Protostars HOPS 150 and HOPS 153 reshape their surroundings
Jets from HOPS 153 influence star formation in the nebula
Discover Hubble's breathtaking glimpse of the Orion Nebula and its emerging protostars
Photo Credit: ESA/Hubble/ NASA/ T. Megeath
The Hubble Space Telescope has captured an extraordinary view of the Orion Nebula, the closest star-forming region to Earth, located approximately 1,500 light-years away. This new image highlights protostars HOPS 150 and HOPS 153, which are playing a significant role in reshaping their surrounding environment. The nebula, visible to the naked eye near the constellation Orion's belt, is illuminated by the activities of these young stars, offering scientists a glimpse into the earliest stages of star formation.
Protostars and Their Evolution
According to the Herschel Orion Protostar Survey, conducted using ESA's Herschel Space Observatory, HOPS 150 is a binary star system comprising two young stars encircled by dusty disks. These protostars are still accumulating material from their surroundings, with a massive cloud of gas and dust extending over 2,000 times the distance between Earth and the Sun feeding their growth. As reported by NASA, observations of the emitted infrared light suggest that HOPS 150 is midway through its evolution into a mature star system.
Jets from HOPS 153 Transforming the Nebula
The narrow jet seen in the image originates from HOPS 153, another protostar situated nearby but still embedded in dense gas. Though HOPS 153 remains obscured by its birth nebula, the jet's impact on the surrounding material is clearly visible. This jet carves out regions in the interstellar medium, releasing energy and creating disturbances that may influence the formation of nearby stars. The interactions between the gas inflows and outflows are crucial for understanding how young stars shape their environments.
The findings, supported by data from NASA and ESA, provide insights into how protostars transition into fully developed stars, altering their surroundings and impacting the interstellar medium. These processes hold vital clues about the dynamics of star formation in our galaxy.
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