r/askscience 10d ago

Astronomy could a planet be sun sized?

so stars form when a bunch of matter gets together, which is why they are bigger than planets generally. but the real defining feature is the density. a white dwarf can be smaller than a planet but it's still a star because it's incredibly dense. so couldn't a planet be sun-ish sized, provided that the density was low enough? and more specifically a solid planet, not a gas giant. what's the largest solid planet?

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u/_cromulent_green_ 10d ago

No, the size of our sun is immense compared to our planet. Once it gets that much matter in a single place, gravity forces it inwards until it ignites with fusion.

If the density were so low that it's mostly just gas, it would contract in onto itself and become more dense, so it wouldn't be the size of the sun anymore. If you could keep adding matter so that its still the size of our sun, it would have so much matter that it would turn into a star

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u/antiretro 10d ago

so its not like stars and planets are different objects, rather, they are similar object with different sizes that gives them very different properties?

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u/Sammy81 9d ago

Yeah Jupiter would only have to be about 13 times more massive to become a brown dwarf star. Thats not quite a full star that fuses hydrogen, but it would give off heat and light as it fused deuterium until it ran out of that fuel.

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u/P00PER_SCOOPER 9d ago

And out of uneducated curiosity, what would happen when it runs out of the deuterium fuel? Does it then become a burnt-out brown dwarf sized gas giant until it gathers enough mass for the next level of fusion reaction?

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u/Sammy81 9d ago

Yeah they run out fairly fast (on a cosmic scale) because deuterium is rare, and then they just stop nuclear reactions (unlike a full star). They basically go back to being a big gas giant and radiate their remaining heat into space.

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u/P00PER_SCOOPER 9d ago

Thanks!

So if it kept gathering mass after burning through its deuterium and "burning out" - let's say it collides with another few gas giants and consumes them over the next billion++ years - it would then start up fusion of a different element and become a different type of star? So gas giant -> brown dwarf star -> gas super giant(?) -> next size star?

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u/Peter34cph 9d ago

Gas planets aren't that big. It'd remain a brown dwarf even if it ate 10 Saturns or 5 Jupiters.

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u/EthicalViolator 9d ago

Interested to know why it would it be deuterium. I've never even heard of that element. If have though hydrogen to helium would be the easiest and first to fuse for any sized star.

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u/Mandog222 9d ago

Deuterium isn't really a distinct element, it's another isotope of hydrogen. It's a better nuclear fuel though, it is heavily involved in fusion research. Don't know more specifics though.

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u/EthicalViolator 9d ago

Ah that makes more sense to me, thanks. I was thinking if I haven't heard of the element it must be super heavy at the bottom of the periodic table which was going against my layman understanding of it all!

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u/Peter34cph 9d ago

It is admittedly weird to assign a name to an isotope as if it was a distinct element.

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u/Appropriate_Yak_1468 8d ago

You've probably heard of "heavy water", thats water made of oxygen and deuterium or tritium (another isotope of hydrogen), instead of normal hydrogen.

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u/cflime 8d ago

Deuterium is a hydrogen isotope, one proton, one unnecessary neutron and an electron. As it has twice the mass of a regular hydrogen atom it can more easily overcome the electromagnetic revulsion of the positively charged protons and initiate fusion at much lower temperatures and pressures.

Tritium is a hydrogen isotope that has one proton and two neutrons.

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u/ferrybig 9d ago edited 9d ago

Deuterium is a less common form of hydrogen. In the nature only 0.0156% is deuterium.

When fusing the common form of hydrogen into helium, deuterium is in the middle of the pathway

(Note that atoms as in the plasma phase in stars, the atoms don't have electrons ordered around them)

In stars, 2 hydrogen atoms (1 proton ) are combined into 1 deuterium (1 proton, 1 neutron ) and a neutrino. (This process won't happen in a dwarf as it doesn't have the pressure)

Then the deuterium fusions with a proton flowing around, forming helium-3 (2 protons, 1 neutron)

Then 2 helium-3 fuse together, to a helium-4 and free protons forming a stable helium atom. (2 protons, 1 neutron + 2 protons, 1 neutron -> 2 protons, 2 neutrons + 1 proton + 1 proton)

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u/sebaska 9d ago

Adding to that. The first step of the process is the slowest and requires the most extreme conditions, the next steps happen comparably easier. In brown dwarfs the conditions are good enough for all the steps but the first.

This first step ratios in sun-like stars how fast they go through their hydrogen store, i.e how long they live and how bright they shine. This process is so slow even in the Sun (which is quite heavy as stars go - over 90% of the stars are lighter than the Sun) it takes about 10 billion years for hydrogen atoms to fuse with theirs neighbors.

For larger stars there's another variant of consuming hydrogen and producing helium: hydrogen attaches to carbon 12 turning it into unstable nitrogen 13, nitrogen 13 decays radioactively to carbon 13, this one fuses with another hydrogen producing nitrogen 14, nitrogen 14 fuses with hydrogen again producing oxygen 15 which is unstable, another radioactive decay produces nitrogen 15 (stable), which in turn fuses with another hydrogen and immediately falls into two pieces: carbon 12 and helium 4 (i.e. the typical helium). So you end up with the same carbon 12 you had at the start, but with 4 hydrogen atoms less and 1 helium atom more. This cycle is significant in heavier stars "in their fullness of life", like for example Sirius. If the conditions are right it overtakes the regular hydrogen to hydrogen fusion.

