Neptunus panas

Neptunus panas^[1] adalah sejenis planet raskasa dengan sebuah massa yang mirip dengan Uranus atau Neptunus yang mengorbit dekat dekat bintangnya, biasanya dalam jarak kurang dari 1 SA.^[2]

Referensi

^ Dong; et al. (23 June 2017). "LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements". Proceedings of the National Academy of Sciences. 115 (2): 266–271. arXiv:1706.07807 . doi:10.1073/pnas.1711406115. PMC 5777037 . PMID 29284755.
^ G. Wuchterl. "Hot Neptunes: A Key To Giant Planet Formation" (PDF). cosis.net. Diakses tanggal 3 August 2015.

Sumber

Gillon; et al. (September 2007). "Detection of transits of the nearby hot Neptune GJ 436 b". Astronomy and Astrophysics. 472 (2): L13–L16. arXiv:0705.2219 . Bibcode:2007A&A...472L..13G. doi:10.1051/0004-6361:20077799.
Paul Gilster (2007-05-16). "Transiting 'Hot Neptune' Found". Centauri Dreams. A discussion of the "Detection of transits of the nearby hot Neptune GJ 436 b" paper.

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[1] Dong; et al. (23 June 2017). "LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements". Proceedings of the National Academy of Sciences. 115 (2): 266–271. arXiv:1706.07807 . doi:10.1073/pnas.1711406115. PMC 5777037 . PMID 29284755.

[2] G. Wuchterl. "Hot Neptunes: A Key To Giant Planet Formation" (PDF). cosis.net. Diakses tanggal 3 August 2015.

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Neptunus panas

Referensi

Sumber

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