Astrophysics

    

The Planets of the Binary Star RR Caeli

Authors: Herbert Weidner

The two stars in RR Caeli emit gravitational waves with a frequency of 76.22 $mu$Hz, which may be measured here on Earth. The decoding of the phase modulations of the GW shows nine companions -- including the planet already discovered with electromagnetic waves. Identical values of the orbital frequency are measured with both methods. The orbital times of the remaining planets fit well with the predictions of Dermott's law. The physical interpretation of the result of the phase modulation is difficult, but allows the masses of the planets to be estimated.

Comments: 8 Pages.

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[v1] 2023-08-27 14:20:13

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