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HD 164595 b es un exoplaneta confirmado orbitando alrededor de HD 164595 cada 40 días; a la distancia de su estrella de 0.230 UA o 34.407.510,252 km. A 94.36 años luz de nuestro Sistema Solar. Tiene una masa equivalente a 16 Tierras.[1]

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  • HD 164595 Signal - Is it Aliens? What does SETI think? [Space Engine]
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Transcription

Señal candidata de SETI

Una reciente (2015) señal de radio en los 11 GHz (2.7 cm) ha sido observada en la dirección de HD 164595 por el equipo de Claudio Maccone en el observatorio de radio RATAN-600. Se desconoce qué planeta del sistema estelar está implicado. Podría ser en cambio un lente gravitacional de una fuente más distante.[2]

Referencias

  1. «HD 164595 b CONFIRMED PLANET OVERVIEW PAGE». NASA. Consultado el 8 de octubre de 2015. 
  2. SETI observations on the RATAN-600 telescope in 2015 and detection of a strong signal in the direction of HD 164595 BURSOV N., FILIPPOVA L., FILIPPOV V., GINDILIS L., MACCONE C. et al. 2016 | in " IAA SETI Permannent Committee", Guadalajara, Mexico, ,
Esta página se editó por última vez el 11 jun 2020 a las 08:47.
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