Rocky Planets Can Form in Extreme Environments

Image: Protoplanetary Disk (Artist Concept)
Composed by the FreeAstroScience.com team, this blog post delves into the remarkable exploration of a planetary formation disk by an international consortium of astronomers utilizing the James Webb Space Telescope. The primary mission was to hunt for water molecules and other constituents within one of the galaxy's most intense environments.



This research is part of the James Webb Space Telescope eXtreme Ultraviolet Environments (XUE) program, which concentrates on studying these colossal, spinning clouds made up of gas, dust, and rock fragments—the birthplaces of planets. Comprehending the influence of the stellar environment on planetary genesis is an essential step for scientists in understanding the exoplanets' diversity.


The team ventured into examining the Lobster Nebula's physical attributes and chemical makeup using Webb's MIRI spectrometer. This exploration centered on the protoplanetary disk XUE 1, nestled in the Pismis 24 star cluster. Given its proximity to several massive stars, scientists anticipated that XUE 1 was subjected to high doses of ultraviolet radiation. Interestingly, despite such harsh conditions, the researchers succeeded in detecting several molecules that constitute the foundation of rocky planets.


Image: XUE 1 spectrum detects water


Lars Cuijpers of Radboud University, expressing the team's astonishment and excitement, stated, "This is the first time these molecules have been detected in these extreme conditions." In addition, the team discovered traces of silicate dust on the disk's surface, a crucial component in the formation of rocky planets, solidifying the importance of this extraordinary discovery.


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