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Start all of your commands with a comma

https://rhodesmill.org/brandon/2009/commands-with-comma/
58•theblazehen•2d ago•11 comments

OpenCiv3: Open-source, cross-platform reimagining of Civilization III

https://openciv3.org/
637•klaussilveira•13h ago•188 comments

The Waymo World Model

https://waymo.com/blog/2026/02/the-waymo-world-model-a-new-frontier-for-autonomous-driving-simula...
935•xnx•18h ago•549 comments

What Is Ruliology?

https://writings.stephenwolfram.com/2026/01/what-is-ruliology/
35•helloplanets•4d ago•31 comments

How we made geo joins 400× faster with H3 indexes

https://floedb.ai/blog/how-we-made-geo-joins-400-faster-with-h3-indexes
113•matheusalmeida•1d ago•28 comments

Jeffrey Snover: "Welcome to the Room"

https://www.jsnover.com/blog/2026/02/01/welcome-to-the-room/
13•kaonwarb•3d ago•12 comments

Unseen Footage of Atari Battlezone Arcade Cabinet Production

https://arcadeblogger.com/2026/02/02/unseen-footage-of-atari-battlezone-cabinet-production/
45•videotopia•4d ago•1 comments

Show HN: Look Ma, No Linux: Shell, App Installer, Vi, Cc on ESP32-S3 / BreezyBox

https://github.com/valdanylchuk/breezydemo
222•isitcontent•13h ago•25 comments

Monty: A minimal, secure Python interpreter written in Rust for use by AI

https://github.com/pydantic/monty
214•dmpetrov•13h ago•106 comments

Show HN: I spent 4 years building a UI design tool with only the features I use

https://vecti.com
324•vecti•15h ago•142 comments

Sheldon Brown's Bicycle Technical Info

https://www.sheldonbrown.com/
374•ostacke•19h ago•94 comments

Hackers (1995) Animated Experience

https://hackers-1995.vercel.app/
479•todsacerdoti•21h ago•237 comments

Microsoft open-sources LiteBox, a security-focused library OS

https://github.com/microsoft/litebox
359•aktau•19h ago•181 comments

Show HN: If you lose your memory, how to regain access to your computer?

https://eljojo.github.io/rememory/
279•eljojo•16h ago•166 comments

An Update on Heroku

https://www.heroku.com/blog/an-update-on-heroku/
407•lstoll•19h ago•273 comments

Vocal Guide – belt sing without killing yourself

https://jesperordrup.github.io/vocal-guide/
17•jesperordrup•3h ago•10 comments

Dark Alley Mathematics

https://blog.szczepan.org/blog/three-points/
85•quibono•4d ago•21 comments

PC Floppy Copy Protection: Vault Prolok

https://martypc.blogspot.com/2024/09/pc-floppy-copy-protection-vault-prolok.html
58•kmm•5d ago•4 comments

Delimited Continuations vs. Lwt for Threads

https://mirageos.org/blog/delimcc-vs-lwt
27•romes•4d ago•3 comments

How to effectively write quality code with AI

https://heidenstedt.org/posts/2026/how-to-effectively-write-quality-code-with-ai/
245•i5heu•16h ago•193 comments

Was Benoit Mandelbrot a hedgehog or a fox?

https://arxiv.org/abs/2602.01122
14•bikenaga•3d ago•2 comments

Introducing the Developer Knowledge API and MCP Server

https://developers.googleblog.com/introducing-the-developer-knowledge-api-and-mcp-server/
54•gfortaine•11h ago•22 comments

I spent 5 years in DevOps – Solutions engineering gave me what I was missing

https://infisical.com/blog/devops-to-solutions-engineering
143•vmatsiiako•18h ago•65 comments

I now assume that all ads on Apple news are scams

https://kirkville.com/i-now-assume-that-all-ads-on-apple-news-are-scams/
1061•cdrnsf•22h ago•438 comments

Learning from context is harder than we thought

https://hy.tencent.com/research/100025?langVersion=en
179•limoce•3d ago•96 comments

Understanding Neural Network, Visually

https://visualrambling.space/neural-network/
284•surprisetalk•3d ago•38 comments

Why I Joined OpenAI

https://www.brendangregg.com/blog/2026-02-07/why-i-joined-openai.html
137•SerCe•9h ago•125 comments

