Palaeocene Rosencrantz & Guildensterns

I’ve been quiet for two reasons. One is that I’m trying to put something complicated in simple terms about madness and the state of the human race. I’ve written quite a lot on this but haven’t published it yet. The other is that we’re about to leave England, probably for good, and that takes a lot of doing. Given the state of things, it seems insensitive to write about anything else than the madness afflicting the West, if indeed “afflicting” is the right word.

Nonetheless, something has come to occupy my mind and operate as a distraction from the insanity, and perhaps put it in context. Whereas we’re in the midst of a mass extinction which may shortly bring the lives of all vertebrates to an end, we are at the end of a long history more than half an aeon in length with its own ups and downs. The biggest of these was the end-Permian mass extinction, whose causes are still not established, but involved the extinction of all but four percent of all species and leading to what’s been described as “a world of pigs”, since Pangaea became dominated by pig-like animals called Lystrosaurs for a long time. This was followed by the end-Triassic mass extinction many millions of years later, which had the surprising result of wiping out most of the mammaliforms and leading to the dominance of the up until then rather insignificant dinosaurs. Something like 120 million years after that came the K-T Event, which I’m often tempted to call the “left hand down a bit” disaster for reasons which reveal possible first-hand experience of the aforementioned mental condition of the world, but which basically involved a massive chunk of something rich in iridium hitting the Gulf of Mexico and killing every animal with a mass over twenty-five kilogrammes. I want now to talk about what happened after that.

I’ve mentioned multituberculates before as the most long-lived ever order of mammals, first appearing 167 million years ago and surviving in some form until millions of years after the extinction of non-avian dinosaurs in the late Eocene, 130 million years later. In other words they lasted longer than the non-avian dinosaurs. These are impressive and could be quite large, fox- or beaver-sized, and superficially resembled rodents although they weren’t closely related, but I haven’t come here to talk about that today. No, I want to talk about pantodonts, because I’ve recently had a bit of a revelation about them.

Pantodonts are somewhat enigmatic early Cenozoic mammals. I should explain that surviving mammals today comprise three main types. There are the monotremes, including the echidnas and the duck-billed platypus, whose group is unclear. The other two are the marsupialiformes and the eutheria, both of which are classed as theria. Multituberculates were in a different group again, the allotheria. Marsupials and their close relatives are well-known for having very short pregnancies and often keeping their young in a pouch physically attached to their nipples. The eutheria include all placental mammals, such as humans, but also other mammals who are not placental. Their traits include skeletal details such as a large malleolus at the bottom of the tibia, and although nowadays all eutheria are placental, there was a time when there were non-placental eutheria distinguished by those other characteristics, and probably more but soft parts are not preserved and there’s no surviving genome from them to work out the fine details. There was once a native New Zealand mammal, who went extinct in the Miocene and may or may not have been therian or eutherian but not placental. I mention all this because pantodonts may have been non-placental eutherians.

Tom Stoppard wrote a play called ‘Rosencrantz And Guildenstern Are Dead’, concentrating on the minor characters from ‘Hamlet’ in question, who are really just a footnote in the play. Stoppard’s play focusses on the random, arbitrary nature of the world and the framing of events in narratives, when something else is also going on. I’ve long since sworn off literary criticism but I tentatively venture to suggest that a major point of the piece is that while the big drama between the “important” people is going on, every bit part player portrays a potential main character who is central to her own life. For another example, consider Regina Spektor’s ‘Samson’:

Samson went back to bed,
not much hair left on his head.
ate a slice of wonder bread, and went right back to bed.
oh, we couldn’t bring the columns down,
yeah, we couldn’t destroy a single one,
and history books forgot about us,
and the Bible didn’t mention us, not even once.

All we “know” about Samson is from the Biblical narrative, but who knows who else was important to him? What about all the other routes not taken in our lives, all the people we knew vaguely as acquaintances but could’ve got to know better, and the various decisions we took and events which overtook us? Something which preoccupies me at times is that I could’ve gone to university in Sheffield instead of Leicester and maybe would still be living there today for all I know, but instead I did go to Leicester, met Sarada, we had children and now have grandchildren and for some reason I don’t understand, somehow I have never been to Sheffield, not even once. I know Leeds well, regularly go to Doncaster, have visited York a few times, have been to Bradford a fair bit, have stayed in Huddersfield and so on, but I have never, ever been to Sheffield. But in another world, Sheffield is my home city, and presumably in that world I’ve never been to Leicester instead of living there for thirty-two years. There are also, I guess, hundreds of people who have lived or do live in Sheffield whom I would’ve got to know, loved, hated, just vaguely known. As it is, I know two people in Sheffield and about two hundred in Leicester.

