Is Hydrodynamic Escape from Small Orbit Extrasolar Planets Fast or Slow? New Solution of Hydrodynamic Equations and Its Applications

Statistics – Applications

Scientific paper

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0325 Evolution Of The Atmosphere, 0343 Planetary Atmospheres (5405, 5407, 5409, 5704, 5705, 5707)

Scientific paper

Hydrodynamic escape has important applications in the formation and evolution of planetary atmospheres. Solutions to the time-independent hydrodynamic equations are difficult to find due to the existence of a singularity point. New method to solve time-dependent hydrodynamic equations is developed and validated. When applied to extrasolar planets under intense radiation from parent stars (HD209458b), we tried to answer the following 2 questions: 1) are these planets undergoing hdyrodynamic escape; 2) how fast are they losing their mass. Simulation results are compared with observations.

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