What is the last stage in the evolution of the Sun before it turns into a planetary nebula?
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After 500,000 years or so, only half of the Sun's current mass will remain and its outer envelope will begin to form a planetary nebula. The post-AGB evolution will be even faster, as the ejected mass becomes ionized to form a planetary nebula and the exposed core reaches 30,000 K.
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⏬⏬ANSWER⏬⏬
✨After 500,000 years or so, only half of the Sun's current mass will remain and its outer envelope will begin to form a planetary nebula. The post-AGB evolution will be even faster, as the ejected mass becomes ionized to form a planetary nebula and the exposed core reaches 30,000 K.✨
✌HOPE IT HELPS YOU !!✌
⏬⏬ANSWER⏬⏬
✨After 500,000 years or so, only half of the Sun's current mass will remain and its outer envelope will begin to form a planetary nebula. The post-AGB evolution will be even faster, as the ejected mass becomes ionized to form a planetary nebula and the exposed core reaches 30,000 K.✨
✌HOPE IT HELPS YOU !!✌
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