NIS FINAL 9: pagamentos do Bolsa Família começam nesta quarta-feira (30)
A CAIXA inicia nesta quarta-feira (30) o pagamento do Bolsa Família referente ao mês de julho para os beneficiários com o Número de Identificação Social (NIS) terminado em 9.
O pagamento é realizado preferencialmente na Poupança CAIXA ou Poupança no CAIXA Tem.
Com o CAIXA Tem, os beneficiários podem pagar contas e fazer transferências diretamente pelo aplicativo no celular.
O benefício também pode ser movimentado com o cartão de débito da conta em comércios, Unidades Lotéricas, Correspondentes CAIXA Aqui, terminais de autoatendimento e Agências da CAIXA. Além disso, é possível realizar saques sem cartão nos terminais de autoatendimento e Unidades Lotéricas, utilizando a identificação biométrica previamente cadastrada em uma agência da CAIXA.
No aplicativo Bolsa Família é possível acompanhar as informações do benefício, além de receber atualizações e novidades sobre o Programa.
Para baixar os aplicativos CAIXA Tem e Bolsa Família, basta acessar a loja de aplicativos do seu smartphone. É gratuito.
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This image set showcases three views of the Butterfly Nebula, also called NGC 6302. The Butterfly Nebula, located about 3400 light-years away in the constellation Scorpius, is one of the best-studied planetary nebulae in our galaxy. Planetary nebulae are among the most beautiful and most elusive creatures in the cosmic zoo. These nebulae form when stars with masses between about 0.8 and 8 times the mass of the Sun shed most of their mass at the end of their lives. The planetary nebula phase is fleeting, lasting only about 20 000 years. The Butterfly Nebula is a bipolar nebula, meaning that it has two lobes that spread in opposite directions, forming the ‘wings’ of the butterfly. A dark band of dusty gas poses as the butterfly’s ‘body’. This band is actually a doughnut-shaped torus that’s being viewed from the side, hiding the nebula’s central star - the ancient core of a Sun-like star that energises the nebula and causes it to glow. The dusty doughnut may be responsible for the nebula’s insectoid shape by preventing gas from flowing outward from the star equally in all directions. The first and second of the three images shown here highlight the bipolar nature of the Butterfly Nebula in optical and near-infrared light captured by the NASA/ESA Hubble Space Telescope. The new Webb image on the right zooms in on the centre of the Butterfly Nebula and its dusty torus, providing an unprecedented view of its complex structure. The Webb data are supplemented with data from the Atacama Large Millimetre/submillimetre Array, a powerful network of radio dishes. While the nebula’s central star is blanketed with thick, dusty gas at optical wavelengths, Webb’s infrared capabilities reveal the central star and show the doughnut-shaped torus and interconnected bubbles of dusty gas that surround it. [Image description: Three views of the same nebula, presented side by side. The left and middle images, which are labeled ‘Hubble Optical’ and ‘Hubble Near
