Solar Models with Dynamic Screening and Early Mass Loss Tested by Helioseismic,Astrophysical, and Planetary Constraints |
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| Authors: | Suzannah R Wood " target="_blank">Katie Mussack " target="_blank">Joyce A Guzik |
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| Institution: | 1.Los Alamos National Laboratory,Los Alamos,USA;2.Los Alamos National Laboratory,Los Alamos,USA |
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| Abstract: | The faint young Sun paradox remains an open question. Presented here is one possible solution to this apparent inconsistency, a more massive early Sun. Based on the conditions on early Earth and Mars, a luminosity constraint is set as a function of mass. We examine helioseismic constraints of these alternative mass-losing models. Additionally, we explore a dynamic electron screening correction in an effort to improve helioseismic agreement in the core of the early mass-losing model. |
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