Catching the first “space wind” by James Webb. The James Webb Space Telescope has captured the first image of winds coming from a planet-forming disk around a young star.
Catching the first “space wind” by James Webb
Planet formation is a complex and long process, and scientists have been trying to understand the many underlying processes that govern the formation of planets, and now a new generation of space telescopes called James Webb has come to their aid.
The James Webb Space Telescope has captured the first image of winds coming from a relatively old planet-forming disk.
Researchers from the University of Arizona and the Search for Extraterrestrial Intelligence Institute (SETI) used the James Webb Space Telescope to study the disk surrounding the young star TCha.
Dispersed Gas
The star TCha is a relatively young star compared to our magnificent Sun. This star is located in an erosion disk with a large dust gap with a radius of about 30 AU.
This disk is actively dispersing its gas content, or in other words, producing a wind. Now this scattering gas is imaged with the help of four lines of noble gases neon (Ne) and argon (Ar).
The neon line was first observed in 2007 using the Spitzer Space Telescope, and experts identified this line as an indicator of winds.
In this new study, the researchers found the reason for the formation of these scattered gas winds.
These winds could be driven by energetic stellar photons (starlight) or the magnetic field that surrounds the planet’s forming disk, says study leader Naman Bajaj of the University of Arizona.
Researchers say that this finding can expand their understanding of the formation of planets.
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Insights into planet formation
“Knowing when the gas dissipates is important because it limits the time left for young planets to consume gas from their surroundings,” the researchers said in a press release.
Additionally, these findings could provide insights into the underlying process that led to the evolution of planets in our solar system.
Our solar system consists of rocky and gaseous planets. Its inner planets, Mercury, Venus, Earth, and Mars, are all stone. At the same time, its four outer planets, Jupiter, Saturn, Uranus, and Neptune, are all gas giants.
However, it has been hypothesized that the initial mass in planet-forming discs is mostly gaseous.
This raises a perplexing question. When and how does this gas disperse and how does it affect the result of planet formation?
The implications of these findings provide new insight into the complex interactions that lead to the dispersal of gas and dust critical to planet formation.
The researchers’ press release explains that by understanding the mechanisms behind disc fragmentation, scientists can better predict the timing and environments favorable for the birth of planets.
The researchers also performed simulations to better understand the scattering caused by stellar photons, and these simulations were compared to real data.
Simulations confirmed that this finding is explained by scattering from high-energy stellar photons.
Measurements of all four noble gas lines by James Webb also provided insights into the amount of gas dispersed.
These findings have been published in the Astronomical Journal.