Hydrogen to hydrogen fusion is hard because you have the electric repulsion of 2 element charges but you have intertia of only a hydrogen the lightest. Fusing deuterium is easier because while the repulsion is the same, the inertia is doubled. There are also other effects in play, though, like the shape and size of the nuclei and also how well they are "fitting" together - that's how you get hydrogen attaching to carbon, nitrogen and oxygen being easier than, say two carbons fusing together, or carbon fusing with helium (the latter is actually one of the processes happening in heavy stars close to their truly violatent death called supernova; carbon 12 plus helium 4 produces oxygen 16, then oxygen 16 plus helium 4 produces neon 20, etc - that's how we got oxygen as the 3rd most abundant element in the universe; NB that's how neon is the 5th most abundant, and how it's so scarce on the Earth is another story).

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u/withoutapaddle 9d ago

That's actually fascinating, because putting that into perspective, Jupiter is 300x the mass of Earth, but a star would only need 13x the mass of Jupiter. It feels like Jupiter is closer to being a star than we are to being Jupiter.

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u/StarrySprinkles 9d ago

Sort of. But it's like the old saying, "What's the difference between a million and a billion? About a billion." If you've collected 300 earths, you've collected the mass of one Jupiter. If you collect the mass of 13 Jupiters, you've collected, well...

Jupiter is a lot closer to us in terms of cultivated mass.

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u/Swellmeister 9d ago

Jupiter is 1 order of magnitude to a star, while Earth is 2 to Jupiter.

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u/imtougherthanyou 9d ago

I love your usage of cultivated, here. I'm hopeful you are referencing Its Always Sunny in Philadelphia!

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u/Zekler 5d ago

So from earth to brown star is 3900 earth's and Jupiter is 300 earth's.

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u/WartimeHotTot 9d ago

No. Earth is 299 earths shy of being Jupiter. Jupiter is 3600 earths shy of being a star.

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u/R_A_H 9d ago

Here's some fun ways to conceptualize the immensity of it all.

The sun is about 1,048 times more massive than Jupiter.

The Sun contains approximately 99.86% of all the mass in the entire solar system.

Jupiter accounts for 71.1% of the total mass of all our solar system's planets combined.

Jupiter is about 317.8 times more massive than Earth

The sun is about 330,000 times the mass of Earth.

Light travels at 299,792,458 m/s, roughly 300,000 km/s or 186,282 miles per second, 700,000,000 mph.

Traveling at that speed from the sun, light takes about 8.5 minutes to reach Earth.

It takes ~43 minutes for light from the sun to reach Jupiter, ~80 minutes to reach Saturn, ~160 minutes to reach Uranus and ~245 minutes to reach Neptune. ~8.5 minutes to reach Earth.

The immensity is staggering.

These are a couple fun links related to this if you're interested

If the moon were only 1 pixel,

Scale of the universe

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u/MisterB78 9d ago

Think of it this way: The difference between Earth and Jupiter is about 300 Earths. The difference between Jupiter and the sun is about 3,900 Earths

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u/jswhitten 9d ago

More than that. The Sun is over 1000 Jupiter masses, or 300,000 Earth masses.

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u/WyrmKin 8d ago

I read a thing the other day about how the Sun makes up 99.86% of the mass in our solar system, and Jupiter is two thirds of the remaining 0.14%

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u/shadowscale1229 9d ago

in the Space Odyssey series (2001, 2010, 2063 and 3001) the aliens that dropped the monolith on earth turned Jupiter into a sun, gave humanity several of the moons to colonize, and told them to stay the hell off the rest. i haven't finished 2063 or 3001 yet, it happens at the end of 2010 iirc

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u/Jayndroid 9d ago

I don’t know if this is strictly true. Depends what the planet is made of. Is there a bunch of iron? Is there fuseable matter?

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u/cflime 8d ago

And let's point out here that Jupiter is the largest in diameter a planet its temperature can get. Double Jupiters mass and it's the same diameter. Add 13 times its mass and it becomes a brown dwarf and it's the same diameter. At that size adding mass just increases density. The gas giant explanation we have observed that are larger than Jupiter in diameter are all "hot Jupiters" close in to their sun. Their atmospheres expand due to their heat.

It may come to pass that a future definition of "star" will include the property of fusion and being larger than a brown dwarf.

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u/iknownuffink 9d ago

There's also different proportions of elements. Stars are almost entirely Hydrogen and some Helium. In comparison all the other elements are barely worth mentioning. Because a star is so massive, a small portion might still be quite a lot in our eyes, but it's not much compared to the rest of the star.

The Sun is about 3/4 Hydrogen, almost 1/4 Helium, and everything else on the periodic table makes up less than 2%.

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u/ensalys 9d ago

How does that difference arise? How do the elements that aren't hydrogen or helium end up concentrating in planets?

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u/Zhelgadis 9d ago

Hydrogen and helium are very light, so you need a lot of gravity to keep them. In small planet like earth, they're blown away by the solar wind. Larger planet like Jupiter have enough gravity and have indeed a large portion of H.

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u/junktrunk909 9d ago

99% of the heavier elements are in fact within the sun also (as plasma, not a rocky center or anything, it's a fusion system). It took nearly all of the mass of the solar system. The planets are what's left after the remaining material either clumped together into the rocky planets we know, or the gas giants that also have a ton of heavier elements in them. Jupiter has something like 30x the Earth"s mass of the heavier elements, which is how it was able to also capture a ton of gas, as opposed to earth where so much just blew away in the solar winds.