The pantodonts are like Sheffield, or Rosencrantz and Guildenstern, with respect to the dominant narrative of prehistory. The multituberculates are also like this to some extent. We have this popular view that there was a time we call the Age Of Dinosaurs, where giant reptiles dominated the planet on land and sea while mammals were tiny and insignificant, then an asteroid collided with us and wiped out all the giant reptiles, who were then replaced by mammals who became dominant. This is partly true, but the details are wrong. The multituberculates, along with various other species related to mammals, were around for a hundred million years before most of the dinosaurs were killed. After the event, it’s possible that hadrosaurs survived for a million years or so, but this is very doubtful. Less doubtful is the somewhat surprising survival of cursorial crocodiles. These were predatory like other crocodiles but with running underslung legs like those of dinosaurs, and terrestrial. Technically they weren’t dinosaurs but this didn’t matter to them or any of the prey they chomped down on for millions of years. At the same time, it would be equally false to over-emphasise these apparent anomalies, because that’s still what they are. And that brings me back to the pantodonts.

Apart from the multituberculates, and for some reason also the cursorial crocodiles, the post-apocalyptic landscape left by the Chicxulub Impactor was probably devoid of any large animals. This situation wouldn’t last, but I don’t want to pass over the immediate aftermath without comment. After the rather dramatic cock-up one Tuesday in May seen as killing off all the large animals here, including the ones living in the seas and oceans, it’s possible that a few scavengers such as pterosaurs survived and actually did really well for a bit and also that there were in fact a few dinosaurs dotted about here and there who had by some happy-ish accident not been killed, but never met another member of their species again and failed to breed. There was also a major rodent “problem”. The rodents, who had evolved in the late Cretaceous, proliferated like anything along with other small mammals, able to thrive in such an environment with few predators. Many of them were largely herbivorous, which helped. The ancestors of today’s hoofed mammals were there too, though they had yet to become hoofed and remarkably a lot of them were going to evolve into apparent apex predators and weren’t herbivorous at all.

By three million years after the K-T Event, one of the earliest pantodonts had appeared. This was Bemalambda:

8 March 2024, 14:44:45
Source: Own work. Author: ДиБгд

As can be seen from this picture, Bemalambda was around a metre long, so about the size of many dogs or perhaps a badger. It was herbivorous, but not a grazer because although grass did exist back then, grasslands didn’t. Grass was just one type of plant among many and much of the planet was covered in forest by then, so grazing didn’t happen and running either after prey or away from predators was difficult over long distances. By the way, this is my view and may not be backed up by evidence. Suppose this animal lived an average of ten years. There are therefore 300 000 generations maximum between the K-T Event and the presence of this specific animal. That’s a mean increase in length by a millimetre every nine thousand years, assuming the original ancestor to be infinitely small, which is obviously false – this is along the lines of “assume a spherical cow”. The significance of these animals is that they were to become the earliest large herbivorous mammals. At this point, this largest herbivorous mammal was the same size as the largest multituberculates had been, so the record was about to be broken.

Relatives and perhaps descendants included Barylambda, Pantolambda and Coryphodon. The occurrence of the word “lambda”, i.e. “Λ”, is incidentally to do with the arrangement of the cusps on their teeth. Speaking of teeth, unlike multituberculates or the more modern rodents, lagomorphs, even-toed ungulates and odd-toed ungulates, pantodonts didn’t have a gap in their teeth between their incisors and molars but just had a load of the primitive canines and premolars between them without any spaces at all. Just to cover the details a bit, they lived in North America and Eurasia but managed to spread to South America and became almost ubiquitous on land except for Antarctica, India (a continent at the time) and Australasia. The smaller species were Asian – one even lived in trees – and the larger North American. At the time, North America seems to have had very different fauna, since a few million years later our own ancestors the omomyids evolved on that continent. I envisage a continent covered in tropical rain forests.

2010 Source: dmitrchel@mail.ru Author: Creator:Dmitry Bogdanov

Barylambda was a late Palaeocene ground sloth-like animal weighing two thirds of a tonne and apparently able to rear up on her hind legs, since she had a heavy tail.

