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Revisi per 23 Maret 2017 15.22

Atmosfer Yupiter adalah atmosfer keplanetan terbesar dalam Tata Surya. Atmosfernya sebagian besar terbentuk dari hidrogen molekuler dan helium dalam proporsi solar secara kasar; senyawa kimia lainnya hanya ada dalam jumlah kecil dan meliputi metana, amonia, hidrogen sulfida, dan air. Meskipun air diduga berada jauh di dalam atmosfer, konsentrasi terukur langsungnya sangat rendah. Nitrogen, sulfur, dan gas mulia melimpah dalam atmosfer Yupiter melebihi nilai solar yang disebabkan oleh sekitar tiga faktor.^[1]

Atmosfer Jupiter tidak memiliki batas bawah yang jelas dan secara bertahap bertransisi menjadi bagian dalam planet yang cair.^[2] Dari yang terendah sampai tertinggi, lapisan atmosfer adalah troposfer, stratosfer, termosfer, dan eksosfer. Setiap lapisan memiliki karakteristik gradien suhu.^[3] Lapisan terendah, troposfer, memiliki sistem awan dan kabut yang rumit, yang terdiri dari lapisan amonia, amonium hidrosulfida, dan air.^[4]

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Pranala luar

Media tentang Atmosphere of Jupiter di Wikimedia Commons

[FOOTNOTEAtreya_Mahaffy_Niemann_et_al.2003-1] Atreya Mahaffy Niemann et al. 2003.

[Guillot1999-2] Guillot (1999)

[Sieff1998-3] Sieff et al. (1998)

[FOOTNOTEAtreyaWong2005-4] Atreya & Wong 2005.

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@@ Baris 1: / Baris 1: @@
 [[Berkas:Jupiter Belt System.svg|thumb|300px|Pola awan di Yupiter tahun 2000]]
-'''Atmosfer [[Yupiter]]''' adalah [[atmosfer keplanetan]] terbesar dalam [[Tata Surya]]. Atmosfernya sebagian besar terbentuk dari [[hidrogen molekuler]] dan [[helium]] dalam [[Matahari#Komposisi|proporsi solar]] secara kasar; senyawa kimia lainnya hanya ada dalam jumlah kecil dan meliputi [[metana]], [[amonia]], [[hidrogen sulfida]], dan [[air]]. Meskipun air diduga berada jauh di dalam atmosfer, konsentrasi terukur langsungnya sangat rendah. [[Nitrogen]], [[sulfur]], dan [[gas mulia]] melimpah dalam atmosfer Yupiter melebihi nilai solar yang disebabkan oleh sekitar tiga faktor.{{sfn|Atreya Mahaffy Niemann et al.|2003}}
+'''Atmosfer [[Yupiter]]''' adalah [[atmosfer benda langit|atmosfer keplanetan]] terbesar dalam [[Tata Surya]]. Atmosfernya sebagian besar terbentuk dari [[hidrogen molekuler]] dan [[helium]] dalam [[Matahari#Komposisi|proporsi solar]] secara kasar; senyawa kimia lainnya hanya ada dalam jumlah kecil dan meliputi [[metana]], [[amonia]], [[hidrogen sulfida]], dan [[air]]. Meskipun air diduga berada jauh di dalam atmosfer, konsentrasi terukur langsungnya sangat rendah. [[Nitrogen]], [[sulfur]], dan [[gas mulia]] melimpah dalam atmosfer Yupiter melebihi nilai solar yang disebabkan oleh sekitar tiga faktor.{{sfn|Atreya Mahaffy Niemann et al.|2003}}
 Atmosfer Jupiter tidak memiliki batas bawah yang jelas dan secara bertahap bertransisi menjadi bagian dalam planet yang cair.<ref name=Guillot1999>[[#Guillot|Guillot (1999)]]</ref> Dari yang terendah sampai tertinggi, lapisan atmosfer adalah [[troposfer]], [[stratosfer]], [[termosfer]], dan [[eksosfer]]. Setiap lapisan memiliki karakteristik [[gradien suhu]].<ref name=Sieff1998>[[#Sieff|Sieff ''et al.'' (1998)]]</ref> Lapisan terendah, troposfer, memiliki sistem awan dan kabut yang rumit, yang terdiri dari lapisan amonia, [[amonium hidrosulfida]], dan air.{{sfn|Atreya|Wong|2005}}