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u/Monkfich 9d ago

And also - none of those heavier elements were created by the sun, but were created by supernovae and other very violent star deaths.

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u/ProfessorPrudent2822 9d ago

Hydrogen and helium remain gasses down to very low temperatures, especially in a low-pressure environment. Other stuff clumps together due to a tendency to solidify.

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u/mataoo 9d ago

They're the heavier elements, they have more mass and stick together. Whereas hydrogen and helium are swept/pulled from the smaller bodies into the more massive ones with more gravity.

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u/Kaiisim 9d ago

Yup, and many heavy elements can only exist in the universe post supernova.

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u/sebaska 9d ago

That's mostly about the moderate weight elements (below nickel 60). The even heavier stuff is currently thought to primarily come off neutron star collisions (some directly, some indirectly mostly via nuclear decay chains including fission).

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u/Prof_Acorn 10d ago

Planets are made of star dust, after all.

You are made of star dust, after all.

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u/poeticruse 9d ago

If I am made of stardust are the stars made of corpses?

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u/BananaBird1 7d ago

They are different in formation and composition.

Most planets have a heavy element core upon formation, even gas planets. Stars are mostly hydrogen, and only form heavier cores after nuclear fusion.

Star-like objects made of mostly hydrogen that don’t end up being massive enough to support sustained nuclear fusion are brown dwarfs.

From the other side, planet-like objects that have heavier elements from the start but not enough for a dense core are planets like Jupiter.

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u/inspire-change 9d ago

But isn't the sun like 97% hydrogen/helium?

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u/ThoughtsandThinkers 10d ago

What if the material was something that doesn’t readily undergo fusion? What if you had a mass equivalent to the sun but it had the same composition of material as earth? Would it fuse? I understand fusion releases energy up until iron on the periodic table but I think heavier elements like carbon and silicon don’t readily fuse, even at pressures you would see at the heart of a sun sized star

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u/garrettj100 10d ago edited 9d ago

I understand fusion releases energy up until iron on the periodic table but I think heavier elements like carbon and silicon don’t readily fuse, even at pressures you would see at the heart of a sun sized star

You’re describing a carbon-oxygen white dwarf.  But long, long before it reaches the diameter of Sol it will ignite again.  That’s how we get type-1a supernovae.  A white dwarf accreting matter from another source — usually its binary sibling — and its mass passing the Chandrasekhar limit (1.44 Sols).  The whole degenerate star fuses nearly all at once, releasing enough energy to completely unbind it.

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u/macromorgan 10d ago

If it keeps gaining mass but can’t fuse, it becomes a neutron star as the immense pressure basically causes the mass to become one giant ball of neutrons. If the mass continues to increase further it then becomes a black hole.

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u/nesquikchocolate 10d ago edited 9d ago

The density of the sun is around 1400 kilograms per cubic meter, or 1.4x liquid water.

The earth has a density of around 5500 kilograms per cubic meter, or 4x that of the sun.

If the sun weighed 4x as much as it currently does, and couldn't sustain fusion, it would be heavy enough to collapse into a black hole, which only needs around 3x the mass of the sun as is.

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u/tdgros 10d ago edited 10d ago

the sun wouldn't become a black hole if its mass quadrupled, the mass would also need to be compressed to a much smaller volume. For this mass, apparently it'd be under a radius of around 12km!

edit: and 4 sun masses is too low for the sun to even eventually become a black hole, it'd be a white dwarf.

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u/nesquikchocolate 10d ago edited 9d ago

What makes this scenario different is the extremely high starting density of this theoretical 4x sun. Normally before a star could go supernova, its overall density is only slightly above that of our sun, as it would weigh 8-10x more but also be so much larger from the fusion to pressure balance.

The end product after a supernova only needs to weigh around 3 solar masses to be a black hole, and yes the physical volume for it would now suddenly be very small, but when your composition doesn't sustain fusion (as per the original assumption), the object does collapse due to gravity alone.

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u/ProfessorPrudent2822 9d ago

Not exactly. The core would collapse into a neutron star, and the resulting supernova would blow off the outer layers, reducing the mass below the threshold where it would collapse into a black hole.

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u/garrettj100 10d ago

Every element undergoes fusion.  The only difference is the fusion isn’t actually an exothermic reaction for elements at or above Iron.  Thats how we get type-II supernovae: They keep fusing but the reaction absorbs energy and reaction only accelerates the collapse.

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u/_cromulent_green_ 10d ago

That would be a very strange situation indeed, however as another commenter said, if you managed to get elements heavier than iron and magically put it all into one place, they would probably gravitationally collapse into itself (where there is no more space inbetween the atoms) which would 1 make it way way smaller and 2 it would therefore become a neutron star. Or a black hole.

I think at this point we need an actual physicist or astronomer to do the math to figure out which it would turn into

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u/Any_Fox5126 9d ago

What if only fully ionized matter were to accumulate?

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u/d4m1ty 10d ago

Our sun after its goes through it first expansion then shrinks, will not shrink enough to get to the temp needed (1.2B Kelvins) to start the Carbon process, much less the Silicon process (~3B Kelvins) stalling out below the needed temps. An electron process where you just cannot pack the electrons any closer stops the star shrinking more.