Show HN: R3forth, a ColorForth-inspired language with a tiny VM

https://github.com/phreda4/r3
70•phreda4•12h ago•14 comments

Female Asian Elephant Calf Born at the Smithsonian National Zoo

https://www.si.edu/newsdesk/releases/female-asian-elephant-calf-born-smithsonians-national-zoo-an...
29•gmays•8h ago•11 comments

FORTH? Really!?

https://rescrv.net/w/2026/02/06/associative
63•rescrv•21h ago•23 comments
Open in hackernews

Jupiter was formerly twice its current size, had a much stronger magnetic field

https://phys.org/news/2025-05-jupiter-current-size-stronger-magnetic.html
128•pseudolus•8mo ago

Comments

rwmj•8mo 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?
elashri•8mo ago
A prepublished version of the paper is available on arxiv [1]

[1] https://arxiv.org/abs/2505.12652

lazide•8mo 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.

HappMacDonald•8mo 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.

skywhopper•8mo 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.
raattgift•8mo 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.

greggsy•8mo 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•8mo 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.
anton-c•8mo ago
That's wild to think about. My mind is struggling to picture 'liquids on the surface' of Jupiter. No idea what that would look like.
jessriedel•8mo ago
I am deeply looking forward to the dragonfly mission to Titan, since we'll finally get high-resolution color images from the surface, which has liquid seas of hydrocarbons like methane and ethane at -290 F.

https://en.wikipedia.org/wiki/Dragonfly_(Titan_space_probe)

The single image from the surface by the Huygens probe leaves a lot to be desired.

https://en.wikipedia.org/wiki/Titan_(moon)#/media/File:Huyge...

anton-c•8mo ago
Yeah this is gonna be awesome, appreciate the heads up!
lazide•8mo 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.
queuebert•8mo 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•8mo ago
In the sense that higher gravity increases density all other things being equal. yes, absolute size will slowly increase - until it collapses, anyway.
lazide•8mo ago
Gas giants generally only get slightly larger than Jupiter (even with adding a lot of mass), until they start to shrink - and eventually with enough mass, turn into actual stars [https://en.m.wikipedia.org/wiki/Gas_giant]

So generally, gas giants don’t get much bigger than Jupiter.

Zardoz84•8mo 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.
DonHopkins•8mo ago
aka "fluffier"
exe34•8mo ago
Probably contracted as it's mostly gas.
adrian_b•8mo ago
The mass did not differ much from the present mass, but the planet was less dense and with a more rapid rotation.
est31•8mo 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.
Maxatar•8mo 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•8mo ago
It's a matter of definitions, so we skip them and just choose something that makes sense to humans.
philipov•8mo 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•8mo 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•8mo 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.
jessriedel•8mo 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.
gus_massa•8mo ago
For comparison, extracting the numbers from the graphic in page 3 of https://projects.iq.harvard.edu/files/acmg/files/intro_atmo_... 1 microbar on Earth is like 50Km, that is 50/6400 ~= 0.8%
queuebert•8mo ago
Venus would get a slight radius buff, too, if we applied that metric.
hnuser123456•8mo ago
But Venus has a solid surface.
queuebert•8mo 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.)
hnuser123456•8mo ago
Ah, I see what you're saying, didn't know the surface pressure was so high! I suppose Titan would also get an atmosphere radius buff!
layer8•8mo 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•8mo ago
This is because of Newtonian gravity being inversely proportional to the square of the radius, right?
skykooler•8mo 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•8mo ago
What makes that curve exponential?
westurner•8mo 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.

westurner•8mo ago
Was there an issue with this answer about why water pressure is?

Are you donvoting according to preference or to Terms of Service?

skykooler•8mo 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).
nh23423fefe•8mo ago
via feynmann

> 40–1 The exponential atmosphere

https://www.feynmanlectures.caltech.edu/I_40.html

marcosdumay•8mo 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.
yubblegum•8mo 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?
GolfPopper•8mo ago
I am not an astronomer (save in the very amateur sense), but I think it has to do with Jupiter forming both early in the history of solar system, and, as you guess, beyond the Sun's 'snow line'.

