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.

Restoring Pluto And Elevating Cynthia

I was going to blog about the larger asteroids at this point, but in recent days it’s been borne in upon me that there’s a current issue in astronomy, perhaps over-emphasised but definitely there, over whether Pluto was unfairly demoted. The reason I mention this now is Steve’s comment about what the difference between Phobos and Deimos and asteroids might be. It’s a very good question and I’ll address this first.

Phobos and Deimos, the moons of Mars, are a little puzzling. There are two hypotheses about where they come from. One is that they’re main-belt asteroids which were captured by Mars. At first glance this sounds very sensible and logical. After all, Mars is next to the asteroid belt, it could be expected to gather up a few stones from it from time to time and the pair seem to be only the latest representatives of a whole series which have scarred Mars with chains of craters as they broke up and impacted. However, there are problems with it. Firstly, the common type of asteroid found near the edge of the belt closest to Mars is different from the type of asteroid Phobos and Deimos would be if they are asteroids. That type is found near Jupiter. This is due to the inner belt being warmer than the outer belt, so the composition differs because temperature makes a difference to them. Secondly, both moons have almost perfectly circular orbits over the Martian equator, and if they were captured, they would usually have come in at a high angle to the equator and have markèdly elliptical orbits. This can be seen with Nereid, Neptune’s third largest moon, and Saturn’s moon Phoebe orbits backwards compared to most other bodies in the system. Therefore, if Mars’s moons are asteroidal in origin, something needs to be evoked to explain that. A simpler explanation would be that they emerged from the cloud which was forming Mars. This would be spinning in the same plane as any moons which formed from it, and if they were formed in situ they would be more likely to have almost circular orbits. However, as Steve astutely pointed out, the actual nature of the bodies themselves is very close to being asteroidal, and in fact is asteroidal, so maybe it doesn’t matter in most ways. In the sense of the physical nature of the two moons, they basically are asteroids. The way in which they aren’t is to do with their history and orbits, which may not be a sensible thing to focus on. The only thing which goes against this is that both are directly affected by orbiting Mars. Phobos has streaks because of the tidal forces of its planet, and Deimos accumulates fragments and dust from itself as it moves through its rather short orbit. If they were orbiting in the asteroid belt itself, neither of these things would be happening. All that said, I can totally see the argument that they are in fact just asteroids in an unusual place which are also moons rather than minor planets. So I agree with you Steve.

This connects to a wider issue which affects Pluto, and it also affects a number of other worlds in the system which if addressed could solve the problem of knowing what to call the big round things in our Solar System. It could also address the peculiarity of our own “moon”. The 2006 CE definition of a planet by the International Astronomical Union is:

The IAU members gathered at the 2006 General Assembly agreed that a “planet” is defined as a celestial body that

(a) is in orbit around the Sun,

(b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and

(c) has cleared the neighbourhood around its orbit.

This definition was motivated by the discovery of a number of relatively large trans-Neptunian objects. Eris, discovered at the start of the previous year, has now been established to have a diameter of 2326 kilometres and a mass of 1.6466 x 1022 kilogrammes. Sedna, discovered in 2003, has a diameter of around a thousand kilometres and an unknown mass because unlike Eris it seems to have no moons. Sedna is less of a threat to the status quo but Eris was initially thought to be larger than it has now turned out to be. For comparison, Pluto is 2376.6 kilometres and it has a mass of 1.303 x 1022 kilogrammes, so it’s actually slightly larger than Eris but also less massive, so the question arose of whether it would be acceptable to admit a potential host of newly discovered planets, thereby reducing the “specialness” of planets, or to invent a new category. This last idea, of “dwarf planets”, seems very odd to me because the category of “minor planet” had existed for a very long time up until that point and instead of inventing an entirely new class of object, it would’ve made more sense, if they were going to do this. Whether or not I agree with the decision, there seems to be no merit in creating a whole new category of “planet” when “minor planet” already existed. I honestly don’t know why they did this.

Many people have disagreed with the decision to demote Pluto. It did elevate Ceres, previously considered a mere asteroid, at the same time. Before that point, for most of its history since discovery Ceres was considered an asteroid, but it’s the only body in the asteroid belt which has managed to make itself round due to its own gravity (there might be other bodies which just happen to be round-ish through chance because asteroids are irregular and could hypothetically be many shapes, including spheroidal), so it probably does deserve special recognition.

