Relativistic redshift of the star S0-2 orbiting the Galactic Center supermassive black hole

@article{Do2019RelativisticRO,
  title={Relativistic redshift of the star S0-2 orbiting the Galactic Center supermassive black hole},
  author={T. Do and A. Hees and A. Ghez and G. Martinez and D. Chu and Siyao Jia and S. Sakai and J. Lu and A. Gautam and K. O'Neil and E. Becklin and M. Morris and K. Matthews and S. Nishiyama and R. Campbell and S. Chappell and Z. Chen and A. Ciurlo and A. Dehghanfar and E. Gallego-Cano and W. E. Kerzendorf and J. Lyke and S. Naoz and H. Saida and R. Schoedel and M. Takahashi and Yohsuke Takamori and G. Witzel and P. Wizinowich},
  journal={Science},
  year={2019},
  volume={365},
  pages={664 - 668}
}
  • T. Do, A. Hees, +26 authors P. Wizinowich
  • Published 2019
  • Physics, Medicine
  • Science
  • Gravitational redshift in the Galactic Center General relativity predicts that light emitted by an object in a strong gravitational field—for example, close to a black hole—should be shifted to longer wavelengths. This gravitational redshift does not exist in the Newtonian theory of gravity. Do et al. monitored the position and spectrum of the star S0-2 as it passed Sagittarius A*, the supermassive black hole at the center of the Milky Way. Around the closest part of S0-2's 16-year orbit, they… CONTINUE READING
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