First pic of asteroid belt outside our solar system released
Webb‘ Mid-Infrared Instrument (MIRI) captured the warm dust around the young star Fomalhaut and found that the dusty structures are much more complex than the asteroid and Kuiper dust belts of our solar system.
Astronomers used the powerful James Webb Space Telescope to study Fomalhaut — the first asteroid belt ever seen outside of our solar system in infrared light.
The James Webb Space Telescope is the world’s premier space science observatory. It is an international program led by NASA with its partners, ESA and the Canadian Space Agency.
Overall, there are three nested belts extending out to 23 billion km from the Fomalhaut; that’s 150 times the distance of Earth from the Sun.
The scale of the outermost belt is roughly twice the scale of our solar system’s Kuiper Belt of small bodies and cold dust beyond Neptune. The inner belts — which had never been seen before — were revealed by Webb for the first time.
The belts encircle the young hot star, which can be seen with the naked eye as the brightest star in the southern constellation, Piscis Austrinus. The dusty belts are the debris from collisions of larger bodies, analogous to asteroids and comets, and are frequently described as ‘debris disks’.
“I would describe Fomalhaut as the archetype of debris disks found elsewhere in our galaxy because it has components similar to those we have in our own planetary system,” said Andras Gaspar of the University of Arizona in Tucson, the lead author of a new paper describing these results.
“By looking at the patterns in these rings, we can actually start to make a little sketch of what a planetary system ought to look like – if we could actually take a deep enough picture to see the suspected planets,” he added.
The Hubble Space Telescope and Herschel Space Observatory, as well as the Atacama Large Millimetre/Submillimetre Array (ALMA), have previously taken sharp images of the outermost belt. However, none of them found any structural interior to it.
The inner belts have been resolved for the first time by Webb in infrared light.
Fomalhaut’s dust ring was discovered in 1983 in observations made by NASA’s Infrared Astronomical Satellite (IRAS). The ring’s existence has also been inferred from previous and longer-wavelength observations using submillimeter telescopes on Mauna Kea, Hawaii, NASA’s Spitzer Space Telescope, and Caltech’s Submillimeter Observatory.
“The belts around Fomalhaut are kind of a mystery novel: Where are the planets?” said George Rieke, another team member and US science lead for Webb’s MIRI.
“I think it’s not a very big leap to say there’s probably a really interesting planetary system around the star.”
In the paper published in the journal ‘Nature Astronomy‘, the astronomers said they didn’t expect “the more complex structure with the second intermediate belt and then the broader asteroid belt”.
[With Inputs from IANS]
PGurus is now on Telegram. Click here to join our channel and stay updated with all the latest news and views
For all the latest updates, download PGurus App.
- Durga idol vandalized at Hyderabad’s exhibition grounds, sparks outrage - October 11, 2024
- Demat accounts in India surge to 175 million as NSE active clients hit 47.9 million: Report - October 11, 2024
- PM Modi advocates for peace and cooperation at East Asia Summit - October 11, 2024
[…] Source link […]