In spite of this definition, which is quite unpopular, a paper has recently been published on the subject arguing that Pluto, among other worlds, does in fact merit planethood. The paper can be found here. It’s sixty-eight pages long and I haven’t read the whole thing but the general gist of it seems to be that there used to be a scientifically arrived-at understanding of what a planet was, but over a period in the early twentieth century when astronomers focussed more on what was happening outside the Solar System, the popular uneducated public understanding of what a planet was took over. I have to say this doesn’t reflect my perception of what happened based on my knowledge of astronomy. I’m aware of the controversy about the canals, the discovery of Pluto, the idea that Mercury always faced the Sun and so on, all ideas which resulted from astronomical research at around that time. I’m aware of the research that was being done at the time about stellar evolution and the realisation that there were other galaxies, but it really doesn’t seem like they were concentrating that much on that more than this Solar System, but anyway, that’s what this paper claims.

Further, it claims that because they adopted a kind of folk understanding of what a planet was, it had led to them adopting earlier, non-scientific ideas about it. So for example, the public was really into astrology and had only recently got used to the idea that the Sun was at the centre of the Solar System rather than Earth. The authors of the paper give examples of how scientific classifications differ from public ones. For instance, most people think of fruit and vegetables as two different things but when it comes to botany, vegetables include fruits, which are the reproductive organs of plants, so from a culinary viewpoint fruit and veg are separate but scientifically they aren’t. To this I would add a couple of things which are I hope relevant to astronomy. One is that I think of a lot of things as fruit, such as tomatoes, aubergines, courgettes, peppers and tomatoes, which other people seem to think of as vegetables because it makes sense to me to think of them nutritionally and in terms of flavour in that way. The other is that the culinary arts are also sciences, and it seems a bit hierarchical to see them as inferior to botany for some reason. After all, we all need to eat. Applying that to astronomy and planets, that would mean that although some things are planets and some things aren’t according to astronomers of a particular vintage, that doesn’t mean there isn’t another branch of science which would view them differently. For instance, everything is subject to the laws of physics, and geology would seem to apply pretty much equally to planets, moons and asteroids in their own way. They’re just bodies in space like everything else. Therefore, I’m not convinced about this. Also, the general public were specifically irritated at the idea of Pluto not being a planet any more, so I don’t see how exactly they were using the public view of what planets were if they managed to annoy so many non-astronomers with their assertion that Pluto wasn’t one.

What seems to have happened is that the problem crept up on astronomers and they kind of panicked and made a fairly slapdash and hasty decision. As various large bodies were discovered on the edge of the Solar System, they became uncomfortable with the idea that they were probably going to end up with a very long list of planets, which seemed unwieldy and not very “neat”, and they also perceived it as an imposition on education that people were going to have to learn about so many worlds. They seemed to feel like this would be regarded as off-putting. The paper compares the situation with how mammals are defined. The official definition of a mammal is now rather abstruse, because it actually hinges on how many bones are in the jaws and the ears, but this is partly because of the need to identify fossil mammals. The widely-used definition is “animals who suckle from their mothers as infants, maintain a different body temperature from their environment, are often covered in fur or hair and mostly give birth to live young”, and the first criterion is the most important. There are exceptions to most of these. For instance, some hibernating mammals don’t keep their body temperatures above their surroundings and humans, whales and elephants are largely hairless, but this is a fairly good definition. However, claim the authors, astronomers have taken a weird approach to planets, having concentrated on whether they dominate their local region, which is in any case vague because what’s local? They’ve also looked at how they move. If mammals had been defined in this way, as warm-blooded vertebrates who walk in herds on land for example, a lot of mammals would’ve been excluded. Bats and whales would then not be mammals and any mammal who has a largely solitary life, such as leopards or sloths, would not then count as mammals either.

Looking at the history of the idea of planets, for a long time any round object in the sky which didn’t appear to stay in the same place was a planet. This used to include Cynthia and the Sun, when people thought Earth was at the centre of the Universe, and it didn’t include Earth. Later on, the four largest moons of Jupiter were discovered and also referred to as planets, and even the thick parts of the rings on either side of Saturn due to the poor quality of telescopes at the time. Later still, Ceres was called a planet because it seemed to fit into Bode’s Law, and turned up where it was expected. By that time, however, the known satellites had been relegated to moons, and soon after Ceres was also demoted because it was realised that there were thousands of other bodies between Mars and Jupiter, some even quite large.

