JWST zooms in on Horsehead Nebula’s mane
The James Webb Space Telescope (JWST) has captured the sharpest infrared images to date of a zoomed-in portion of the iconic Horsehead Nebula. These observations offer an unprecedented view of the “mane” or edge of this renowned nebula, revealing its intricate complexity with remarkable spatial resolution.
The new images unveil a region within the constellation Orion, specifically the Orion B molecular cloud’s dense western area. Here, the Horsehead Nebula, also known as Barnard 33, rises majestically from turbulent waves of dust and gas, approximately 1,300 light-years from Earth.
The Horsehead Nebula formed from a collapsing interstellar cloud of material and glows due to the illumination of a nearby hot star. While the surrounding gas clouds have dissipated, the jutting pillar remains composed of thick clumps of material, making it more resistant to erosion. Astronomers estimate that the Horsehead has approximately five million years left before it too disintegrates. Webb’s new view zooms in on the illuminated edge of the top of this distinctive dust and gas structure.
The image showcases three perspectives of the Horsehead Nebula:
- The left image, released in November 2023, features the Horsehead Nebula as seen in visible light by the Euclid telescope.
- The middle image shows the Horsehead Nebula in near-infrared light from the Hubble Space Telescope, featured as the telescope’s 23rd anniversary image in 2013.
- The right image unveils the new view of the Horsehead Nebula from JWST.
The Horsehead Nebula is a renowned photodissociation region (PDR), where ultraviolet (UV) radiation from massive, young stars creates a mostly neutral, warm area of gas and dust. This region lies between the fully ionized gas surrounding the massive stars and the clouds from which they were born. The UV radiation profoundly influences the chemistry of these regions and serves as a significant source of heat.
PDRs occur where interstellar gas is dense enough to remain largely neutral, yet not too dense to prevent the penetration of UV light from massive stars. The light emitted from such PDRs provides a unique tool to study the physical and chemical processes that drive the evolution of interstellar matter in our galaxy and throughout the universe, from the early era of vigorous star formation to the present day.
Due to its proximity and nearly edge-on geometry, the Horsehead Nebula is an ideal target for astronomers to investigate the physical structures of PDRs and the molecular evolution of gas and dust within their respective environments, as well as the transition regions between them. It is considered one of the best regions in the sky to study how radiation interacts with interstellar matter.
Thanks to JWST’s MIRI (Mid-Infrared Instrument) and NIRCam (Near-Infrared Camera) instruments, an international team of astronomers has revealed, for the first time, the small-scale structures of the illuminated edge of the Horsehead. As UV light evaporates the dust cloud, dust particles are swept away, carried with the heated gas. Webb has detected a network of thin features tracing this movement. The observations have also allowed astronomers to investigate how the dust blocks and emits light, and to better understand the multidimensional shape of the nebula.
Next, astronomers intend to study the spectroscopic data obtained to gain insights into the evolution of the physical and chemical properties of the material observed across the nebula.