By Heinrich Harder (1858-1935) – The Wonderful Paleo Art of Heinrich Harder, Public Domain, https://commons.wikimedia.org/w/index.php?curid=1141375

Pantolambda was smaller at up to 178 kilogrammes but there was a smaller species of the same genus whose mass was only twenty-eight or lower. She was found in both North America and Eurasia and seems to have eaten soft plants in the summer and leaf litter and fungi in the winter, bearing in mind that she lived in the Arctic, which despite having what we would perceive as semi-tropical forests still had 24-hour daylight in the summer and completely nocturnal conditions in the winter, possibly for months on end, during which apparently loads of mushrooms grew. This particular fact about the Arctic in the early Cenozoic always does my head in: yes there were basically tropical rain forests inside the Arctic circle and yes they had twenty-four hours of darkness in the winter and permanent daylight in the summer.

By Heinrich Harder (1858-1935) – The Wonderful Paleo Art of Heinrich Harder, Public Domain, https://commons.wikimedia.org/w/index.php?curid=1141305

Coryphodon was about two metres long and more common in North America though also present in Europe and the rest of Eurasia. They’re remarkable for having tiny brains. The body weighs up to seven hundred kilogrammes and the brain only ninety grammes, a ratio of nearly eight thousand to one. This compares to the human figure of about forty-five to one and the rhino’s of about five thousand, which is the same as a whale’s, and a bovine’s is about a thousand. This kind of brain size is quite extreme for a mammal and doesn’t compare even to contemporary or earlier such animals.

It seems that the chief means of defence offered by pantodonts was their sheer size compared to the predators, since it seems unlikely they were intelligent enough to outwit them and they couldn’t run, something I’ll get back to. Their chief mammalian threat was the mesonychids, as at this point the predatory artiodactyls and creodonts had yet to evolve. Ankalagon was an early mesonychid appearing soon after the K-T Event and was the size of a bear.

The possibility that the pantodonts were not placental mammals but were eutherian might provide extra information regarding their nature. First of all, today’s ungulates are precocial. That is, their young can stand and walk (or swim in the case of whales) almost immediately after they’re born, possibly because they may have to escape predators very early on. Human babies, by contrast, are altricial. We are helpless at birth and can’t possibly fend for ourselves for a very long time. Although for humans this relates directly to the way we use our intelligence and technology, many other mammals are also altricial, such as dogs and mice. Pantodonts, having less advanced placentae, may have been altricial too, and this is not a good combination with being potential prey living out in the open from birth. It seems unlikely they lived in burrows and in most cases they couldn’t have climbed trees, so they’d have to tend their young and prevent them from being picked off by mesonychids or cursorial crocodilians (dinosaurs in all but name really) to some extent, although presumably thick undergrowth helped. Maybe they had nests? Once artiodactyls had evolved, with their precocial young, they would’ve had a big advantage over them, hence their early extinction.

There may be another way of understanding this group corresponding to the ancestry and nature of other clades of mammals. Pantodonts were graviportal. That is, they moved as slowly as tortoises or sloths, and this last is crucial. Before sophisticated DNA sequencing and maybe other more accurate techniques, a lot of guesswork was involved in tracing the ancestry of species. In the case of placental mammals, it was thought for a long time that there was a group called the “insectivores” who were close to the ancestors of all placental mammals. It’s still possible this is true, but “insectivores” no longer exist. Tupaias, colugos, tenrecs and elephant shrews, for example, were all placed within this order as well as hedgehogs, moles and shrews. It turns out that elephant shrews are more closely related to actual elephants, tupaias and colugos are close to primates and also rodents and tenrecs, despite being almost indistinguishable from hedgehogs, actually have no connection to them and are almost as distantly related as they could be and still be placental mammals. Almost, and this is where it gets a bit more relevant.

The group of placental mammals least closely related to the others is the xenarthra, formerly known as the edentates or “toothless mammals”. This description is completely wrong as in fact the armadillos have more teeth than any other species of mammals. They’re apparently in three groups: armadillos, anteaters and sloths. Nowadays, armadillos are grouped separatedly from the other two, who are considered to belong to the same order, but the three still have much in common with each other, rather like rodents and lagomorphs have. Xenarthrans diverged from the rest of us placental mammals around a hundred million years ago, and of course since then they have been evolving just like the rest of us, but they also have unusual features compared to others. They have the lowest metabolic rate, no milk teeth, often no teeth at all, no colour vision, seem to have regulated their temperature by burrowing in the past, extra vertebral joints (lost in sloths) to stiffen the spine and aid burrowing, no enamel on their teeth and sloths have either more or fewer neck vertebrae than other mammals and several times the number of ribs at fifty-six.

