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1988•Progress of Theoretical Physics SupplementOpen access

Chapter 14. Dissipation of the Solar Nebula

Keiji Ohtsuki, Yoshitsugu Nakagawa

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Abstract

The solar nebular gas, which must have played quite important roles in various stages of planetary formation, disappeared at some stage of evolution of the solar system and no longer exists at present. The dissipation process of the solar nebula must be closely related to interaction with the Sun, which has not been well understood. In this chapter, we will review the previous work on the dissipation of the solar nebula, although they are still preliminary.

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The solar nebular gas, which must have played quite important roles in various stages of planetary formation, disappeared at some stage of evolution of the solar system and no longer exists at present. The dissipation process of the solar nebula must be closely related to interaction with the Sun, which has not been well understood. In this chapter, we will review the previous work on the dissipation of the solar nebula, although they are still preliminary.

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Available abstract

The solar nebular gas, which must have played quite important roles in various stages of planetary formation, disappeared at some stage of evolution of the solar system and no longer exists at present. The dissipation process of the solar nebula must be closely related to interaction with the Sun, which has not been well understood. In this chapter, we will review the previous work on the dissipation of the solar nebula, although they are still preliminary.

Key concepts: Formation and evolution of the Solar System, Nebula, Astrobiology, Solar System, Dissipation, Physics, Astronomy, Planetary nebula

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