Undergrad Solar System Diameter: Calculating Distances & Multi-Star Systems

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SUMMARY

The calculation of a solar system's diameter is not simply a matter of doubling the distance of the furthest planet from its star. The boundaries of a solar system are influenced by the solar wind and the Sun's gravity, with the heliopause marking the transition to interstellar space at approximately four times Pluto's distance from the Sun. The Sun's gravitational influence extends up to two light years (125,000 AU), while the Oort cloud's radius is estimated to be around 50,000 AU. Current knowledge indicates that the furthest known objects, such as Comet West, have aphelia of about 70,000 AU from the Sun, suggesting that our understanding of the solar system's extent is still evolving.

PREREQUISITES
  • Understanding of heliopause and its significance in solar system boundaries
  • Knowledge of the Sun's gravitational influence and its Hill sphere
  • Familiarity with the Oort cloud and its estimated dimensions
  • Basic concepts of solar wind and its effects on solar system boundaries
NEXT STEPS
  • Research the properties and boundaries of the heliosphere
  • Study the gravitational dynamics of multi-star systems
  • Explore the characteristics and significance of the Oort cloud
  • Investigate the latest discoveries regarding distant solar system objects
USEFUL FOR

Astronomers, astrophysicists, and space enthusiasts interested in understanding the structure and boundaries of solar systems, particularly in relation to gravitational influences and multi-star systems.

exxon_valdez
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TL;DR
Method to calculate a solar system diameter.
What is the method of calculating the diameter of a solar system knowing each of its planets distance to the star? Is it a matter of doubling the distance of the furthest planet?
What about when a solar system has more than one star?
 
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exxon_valdez said:
What is the method of calculating the diameter of a solar system knowing each of its planets distance to the star?
The boundaries of solar system are not exactly defined. See wiki:
The point at which the Solar System ends and interstellar space begins is not precisely defined because its outer boundaries are shaped by two forces, the solar wind and the Sun's gravity. The limit of the solar wind's influence is roughly four times Pluto's distance from the Sun; this heliopause, the outer boundary of the heliosphere, is considered the beginning of the interstellar medium.[63] The Sun's Hill sphere, the effective range of its gravitational dominance, is thought to extend up to a thousand times farther and encompasses the hypothetical Oort cloud.
Much of the Solar System is still unknown. The Sun's gravitational field is estimated to dominate the gravitational forces of surrounding stars out to about two light years (125,000 AU). Lower estimates for the radius of the Oort cloud, by contrast, do not place it farther than 50,000 AU.
...
Currently, the furthest known objects, such as Comet West, have aphelia around 70,000 AU from the Sun, but as the Oort cloud becomes better known, this may change.

exxon_valdez said:
Is it a matter of doubling the distance of the furthest planet?
Surely not, see previous quotes.
 
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