Sloths are particularly unusual. They sleep most of the time, their claws relax in a grasping position meaning that when they die they may not fall from the branch they were living on, they’re capable of starving with a full stomach because their bodies may get too cold for their digestive enzymes to work, and have algae living on the side of their fur away from the Sun. Ground sloths in particular somewhat resemble Barylambda:

It’s thought that the very first mammals were not able to control their body temperatures internally, because the growth patterns in their teeth seem to indicate that they lived about as long as lizards of the same size. Monotremes also have quite labile body temperatures, marsupials somewhat so and xenarthrans also to some extent. I think, not rigorously or scientifically but I have a hunch, that pantodonts and probably other mammals at the time who were not closely related to any of the eutherian mammals around today, shared characteristics with sloths and that the other placental mammals have lost them.

Here, then, is a scenario: pantodonts were sloth-like. They moved extremely slowly, might have had algae growing on the side away from the equator and had quite variable body temperatures. Their metabolism was sufficiently slow that they wouldn’t be able to digest food below a certain temperature, although in the Eocene this probably didn’t matter because practically the whole planet was too hot to endanger them. They also gave birth to tiny, naked and helpless young after short pregnancies whom they tended away from predators as far as possible but weren’t very good at keeping them safe, and once the true ungulates came along they couldn’t compete and died out. They’re really quite unlike most of the mammals Europeans would be familiar with. Those are my thoughts on the subject, and they’re quite unscientific and involve quite a few leaps of logic, but we’re never going to know.

Most of the time when people think about prehistoric animals, they think of dinosaurs, giant dragonflies, sea monsters, mammoths, trilobites and various other species, and all of those are very interesting, but I don’t think many people think about pantodonts even though they were of record-breaking size at the time, managed to evolve very quickly just after the non-avian dinosaurs died and were the first browsing herbivores. Hence, as I said, they’re the Rosencrantz and Guildenstern of the mammal world and they’re excluded because we tend to tell certain stories which miss details out. Thus their significance is akin to me not going to Sheffield and not meeting anyone there whom I might otherwise have got to know and Regina Spektor’s imaginary first lover of Samson. Like her, (pre)history books forget about them and the “Bibles” of palaeontology don’t really mention them, but for millions of years they existed before they vanished without trace. In a way, they’re like the Goths. I make a point of mentioning people’s names to those who never met them but whom I used to know because I think their existence should be honoured. Likewise, I mentioned the pantodonts here.

Middle-Sized?

I don’t know if you’ve ever seen the short film “Powers Of Ten”. It starts with a photo of a picnic and zooms out to one hundred million light years, then zooms in to a hundred attometres. It can be seen here:

I have a distinct memory of a different film and wonder if it’s been remade. Despite the date on this I think this is the 1968 version. ‘The Voices Of Time’ was published in 1966. The maximum zoom out is to 1024 and the maximum zoom in is to 10-16 metres, neither of which are absolute limits. Nor does the upper bound correspond to the limits of knowledge at the time so far as I can tell, and a metre is not in the middle of that range. The middle would be somewhere like ten kilometres, which is of the order of the width of Chicago, probably somewhat smaller. The idea of it being in the middle is a bit nebulous-sounding. What I mean to ask is, how big are we in terms of powers of ten, or for that matter any other number, in the scheme of things? Are we as much bigger than the smallest possible length as we are smaller than the largest length, or are we off to one side, and if so, which?

The smallest possible length is the Planck Length. This is 1.616255(18)×10−35 metres. Strictly speaking there is no upper limit because it appears that space will continue to expand for ever, and even if it doesn’t it isn’t because there’s a geometrically ordained maximum size, but the diameter of the Universe is said to be 28 gigaparsecs, which is 8.635317 x 1026 metres. Incidentally, the upper figure has spurious accuracy. While we’re “out here”, I may as well work out the volume of the Universe, and I may have this wrong. The Universe is not spherical but hyperspherical, and its volume corresponds to the surface area of a sphere in the same was as that corresponds to the circumference of a circle. The formula for the circumference of a circle is of course 2πr and the surface area of a sphere is 4πr2, so I, perhaps naïvely, would deduce that the formula for the volume of a hypersphere is 16πr3. It’s a bit difficult to work out what the “diameter” of the Universe means because it isn’t spherical, but assuming it means the diameter of the hypersphere which in practical terms constitutes space, this gives it a volume of 4 x 1081 metres. It’s also worth using these figures to calculate the difference between this and the volume of a sphere of the same size, that formula being (4/3)πr3, which would give the Universe a volume of “only” 3.37158 x 1080 metres, which is only a dozenth of the size. This illustrates the significance of the fact that Euclidean geometry doesn’t apply at this scale, and it also means that a sphere exactly half the size of the Universe is twelve times bigger on the inside than it is on the outside. In Whovian terms, it’s dimensionally transcendental. It’s also possible to stick these two big figures together and work out one in terms of the other: how many Planck volumes are there right now? The answer is a figure with a hundred and eighty-seven digits, which permits an upper limit to the useful value of π, although as time goes by it would drift out of kilter so many more places may in fact be necessary. In the unlikely event that you need this figure, go here, which gives it to a million decimal places. I find this quite reassuring because it suggests that memorising the number in question isn’t entirely pointless, or maybe that’s disappointing.

