Novas imagens de Júpiter revelam características misteriosas do planeta

[{"selector":"#anim-0df6aa07-8c69-40d4-8c1b-755b065e93fe","keyframes":{"transform":["translate3d(-108.92857%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-186d527a-bab2-4fc5-bd42-30c0910f582d","keyframes":{"opacity":[0,1]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.4, 0.4, 0.0, 1)","fill":"both"}] [{"selector":"#anim-b643a646-db61-4b72-ba4d-365ccf4d7452 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-47.67045422792089%, 0, 0)","translate3d(0%, 0, 0)"]},"delay":0,"duration":1000,"fill":"both"}] O MAIOR PLANETA AURA/NSF/NOIRLAB/ESA/NASA/INTERNATIONAL GEMINI OBSERVATORY Novas imagens de Júpiter revelam características misteriosas do planeta

[{"selector":"#anim-7d859474-f1e1-41a9-8a20-cc16671531bc","keyframes":{"transform":["translate3d(-83.59621%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":2500,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-cd9961c4-1477-48bb-aa3c-aacc5e293857","keyframes":{"transform":["translate3d(0px, -149.08076%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] Imagens capturadas por dois telescópios diferentes mostram o maior planeta do nosso sistema solar sob uma nova luz Giphy

[{"selector":"#anim-c037af6f-51aa-4997-9338-b91b788bd3cb","keyframes":{"opacity":[0,1]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.4, 0.4, 0.0, 1)","fill":"both"}] [{"selector":"#anim-3249b3b0-63d0-460f-b5a6-8ce87d7cf4f3","keyframes":{"opacity":[0,1]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.4, 0.4, 0.0, 1)","fill":"both"}] [{"selector":"#anim-80df1589-abc2-4ec5-9ffd-53766b5cde5f [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(0, 12.121212121212123%, 0)","translate3d(0, 0%, 0)"]},"delay":0,"duration":1000,"fill":"both"}] O telescópio Gemini North, no Havaí, e o Telescópio Espacial Hubble capturaram Júpiter em luz visível, infravermelha e ultravioleta, revelando características atmosféricas impressionantes em detalhes AURA/NSF/NOIRLAB/ESA/NASA/INTERNATIONAL GEMINI OBSERVATORY

[{"selector":"#anim-0b543464-ec46-4309-930e-1ad07d1634d5","keyframes":[{"offset":0,"transform":"translate3d(0, -256.27499%, 0)","easing":"cubic-bezier(.5, 0, 1, 1)"},{"offset":0.29,"transform":"translate3d(0, 0%, 0)","easing":"cubic-bezier(0, 0, .5, 1)"},{"offset":0.45,"transform":"translate3d(0, -72.064527188%, 0)","easing":"cubic-bezier(.5, 0, 1, 1)"},{"offset":0.61,"transform":"translate3d(0, 0%, 0)","easing":"cubic-bezier(0, 0, .5, 1)"},{"offset":0.71,"transform":"translate3d(0, -24.499889044%, 0)","easing":"cubic-bezier(.5, 0, 1, 1)"},{"offset":0.8,"transform":"translate3d(0, 0%, 0)","easing":"cubic-bezier(0, 0, .5, 1)"},{"offset":0.85,"transform":"translate3d(0, -9.200272141000001%, 0)","easing":"cubic-bezier(.5, 0, 1, 1)"},{"offset":0.92,"transform":"translate3d(0, 0%, 0)","easing":"cubic-bezier(0, 0, .5, 1)"},{"offset":0.96,"transform":"translate3d(0, -3.997889844%, 0)","easing":"cubic-bezier(.5, 0, 1, 1)"},{"offset":1,"transform":"translate3d(0, 0%, 0)","easing":"cubic-bezier(0, 0, .5, 1)"}],"delay":0,"duration":1600,"fill":"both"}] [{"selector":"#anim-16f9f3a3-8c84-4b61-9d35-64a6a268b914","keyframes":{"transform":["translate3d(3999.97528%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":2000,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] As imagens foram feitas ao mesmo tempo, em 11 de janeiro de 2017, para permitir uma comparação. E em cada uma delas, Júpiter parece totalmente diferente Giphy

