Abstract
Assuming that the terminated mass is confined within the range of 0.4551–0.5813 M ⊙ when the sun is going to evolve into a white dwarf, the velocity of the sun projecting the shell in the PN stage is much greater than the revolving velocity of the earth-like planet, therefore, we think that the solar mass change is instantaneous.
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References
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Acknowledgements
This work is supported by the Guangxi Natural Science Foundation (2012jjAA10090), the National Natural Science Foundation of China (NSFC 11173009, 11203007), the Bureau of Education of Guangzhou Municipality (No. 11 Sui-Jiao-Ke [2009]), Guangdong Province Universities and Colleges Pearl River Scholar Funded Scheme (GDUPS) (2009), Yangcheng Scholar Funded Scheme (10A027S), and support for Astrophysics Key Subject of Guangzhou city.
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Zhu, Y., Pan, C., Pan, D. et al. Influence of Sudden Change of Solar Mass in the PN Stage on the Orbit of Earth-Like Planet. J Astrophys Astron 35, 581–583 (2014). https://doi.org/10.1007/s12036-014-9292-y
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DOI: https://doi.org/10.1007/s12036-014-9292-y