Why is a Planck Length the shortest possible length? The reason for this originates in the “ultraviolet catastrophe”. It’s been known for thousands of years that when an object gets hot, it glows red, then orange, then yellow, then white. However, nobody knew why for most of our history. Given classical physics, why is it that hot objects don’t simply glow white and get brighter as they get hotter? There would, however, be a problem with them doing this. If they just glowed at the entire range of frequencies of light, this would include all frequencies shorter than visible light and this would be infinite if the variation of frequencies could be any figure at all between any two other figures. Obviously a hot object is not infinitely bright, but why?

The answer is that there is a minimum difference between frequencies of the light emitted by a hot object. This means that physical reality has a granularity to it. It has, in terms of computer graphics and video, a frame rate and a resolution, all determined by Planck’s constant, h, and the speed of light, c. Light can only be omitted in discrete quantities. There is not an intermediate energy level below a certain fineness and instead energy leaps between these levels without having any values in between. The minimum quantity is known as a quantum, and the energy of a photon is equivalent to its frequency multiplied by h. It solves a lot of problems. For instance, if electrons in orbitals constantly radiated energy over a continuous range, they would spiral into the nucleus and the atom would collapse. Instead, an electron can only have certain clearly defined energy levels. The Planck Length is given by the formula:

. . . where G is the gravitational constant and ℏ is h divided by 2π. The Planck Time is then the time taken for light to travel this distance.

The thing about the Planck Length in terms of scale is that it’s so much smaller than anything significant which seems to be happening, such as the size of the “smallest” subatomic particles. A zoom into the Planck Length would mainly be very boring because it’s nineteen orders of magnitude smaller than the limit in ‘Powers Of Ten’, which is equivalent to a speck of dust compared to something like ten dozen times the diameter of the orbit of Neptune. However, assuming that the film was made in 1968, certain fundamental particles such as quarks had not been established to exist yet, so nowadays it would be possible to go further. At this scale, it’s conceivable that “quantum foam” exists. Spacetime may be fluctuating in nature at these dimensions like a stormy sea, which also suggests that there is energy present in a pure vacuum. How this might be extracted, and whether it would be desirable to do so, is another question. It’s sometimes thought that the Universe is not at its lowest energy level and if that level were to be reduced to zero, for instance by “mining” the energy of quantum foam, that true vacuum would spread out at the speed of light from where it was formed and destroy everything.

Getting back to the question in hand, the smallest possible scale is the Planck Length of the order of 10-35 metres, and the largest possible scale is the Universe itself, whose current diameter is of the order of 1026 metres. This means we are on the large size. Of the sixty-one orders of magnitude possible at the moment, we’re the thirty-fifth smallest and the twenty-sixth largest. Middle-sized is around the thirtieth from either end, which is around ten microns or somewhere between the size of a white blood cell and a red blood corpuscles. Organisms of this size include protists and single-celled algæ. They are to the Universe as the Planck length is to them. Even so, we are close to being middle-sized in the grand order of things in that a factor of a million is not hugely significant when the number considered is around ten decillion. A hundred thousand times bigger than we is the size of a region of England such as the Midlands, and that’s not terrifyingly and incomprehensibly enormous. Therefore we are, very roughly, in the middle.

A More Literary Bit

I don’t know what pretensions I have to dare describe anything I write as appropriate for the above heading, but there it is. Yesterday I made this YouTube video:

Incidentally, I’m thinking of going back to making YouTube videos, but in future they’re likely to include no speaking and I won’t be showing my face on them, if I bother at all.

