Neptune may be the outermost planet. After the torridity of having to refer to the previous planet by a silly name or bear the brunt of using an unofficial name, it’s nice to have the calm of just being able to call it “Neptune” without the irritation of puerile jokes. That said, things could’ve turned out very differently because one of the names considered for the seventh planet was actually Neptune!
The two planets are the most similar pair in the entire system. That said, having fixated on Hamlet for so long, right now the two don’t look that alike to me. Neptune has no obvious rings, spins more upright and is a much clearer and more vivid (livid?) blue than the hazy and almost featureless Hamlet. The further out a gas giant is, the more likely it is, even if bigger than Jupiter, to look like Neptune. If Tyche exists, it will be blue, and outer planets in other star systems whose stars provide less radiation than about a thousandth of solar intensity at our distance from it are also probably going to look like this, although much dimmer. The above image is actually more colourful than it would look to the unaided human eye, at least at first. At Neptune’s distance, the Sun is nearly a thousand times dimmer than at Earth’s. The logarithmic nature of senses means that this wouldn’t seem as dim as that suggests. It’s still about 360 times brighter than Cynthia ever gets. Moonlight is insufficient to make out colour, but I don’t know about sunlight on Neptune. In a way it’s odd even to consider what colour Neptune would look like to human vision as nobody will ever see it in person and it would appear to be coloured to some species who live on this planet, particularly nocturnal ones.
The Titius-Bode series does not apply to Neptune. It’s actually 30.1 AU from the Sun rather than the predicted 38.8, although Pluto is much closer to that distance. That doesn’t mean Pluto is or isn’t a planet by the way, but that astronomers expected there to be one there and therefore called it one. What’s actually happening there is quite interesting, but I’ll leave that for now. Neptune was discovered in 1846, by which time a large number of asteroids had also been found and Ceres was no longer considered a planet, which led to the idea that Bode’s Law was mere coincidence. The revision which was able to include Hamlet’s major satellites could be seen, again, as a form of pareidolia, where an increasingly vague formula is used to fit observed phenomena which actually doesn’t reflect any real process or effect but just corresponds to the various coincidences. The sequence was originally n+4, with n=0 for Mercury, rather than a simple doubling sequence, and the fact that the asteroid belt intervenes and Neptune doesn’t fit makes the idea that it’s an actual law more doubtful because there are then three out of ten exceptions to the rule. A side issue, probably not important, is the surprising convenience of Earth being at a round ten units from the Sun. The question arises, then, of whether there really is something about Neptune which puts it in the “wrong” place or whether it’s just that the spurious correlation was revealed by it. Most astronomers would agree with the latter possibility.
Neptune is not the coldest planet in the system in spite of being further from the Sun than any other known planet, at least consistently. This is because, unlike the seventh planet, it has a significant internal heat source. It takes 165 years to orbit the Sun, and having a moderate axial tilt this gives the temperate regions four-decade-long seasons. The axial tilt is 28° and the day lasts sixteen hours, which is technically close to Hamlet’s but differs in that the poles don’t spend most of their time pointing towards or away from the Sun. It might therefore be expected to have seasons dominated by the Sun, but this isn’t obvious because unlike its twin, Neptune is heated internally. This leads to Neptune being warmer than the other ice giant at cloud top level. Like the other outer planets, this heat is due to contraction of the planet from the part of the solar nebula it formed from, but in Neptune’s case there may be an extra factor in the form of its large moon Triton’s tidal influence. The centre is at around 7000°C compared to the other giant’s 5000, possibly because Neptune wasn’t disrupted, but it could also be that both planets go through warmer and colder phases and we happen to be living at a time when it’s that way round. I don’t actually know how they arrived at these figures considering that there are theories that the clouds are cold due to insulating convection layers, meaning that heat doesn’t leak out and is therefore presumably undetectable, but this is what they say. Neptune’s centre is therefore hotter than the surface of the Sun.