[{"selector":"#anim-85429239-db0e-44d9-8f18-cd5c688cf82a","keyframes":{"transform":["translate3d(90.50445%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":2500,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-6a900fff-58fc-414d-a321-fb0cb7f56617","keyframes":{"transform":["translate3d(101.33334%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-780d2ce0-31d6-47e6-a924-32f18d8d687b","keyframes":{"transform":["translate3d(-5449.96498%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":2000,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-61e0b2b3-0bb8-4d04-92fc-3c5b1e604c3a [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-23.83522711396044%, 0, 0)","translate3d(0%, 0, 0)"]},"delay":0,"duration":1000,"fill":"both"}] Isso inclui super tempestades, ciclones massivos e, é claro, a Grande Mancha Vermelha - a tempestade de séculos na atmosfera de Júpiter, tão grande que poderia engolir a Terra AURA/NSF/NOIRLAB/ESA/NASA/INTERNATIONAL GEMINI OBSERVATORY

[{"selector":"#anim-aea0b27c-6fa3-4937-8223-54e130ac4fac","keyframes":{"opacity":[0,1]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.4, 0.4, 0.0, 1)","fill":"both"}] [{"selector":"#anim-e6ecf740-991d-46d9-a0d1-9f1e9cd67f47","keyframes":{"transform":["translate3d(-100%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":2500,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] Giphy Ter um planeta em diferentes comprimentos de onda de luz pode revelar aspectos e características que de outra forma seriam invisíveis. Compará-los permite uma maior compreensão do planeta gigante

[{"selector":"#anim-e877e5c8-4098-487c-b966-0fc1fc5915e4","keyframes":{"transform":["translate3d(0px, -108.90846%, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":2500,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-51ec1671-babc-4c80-b928-510834d099ff","keyframes":{"transform":["translate3d(104.99999%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-a88f317c-f2d8-46a7-a193-42e5585523a3","keyframes":{"transform":["translate3d(-4949.9691%, 0px, 0)","translate3d(0px, 0px, 0)"]},"delay":0,"duration":2000,"easing":"cubic-bezier(0.2, 0.6, 0.0, 1)","fill":"both"}] [{"selector":"#anim-127e4eab-6a20-4960-b64a-b3f7703158cb [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(12.470702897273686%, 0, 0)","translate3d(0%, 0, 0)"]},"delay":0,"duration":1000,"fill":"both"}] A Grande Mancha Vermelha quase desapareceu no infravermelho, mas uma região escura da tempestade parece maior do que a luz visível. Isso porque diferentes comprimentos de onda de luz mostram estruturas variadas dentro da tempestade NASA/Caltech/SwRI/MSSS/Kevin M. Gill

A combinação das imagens da tempestade em luz visível do Hubble com as observações infravermelhas do Gemini revelou que as feições escuras são buracos na camada de nuvens Giphy

[{"selector":"#anim-0d05596e-e56e-469d-a992-ef40b5da4eda","keyframes":{"opacity":[0,1]},"delay":0,"duration":3000,"easing":"cubic-bezier(0.4, 0.4, 0.0, 1)","fill":"both"}] [{"selector":"#anim-0d21e2b3-3772-4c47-b953-9f4900700c79 [data-leaf-element=\"true\"]","keyframes":{"transform":["translate3d(-2.747201137053819%, 0, 0)","translate3d(0%, 0, 0)"]},"delay":0,"duration":1000,"fill":"both"}] Leia a reportagem no site da CNN Brasil AURA/NSF/NOIRLAB/ESA/NASA/INTERNATIONAL GEMINI OBSERVATORY