The 2006 definition also has a rather silly consequence which a few people have noticed: it means Earth isn’t a planet! As I’ve mentioned before, from the Sun’s perspective Cynthia doesn’t orbit Earth, but the two weave in and out of each other’s orbits. I’m not completely clear what the astrological influence is supposed to be, but I think it’s the emphasis on orbits, i.e. the kind of definition which would’ve excluded bats, whales and leopards from being mammals. Whatever the definition of a mammal is, it seems to make more sense to use their anatomy and physiology than other more dubious criteria. Both of the definitions I mentioned above do this. The first is rather abstract and strange to most people, although there are good reasons for it – mammal jaws and teeth survive better than the rest of their bodies so it’s like identifying a body by dental records – but both of them focus on what their bodies are like, which seems entirely sensible compared to that fictional other definition.

What, then, is proposed as a more sensible definition of a planet? Well, it’s closer in spirit to that way of defining a mammal. A planet is a geologically active body. I have to admit I’m not sure about this because of various things, such as “eggshell planets”, and I’d also want planets to be round and I can’t tell if they also stipulated that. What it means (I’ll get back to eggshell planets in a moment) is that Pluto’s Sputnik Planitia which is created by frozen nitrogen and is active even though the Sun isn’t strong enough at that distance to have that effect. In talking about asteroids, I’ve mentioned the fact that the larger ones tend to be layered like Earth is, but the smaller ones are either rubble piles or mixtures of different minerals and other substances which aren’t separated out in the same way. A geological process has done this sorting in the larger ones, and consequently Ceres, for example, could count as a planet: it has been geologically active.

This applies also to some moons. Io, the innermost large moon of Jupiter, is intensely active with continual volcanic eruptions, to the extent that it’s thought to “turn itself inside out” every few years – some much of its interior is spewed onto the surface that the former surface becomes the interior and proceeds to get thrown out itself a few years later. This is because of the tidal forces effectively “wringing” the moon all the time, with the other large moons in the Jovian system along with Jupiter itself wreaking havoc on the place. By this standard, Io is definitely a planet, albeit a planet which is also a moon.

I’ll now permit myself a digression into eggshell planets. An eggshell planet is a surprising kind of “planet” which kind of “does nothing”. It isn’t necessarily possible to tell from a distance which planets are like this. Earth’s crust is divided into plates, and other planets have a thick, solid layer all the way round, but there is another possibility or which at least three examples may have been found already. This is where the crust is thin and fragile, and so cannot have plates or thick layers, and also can’t even support mountains or hills, so the surface is solid and also smooth, and nothing happens there – no volcanic eruptions, continental drift or erosion, because there’s nothing to erode. The question arises of whether this even counts as a planet under this new definition, since it isn’t geologically active. However, there are no such planets in our Solar System as far as anyone knows, and they’re probably quite rare.

There are three categories of planets suggested in this new definition: terrestrial planets; giant planets; satellite and dwarf planets. The last category is the largest. It includes the large moons of Jupiter, Ceres, Titan, Pluto, Charon, Eris and Sedna, and in fact there are more than a gross of these. Far from the expected response, apparently people tend to be quite excited at the idea that there are so many planets around the Sun. The giant planets include Jupiter, Saturn, Uranus and Neptune, so no surprises there, although this clear-cut division may be an artifact of how our own Solar System is, with its complete absence of the very commonest type of planet, the mini-Neptune, intermediate between Earth and Neptune in size.

There are five planets in the terrestrial category rather than four, because once the criterion for dominating its orbit has been removed, Cynthia becomes eligible, which makes me very happy! Cynthia is not even in the same group as the satellite and dwarf planets, but a planet just like Mars and Mercury. This also means that the Apollo astronauts landed on another planet, not just our moon. As well as that, Earth now has no moon!

It seems that the process leading to the decision to redefine planets was not very scientifically grounded and was in fact rather acrimonious. The orbital dynamics people took umbrage at the geophysical definition and there were only a few days available for debate, forcing people to take sides quickly without due consideration. Planetary scientists were underrepresented because they’re apparently not officially astronomers, which is a bit astonishing. Another motivation was to keep the number of official planets low because the IAU didn’t expect the alternative to go down well with the public because previously, i.e. in Victorian times, they’d felt more comfortable with a small number of planets. They were used to seven at that point, including the Sun and Cynthia. This is probably no longer the case, so in 2006 they made a decision based on misjudging the mood of the general public.

To finish, I’m going to make a commitment. Henceforth I will be referring to every spheroidal body in the Solar System as a planet, although I will also acknowledge what kind of planet it is, such as a moon or dwarf planet. And Pluto is a planet!

I’d be delighted to hear your views on this.