Regardless of the temperature at the core, the cloud tops are still very cold at around -200°C. Before Voyager 2 got there, it was speculated that the low temperature could give rise to fast winds in the atmosphere because the vibration of gas molecules at higher temperatures was absent, leading to a low-friction environment, and this did in fact turn out to be so. The winds are the fastest recorded in the system at over 2000 kph. At the equator, the average wind speed is around 1100 kph, which is about the same as the speed of sound at sea level on Earth. On Earth, the Coriolis Effect is somewhat significant in generating wind but the main driver is the primary or secondary solar heating and cooling. The Sun heats the air on this planet, causing it to expand, or cooler areas have contracting air over them, allowing the warmer air to move in and occupy the space due to the pressure difference, or in a more complicated process, land and water change temperature at different rates, causing air movement. Although the core of Neptune is far hotter than its exterior, this doesn’t seem to drive the extreme high velocity winds near the cloud tops. My guess is that it’s somewhat similar to a perpetual motion machine, which of course cannot exist. The input from whatever source to the weather systems, such as the Coriolis Effect, tidal forces and the hot interior of the planet, puts the atmosphere in motion and due to the lack of friction that energy is only lost very slowly, and consequently the winds accelerate until they reach the speed of sound, which prevents them from moving any faster. This is not a detailed explanation and may well be completely incorrect. It’s just a guess.
Neptune has more visible banding than the other ice giant, and also has rotating storms in its atmosphere which have been observed to last up to six years. This is far less durable than Jupiter’s storms, but the size and energy input are smaller so this might be expected. Neptune’s Great Dark Spot is visible in the lower part of the picture at the start of this post, but here it is again:
The spot was 13 000 kilometres long by 6 000 wide, and is a hole in the cloud deck. The white clouds around it are cirrus made of frozen methane and were instrumental in enabling the wind speed to be measured. It’s thought that the spots disappear as they approach the equator, which can take years. As I may have mentioned before, the Great Dark Spot was at the same latitude as Jupiter’s Great Red Spot, and this suggests it’s recurrent. If it is, it also shares with the GRS a tendency to appear and disappear. I’ve mentioned elsewhere that it seems to be more than coincidence that planets tend to have a fluid-related feature at this latitude, including Hawaiʻi, Olympus Mons, the Great Red Spot and this storm, which is intermittent, and although I have a vague impression of a pyramid superimposed on the bodies in question with the apex at one pole, I can’t put my finger on why this would happen or whether it actually is more than cherrypicking.
Neptune’s blueness can’t be explained simply through Rayleigh scattering and there must actually be something blue in its atmosphere which isn’t in Hamlet’s, but what this is exactly is another question entirely. Even so, it is true that the methane contributes by absorbing red light. The different hydrocarbon content contributes to it being warmer than Hamlet due to a greenhouse effect, although this is only relative as it’s still at the temperature of liquid nitrogen on Earth.
This is a fairly well-known image of clouds on Neptune above the more generally blue cloud deck. These clouds are frozen methane, but the picture also seems to show that not far below them is a blue haze with a definite level top to it. The clouds are about fifty kilometres above the haze and are casting such definite shadows because the Sun is low in the sky at this point, as evinced by the night on the right hand side of the image. Although the widths of the clouds here varies between around fifty and two hundred kilometres, I don’t know how that scale compares to the clouds in our own sky. It does sound rather larger at first consideration. I’m also tempted to see them as having been streamlined by the powerful winds and feel they don’t have much chance to be wispy, unlike Earth’s cirrus clouds. They’re almost like contrails in a way.
One theory about Neptune’s clouds is that the planet’s atmosphere is effectively a giant cloud chamber. A cloud chamber is a delicately balanced humid atmosphere used to detect subatomic particles, whose energy as they move through it leaves wakes in the form of clouds. This can be created using the steam from dry ice. The planet in question is of course very cold at the height the clouds can be seen, and it’s been theorised that galactic cosmic rays stimulate the atmosphere into producing these streaks. The coolness of the atmosphere makes these things much more significant for Neptune than here, so if this is how it happens, the cause is similar to the high winds. Ultraviolet light from the Sun is also probably responsible for features in the atmosphere, but probably the haze more than the clouds.
The rate of rotation has the same features as that of the bigger gas giants, as the planet does not rotate as a solid body would. The magnetosphere can be taken as a guide to the rotation period if you like, but it isn’t necessarily any more “real” than anything else and we only think it is because we’re from a planet with a solid surface and a shallow atmosphere. The magnetosphere takes sixteen hours, the equator eighteen and the poles twelve. All of this also raises the question of whether it even means anything to assert that Neptune has powerful winds. Maybe that’s just the rotation of the planet, which varies, but it doesn’t mean they actually amount to winds just because different parts rotate at different rates. The understanding of fluid movement used with Jupiter, that they’re cylinders rotating independently, actually cancels out the idea that there are such winds, although there could still be slipstream areas where the wind would be felt.
