Are there undiscovered sister stars in our solar system?

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SUMMARY

The discussion centers on the hypothesis of undiscovered sister stars in our solar system, particularly in relation to Alpha Centauri, which is measured at 742 marcs parallax (approximately 1.3 parsecs or 4.3 light-years away). While the idea that our sun has sister stars at closer distances is proposed, it is countered by observational evidence suggesting otherwise. The use of infrared telescopes to search for cold gas giants and the implications of the Oort cloud's structure are also examined, concluding that no definitive evidence for nearby sister stars has been found, and the search for such celestial bodies continues.

PREREQUISITES
  • Understanding of stellar parallax and distance measurement
  • Familiarity with infrared astronomy and telescope technology
  • Knowledge of the Oort cloud and its significance in astrophysics
  • Basic concepts of stellar formation and multiple star systems
NEXT STEPS
  • Research the capabilities and findings of infrared telescopes in stellar surveys
  • Explore the current status of the Brown dwarf survey and its implications
  • Investigate the structure and dynamics of the Oort cloud in multi-stellar systems
  • Study the historical context and theories surrounding the hypothetical 'Nemesis' star
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Astronomers, astrophysicists, and space enthusiasts interested in stellar formation, the search for celestial bodies, and the dynamics of our solar system.

cph
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Hipparcus indicates that our supposed closest star alpha centuari is 742 marcs parallax, which corresponds to about 1.3 pc or 4.3 yrs away. Since stars form in multiple; hence our sun has sister stars at much closer distance, with higher parallax values. Also infrared telescope could be used to look for cold gas giants, and compare image size for relative closesness. In fact does the Brown dwarf survey, and other surveys, include some large infrared planets which indicate a nearby sister star? Such sister stars would have a center of mass, and hence via central force, one would have a spherical distributed cometary cloud - a common Oort cloud. So does our Oort cloud enclose a multi-stellar system?
 
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cph said:
Hipparcus indicates that our supposed closest star alpha centuari is 742 marcs parallax, which corresponds to about 1.3 pc or 4.3 yrs away.

So far so good.

cph said:
Since stars form in multiple;

Sometimes.

cph said:
hence our sun has sister stars at much closer distance, with higher parallax values.

This doesn't logically follow. Observationally, it appears to be untrue.

cph said:
Also infrared telescope could be used to look for cold gas giants, and compare image size for relative closesness.

Yes, but a gas giant is not a star.

cph said:
In fact does the Brown dwarf survey, and other surveys, include some large infrared planets which indicate a nearby sister star?

No.

cph said:
Such sister stars would have a center of mass, and hence via central force, one would have a spherical distributed cometary cloud - a common Oort cloud. So does our Oort cloud enclose a multi-stellar system?

And no.
 
Uh, IIRC, the infrared survey results are not all in. However, no obvious candidates for red or brown dwarf stars have yet jumped out of the search. There may be ultra-dim stars, there may be ice-planets, but they'll take some finding and much confirmation.

Odds are good on lots of 'plutoid' objects, and possibly a couple of distant 'neptunians'. IMHO, finding 'Nemesis' is unlikely...
 

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