est31 a day ago

How is the size defined for a gas planet? The gas density just keeps dropping, where do you draw the line (isosurface, rather)? Earth's radius is always the one without earth's atmosphere.

  • jessriedel a day ago

    As others note, the definition of Jupiter’s radius is set by where the pressure is 1 bar. This is somewhat arbitrary, but the arbitrariness doesn’t matter much: the pressure drops to 1 microbar just 320 km higher, which is <0.5% of Jupiter’s ~70,000 km radius.

    • queuebert a day ago

      Venus would get a slight radius buff, too, if we applied that metric.

      • hnuser123456 18 hours ago

        But Venus has a solid surface.

        • queuebert 9 hours ago

          Yes, that's why I said buff. The radius as defined would increase, because surface pressure is 90 bar, so at 1 bar, you're pretty high in the atmosphere. I can see merit in such a definition because that is the level at which we wouldn't have to pressurize our space stations to be comfortable. (Really 1/3 bar is fine too.)

  • layer8 a day ago

    The density falls off pretty steeply at the “edge”, so the exact definition only makes little difference for the radius: https://www.researchgate.net/figure/Density-vs-radius-for-a-...

    • formerly_proven 20 hours ago

      This is because of Newtonian gravity being inversely proportional to the square of the radius, right?

      • marcosdumay 15 hours ago

        It's related to the Boltzmann distribution being an exponential. But there are all kinds of effects that make a planet's atmosphere deviate from an ideal gas at rest in a homogeneous container.

      • skykooler 19 hours ago

        Gravity changes little over that distance - it's more because of the compounding effect of atmospheric pressure (the deeper you go, the more air you have above you which raises the pressure, raising the density and meaning that pressure increases exponentially faster).

        • vecter 17 hours ago

          What makes that curve exponential?

          • skykooler 7 hours ago

            Starting at an initial density of air, suppose you descend a distance D such that the air density doubles. Now your air is twice as dense, which doubles the pressure underneath it, meaning if you descend a further D the density will double again. Continue ad infinitum (or at least until the ideal gas law stops being a good approximation).

          • westurner 16 hours ago

            Newtonian gravity (classical mechanics).

            Two-body gravitational attraction is observed to be an inverse square power law; gravitational attraction decreases with the square of the distance.

            g, the gravitational constant of Earth, is observed to be exponential; 9.8 m/s^2.

            Atmospheric pressure: https://en.wikipedia.org/wiki/Atmospheric_pressure#:~:text=P... :

            > Pressure (P), mass (m), and acceleration due to gravity (g) are related by P = F/A = (m*g)/A, where A is the surface area. Atmospheric pressure is thus proportional to the weight per unit area of the atmospheric mass above that location.

  • Maxatar a day ago

    It's defined as the distance from the center of mass to the point where the pressure is equal to the pressure on Earth at sea level.

  • amelius a day ago

    It's a matter of definitions, so we skip them and just choose something that makes sense to humans.

    • philipov 20 hours ago

      The most important thing about definitions is that we apply them consistently. A different definition might give different answers, but it's fine as long as it does so uniformly.

      • JumpCrisscross 19 hours ago

        > most important thing about definitions is that we apply them consistently

        The most important consideration for a definition is its practical consequence.

        In this case, whether the line is drawn at 1 bar or an order of magnitude more or less doesn’t materially change that, on the same measure, Jupiter was 2x larger in the past. (Less than 1% in both cases.)

        In a different context, that difference may be meaningful and should thus be noted and tested for robustness.

      • amelius 18 hours ago

        The point is that there will be multiple definitions, so which one do you choose? From there your conclusion can be that we just use a loose definition that humans can easily grasp.

yubblegum a day ago

I've always wondered about the core of these gas giants. I assume it is some liquid form of light elements. What is puzzling is the presence of the gas giants in the middle of solar system's planetary line up: why are they in the middle and the ones closer or further away from the central star are not like them? Is it the temperature gradient?

