File:NGTS-12 b render in Celestia.png

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Original file(1,920 × 2,036 pixels, file size: 1.64 MB, MIME type: image/png)

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The Hot Jupiter exoplanet NGTS-12 b rendered in the application Celestia

Summary[edit]

Description
English: NGTS-12 b is a sub-Saturn mass Hot Jupiter orbiting the slightly evolved G4V star NGTS-12. The planet has an orbital period of seven and a half days, which, at the time of its discovery, made it the longest period planet discovered by the main NGTS survey. It was later beaten by NGTS-19b and NGTS-20b. I say that it is "inflated" because it has a size slightly larger than that of Jupiter, but less than that of Saturn, meaning it has a low density and is thus "inflated". NGTS-12 b might be nearing the end of its lifetime, as its star may be beginning to transit into the subgiant phase, meaning that the planet could soon be engulfed by its parent star.)
Русский: NGTS-12 b — это Горячий Юпитер с массой субсатурна, вращающийся вокруг слегка эволюционировавшей звезды G4V NGTS-12. Планета имеет период обращения семь с половиной дней, что на момент ее открытия делало ее самой длиннопериодической планетой, обнаруженной основным обзором NGTS. Позже его обыграли НГТС-19б и НГТС-20б. Я говорю, что он «раздут», потому что его размер немного больше, чем у Юпитера, но меньше, чем у Сатурна, а это означает, что он имеет низкую плотность и поэтому «раздут». NGTS-12 b может приближаться к концу своего существования, так как его звезда, возможно, начинает переходить в субгигантскую фазу, а это означает, что планета вскоре может быть поглощена родительской звездой.)
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This image was created with Celestia.
Author TheLostProbe

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Date/TimeThumbnailDimensionsUserComment
current03:50, 13 July 2022Thumbnail for version as of 03:50, 13 July 20221,920 × 2,036 (1.64 MB)TheLostProbe (talk | contribs)more realistic
11:58, 23 October 2020Thumbnail for version as of 11:58, 23 October 20201,761 × 1,768 (1.32 MB)TheLostProbe (talk | contribs)Uploaded own work with UploadWizard

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