The Closest Gas Giant: Why is Jupiter so Big?

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Discussion Overview

The discussion revolves around the reasons for Jupiter's large size compared to other planets in the solar system, exploring theories related to planetary formation, atmospheric retention, and the distinctions between stars and planets. Participants examine the implications of these factors on the characteristics of gas giants versus rocky planets.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants suggest that the inner planets are rocky because the Sun boiled off their atmospheres, while gas giants like Jupiter retained theirs due to their distance from the Sun.
  • Others propose that Jupiter's size is influenced by the density of the protoplanetary disc during formation, allowing it to accumulate more material.
  • A participant mentions that turbulence in the disc may have led to the clumping of gases, contributing to the formation of gas giants.
  • It is noted that larger planets can hold onto lighter gases due to their stronger gravitational pull, while smaller planets cannot.
  • Some argue against the idea that Jupiter's atmosphere was formed from gases boiled off other planets, asserting that each planet developed its own atmosphere during formation.
  • Disagreement arises regarding whether Jupiter should be classified as a "brown dwarf" star, with some asserting it is a planet based on its formation process rather than mass.
  • Participants discuss the implications of Jupiter emitting more heat than it receives from the Sun, questioning its relevance to the star/planet distinction.
  • There is mention of the discovery of extrasolar planets that challenge existing models, suggesting that planetary migration may have occurred in the solar system.
  • Some participants express skepticism about the planetary migration theory while others find it gaining credibility.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the factors influencing Jupiter's size and classification, and the discussion remains unresolved with no consensus reached on several points.

Contextual Notes

Participants reference various theories and models related to planetary formation, but there are limitations in the assumptions made about the processes involved and the definitions of terms like "star" and "planet." The discussion reflects ongoing debates in the field without definitive conclusions.

Who May Find This Useful

Readers interested in planetary science, astrophysics, and the formation of celestial bodies may find the discussion relevant and informative.

Nim
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How I understand it, the four inner planets are rocky planets because the Sun boiled off most of their atmospheres, while the planets past Mars retained there's.

I was wondering if the reason why Jupiter is so big is because it is the closest planet to Mars, so it caught most of the atmosphere that was boiled away by the Sun. Plus, the planets get smaller and smaller after Jupiter. Although maybe that has more to do with the density of the disc near the edges when the planets were forming.
 
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My guess would be its the density of the disc. Not sure though.
 
I believe the current theory to the creation of the gas giants relies on turbulence developing in the disc, swirling some gases into clumps. In this case, the fact that Jupiter is the innermost is probably because Jupiter was a disturbance that started in a patch of high density gases.

I don't think the atmosphere of Mars is a significant factor.
 
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Actually, Nim, it is held that planets have to be very large, in order to produce enough gravity to hold in lighter gases. Earth is only large enough (IIRC) to hold in Oxygen and heavier gases/elements.

So, the atmospheres were not blown off of other planets onto gas giants, but rather each planet developed it's own atmosphere as it was forming, and the bigger ones could hold in lighter gases.

Jupiter, btw, is considered to be a "brown dwarf" star, which is star that never "ignited".
 
Originally posted by Mentat
Jupiter, btw, is considered to be a "brown dwarf" star,
which is star that never "ignited".
Nope, as far as I remember it'll have to be 8-10 times
more massive for that.

Peace and long life.
 
Nim How I understand it, the four inner planets are rocky planets because the Sun boiled off most of their atmospheres, while the planets past Mars retained theirs.
Close. The inner planets formed in a region where the volatiles (water, methane, ammonia, etc) had been 'boiled off' while the proto-solar system disk was collapsing; their atmospheres came later, from comets (tho' not the Earth's oxygen Mentat, that came much later, from plants).

All the planets were formed by collisions (rocky planets) or gravitational accretion (gas planets) of planetesimals.
Nim I was wondering if the reason why Jupiter is so big is because it is the closest planet to Mars, so it caught most of the atmosphere that was boiled away by the Sun. Plus, the planets get smaller and smaller after Jupiter. Although maybe that has more to do with the density of the disc near the edges when the planets were forming.
Jupiter, like the other gas giants, could grow bigger than the rocky planets because there was much more material from which it could form (all those volatiles).

The planets get smaller and smaller after Jupiter because of the way the remaining gas, dust, and planetesimals were swept up by the growing planets.

Here's a link that gives a good overview:
http://www.pha.jhu.edu/~akir/Seminar/seminar.html
Mentat Jupiter, btw, is considered to be a "brown dwarf" star, which is star that never "ignited"
No, it's still a planet. Although the terminology is somewhat inconsistenly applied, the star/planet distinction refers to the formation process, not the mass, nor whether ignition took place or not. Stars form by the collapse of a gas/dust cloud; planets by accretion.
 