  • mnky9800n 2 hours ago

    Because of solar wind. After the sun formed from the material of the proto solar system it started producing solar winds. This pushes light elements to the edge of the solar system but heavy elements stay. So rocky planets form. Then the light elements collect as well and reenter the interior solar system as comets which redeposit light elements on the surface of rocky planets. In the mean time the light elements that collected together in great quantities formed the gas planets.

    This is all a very traditional view afaik and doesn’t explain where mantle light elements come from. For example there is a great deal of water that is in the mantle that drives geochemical changes in the mantle rocks. Was that there originally? Or was it put their after plate tectonics started and subduction sucked water into the mantle? I don’t know but I would assume there are plenty of geodynamics people who would have opinions more deeper than mine on the topic.

  • yencabulator 19 hours ago

    > Data from the Juno mission showed that Jupiter has a diffuse core that mixes into its mantle, extending for 30–50% of the planet's radius, and comprising heavy elements with a combined mass 7–25 times the Earth.

    https://en.wikipedia.org/wiki/Jupiter#Internal_structure

    > This has resulted in the theory that Jupiter does not have a solid core as previously thought, but a "fuzzy" core made of pieces of rock and metallic hydrogen.

    https://en.wikipedia.org/wiki/Juno_(spacecraft)#Scientific_r...

  • Tepix a day ago

    > I assume it is some liquid form of light elements.

    Why would you assume that? The heavier elements such as iron are likelier to move to the center of gravity.

    • k__ a day ago

      I'd assume these elements would be created in the sun and keep close to the sun, because of their higher mass.

      • frutiger a day ago

        All the heavier elements were created in a former star that went supernova. The solar system formed from the gas/dust after that.

        The heavier elements being formed in our sun now are going to stay there until something can tear it apart.

        • pfdietz 21 hours ago

          Some will be ejected back into space when the aged Sun becomes a planetary nebula (with a white dwarf at the center).

      • bell-cot 17 hours ago

        Until several billion years in the future, our sun will create no element heavier then helium.

        IIR, our sun's mass is far too low to ever create any element heavier than carbon.

  • everyone 20 hours ago

    In an Arthur C Clarke story (I forget which one) the core of jupiter is a planet sized diamond.

    • ReptileMan 20 hours ago

      Space Odyssey one of the sequels.

      • teamonkey 19 hours ago

        2061. Not his best work, alas.

        • bell-cot 17 hours ago

          Actually 2010, in the closing words of Chap. 38.

          Though I agree that 2061 fell rather short of his usual.

lukan 16 hours ago

That seems at odds, with something I previously learned about Jupiter:

"As a result, Jupiter is thought to have about as large a diameter as a planet of its composition and evolutionary history can achieve."

https://en.wikipedia.org/wiki/Jupiter

So is this a significant new finding, changing previous assumptions, or is it part of the "evolutionary history" meaning it was assumed before, that in early times it was bigger?

  • vlovich123 13 hours ago

    The new part is probably the precise details about size and strength of the magnetic sphere in the past and that they used a different mechanism to fill in gaps in existing theories.

    > Importantly, these insights were achieved through independent constraints that bypass traditional uncertainties in planetary formation models—which often rely on assumptions about gas opacity, accretion rate, or the mass of the heavy element core

    > The results add crucial details to existing planet formation theories, which suggest that Jupiter and other giant planets around other stars formed via core accretion, a process by which a rocky and icy core rapidly gathers gas. These foundational models were developed over decades by many researchers, including Caltech's Dave Stevenson, the Marvin L. Goldberger Professor of Planetary Science, Emeritus. This new study builds upon that foundation by providing more exact measurements of Jupiter's size, spin rate, and magnetic conditions at an early, pivotal time

    https://www.caltech.edu/about/news/jupiter-was-formerly-twic...

waynecochran 20 hours ago

    > Because Amalthea and Thebe have slightly tilted orbits, Batygin and Adams analyzed these small orbital discrepancies to calculate Jupiter's original size…
This seems like a non-sequitur. What do tilted orbits have to do with size?
bethekidyouwant 21 hours ago

When the solar system was young, Jupiter was hotter and spun faster. (which affects its radius, but not its mass) This is not new information.

rwmj a day ago

Couldn't read the actual paper as it is paywalled, but does "twice its current radius" mean that it had a larger mass, and if so what happened to all that extra mass?

