The Sun's Journey Through the Local Interstellar Medium: The PaleoLISM and Paleoheliosphere

Abstract

Over the recent past, the galactic environment of the Sun has differed substantially from today. Sometime within the past ~130,000 years, and possibly as recent as ~56,000 years ago, the Sun entered the tenuous tepid partially ionized interstellar material now flowing past the Sun. Prior to that, the Sun was in the low density interior of the Local Bubble. As the Sun entered the local ISM flow, we passed briefly through an interface region of some type. The low column densities of the cloud now surrounding the solar system indicate that heliosphere boundary conditions will vary from opacity considerations alone as the Sun moves through the cloud. These variations in the interstellar material surrounding the Sun affected the paleoheliosphere.

To be published in Astrophysics and Space Sciences Transactions (ASTRA), for the proceedings of the workshop "Future Perspectives in Heliospheric Research: Unsolved Problems, New Missions - New Sciences" Bad Honnef, Germany, April 6-8, 2005, held in honor of Prof. Hans Fahr's 65th birthday

Cited by in corpus (7)

• The interstellar cloud surrounding the Sun: a new perspective
• Heliospheric Compression due to Recent Nearby Supernova Explosions
• Can IBEX Identify Variations in the Galactic Environment of the Sun using Energetic Neutral Atom (ENAs)?
• The S1 Shell and Interstellar Magnetic Field and Gas near the Heliosphere
• A search for lithium in metal-poor L dwarfs
• The Heliosphere in Time
• Influence of interstellar environment near the solar system on cosmic-ray spectra and dipole anisotropy