Английская Википедия:HD 142022 Ab

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Шаблон:Short description Шаблон:Infobox planet HD 142022 Ab is an exoplanet discovered by the radial velocity method by Eggenberger et al. in 2005, after finding that HD 142022 A is wobbling which indicated the presence of a massive planet, with a minimum mass 4.5 times Jupiter. It has a relatively wide separation between the planet and the star of nearly 3 AU, and takes 1928 days or 5.28 years to revolve. As is common for long-period planets, it has a relatively high eccentricity of 53±20%.[1] In 2023, the inclination and true mass of HD 142022 Ab were determined via astrometry.[2]

See also

References

Шаблон:Reflist

External links

Шаблон:Sky

Шаблон:Octans

Шаблон:Extrasolar-planet-stub

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  2. Ошибка цитирования Неверный тег <ref>; для сносок Xiao2023 не указан текст