  • adrian_b a day ago

    The mass did not differ much from the present mass, but the planet was less dense and with a more rapid rotation.

  • lazide a day ago

    It was hotter, a lot hotter.

    Like stars, radius for a gas giant is increased by heat, and decreased by increased mass.

    These two factors are rarely completely independent, of course, so it gets complicated. Especially in a star where masses are large enough to result in densities sufficient to cause fusion - and large releases of heat, which then cause decreased density, etc.

    But all other factors being constant, the volume of a gas increases (and density decreases) as temperature increases.

    See page 6 and the first couple paragraphs of page 7 in the paper for a breakdown.

    Eventually Jupiter will cool enough it will be a small fraction of it’s current size, assuming that our understanding is correct and it doesn’t have enough mass to meaningfully result in fusion regardless of how dense it gets. [https://www.pas.rochester.edu/~blackman/ast104/jinterior.htm...]

    In theory, it will even eventually cool to the point all those clouds and atmosphere are liquid (or even solid!) gas oceans. That is going to take awhile.

    • queuebert 21 hours ago

      > ... decreased by increased mass.

      I don't think this is in general true for planets or stars. You're confounding multiple effects. For a fixed number of particles, increasing metallicity, which follows average particle mass, should reduce radius, but for a fixed metallicity and temperature, increasing particles will increase radius. Temp has the effects stated. You can roughly validate this by the fact that massive planets and stars are bigger than less massive ones. Obviously many other things start happening as stars reach end of life...

      • lazide 2 hours ago

        In the sense that higher gravity increases density all other things being equal. yes, absolute size will slowly increase - until it collapses, anyway.

    • greggsy a day ago

      Could it cool and crystallise?

      Could those crystals then erode and reform again as sedimentary rocks to be come a solid planets like earyh?

      I understand that’s not how earth itself came to be, but it’s an interesting metamorphosis that I hadn’t previously considered.

      • jessriedel a day ago

        Like the interior of the planet, the atmosphere is overwhelmingly hydrogen and helium. And helium is liquid even at 0 temperature unless under pressure, so presumably (?) would be liquid on the surface. These materials are mechanically very different than the silcates and metals dominating the Earth’s crust, and I don’t think we even have well measured bulk properties? Not sure what erosion processes would look like.

      • lazide a day ago

        At the point hydrogen, helium, ammonia, etc. have cooled to solid ‘rock’, chemistry and weather as we’re familiar with it doesn’t really apply anymore. Pluto has been that way for a long time though, albeit good luck spending enough time there to get very familiar with it.

    • HappMacDonald a day ago

      > Like stars, radius for a gas giant is [..] decreased by increased mass.

      If this is the case then do you have any intel on why do the gas giants in our system appear to more closely directly correlate mass with radius instead of inversely?

      https://nssdc.gsfc.nasa.gov/planetary/factsheet/ Mass: Jupiter = 3.3 x Saturn = 22 x Uranus = 19 x Neptune Radius: Jupiter = 1.2 x Saturn = 3 x Uranus = 3 x Neptune

      I mean Saturn's density is far less than either of the other three planets, despite being smaller and less massive than Jupiter but larger and more massive than Uranus/Neptune, as well as slightly cooler than Jupiter and far warmer than Uranus/Neptune. And Saturn has the lowest angular velocity among the four, which it would make sense might have the opposite relative effect on density.

      • raattgift a day ago

        Neither Jupiter nor Saturn is close to thermal equilibrium, whereas the sun is. Bounded self-gravitating gas spheres in thermodynamic equilibrium can show negative specific heats [The classic LBLB, Lynden-Bell & Lynden-Bell, 1977 <https://adsabs.harvard.edu/full/1977MNRAS.181..405L>]. A negative specific heat capacity reducews the gas's volume as its temperature increases. Temperature in stars and gas giants is mostly lowering due to outward radiation driven by internal processes. Unlike a star, Jupiter's specific heat capacity is positive. Very roughly the sun's excess power output will cause it to grow (this handwaves a complex balance of temperature, pressure, mass, and nuclear fusion as it rises in the main-sequence part of the H-R diagram <https://chandra.harvard.edu/graphics/edu/formal/variable_sta...> -- as it climbs in that region with similar temperature the sun gets brighter because it gets bigger), while Jupiter's power output has been higher (presently about 2.5x) than its solar radiation input yet the planet has probably been shrinking.

