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The Sun and Earth in the distant future Evolution of the Sun: With

The Sun and Earth in the distant future Evolution of the Sun: With mass loss. Solar wind mass-loss is negligible (~10-14 Msun/year). Mass loss is much greater at RGB and AGB stages. We use a new semi-empirical formula, calibrated from globular cluster giants and nearby galactic giants (Schr?der & Cuntz, ApJ, 630, L73, 2005 and A&A, 465, 593, 2007): where ? = 8?10-14 solar masses/year. This leads to a loss of 0.332 Msun by the tip RGB.

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