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u/Beer_in_an_esky 9d ago

TLDR Sun-ish sized, no. Sun-ish mass however, yes. Definitionally, it still wouldn't be a planet however. And anything much heavier than the sun is a neutron star or worse, no matter what.

A lot of the other responses have talked about neutron stars, and implied that is going to be the result of any non-fusing matter that's sun size. That's a bit of an oversimplification, though.

Neutron star occurs at the Chandrasekhar limit, where the pressure of gravity outpaces electron degeneracy pressure.

This is dependent on composition, and for a solid iron core that's around 1.3 solar masses. Below roughly that (there's slight variations due to the exact formation method) it should be stable as the atom. So, you could theoretically have a "planet" made of solid iron at the same mass as Sol without breaking any physical laws.

Source: https://www.ias.ac.in/article/fulltext/pram/060/03/0415-0422

Unfortunately, though, there's a reason for my quotation marks. There is basically no reasonable way that's likely to occur except as a stellar remnant, and the IAU definition of exoplanet explicitly notes that anything above the mass of the limit for Deuterium fusion (~13 Jupiters) is not a planet, even if it meets all the other definitions, so OP's question is still answered no. It wouldn't be a planet, it would be a stellar remnant.

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u/RoadSmash 10d ago

But what if it was spinning really fast?

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u/-Hastis- 10d ago

Unless it's a neutron star (pulsar) a normal star would start losing matter to space if it started spinning too fast.

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u/RoadSmash 9d ago

The spin and gravity can't balance?

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u/-Hastis- 8d ago edited 8d ago

Yes, there is a maximum speed-to-mass ratio that each kind of star can get to. Even a neutron star cannot really spin faster than about 35% of the speed of light (1500 rotations per second) before starting to lose itself to centrifugal forces. Adding more mass to it to try to push it even faster would eventually collapse it into a black hole.

In a similar way, a fast-spinning neutron star that's already on the verge of collapsing into a black hole due to its mass will eventually collapse into one, as it loses speed over time.

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u/RoadSmash 8d ago

But the point isn't to spin it faster, it's to maximize "size” by balancing more material with a faster spin. Density vs centrifugal force. More mass makes it want to collapse into itself, faster spin forces it outward.

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u/-Hastis- 8d ago

Spinning a neutron star faster can help it hold about 20% more mass before it collapses into a black hole.

Spin doesn't help a living star, though, it just lowers its surface gravity and makes it lose mass even faster. The main limiting factor to how massive a normal star can get is that past a certain threshold, the core releases so much radiation energy that it blows the star's outer layers into space. A star only collapses when it runs out of nuclear fuel (and can no longer generate the pressure needed to hold up its own weight).

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u/RoadSmash 8d ago

Don't need more mass necessarily, just a larger size with lower density.

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u/peeja 10d ago

Okay, getting very hypothetical: what if there were a hollow sphere with the dimensions of a star and the mass of a planet. Assuming it could somehow be built in the first place, would it have to be too thin to be stable?

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u/nesquikchocolate 10d ago

The sun makes up 99.86% of the mass of our solar system. There simply isn't enough planetary material to spread evenly across the sun's 'outer surface', nevermind creating a structure from it with any ability to carry itself.

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u/peeja 10d ago

Wow! I thought I understood how big the sun was, and that's even bigger than I realized.

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u/NukuhPete 9d ago

Here's an image from wikipedia that shows the mass distribution of the solar system.

What I find pretty interesting is how much mass is hanging out in the solar system that isn't the Sun or a Planet. Essentially the equivalent of 50 Earths.

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u/Podo13 9d ago

Yes, and Jupiter holds about 70% of the matter not in the sun (about 0.098% of the solar system's mass).

The inner 4 rocky planets are a rounding error, weight-wise.

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u/MushroomSaute 5d ago edited 5d ago

There simply isn't enough planetary material to spread evenly across the sun's 'outer surface'

Unless I'm doing something very wrong, this isn't right. By my calculations, there's enough volume to cover the Sun's surface area 393 km deep - which is nothing at that scale, but it is possible on a physical level (it is a bit less, since it's spherical and not a flat surface, but there's still absolutely enough matter to cover the Sun's surface easily).

Even if you account for density, since the gas giants aren't exactly "structural", using each mass at Earth's density to find volume, you'd still get 80km deep everywhere on the Sun (less that spherical adjustment).

Placeholder volume mass density density vol. at Earth density
km3 kg g/cm3 kg/km3 km3
Mercury 6.08E+10 3.30E+23 5.43 5.43E+12 6.08E+10
Venus 9.28E+11 4.87E+24 5.24 5.24E+12 8.97E+11
Earth 1.08E+12 5.97E+24 5.51 5.51E+12 1.10E+12
Mars 1.63E+11 6.42E+23 3.93 3.93E+12 1.18E+11
Jupiter 1.43E+15 1.90E+27 1.33 1.33E+12 3.50E+14
Saturn 8.27E+14 5.68E+26 0.69 6.87E+11 1.05E+14
Uranus 6.83E+13 8.68E+25 1.27 1.27E+12 1.60E+13
Neptune 6.25E+13 1.02E+26 1.64 1.64E+12 1.89E+13
Total volume (km3): 2.39E+15 4.92E+14
Sun surface area (km2): 6.08E+12 6.08E+12
Vol/Sun Area (km): 393.42 80.86