        The energy input and internal heat budgets are under active study for Jupiter <https://www.nature.com/articles/s41467-018-06107-2> (open access), and will supply further evidence for various hypotheses about "primordial Jupiter", one of which is the topic here. One of the major points of comparison with a star here would be how the former is much more like an ideal blackbody than our local gas giants. And of course there is a dark side of Jupiter, while there is no dark side of the sun.

      • skywhopper a day ago

        They’re all made out of different mixes of gases and other elements, and are different distances from the sun, and any number of other variables.

  • exe34 a day ago

    Probably contracted as it's mostly gas.

  • Zardoz84 a day ago

    Not larger mass. Simply, was less dense. In layman terms, and if I understand correctly, was the result of the interactions of Jupiter, Jupiter's magnetosphere and Jupiter's circumplanetary disk.

WalterBright 15 hours ago

Presuming that Jupiter got its start from a cloud of gas and dust, far far larger, at what point did its gradual compression make it a planet?

As its rotation slows, it will shrink even further.

Civitello 17 hours ago

It shrank because of all the boys going there to get stupider.

fasteddie31003 a day ago

I am deeply skeptical of any "research" that concludes something in the past. The scientific method relies on observation, experimentation, and replication, but these aren't possible with past events, so we can't directly test or falsify historical claims. Instead, researchers infer conclusions based on indirect evidence like documents, artifacts, or statistical patterns—often without being able to isolate variables or rule out alternatives.

If something is not falsifiable, it is not science in my book. Research that is falsifiable uncovers deep truths of nature that will benefit humanity's progress, which this kind of research will not.

Sorry to be a downer. I haven't had my morning coffee yet.

  • layer8 a day ago

    Observations are inherently always about the past.

    • fasteddie31003 a day ago

      That’s true in a narrow sense—every observation records something that has already happened. But in science, observations can be tested, replicated, and used to predict future outcomes. The kind of "research" I'm skeptical of draws broad, causal conclusions about unique, unrepeatable past events where none of that is possible.

      • layer8 a day ago

        Usually these are predictions made by a model that has explanatory power for things that we can observe. The model might be wrong, or there might be a better model. That’s always the case in science. Observations that confirm a model also increase the credence for its predictions that we can’t directly observe. It means that given our best current understanding of X, it also implies Y. Yes, Y might be wrong, but then that implies that something is likely also wrong with our current understanding of X. The predictions (or retrodictions) aren’t black and white. They always have some associated level of credence, which depends on how well we think we understand the kind of system we are talking about.

      • drob518 21 hours ago

        It’s always a theory, but what choice do you have? You can’t rerun the experiment again under controlled conditions. Your only choice is to theorize or not. Sure, there is more possible error in such theories compared to other theories where you can rerun the experiment multiple times to test it, but that doesn’t mean that a theory that can’t be tested is wrong.

  • impendia 21 hours ago

    If we're to take your claims at face value, can we make any conclusions about the past at all?

    For example, suppose that I were to claim that the universe is exactly one hundred years old. George Washington, Genghis Khan, Julius Caesar, dinosaurs, etc. are all figments of our collective imagination.

    If you deny the validity of research that makes conclusions about the past, on the grounds that such claims can't be tested or falsified -- then have you left yourself any means of making a counterargument?

  • SJC_Hacker 19 hours ago

    So I guess you’re skeptical about continental drift theory and universal common descent ?

  • iwontberude 20 hours ago

    This is how young earth type misunderstandings begin. Thanks for bringing us inside the mind.

    • ricksunny 19 hours ago

      parent commenter invokes Popperian epistemology. Your comment aligns Popper with flat-earth thinking. One of you is engaging in pseudoscience.