone missing over the years – sold, stolen, eaten by wolves.

While the Goodwill pieces can’t be legally traded, there is a global market for meteorites; lunar meteorites included. So it is possible to own a little piece of the moon. There is an international group of over 1,000 scientists and enthusiasts called the Meteoritical Society, who issue a regular bulletin documenting and classifying each and every meteorite find. All known meteorites are given a name – some more inspiring than others – making things easier for everybody. The NWA number shown on the boxed example pictured is its name – the letters simply standing for North West Africa, where it was found. Sometimes more information is known; a more specific find locality, a date, the name of the collector, etc, but there will always be a description of the type of rock and basic chemistry.

Whatever happens next in our attempts to explore our cosmic surroundings, Neil Armstrong’s first step on the moon will forever remain one of humanity’s crowning achievements, and the celebrations and commemorations are entirely justified.