NGC 6302 (also known as the Bug Nebula, Butterfly Nebula, or Caldwell 69) is a bipolar planetary nebula in the constellation Scorpius. The structure in the nebula is among the most complex ever seen in planetary nebulae. The spectrum of Butterfly Nebula shows that its central star is one of the hottest stars known, with a surface temperature in excess of 250,000 degrees Celsius, implying that.
Butterfly Nebula - Facts and Info About NGC 6302 This beautiful nebula is named for its resemblance to the winged insect, the "butterfly" colored with brilliant blues and clouds of purple and red. The Butterfly Nebula is among the most complex ever observed in planetary nebulae, located in the constellation of Scorpius. It has a dense disc of dust and gas surrounding it at the equator, which.
The planetary nebula NGC 6302 is one the most-studied of cosmic entities of its kind, with a familiar shape and dazzling colors that live up to its " Butterfly Nebula " nickname. But thanks to. A color rendition of NGC 6302, the Butterfly Nebula, created from black-and-white exposures taken by the Hubble Space Telescope in 2019 and 2020.
In the violet-colored regions, strong stellar winds are actively reshaping the nebular wings over the past 900 years. Butterfly Nebula images reveal colors and structures shaped by the intense heat and radiation. The Hubble Space Telescope captured an image of NGC 6302 in 2009, showcasing its complex details.
Hubble was recently retrained on NGC 6302, known as the "Butterfly Nebula," to observe it across a more complete spectrum of light, from near-ultraviolet to near-infrared, helping researchers better understand the mechanics at work in its technicolor "wings" of gas. The observations highlight a new pattern of near-infrared emission from singly ionized iron, which traces an S shape from lower. This view of the Butterfly Nebula, NGC 6302, comes from the NASA/ESA Hubble Space Telescope.
Compared to its appearance in visible light, the Butterfly Nebula looks gauzy at near-infrared wavelengths. The red colour that's most prevalent in this view shows light from hydrogen, while green and blue come from iron that has been ionised. NASA video show off the shimmering colors and remarkable complexity of the Butterfly Nebula (sometimes called the Twin Jet Nebula).
Two iridescent lobes of material stretch outwards from a central. The NASA/ESA/CSA James Webb Space Telescope has revealed new details in the core of the Butterfly Nebula, NGC 6302. From the dense, dusty torus that surrounds the star hidden at the centre of the nebula to its outflowing jets, the Webb observations reveal many new discoveries that paint a never.
The Butterfly Nebula is changing, and astronomers are puzzled as to why these changes are occurring. Observations of this planetary nebula show dramatic changes in the butterfly's 'wings' in just.