Unsurprisingly, the interior of the planet closely resembles the other ice giant’s. As I mentioned before, Olaf Stapledon described Neptune, important in ‘Last And First Men’, thus: “. . . the great planet bore a gaseous envelope thousands of miles deep. The solid globe was scarcely more than the yolk of a huge egg.” The upper atmosphere is mainly hydrogen and helium with some methane. Deeper inside is a liquid, becoming solid, layer composed of water, ammonia and methane, and at the centre is a core somewhat larger than Earth made of silicate rock and iron. Like Hamlet, it probably rains diamonds and there are likely to be diamond-bergs floating in the ocean. There may even be a whole layer of diamond deep within the planet.
There being two similar planets of this kind in the system might be seen as coincidence, but in a cosmic context seems not to be. In fact, Neptune-like planets are more common in the Galaxy than Jupiter- or Saturn-sized ones, and the fact that only one spacecraft has ever visited either hampers understanding of a disproportionately large number of worlds. There are nearly 1 800 known Neptune-like planets, notably referred to as “Neptune-like” rather than “Uranus-like”, which makes me wonder again about that ridiculous name although Neptune is more “typical” seeming since it isn’t tipped on its side. Even more common, and absent from the known Solar System, is the intermediate-mass type of planet both smaller than Neptune and larger than Earth. Some of these are much closer to their stars than our own ice giants, and can’t therefore really be classified as such. Nonetheless, this size and mass of planet is common in the Universe.
Getting back to our own Neptune, one surprising finding was that like Hamlet’s magnetic field, Neptune’s is off-centre and at a radically different angle to its axis of rotation. This creates another puzzle because the orientation of Hamlet’s magnetosphere was attributed to its peculiar tilt and misadventure with a large body in the distant past, but given that Neptune’s is also like that suggests that this is irrelevant and makes me wonder if that ever happened, although the tilt does need to be explained. It’s offset by 55% of the planet’s radius and the magnetic poles are 47° from the axis of rotation, yet no explanation based on collisions or close encounters with large objects has been offered so far as I know.
That said, Neptune does in fact show some evidence for this. Discounting Pluto and Charon, the planet has the largest proportionate satellite of any planet in the system but Earth, namely Triton, which is also the only large moon to orbit backwards, and appears to be a captured dwarf planet. Also, the moon Nereid has a comet-like orbit with its closest approach to the planet being much greater than its greatest distance, making it elongated and highly elliptical. Hence one catastrophe may have occurred to Hamlet and another radical event to Neptune, and the question then arises of what was happening in the outer solar system early in its history. Neptunian auroræ are not distributed like terrestrial ones due to the different magnetic field and the presence of rings, which reduces the quantity of charged particles trapped in the magnetosphere. Neptune and Triton also interact magnetically in a similar manner to Jupiter and Io, although not so strongly. There are diffuse auroræ close to the equator to just over half way to the poles, and more definite rings of auroræ closer to the poles, and brighter near the south pole at the time of the Voyager 2 encounter. Neptune has the weakest magnetosphere of any gas giants.
As mentioned above, Neptune has rings. Once Jupiter’s rings had been discovered by the Voyagers, Hamlet already having had them detected, it seemed inevitable that it would have them too, and it has. They were discovered from Earth in 1984 CE but had been seen occulting a star in 1981 in a manner compatible with them not being complete. That is, it was established that there were curved objects orbiting the planet but not that they went all the way round. This is probably because their width varies more than the other three planets’. There was an uncomfortable period in the early ’80s when for me it seemed inevitable that Neptune would be ringed but there was no evidence either way on the issue. I wanted the giant planets to be uniform. For some reason its ringedness is less emphasised than the others’, maybe because it had become routine by that time and it would’ve been more surprising if it hadn’t been.
