Common Envelope

Definition

The common envelope is a phase in the evolution of a binary star system where the two stars become enveloped in a shared, extended atmosphere. This critical stage can significantly impact the future evolution and interaction of the binary components.

5 Must Know Facts For Your Next Test

1. The common envelope phase occurs when one of the stars in a binary system expands to the point where it engulfs its companion star.
2. This can happen when a more evolved, larger star transfers mass to its less massive companion, leading to the formation of the common envelope.
3. The common envelope phase is a crucial stage in the evolution of many binary systems, as it can significantly alter the final configuration and properties of the system.
4. During the common envelope phase, the orbital separation of the two stars decreases rapidly, which can lead to the merger of the stars or the ejection of the common envelope.
5. The outcome of the common envelope phase depends on factors such as the mass ratio of the two stars, the initial orbital separation, and the efficiency of the energy transfer within the envelope.

Review Questions

• Explain the formation and significance of the common envelope in the evolution of binary star systems.
  • The common envelope phase occurs when one star in a binary system expands and engulfs its companion star, forming a shared, extended atmosphere around the two stars. This critical stage can significantly impact the future evolution of the binary system. During the common envelope phase, the orbital separation of the two stars decreases rapidly, which can lead to the merger of the stars or the ejection of the common envelope. The outcome of this phase depends on factors such as the mass ratio of the stars, the initial orbital separation, and the efficiency of energy transfer within the envelope. The common envelope phase is a crucial stage in the evolution of many binary systems, as it can determine the final configuration and properties of the system.
• Describe the role of mass transfer in the formation of the common envelope and its impact on the binary system's evolution.
  • Mass transfer between the stars in a binary system is a key factor in the formation of the common envelope. When a more evolved, larger star transfers mass to its less massive companion, it can lead to the expansion of the larger star to the point where it engulfs its companion, creating the common envelope. This mass transfer and the subsequent common envelope phase can significantly alter the future evolution of the binary system. The rapid decrease in orbital separation during the common envelope phase can result in the merger of the stars or the ejection of the common envelope, ultimately shaping the final configuration and properties of the binary system.
• Analyze how the Roche lobe and the common envelope are interconnected in the context of binary star system evolution.
  • The Roche lobe, which defines the region around a star in a binary system within which orbiting material is gravitationally bound to that star, is closely related to the formation of the common envelope. When one of the stars in a binary system expands to the point where it fills its Roche lobe, the mass transfer from the larger star to its companion can lead to the creation of the common envelope. The common envelope then encompasses both stars, altering the Roche lobes and the gravitational interactions within the system. The evolution of the Roche lobe and the common envelope are thus interdependent, as the former can trigger the formation of the latter, which in turn shapes the future evolution of the binary system through processes such as orbital separation changes and potential mergers or envelope ejection.

Related terms

Binary Star System: A system of two stars that orbit around their common center of mass, held together by gravitational attraction.

Mass Transfer: The process by which material is transferred from one star to the other in a binary system, often through the common envelope.

Roche Lobe: The region around a star in a binary system within which orbiting material is gravitationally bound to that star.