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> M57 (NGC 6720) planetary nebula in Lyra

M57 (NGC 6720) planetary nebula in Lyra

author: ESA/NASA/CSA/Novapix

reference: a-nep67-20012

Image Size 300 DPI: 34 * 35 cm

The NASA/ESA/CSA James Webb Space Telescope has observed the well-known Ring Nebula with unprecedented detail. Formed by a star throwing off its outer layers as it runs out of fuel, the Ring Nebula is an archetypal planetary nebula. Also known as M57 and NGC 6720, it is both relatively close to Earth at roughly 2,500 light-years away. This new image provides unprecedented spatial resolution and spectral sensitivity. For example, the intricate details of the filament structure of the inner ring are particularly visible in this dataset. There are some 20,000 dense globules in the nebula, which are rich in molecular hydrogen. In contrast, the inner region shows very hot gas. The main shell contains a thin ring of enhanced emission fromcarbon-based molecules known as polycyclic aromatic hydrocarbons (PAHs). Roughly ten concentric arcs are located just beyond the outer edge of the main ring. The arcs are thought to originate from the interaction of the central star with a low-mass companion orbiting at a distance comparable to that between the Earth and the dwarf planet Pluto. In this way, nebulae like the Ring Nebula reveal a kind of astronomical archaeology, as astronomers study the nebula to learn about the star that created it.

Keywords for this photo:

2023 - ASTRONOMY - DWARF - EVOLUTION - JAMES WEBB SPACE TELESCOPE - JWST - LYRA - M57 - NEBULA - NGC 6720 - PLANETARY NEBULA - STAR - WHITE DWARF -