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Atmosfer Jupiter

Atmosfer Jupiter

330px-Jupiter_Belt_System.svg.png?utm_source=id.wikipedia.org&utm_campaign=parser&utm_content=thumbnail — Pola awan di Jupiter tahun 2000

Atmosfer Jupiter adalah atmosfer keplanetan terbesar dalam Tata Surya. Atmosfernya sebagian besar terbentuk dari hidrogen molekuler dan helium dalam proporsi solar yang lebih kurang sama; 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 Jupiter 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]

Referensi

Sumber kutipan

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Pranala luar

Media terkait Atmosphere of Jupiter di Wikimedia Commons

Basis data pengawasan otoritas
Nasional	Amerika Serikat Israel
Lain-lain	Yale LUX

Konten disalin dari Wikipedia Bahasa Indonesia (lisensi CC BY-SA) Lihat versi asli di Wikipedia

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