Astrophysics

   

The Planets of the Binary Star Epsilon Ursae Minoris

Authors: Herbert Weidner

So far, no planets have been discovered in the binary star system, which is 300 LY away. The two stars emit gravitational waves with a frequency of 586 nHz, which can be measured here on Earth. The decoding of the phase modulations of the GW shows textit{eleven} companions -- unseen by electromagnetic waves. The orbital times 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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Submission history

[v1] 2023-08-21 09:50:32

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