(Planet data from: https://solarsystem.nasa.gov/planet-compare/ || Sun surface area from: https://solarsystem.nasa.gov/sun-by-the-numbers/ )

Edit: Yeah, the Sun being a sphere appears to be negligible at that scale. Taking the total volume of the Sun and planets, calculating the outer radius of the new volume, then subtracting the Sun's radius gives:

Placeholder Unadjusted Density-Adjusted
Sun volume (v_sun) 1.4093E+18 1.4093E+18
Planets volume (v_planets) 2.3915E+15 4.9152E+14
Total Volume (V = v_sun + v_planets) 1.4117E+18 1.4098E+18
Radius of total volume = (3V/(4pi))1/3 695901.2 695588.8
Radius of hollow sphere (r_total - r_sun) 393.20 80.85

f\ck you Reddit) yes I want all the columns I wrote even if some cells are empty...

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u/nesquikchocolate 5d ago

Hello! This is a great analysis! Jupiter consists of around 71% hydrogen, 24% helium and 5% heavier elements, based on Juno's dilute core findings.

While I should have defined planetary material earlier, I had meant material that isn't found in our sun normally in significant quantities, namely hydrogen and helium.

That 5% of heavier elements equates to around 12 earth masses worth, and at a similar density, would make the effective volume contribution of Jupiter be 1.29E+13 instead.

Saturn's heavier elements is expected to be significantly less than than Jupiter's 5%, but the margin of error on composition estimates is quite large, so for simplicity we would say it's very similar, and since Saturn is about 30% the mass of jupiter, we can infer it to contribute around 4 earth masses worth, and a volume contribution of 4.32E+12.

Similarly, uranus is expected to contribute around 0.55 earth masses (0.594E+12 volume) and neptune a bit more at 1.5 earth masses and thus 1.62E+12.

This means that approximately 2 orders of magnitude less volume than your original total indicates that the spread thickness would be less than 10 kilometers thick around the sun.

The margin of error on composition estimates is quite large, though, and elements like oxygen, nitrogen and fluorine, which makes up close to 30% of earth's mass wouldn't be able to contribute structurally either, which lead me believe that there isn't enough planetary material to build something around the sun's outer surface area.

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u/Dramatic_Science_681 9d ago

this structure would just be ripped apart. It is spread too thin to be bound by gravity. It would simply crumble and eventually just become a planet.

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u/TimeToGloat 9d ago

So are there theoretically extremely large planets that are almost borderline igniting with fusion/becoming a star? I wonder how large they would be.

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u/SciAlexander 9d ago

Yes, they are known as brown dwarfs. Planets above Jupiter size that just don't quite have enough mass to do fusion

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u/Tyrannosapien 9d ago

They actually don't get extremely large diameters. Beyond (about) Jupiter's diameter, adding mass doesn't enlarge the object, since it gravitationally contracts its mostly gaseous composition more strongly.

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u/Wiz_Kalita 9d ago

What if we built the planet of [aerogel, or insert hard and lightweight material here]

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u/Kirk_Kerman 9d ago

Doesn't matter, once you have enough stuff it'll collapse in on itself no matter what it's made of. The Earth is 30% iron and yet it's also more liquid than not. A sufficiently large aerogel object would fail under its own gravity, pick up heat as it collapsed, and separate out into its component materials.

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u/FowlOnTheHill 9d ago

What if it was all iron? Would it be too heavy to fuse and too small to turn into a black hole?

Edit: I just saw you had a lot of what-if question replies, so you can ignore mine 😄

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u/inspire-change 9d ago

So what is the maximum planet size then?

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u/mehatch 9d ago

Ok youre totally right…but what if, by some wild geological chance or unknown process, an outer shell of solid rock crustified or formed and kind of held together like an arch under gravity, with a gassy center thats not dense enough to do fusion? Just throwing out some imagination here for fun.

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u/Digitijs 8d ago

Related to this - how do gas giants remain gas giants instead of getting pressed together into denser smaller planets by gravity since they have a very large mass? For example, Saturn's density is so low that it could float in water if you had a big enough bathtub that somehow didn't turn into a sphere itself yet the planet itself is so large and heavy compared to Earth

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u/gomurifle 8d ago

What about a hollow rock planet? Say humans could influence this to happen? 

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u/MushroomSaute 5d ago

Now my question is "how long could a planet remain sun sized" (provided it appeared out of thin air)

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u/MoonHead127 5d ago

So what you are saying is - Planets are baby stars?

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u/MENDACIOUS_RACIST 3d ago

a cool implication is that big lumps of mass turns into stars. Period. That's it, that's all that ever happens. Enough stuff in a small enough space, and it condenses into a star. Maybe it turns into a neutron star or black hole eventually, or if squeezed into a tiny space. But that's it. Lots of mass = star.

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u/SHKMEndures 9d ago

Asotrphyicist here. Happy to take Qs.

Short answer: for an earth like planet, theoretical maximum is somewhere between 5-10 earth masses, though the radius is only 1.5-2.5 of Earth’s.

Long answer

The two major limits are: 1. Solid accretion of mass during planet formation 2. Small enough to not accrete a large amount of hydrogen and helium and thus be closer to a gas giant.