There is no uniform scheme for naming planetary rings, as can be seen with Hamlet’s. Neptune’s are named after astronomers associated with the planet, specifically Galle, Le Verrier, Lassell, Arago and Adams. Adams is the one with the wider arcs, which are named Liberté, Egalité, Fraternité and Courage. Egalité is split into 1 and 2. Three small moons orbit between the rings, and there’s another ring associated with the moon Despina. In a way it’s quite nice that there’s a French theme to the naming contrasted with the English theme for Hamlet, but I don’t know if it’s deliberate. One really surprising thing about them is that the supposèd “discovery” was actually an occultation by the moon Larissa, so although they were correct about them being rings, they were correct by chance and misinterpretation of an unusual astronomical event. Neptune is a harder target for ring detection than Hamlet, although that is itself not easy, because it moves so slowly against the background with its 165-year orbit. The rings are, like the other ice giant’s, very dark and of course even dimmer due to the greater distance from the Sun. There’s a big contrast in the widths, with the three inner rings being only about a hundred kilometres wide (i.e. their height) and the others being several thousand, which is unlike Hamlet’s much thinner ones. An image of them with the contrast turned up to show details of the structure looks like this:
It’s really come to something when a planet invisible to the naked human eye is made so bright that its glare almost bleaches out the view of its even dimmer rings. This is a ten-minute exposure made by Voyager 2, which was right there, and still the rings are hard to see without that kind of technique. Whether the average human eye could see them is another question, as ours are very good at adjusting to low-light conditions. It still isn’t that low though, at least compared to bright moonlight, but I fear I’m repeating myself. In fact, all the conditions that apply to sunlight on Pluto also apply to it on Neptune because their orbits overlap distance-wise (they don’t literally). Hence the Sun at Neptune’s distance is just a star. The minimum visible object to someone with good vision is one minute of arc across. After that, it’s visible if it’s luminous but not as an actual shape. This is equivalent to a hair’s breadth viewed from twenty-five centimetres away. From Earth, the Sun appears as a disc thirty times that diameter and is therefore very obviously a ball of light. Neptune, however, is thirty times as far away and the Sun could therefore not be seen as anything more than a star, which is effectively a point source of light. This is, however, quite misleading as it’s still many thousand times as bright as any other star in the sky, and might therefore not appear as a point due to its glare. Lighting conditions on Pluto have been likened to those on Earth after a sunny day shortly after sunset, so the same kind of thing can be expected on Neptune and its moons. In other words, you’d probably hardly notice it at all after a while and it would look like broad daylight, except that the actual illumination is only a thousandth that of the Sun’s here. Looking at it from the other end of the telescope, as it were, Neptune is the only planet in the system, taking Pluto as a non-planet, which is never bright enough to be seen. Its maximum brightness is something like four times dimmer than it would need to be to become visible. Of course there will, as with other celestial bodies, be other species who can see it and in fact Galileo saw it, through a telescope of course, but didn’t notice it was a planet. Likewise, it was reported that it had rings shortly after it was discovered but in this case it was probably an illusion.
Neptune has a rather odd array of satellites. At one point it was thought that Triton might be the largest in the Solar System, and as I mentioned above it orbits backwards compared to most other moons. Nereid has a very eccentric orbit. Up until the 1980s, these were the only two moons known, but Voyager 2 surprisingly discovered a moon, now called Proteus, which is actually larger than Nereid, making it the largest object discovered by the Voyager probes. Due to the mistake leading to the accidentally correct conclusion that the planet has rings, the moon Larissa was also detected in 1981 but it wasn’t realised that this had happened, rather like Galileo and Neptune itself. Voyager 2 found another five, including Proteus, and a further six were discovered this century. Neptune also holds the record for having the most distant moon and the longest time taken for that moon to orbit, Psamathe, which is fifty million kilometres from it and has a period of almost twenty-five years. There are various interesting things going on with Neptune’s moons but that can wait until my next post.
Probably the most prominent appearance of Neptune in science fiction is in Olaf Stapledon’s ‘Last And First Men’. Published in 1930, the science is well out of date, although the description of a yolk in an enormous egg is valid. In this account, our distant descendants are living on Venus an æon hence when they observe a mass of gas on a collision course with the Sun which will cause the Solar System to be disruptd and the Sun to become what we would probably call a red giant the size of the orbit of Mercury. Humanity decides, though not en masse, to escape to Neptune, where it has to contend with enormous gravity and pressure, and first a very cold climate followed by a very hot one. Humans cease to be intelligent and take four hundred million years to evolve into a sentient form again. This is partly because their lifespan is much longer, as most species live at least one Neptunian year. They ultimately become superhuman beings who notably have ninety-six genders and a life expectancy of a quarter of a million years. I find this section of the novel, if that’s an accurate description, to be a particularly satisfying example of speculative evolution, although one which has been left standing by scientific discoveries about the planets involved.
That’s probably a fairly adequate introduction to Neptune. Next time: Triton.





