I found this rather unsatisfactory. I was going for the impression that the rather overgrown back garden was like a jungle at a smaller scale, but there were a couple of issues. One was that most of this wasn’t truly at ground level, and the other was that there seemed to be precious few animals in that video. I may give it another go at a later date. What I wanted was a lush forest-like appearance teeming with animal life, such as spiders, ants, beetles and flies. Something like this but with animals:

We do, to Sarada’s chagrin, have plenty of horsetails in our garden but they’re not forty metres tall. It’s really a testament to them that they’re still around after 300 million years, and to me it raises the question: when you get smaller, is it like going back in time? After all, on a sufficiently tiny level there are no vertebrates, or rather the vertebrates who do exist are great hulking monsters. There’s a frog who is less than eight millimetres long, and in Britain the minimum size seems to be a few centimetres. Mammals and birds as they’re now constituted can’t be smaller than a certain size because they would be physically incapable of eating enough food to keep their body temperatures at the right level to survive, so getting smaller is a journey into the past in terms of the animals all being “cold-blooded”, except of course that as discussed previously a flying insect isn’t really cold-blooded at all if it has to put much effort into flying. However, also at this scale animals don’t so much need to put effort into flying as into not flying, because for them the air is a fairly thick, buoyant fluid which they don’t so much fly through as swim in.

J G Ballard’s novel ‘The Enormous Space’ tells the story of a man who resolves never to leave his house again. As the days go by, his house expands until even the room he’s in is too vast to traverse. It’s been adapted into a TV play by the BBC:

Because of lockdown (I almost gave that a capital letter), some of us have found our homes becoming our worlds like the character in this piece, but to the various denizens of our dwellings they already are. The longest line section (actually geodesic) which can be drawn in the area I have lived my entire life within is about two thousand kilometres long, from Inverness to Rome, so that’s my world, in a way. Reducing this by a thousand gives an area the size of a small town, so for an ant, say, this is their world. The vegetated area of the garden is about twelve metres long, so magnifying that by a thousand makes it twelve kilometres, like a large forest in terms of England today. But this is mainly a bamboo forest with prodigiously high “trees”, since it’s largely grass. The tallest bamboo species is Dendrocalamus giganteus, which is up to thirty-five metres high, and at a scale of one to a thousand this is equivalent to a fairly well-manicured lawn, which we don’t currently have. To an ant, the moderately tall grass in the back garden is something like ten times the height of the tallest bamboo, making it more like a redwood forest, though of course not woody because of the relatively lower gravity.

This is truly a different world. The gravitational acceleration is less important there because the relative masses are a thousand million times lower. An insect could easily fall out of a skyscraper without being harmed, even though the gravity operating on a two millimetre long organism is in a sense a thousand times as strong. The atmosphere becomes a much more important factor, even the dominant one. Water becomes if anything more dangerous because its surface tension not only allows it to be walked on but also to capture an insect permanently even though they wouldn’t sink, and this opens up a whole ecological niche of predators who can prey on the victims of surface tension such as raft spiders and pond skaters. At the same time there are still the more familiar predators and prey in the form of ladybirds, wolf spiders and aphids.

It’s easy to think of oneself as trapped in one’s home, and since I’m a carer that is particularly a hazard for me. However, not only do I continue to have communication with the outside world, but also I have access to the microcosm. Even without a microscope I can observe the relatively large animals living in the house and garden, and when I get down to the middle-sized animals such as the hundred micron Colpoda, which will be present in the soil here like it is all over the place, and the crinoid-like Vorticella likely to be present in the guttering whose stalks are around the same length, the garden is relatively the size of that good old colloquial unit Wales. How could I want for any more? I can also go the other way, though since I live in England with its grey skies, not quite so far. But on a clear night, like anyone else I can realistically see individual stars thousands of light years away. The whole observable Universe is around me and half of it is accessible, though this presumes I have my own observatory and in practical terms is far less so because I’ve only got a pair of binoculars. But even so, I can see the Orion Nebula, 1 300 light years away, and the Pleiades open star cluster, 440 light years from here, and so on.

In the end, then, although it’s important to get out of the house, to some extent it’s what one makes of it, and the scope for what I might call adventure but is probably better called observation, even just from this one small house and garden in an English Midlands town, is vast. Just because the slightly larger than medium scale at which we happen to live lacks, in the East Midlands anyway, rainforests, elephants, lions and whales, doesn’t mean it doesn’t contain an equally fascinating array of wildlife on another level, and just because we’re confined to Earth doesn’t mean we can’t observe a fascinating wider Galaxy. What more could anyone want? Isn’t it great to be middle-sized?