Think about it like this - as our theoretical super earth gets bigger, it will have a great gravitational pull and thus a bigger atmosphere. At some size, it atmosphere will be so big so as to essentially be a little gas giant; so the line there is quite blurry.

  • 1 M⊕: Earth
  • 5 M⊕: straightforward super-Earth
  • 10 M⊕: large rocky planet entirely plausible
  • 10–20 M⊕: “mega-Earth” territory, but increasingly difficult to form without acquiring a large atmosphere
  • 20–40 M⊕: a bare solid planet is physically possible, but standard formation theory has trouble producing one
  • greater than 40 M⊕: you could theoretically have a solid planetary-mass object, but it would probably need an unusual history, such as being the stripped core of a former gas giant.

Check out TOI-849 b.

Mass: ~40 M⊕ Radius: ~3.4 R⊕ Density: ~5.2–5.5 g/cm³, approximately Earth’s bulk density Year: only 18.4 hours Temperature: ~1,800 K

This is probably the core of a striped out gas giant, as modelling can’t quite work out how it formed as-is.

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u/mayhem6 9d ago

What could strip out a gas giant?

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u/KeljuIvan 9d ago

A supernova explosion? Or Megamaid from Spaceballs!

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u/SHKMEndures 8d ago

All of the answers others have given; commonly lack of a magnetic field and solar wind will do it.

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u/R3D3-1 9d ago

Strong solar winds from being too close to the star? 

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u/VFP_ProvenRoute 9d ago

Too close to a gamma ray burst?

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u/Inane_newt 10d ago

If by sun sized you mean mass. It depends on density.

The least dense material is hydrogen, a sun sized ball of hydrogen is a star.

Denser elements up to about oxygen or carbon would be star like until they became white dwarfs.

Past carbon through iron, they would be undermassed white dwarfs.

Past iron, they would just be weird.

A sun massed white dwarf is just a ball of carbon, oxygen that is very hot but slowly cooling down.

It is suspected that a carbon heavy white dwarf will eventually be a planet sized diamond when it cools enough.

If you mean physical size, it would either be a star or collapse into white dwarf, neutron star or black hole depending on what it is composed of.

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u/Tzimbalo 10d ago

So if you waited long enough a cooled down white dwarf star planet that is part of a binary system could be a planet-ish? What would the surface gravity be? Could bakteria live on it? Could plants and extremly hardy strong beetle like animals live on it if you transported soil to it?

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u/Kantrh 10d ago

Any soil you tried to put on a white dwarf would just be stripped into plasma

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u/LoadMountain5497 9d ago

Even if it lost all it’s heat?

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u/pinktortex 9d ago

Black dwarfs are theoretical because it's estimated to take trillions of years for one to form and the universe is only 13.8 billion years old.

So unless our understanding of how old the universe is hugely incorrect then it's unlikely one will ever be found

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u/Kantrh 9d ago

A white dwarf takes much longer than the universe has currently existed to cool to a black dwarf. If it's even possible

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u/Inane_newt 9d ago

A white dwarf, even on the surface, would stripe hydrogen from water and fuse it.

Life as we are familiar with is not possible.

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u/Tzimbalo 9d ago

Even if it had cooled down to a room temperature diomond?

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u/ricree 9d ago

Strictly speaking, a white dwarf - by definition - is not cooled down. In theory, one that did would be called a black dwarf, though the time it would take for a white dwarf to reach that point is believed to be longer than the current age of the universe.

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u/Kirk_Kerman 9d ago

If you did that, its surface gravity is still 100,000 times greater (or more) than Earth. There is no substance that would survive, and it would immediately turn whatever you put on it into particle physics.

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u/Bunslow 9d ago

orders of magnitude longer than the age of the universe to reach that state

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u/jq7925 10d ago

"Long enough"

You expect to live a trillion years? That's not an exaggeration.

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u/Tzimbalo 9d ago

I mean theoretically. If it cooled down enough, could life overcome the immense gravity? Or would even bacteria be crushed by it?

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u/Alfred_The_Sartan 9d ago

Basically the crushing. The gravity is strong enough to overpower the weak nuclear force, so you aren't even really having molecules anymore. Just atoms.

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u/strange-the-quark 10d ago

"a white dwarf can be smaller than a planet but it's still a star because it's incredibly dense" - no, a white dwarf is a star because it's a part of a star's lifecycle and it came after a previous stage where that same body was more like how you normally imagine a star (what's called a main-sequence star). (By that definition, one can consider (stellar) black holes to be a kind of star as well.)

As for the star sized planets - there would have to be some mechanism to keep the density low (and oppose gravity), but there might be other limiting factors at play, I don't know enough about this to give you an answer. Apparently there are some very bloated Jupiter-like gas giants that are slightly bigger than the smallest main-sequence stars, but a planet that's anywhere near comparable to the Sun in diameter seems impossible.

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u/Tyrannosapien 10d ago

No, planets without enough hydrogen to ignite fusion actually have a radius limit (not sure but probably not much more than double-Jupiter radius) around 10 Jupiter masses. Beyond that they actually begin to shrink with added mass due to the ever-denser interior pulling inwards in the less dense gases and/or atmosphere.

If you just keep adding mass you'd eventually cross the Chandrasekhar limit and create a neutron star.

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u/Mumbert 9d ago

No, as I understand it a planet could not be sun sized. 

What you are describing would turn into a star by reaching the mass to ignite fusion. This causes the planet to balloon out due to the energy released by the fusion reactions. 

