Planets <-> solar systems <-> galaxies

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Discussion Overview

The discussion revolves around the observation and definition of planets, particularly focusing on the existence of planets outside of solar systems and solar systems outside of galaxies. Participants explore the challenges of detecting rogue planets and the implications of technological capabilities on these observations.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants question whether planets can exist outside of solar systems, particularly rogue planets that do not orbit a star.
  • There is a discussion on the definition of a planet, with some arguing that it traditionally requires a star, while others suggest that low-mass objects could also be considered planets.
  • Participants note the difficulty of detecting rogue planets due to their lack of illumination and the limitations of current detection methods, which primarily focus on planets around stars.
  • Some propose that while rogue planets are hard to detect, they may exist, and their detection could potentially be achieved through methods like microlensing.
  • There is mention of historical projects like MACHO that have found evidence of low-mass objects, suggesting that there may be many undetected rogue planets or low-mass stars.
  • Discussion includes the possibility of solar systems existing outside of galaxies, which is also framed as a matter of technological capability and the distribution of stars in galaxies.
  • One participant references the ejection of stars from galaxies and questions whether these rogue stars could have accompanying planetary systems.

Areas of Agreement / Disagreement

Participants express differing views on the definition of planets and the feasibility of detecting rogue planets and solar systems outside of galaxies. There is no consensus on these topics, and the discussion remains unresolved.

Contextual Notes

Limitations include the dependence on current technological capabilities for detection and the unresolved nature of definitions regarding what constitutes a planet.

Loren Booda
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Planets <--> solar systems <--> galaxies

Have planets been observed outside of solar systems, or solar systems outside of galaxies?
 
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Loren Booda said:
Have planets been observed outside of solar systems, or solar systems outside of galaxies?

Just a rogue planet floating around without a star?... I though part of the definition of a plant was that it was in orbit around a star...
 


Sorry! said:
Just a rogue planet floating around without a star?... I though part of the definition of a plant was that it was in orbit around a star...
Rogue it is.
 


No. It is hard enough to find planets when we know almost exactly where to look and they're well lit by their star.

Even if we knew exactly where look, a rogue planet would be pretty much invisible in the darkness.
 


Our planet detection methods require them to be around stars.
 


russ_watters said:
Our planet detection methods require them to be around stars.

A sensible definition for the present. It follows that binary planets are precluded.

What about the possibility of solar systems outside of galaxies?
 


Loren Booda said:
A sensible definition for the present. It follows that binary planets are precluded.
I'm not sure you understood me: It's not a definition, it is a matter of technological capability.
What about the possibility of solar systems outside of galaxies?
That, too is a matter of technological capability, but also a matter of the fact that the vast majority of stars are in galaxies.
 


While a 'rogue' planet would be very difficult to detect, that is not to say they don't exist. The question comes down to the definition of a planet. We really don't know very much about the formation of very low mass stars (because they are very hard to see) so it is possible that when star clusters form, there are many 'stars' which form that are not sufficiently massive to start nuclear fusion. Technically, a ball of gas that is not burning at the core is a planet (such as the gas giants in our solar system) and as such there may well be many of these lone planets out there.

Detecting them would be very hard, and certainly the way we hunt for planets around stars would never find them. We could possibly see them via microlensing, if we got lucky.
 


Wallace said:
We could possibly see them via microlensing, if we got lucky.
Now there's an understatement. :wink:
 
  • #10


Not really, the MACHO project in the late 90's found evidence for lone microlensing lenses with masses about twice that of Jupiter, and that was using a 40 inch telescope. In general, MACHO found a lot more microlensing events when looking towards the core of the Milky Way than expected, indicating the possible presence of many low mass stars/lone planets.

Modern microlensing surveys, e.g. see http://bustard.phys.nd.edu/MPS/" are most definitely aimed at addressing this question (amongst others). You have to be lucky to see an individual event, but the theory behind these surveys is that if you keep watching enough stars you're effectively rolling the dice many times, so you end up getting lucky pretty often.
 
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