Assuming a mass loss rate of 3*10^-8 solar masses yr^-1 and a stellar wind velocity of 100 km s^-1 from aT Tauri star, estimate the mass density of the wind at a distance of 100 AU

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Assuming a mass loss rate of 3*10^-8 solar masses yr^-1
and a stellar wind velocity of 100 km s^-1 from aT Tauri
star, estimate the mass density of the wind at a distance
of 100 AU
Transcribed Image Text:Assuming a mass loss rate of 3*10^-8 solar masses yr^-1 and a stellar wind velocity of 100 km s^-1 from aT Tauri star, estimate the mass density of the wind at a distance of 100 AU
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