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NASA Webb’s NIRCam and MIRI reveal new details of the Crab Nebula in infrared light.

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20231102 074259 InfinityCosmos
The James Webb Space Telescope, a remarkable observatory, has recently observed the Crab Nebula, a supernova remnant situated 6,500 light-years away in the Taurus constellation. This celestial event was originally documented in 1054 CE by astronomers from the 11th century. Since then, the Crab Nebula has remained a subject of significant interest and continued scrutiny by scientists who aim to comprehend the conditions, behavior, and consequences of supernovae. It serves as a relatively nearby and essential example for studying these phenomena.
The image captured by the James Webb Space Telescope’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument) reveals new details in infrared light. The supernova remnant is composed of various components, each depicted in distinct colors: doubly ionized sulfur in red-orange, ionized iron in blue, dust in yellow-white and green, and synchrotron emission in white. These colors correspond to different filters used by Webb’s NIRCam and MIRI.
A team led by Tea Temim at Princeton University is utilizing Webb’s NIRCam and MIRI to investigate the Crab Nebula’s origins. They are leveraging the sensitivity and spatial resolution of the James Webb Space Telescope to accurately determine the composition of the ejected material, with a particular focus on iron and nickel content. This investigation may shed light on the type of explosion that gave rise to the Crab Nebula and offer insights into the fascinating world of supernovae.

Crab Nebula captured by Hubble and Webb’s NIRCam and MIRI.

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This side-by-side comparison of the Crab Nebula, as observed by the Hubble Space Telescope in optical light on the left and the James Webb Space Telescope in infrared light on the right, provides valuable insights into this mysterious supernova remnant. By examining the recent data collected by Webb and comparing it to previous observations from telescopes like Hubble, astronomers can construct a more comprehensive understanding of the Crab Nebula.
In this comparison, the general shape of the supernova remnant remains similar to what was seen in the optical wavelength image captured by Hubble in 2005. However, Webb’s infrared observation reveals new details. It shows a distinct, cage-like structure of gaseous filaments in red-orange. Additionally, Webb maps out the emission from dust grains in the central regions, represented in yellow-white and green, for the first time.
The James Webb Space Telescope’s infrared view offers a closer look at various aspects of the Crab Nebula. Notably, it highlights synchrotron radiation, which is produced by charged particles, such as electrons, moving at relativistic speeds along magnetic field lines. This radiation appears as milky, smoke-like material throughout much of the Crab Nebula’s interior.
It’s a product of the nebula’s pulsar, a rapidly rotating neutron star with a strong magnetic field that accelerates particles to high speeds, causing them to emit radiation as they spiral along magnetic field lines. Although this radiation is emitted across the electromagnetic spectrum, Webb’s NIRCam instrument provides an unprecedented level of detail in capturing the synchrotron radiation within the Crab Nebula.

Crab Nebula studied by Webb.

To pinpoint the location of the Crab Nebula’s pulsar at its core, you can follow a set of wispy structures that form a circular ripple-like pattern within the central region. These wisps lead to the bright white dot in the very center of the nebula. Moving outward from the core, you’ll notice thin white ribbons of radiation. The curvy wisps are closely clustered, outlining the structure of the pulsar’s magnetic field, which plays a significant role in shaping and sculpting the overall appearance of the nebula.

At the center-left and center-right of the image, the white material curves sharply inward from the edges of the filamentary dust cage and converges towards the location of the neutron star at the heart of the nebula. This narrowing of the nebula’s waist may be the result of the confinement of the expansion of the supernova wind by a belt of dense gas.
The wind generated by the pulsar heart continues to exert pressure, pushing the surrounding shell of gas and dust outward at a rapid pace. Within the interior of the remnant, you can observe yellow-white and green mottled filaments forming large-scale loop-like structures, indicating areas where dust grains are concentrated.
Astronomers are actively seeking answers about the Crab Nebula’s history and characteristics by closely analyzing the data collected by the James Webb Space Telescope. They are also comparing these findings with previous observations from other telescopes, such as the Hubble Space Telescope. In the coming year, astronomers will have access to newer Hubble data, marking its first observations of the Crab Nebula in over two decades. These fresh observations will help astronomers make more precise comparisons between the data gathered by the James Webb Space Telescope and the Hubble, advancing our understanding of this fascinating celestial object.
NASA Webb’s NIRCam and MIRI reveal new details of the Crab Nebula in infrared light.

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