Wikipedia is a good place to start getting a feel for the possible history of the Solar System:

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

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

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

Tepix•8mo 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__•8mo ago
I'd assume these elements would be created in the sun and keep close to the sun, because of their higher mass.
frutiger•8mo 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•8mo 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•8mo 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.

mystified5016•8mo ago
The core of Jupiter is thought to contain metallic hydrogen.
yubblegum•8mo ago
Found this on the wiki for metalic hydrogen. Apprently there is a liquid phase as well. Apparently there is debate as to whether there is a solid core besides the hydrogen (thought shown in the pic):

https://upload.wikimedia.org/wikipedia/commons/b/b5/Jupiter_...

twic•8mo ago
It's made from something which can generate magnetic fields, since Jupiter has a very strong magnetic field with a lot of distinct inhomogeneous features, resulting in some interesting radio emissions:

https://www.ebsco.com/research-starters/science/jupiters-mag...

https://radiojove.gsfc.nasa.gov/library/sci_briefs/decametri...

The rotation of these features is the basis for the "system III" definition of longitude on Jupiter.

everyone•8mo ago
In an Arthur C Clarke story (I forget which one) the core of jupiter is a planet sized diamond.
ReptileMan•8mo ago
Space Odyssey one of the sequels.
teamonkey•8mo ago
2061. Not his best work, alas.
bell-cot•8mo ago
Actually 2010, in the closing words of Chap. 38.

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

yencabulator•8mo 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...

mnky9800n•8mo 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.

dragonwriter•8mo ago
They aren't in the middle of the “planetary lineup”.

The four inner planets are all terrestrial. The four outer planets are gas (the last fwl sometimes distinguished instead as “ice”) giants.

There are dwarf planets (a separate category from, rather than sibcategory of, planets) closer and farther, but no known rocky planets beyond the gas/ice giants.

fasteddie31003•8mo 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•8mo ago
Observations are inherently always about the past.
fasteddie31003•8mo 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•8mo 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•8mo 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.
AStonesThrow•8mo ago
It’s actually seldom a Theory. In fact, I’d be surprised if scientists were eager to form “Theory on the Formation of Jupiter” [or Venus or the Moon] because those are already quite specific subjects that should be derived from generalized theories.

We’re thinking of hypotheses and proposals and extrapolations here. A few scientists analyzed and compared existing data, and they estimate things and interpolate and ... guess ... And the narrative develops as they give facility tours and answer questions for journalists, 8-year-olds, and 8-year-old journalists.

Theories are hypotheses which were tested and survived falsification attempted against them. You cannot adequately falsify “800 million years ago, and 12 parsecs away...” but you can enjoy your colleagues’ version of the story over drinks with a jazz band.

iwontberude•8mo ago
PC is from the future
impendia•8mo 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?

iwontberude•8mo ago
This is how young earth type misunderstandings begin. Thanks for bringing us inside the mind.
ricksunny•8mo ago
parent commenter invokes Popperian epistemology. Your comment aligns Popper with flat-earth thinking. One of you is engaging in pseudoscience.
SJC_Hacker•8mo ago
So I guess you’re skeptical about continental drift theory and universal common descent ?
mmooss•8mo ago
> I am deeply skeptical ...

Perhaps you mean, you don't understand or you wonder how it reconciles with the scientific method? It's an interesting question about theory.

To be 'deeply skeptical' is not meaningful, imho. All these people - including Newton, Darwin, Einstein, and so many more, including the entire scientific community - believe it. All these experiments replicate it. You are deeply skeptical about all of that and of all of them? What does it mean, even to you?

> 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.

We can directly test the claims through many methods, for example that the stone tool was made 2.58 million years old, but we can't see 2.58 million years ago (except something that is 2.58 million light years away, of course). We can indirectly test claims, e.g., that tool use existed 2.58 million years ago, through many different methods.

You're right that it's not the same. What else can we do? Just quit and live in ignorance?

> 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.

You can call it what you want, but that doesn't change its value. Is this just a question of terminology?

By this proposed theory, we can't know anything that happened before now. We can't know what happened in ancient China - did the Han dynasty even exist? We can't know who won the Olympic marathon in 1928 without witnesses to tell us. We can't know what happened yesterday - human memory is certainly fallible, and otherwise you have only indirect evidence. That applies to every scientific paper, providing indirect evidence to us of what has happened, and mostly based on human memory. Did I write what you are reading? Where is your falsifiable direct observation?

We also can't know much of what is happening now. Most science data is based on indirect observation by devices and machines. Human sensory ability is limited and unreliable in many ways. What color is the light in the experiment? We measure that with a machine that gives us indirect information.

I think a key challenge to your theory is, how do we know anything at all?

bethekidyouwant•8mo 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.
waynecochran•8mo 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?
Civitello•8mo ago
It shrank because of all the boys going there to get stupider.
lukan•8mo 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•8mo 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...

WalterBright•8mo 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.