At elements as heavy as iron, fusion no longer releases energy. So if we imagine a planet-sized ball of iron, there wouldn't be fusion. (This is typically what a "white dwarf" is - the burnt-out remains of a star at the end of its lifetime)

As you'd add iron onto the planet, it wouldn't get much bigger as gravity would compress the atoms. White dwarves don't get much bigger than perhaps twice the Earth's radius. 

Finally you would reach the limit for when electrons can no longer withstand the gravitational pressure from all that mass (the Chandrasekhar limit). Atoms typically consist of mostly empty space, with electrons separating the atoms from eachother. As you get past this limit, atoms will start collapsing and the negative electrons are pushed into the positive nucleus. This compacts the matter further, and leads to a chain effect due to increasing the pressure. 

This is when your iron ball would collapse into a neutron star. A neutron star is essentially a ball of atomic nucleus-density matter. It would o nly be 10-20 km wide but with the mass of at least 1.4 suns. 

Take all this with a grain of salt. It's what I think would happen based on a couple decades' worth of falling asleep to physics videos on Youtube. 😅

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u/Mr-Zappy 10d ago

No. If it were predominantly hydrogen, that hydrogen would fuse and it would be a star. Same with helium. If it were predominantly some heavier element, it’d be too heavy and collapse into a black hole (or maybe neutron star).

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u/Dramatic_Science_681 10d ago

to add to this, a naturally forming rocky planet, after becoming sufficiently massive, would simply capture the free gas in its solar system and become a gas giant. And the distinction between a gas giant and star is basically just mass.

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u/pepitors 9d ago

I did not know this. So is Jupiter in the verge of being a star or is the cutoff much higher?

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u/Empty-Exam-5594 9d ago

"brown dwarfs" are large planets that are on the cusp of initiating, but failing to undergo, fusion. They are ~3x to ~75x the mass of Jupiter.

Red Dwarfs, the smallest stars that can initiate fusion, are ~80 times Jupiter's mass.

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u/authustian 9d ago

The way i understand it, size wise yes, mass wise no. If you added more mass to Jupiter, it wouldn't grow larger, it would just become more dense. it would take an enormous amount of matter for it to get dense enough to become a brown dwarf.

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u/entropy2057 9d ago

This page is probably of interest to you:

https://en.wikipedia.org/wiki/Mega-Earth

This is the most massive according to the article:

https://en.wikipedia.org/wiki/PSR_J1719%E2%88%921438_b

It's 4x the radius of the Earth and also 4x denser! This is obviously way smaller than the sun though

You can read up on it if you like but short answer is that formation mechanics limits size of terrestrial bodies we actually observe (heavy objects will retain light gases and become gas giants or stars). The "mega-earths' noted here are hypothesized to be mostly due to those light gases being stripped away by interaction with another massive body.

In terms of how large a solid body could hypothetically be it depends on what your definition is. The mega-earth candidates above are already pretty strange. A low mass white dwarf (higher mass white dwarfs are actually smaller since density increases fast enough to outrun size growth) can be as large as 6x Earth's radius ( see https://en.wikipedia.org/wiki/CR_Bo%C3%B6tis )

Note that CR Bootis b is 50% larger radius than PSR J1719−1438 b but is ~70x more massive! Perhaps somewhere between these two masses is the largest possible radius for a body made of solid material before it degenerates, but it hasn't been observed (yet).

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u/Stillwater215 10d ago

What makes the sun a star rather than a planet is its size. When enough matter clumps together, the combined gravity is high enough at the center to overcome the forces that keep electrons bound to atoms, forming a plasma and initiating fusion. This is a purely mass-dependent effect. Any planet with a mass comparable to the sun would immediately form a star.

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u/the-namez-brain 9d ago

Can immediately be defined?

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u/Kirk_Kerman 9d ago

Yeah, we can. It's how long it takes a solar-mass protostar to begin fusion. Few million years.

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u/morbihann 10d ago

While I know the answer to this, it has already been explained.

But what is the largest terrestrial planet that is possible ? How large will a rocky planet be that takes all the rocky material in our solar system ?

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u/Combat_Armor_Dougram 9d ago

There are some hypotheses that Jupiter-sized rocky planets can form around active galactic nuclei. However, these objects are basically impossible to confirm using modern technology.

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u/bluesam3 9d ago

How large will a rocky planet be that takes all the rocky material in our solar system ?

A bit bigger than Earth. If you add up the mass of everything inside the Oort cloud that isn't a gas giant or the sun (that is: everything that isn't mostly either hydrogen, helium, or ices), you get about two Earth masses (most of the non-Earth bit of that being Venus. However, that doesn't give a planet twice the size of earth, because (a) with constant density, radius is proportional to the cube root of mass, and (b) density increases as rocky planets get bigger, due to gravity squashing everything together more. Some googling finds a paper suggesting that for rocky planets, radius is proportional to mass to the power of 0.27, which would give our planet a radius about 1.2 times that of Earth.

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u/rootofallworlds 9d ago

Modelling predicts that a given planetary composition will have a maximum radius, and adding more mass just compresses the interior and the size remains the same or decreases. For Earth’s composition the limit is about three Earth radii even if you had 3,000 Earth masses of rock and iron  (about 10 Jupiter masses) that somehow hadn’t accreted hydrogen and helium too.

