HD 20782 b explained

HD 20782 b
Discoverer:Jones et al.
Discovery Site:Anglo-Australian Planet Search
Discovered:March 14, 2006
Apsis:astron
Semimajor:1.36±
Eccentricity:0.97 ± 0.01
Period:585.86 ± 0.03 d
Time Periastron:2451687.1 ± 2.5
Arg Peri:147 ± 3
Semi-Amplitude:115 ± 12

HD 20782 b is an extrasolar planet located approximately 117 light-years away in the constellation of Fornax, orbiting the star HD 20782.

This planet orbits in the most eccentric orbit known (as of November 2012),[1] with a semi-major axis of 1.36 AU, and eccentricity e=0.97+/-0.01.[2] As a result, it also has one of the most extreme temperature swings.

See also

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Notes and References

  1. MNRAS . 0810.1589 . Selection Functions in Doppler Planet Searches . S. J. O'Toole . C. G. Tinney . H. R. A. Jones . R. P. Butler . G. W. Marcy . B. Carter . J. Bailey . 392, 641 . 2009. 2 . 641–654 . 2009MNRAS.392..641O . 10.1111/j.1365-2966.2008.14051.x . free . 7248338 .
  2. https://arxiv.org/abs/0810.1589 Selection Functions in Doppler Planet Searches