He The James Webb Space Telescope of Pot captured the sharpest infrared images to date of an extended section of Horsehead NebulaReveals unprecedented detail of this iconic celestial object.

NASA explains Nebula Like a huge cloud of dust and gas in space. Some nebulae come from gas and dust ejected by the explosion of a dying star, such as a supernova. Other nebulae are regions where new stars begin to form.

Observations centered on the upper part of the nebula's “man,” revealed the complexity of this region with unprecedented spatial resolutionAccording to a study published this Tuesday, April 30, 2024 Astronomy & Astrophysics.

The Horsehead NebulaAlso known as Barnard 33Located approximately 1,300 light-years away in the galaxy Orionwithin a dense region called a molecular cloud Orion b.

According to the US space agency, the nebula formed from a collapsed interstellar cloud, illuminated by a nearby hot star. Although surrounded by gas clouds Horsehead Nebula Already deformed, the protruding pillar is made of thicker material, which is more resistant to corrosion. Astronomers estimate that the nebula is approx Five million years ago it would have disintegrated.

The Horsehead Nebula is a Photosynthetic Area (PDR)Ultraviolet (UV) light from young, massive stars creates a region of mostly neutral, hot gas and dust between the fully ionized gas surrounding massive stars and the clouds from which they were born.

tools MIRI And NIRCam of the telescope James Webb The illumination revealed the small-scale structures of the shore in detail of Nebula. According to the scientists, as UV light vaporizes the dust cloud, the dust particles are pulled from the cloud and carried along with the hot gas.

This phenomenon gives astronomers a deeper understanding of how dust blocks and emits light, the nebula's multidimensional shape.

Studying this data is critical to understanding how radiation interacts with interstellar matter.. Based on its proximity and its almost edge-to-edge geometry, the Horsehead Nebula Provides a better scope for analyzing physical structures PDR and the molecular evolution of gas and dust within their environments, as well as the transition regions between them. It is considered one of the best areas of the sky to study these interactions.

Soon, astronomers will focus on analyzing the collected spectroscopic data Obtaining information on the evolution of physical and chemical properties An object observed through a nebula.

It is true web It has discovered a network of microscopic features that trace the movement of dust and hot gas, opening up new ways of understanding the early universe and the key role UV radiation plays in star formation.

Light emitted by PDR It provides a unique tool to study the physical and chemical processes that drive the evolution of galaxies in our galaxy and throughout the Universe, from the earliest times of intense star formation to the present.