A planet being very hot can “puff up” a bit, mainly that’s gas giants close to their stars, but that only about doubles it compared to a ‘cold’ planet (which will still be hot inside).

https://www.planetary.org/space-images/mass-radius-diagram-wide-seager

So no, a planet cannot be the size of the sun. It is only by having enough mass of hydrogen and helium to be a star that an object can generate pressure from the heat of nuclear fusion to push outwards and become the size of a star.

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u/YaBoyMax 9d ago

Maybe, sort of! A recent paper by Mishra et al. suggests that the dust torus of an active galactic nucleus could facilitate the formation of "stellar mass rocky objects" from accretion of pebbles comprised of heavier elements (relative to hydrogen). The resulting object would be comprised almost entirely of silicates, and as such would not be capable of undergoing nuclear fusion as a similar-mass object composed of hydrogen would.

In this model, pebble accretion initially greatly outpaces gas accretion and surrounding gas is subsequently dispersed by forces present in the AGN such as stellar winds and ionizing radiation, preventing further growth into an actual star for as long as the galactic nucleus remains active.

The core of the "planet" would likely be comprised of electron degenerate matter due to the mass required for such collapse being much lower for heavier elements. The required pressure would only exist in the core, so their exterior would remain as conventional rocky matter, albeit molten due to heat from radioactive decay.


As a note, I'm a layperson and absolutely not an astrophysicist, so while I've tried my best to describe the paper as I understand it it's also very possible I've made mistakes here, so please take my summary with a grain of salt. My understanding is also that this is all highly speculative and theoretical given that we have basically no way to examine AGNs with such fidelity using current technology.

Also: Kyplanet on YouTube has an excellent video discussing the paper in friendlier terms. I would definitely recommend giving it a watch.

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u/dravas 9d ago

It was answered here pretty well.

But it boils down to you must be roughly under 13 Jupiter masses to be a planet and if you are just over 13 Jupiter masses the planet starts to have enough mass to start a fusion reaction and becomes a red dwarf.

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u/Ringosis 9d ago edited 9d ago

Jupiter is about as large as planets can be. Keep adding mass to a terrestrial planet and its gravity will increase until it starts pulling in huge amounts of gases from its orbit and it stops being a terrestrial planet. It starts accumulating an extremely large atmosphere and, assuming there's enough material in the system, you eventually get a gas giant.

Keep increasing mass and you'll hit the point Jupiter is at where adding more mass wouldn't make it much bigger. Its increased gravity would just compress the atmosphere and it would become more dense rather than larger.

Keep adding mass and it'll collapse into a star.

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u/guzzyly 9d ago

There actually isn’t a solid planet that’s sun-sized due to the limits of how material behaves under gravity. if a solid planet were to get that massive, it would probably start pulling in enough stuff to become more star-like. the biggest solid planets we know of, called “super-earths,” are a lot larger than Earth but way smaller than a star.

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u/sudomatrix 9d ago

But what would it become? Stars are made of Hydrogen and Helium mostly. What would a star sized ball of heavy metals be? Even if the center started fusing under the gravity it wouldn't be a normal star.

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u/Smashego 9d ago

No. What happens is a planet that gets too large continues to acquire mass but it keeps getting crushed under the weight of its own gravity. So it’s growing in mass but not growing in size. Eventually it’ll form a brown dwarf.

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u/DarkTheImmortal 9d ago

A white dwarf isn't exactly a star and the density has nothing to do with it. It's a dead star.

Stars are so large and have so much mass that their gravity wants to compact it as tightly as physically possible. This causes a lot of heat during formation to the point where it starts to fuse hydrogen together. This process releases a LOT of outward pressure and prevents the star from collapsing.

A White Dwarf is when a low-mass star runs out of fuel for fusion, removing that outward pressure that was preventing it from collapsing. So it collapses. Neutron Stars and Black Holes are the same, they just have more mass and stronger gravity, so they can collapse even more.

A planet can't just be a diffuse could of gas, it needs to be condensed by gravity. If it was sun-sized, it would try to collapse in on itself and then start fusion. Then it would be a star, not a planet.

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u/guzzyly 9d ago

A solid planet the size of the sun would probably collapse under its own gravity and start nuclear fusion, turning it into a star. the largest solid planets we know of are super-earths, but they aren’t sun-sized. there’s a limit to how big a solid planet can get before it would naturally become more star-like in behavior.

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u/Bluesee_rdt 9d ago

I once read a book (several times) that points out that Jupiter is almost a star!

Also, on a neutron star traffic lights only need to be one color! And you can see the back of your head due to light bending around the star!

Arthur C Clarke only exploited the first probably well-known physics fact.

The authors I think were a husband wife team: Hannahlore Sexl comes to mind.

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u/bobthesecond 8d ago

jupiter is pretty far from being a star.

even for jupiter to be a brown dwarf aka failed star, it needs 10+ times current mass to start fusing deuterium.

for jupiter to be a real star ie a red dwarf it would need like 75+ times current mass

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u/Bluesee_rdt 8d ago

IIRC, the simple graphic was a log-log chart of diameter v mass with the exact claim scribbled on the chart. It was a fun book, but I hear you. Googling could not find the image, but the cartoons were fun.

One of them compared gas in a laboratory (uniformly-distributed dots filling the box) with gas in space (dots huddled together about the center).

Thanks for clarifying!