Introduction and Questions about Asteroid Belt/Jovians

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    Asteroid Introduction
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Discussion Overview

The discussion revolves around the formation of the asteroid belt and the influence of Jupiter's mass on planetary formation in the solar system. Participants explore hypothetical scenarios regarding the size of Jupiter and its implications for the existence of the asteroid belt and potential terrestrial planets.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants propose that if Jupiter were significantly smaller, such as closer to Saturn's mass, it could lead to the formation of a terrestrial planet instead of the current asteroid belt.
  • One participant notes that the asteroid belt's current mass is very small, suggesting that the mass originally present may not have been sufficient to form a larger body than a moon-sized object.
  • Another participant questions how much mass was lost from the asteroid belt due to gravitational interactions with Jupiter and other bodies during the solar system's formation.
  • There is speculation that a smaller Jupiter, possibly an ice giant, might have allowed for a larger body to exist in the belt's orbit, as its gravitational influence would be less disruptive.
  • One participant mentions a paper discussing models of these scenarios but does not provide specific details or references.
  • Another participant expresses uncertainty about the exact amount of mass that would have been ejected from the asteroid belt if Jupiter were smaller.

Areas of Agreement / Disagreement

Participants express varying opinions on the effects of a smaller Jupiter on the asteroid belt and planetary formation, indicating that multiple competing views remain without a consensus on the outcomes.

Contextual Notes

Limitations include the lack of definitive data on the original mass of the asteroid belt and the complexities involved in modeling planetary formation scenarios.

redwood973
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Good evening, everyone.

My name is Steve, I'm 37 and from a small town called Fort Dodge in Iowa (USA). I have no formal education in Astronomy, but have always loved the topic since I was a child (most likely due to having a cousin who was an engineer for NASA who would send me photos and trinkets in the mail from time to time).

I stumbled upon your forum this afternoon and have been enjoying reading many of the threads since finding my way here . My interests will limit my reading and participation to this General Astronomy section of the forum. I may not be able to contribute much to your group, but I will defiantly be stopping by and reading the threads (a lurker, I believe it’s called).

Through my wondering around here I found myself wondering about the asteroid belt and the gas giants. I believe the accepted theory of the belts formation was the inability of the mass present in the belt to form a planetary body due to the effects of Jupiter’s gravity.

Now I was wondering–if Jupiter where much smaller than its actual 318 Earth masses, say closer to Saturn 95 Earth masses, would there still be an asteroid belt, or would we have another terrestrial planet?

Since Uranus (14 Earth masses) and Neptune (17 Earth masses) are considerably smaller, is it a given that there would be another terrestrial planet occupying the orbit of what would have been the asteroid belt if Jupiter were of their mass rather than the 318 it is?

I look forward to your thoughts on this topic.
 
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there's no way to tell for certain, as we cannot go back and time and see everything that was there and that happened when the solar system formed. The current mass of the asteroid belt is very small, only 4% of the moon according to the wikipedia article on the asteroid belt. While its very probably that some of the forming mass was ejected from the belt by Jupiter and other bodies when the belt was forming, I'm not sure there would have been enough mass to form anything larger than a moon sized object.
 
Hello, Drakkith.

Was there an estimate on how much mass was lost from the belt zone? It's only a guess, but I suspect it would be a considerable amount (based on the guess that the mass present in the belt zone would not have been much different from the mass present in the orbits of each of the four terrestrial planets, had the belt zone mass not been cast out by the giants).

I'm really interested in what effect on the belt Juipiter would have if it were smaller, but still a giant. I suspect that had Juipiter been an ice giant, such as Uranus and Neptune, there would be some planetary body in the belts orbit (due to the smaller size of the ice giants, it's not unreasonable to assume such a body in the belt zone would have been larger than 4% of Luna, as the smaller mass of the giant did not result in a scattering of mass the way superjovian Juipter did). But what of a Saturn-sized body at Juipiter's orbit? Would 95 Earth masses be sizeable enough to disrupt planetary formation? Doubtless it would scatter some mass, but would it inhibit planetary formation?

Anymore thoughts on the topic, or any source material anyone knows of?
 
Sorry Redwood, I don't know any details on this. I would definitely think a lower mass Jupiter would have caused less mass to be ejected from the asteroid belt. But I don't know how much was there originally or how much was predicted to have been lost.
 
redwood973 said:
Good evening, everyone.

My name is Steve, I'm 37 and from a small town called Fort Dodge in Iowa (USA). I have no formal education in Astronomy, but have always loved the topic since I was a child (most likely due to having a cousin who was an engineer for NASA who would send me photos and trinkets in the mail from time to time).

I stumbled upon your forum this afternoon and have been enjoying reading many of the threads since finding my way here . My interests will limit my reading and participation to this General Astronomy section of the forum. I may not be able to contribute much to your group, but I will defiantly be stopping by and reading the threads (a lurker, I believe it’s called).

Through my wondering around here I found myself wondering about the asteroid belt and the gas giants. I believe the accepted theory of the belts formation was the inability of the mass present in the belt to form a planetary body due to the effects of Jupiter’s gravity.

Now I was wondering–if Jupiter where much smaller than its actual 318 Earth masses, say closer to Saturn 95 Earth masses, would there still be an asteroid belt, or would we have another terrestrial planet?

Since Uranus (14 Earth masses) and Neptune (17 Earth masses) are considerably smaller, is it a given that there would be another terrestrial planet occupying the orbit of what would have been the asteroid belt if Jupiter were of their mass rather than the 318 it is?

I look forward to your thoughts on this topic.

Hi redwood973

There's a paper which discussed modelling of these very scenarios, but I can't remember the reference. Do a search of either the Internet PrePrint Archive...

http://arxiv.org/"

...or Google or try NASA's Astrophysical Database Server...

http://adsabs.harvard.edu/abstract_service.html"

...all very good reference tools.
 
Last edited by a moderator:
Hello, qrall and thanks!

Very good reference indeed! Just need to refine my search a bit--first searched turned up 527,000 hits, but I've gotten it down to about 8,000 (using SAO/NASA). Just a little more fine tuning to go.
 
My guess is Jupiter, being very massive, inhibited formation of what would have been the fourth planet orbiting the sun. What remains is the asteroid belt.
 

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