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Greetings !

We have to remember that that's the way things happened
in our solar system, but we've already seen many that
acted otherwise.
Originally posted by Nereid
No, it's still a planet. Although the terminology is somewhat inconsistenly applied, the star/planet distinction refers to the formation process, not the mass, nor whether ignition took place or not. Stars form by the collapse of a gas/dust cloud; planets by accretion.
Well, isn't that more of a relative definition, after all
a star can also be orbiting other stars/objects as well
as turning aroung the galaxy center and a planet can
also form individualy without anything nearby to rotate
around, if the amount of gas is too small. Right ?

Live long and prosper.
 
drag wrote: Well, isn't that more of a relative definition, after all a star can also be orbiting other stars/objects as well as turning aroung the galaxy center and a planet can also form individualy without anything nearby to rotate around, if the amount of gas is too small. Right ?
Definitions can be somewhat arbitrary. Among those who work together, or otherwise form a community, you usually find that the terms they use settle down to have fairly narrow ranges of meanings (unless they're politicians, of course!).
Stars form by the collapse of a gas/dust cloud; planets by accretion
That's what astronomers generally mean when they use the terms 'star' and 'planet'. Certainly, stars may form in pairs (the collapse of two blobs of gas, or a cloud which formed two centres), and may form in a galaxy or globular cluster.

An object which forms from a very small gas cloud would be called a brown dwarf. A number of isolated brown dwarfs have been observed, though it's not always clear if they formed in isolation, or were ejected from a binary.
 
Originally posted by Nereid
No, it's still a planet. Although the terminology is somewhat inconsistenly applied, the star/planet distinction refers to the formation process, not the mass, nor whether ignition took place or not. Stars form by the collapse of a gas/dust cloud; planets by accretion.
So the fact that Jupiter gives off lots more heat, then it gets from the Sun, seems to, in your mind, not have anything to do with the distinction 'tween stars and planets, Huh?
 
  • #10
Originally posted by drag
Greetings !

We have to remember that that's the way things happened
in our solar system, but we've already seen many that
acted otherwise.


In fact, these other systems have caused us to re-evaluate the current model. Many of the extrasolar planets so far discovered are planets several timea the size of Jupiter with orbits smaller than Venus. This has lead to the idea of planetary migration, which proposes that Jupiter and possibly the other gas giants formed close to the Sun and then moved outward much later.

I don't really buy that theory yet, but it is gaining credibility. Personally, I think the inner planets are rocky because of the composition of the protosolar accretion at the very beginning. The disk was formed buy gravitational attraction, and so it would seem (to me, at least) to make sense that the heavier elements were closer to the center, sort-of "settled to the bottom". Meanwhile, the lighter elements that we normally think of as gasses would float to the top, leaving them out near the edge. I am hoping that the mission to Pluto will help confirm this idea.
 
  • #11
Originally posted by Mr. Robin Parsons
So the fact that Jupiter gives off lots more heat, then it gets from the Sun, seems to, in your mind, not have anything to do with the distinction 'tween stars and planets, Huh?
Just telling it like it is!

Who sets the rules for how language is used? Let's all vote for Mr. Robin Parsons!

:wink: First order of business, Madame Chair (of the International Astronomical Union), motion to refer all questions of nomenclature to Mr. Robin Parsons for his esteemed, absolute ruling. :wink:
 
  • #12
Originally posted by Nereid
Just telling it like it is!
Who sets the rules for how language is used? Let's all vote for Mr. Robin Parsons!
:wink: First order of business, Madame Chair (of the International Astronomical Union), motion to refer all questions of nomenclature to Mr. Robin Parsons for his esteemed, absolute ruling. :wink:
To whom it might/and/or/does concern, I would respectfully desist from the nomination, as it is deleterious to my current reputation :wink: to have such a nominator at hand.
Thanks, one and all!
 
  • #13
And did you know, those perfidious astronomers, they wanted to demote Pluto! They had this totally :wink: unreasonable, :wink: irrational idea that just 'cause
- there are lots and lots of satellites that are bigger
- it's merely the largest of a class of objects, numbering >1,000 (the Plutinos, EKB objects, SDOs, ... take your pick)
- Ceres* doesn't get to be called a planet
- etc, etc, etc
it didn't deserve to be called a planet. I mean, just look at it - doesn't it look like a planet to you?

Girl, they sure know how to hurt a planet's feelings.

*the largest asteroid. Like the planets, asteroids orbit the Sun. The main belt asteroids' orbits lie between Mars and Jupiter. >200,000 have been observed (only ~10,000 have names). If Ceres isn't a planet, why should Pluto be?
 

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