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DescriçãoThe Twin Jet Nebula.jpg
English: The Twin Jet Nebula, or PN M2-9, is a striking example of a bipolar planetary nebula. Bipolar planetary nebulae are formed when the central object is not a single star, but a binary system, Studies have shown that the nebula’s size increases with time, and measurements of this rate of increase suggest that the stellar outburst that formed the lobes occurred just 1200 years ago.
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Data e hora de geração de dados
15h00min de 26 de agosto de 2015
Software utilizado
Adobe Photoshop CC 2014 (Windows)
Identificação exclusiva do documento original
xmp.did:90ad1b20-5796-aa42-8fdd-2c2450adb3f0
Atribuição/Fornecedor
ESA/Hubble & NASA Acknowledgement: Judy Schmidt
Fonte
ESA/Hubble
Título curto
The Twin Jet Nebula
Título
The Twin Jet Nebula, or PN M2-9, is a striking example of a bipolar planetary nebula. Bipolar planetary nebulae are formed when the central object is not a single star, but a binary system, Studies have shown that the nebula’s size increases with time, and measurements of this rate of increase suggest that the stellar outburst that formed the lobes occurred just 1200 years ago.