Quartz crystals detected swirling in atmosphere of exoplanet WASP-17b

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Astronomers utilizing the James Webb Area Telescope have for the primary time detected tiny quartz crystals containing silica — a standard mineral on Earth — inside the ambiance of a blazing scorching exoplanet.

It’s possible that the nanoparticles of silica, which on Earth seems in seaside sands and is used to provide glass, swirl from the clouds of the exoplanet, often called WASP-17b, in accordance with the researchers.

First found in 2009, WASP-17b is a fuel large planet situated 1,300 light-years from Earth. It has a quantity greater than seven occasions that of Jupiter, making it one of many largest exoplanets identified to astronomers.

This artist's concept shows what the exoplanet WASP-17 b could look like.

WASP-17 b, also called Ditsö̀, is a hot gas giant that orbits its star at a distance of just 0.051 AU (about 4.75 million miles, or one-eighth the distance between Mercury and the Sun), completing one full circuit in about 3.7 Earth-days. The system lies within the Milky Way, about 1,300 light-years from Earth, in the constellation Scorpius.

With a volume more than seven times that of Jupiter and a mass less than one-half of Jupiter, WASP-17 b is an extremely puffy planet. Its short orbital period, large size, and thick, extended atmosphere make it ideal for observation using transmission spectroscopy, which involves measuring the effects of the planet's atmosphere on the starlight filtering through it.

WASP-17 b's atmosphere is composed primarily of hydrogen and helium, along with small amounts of water vapor and hints of carbon dioxide and other molecules. Observations of 5- to 12-micron infrared light from Webb's MIRI (Mid-Infrared Instrument) show that WASP-17 b's atmosphere also contains clouds made of nanocrystals of quartz (SiO2).

WASP-17 b is tidally locked and has a retrograde orbit. Its temperature ranges from about 1,000 kelvins (1,350 degrees F or 725 degrees C) on the cooler nightside to nearly 2,000 kelvins (3,150 degrees F or 1,725 degrees C) on the side in permanent daylight.

The star, WASP-17 (also called Diwö), is an F-type star: slightly larger, more massive, hotter, and whiter than the Sun.

This artist's concept is based on new data gathered by MIRI as well as previous observations from other ground- and space-based telescopes, including NASA's Hubble and retired Spitzer space telescopes. Webb has not captured any images of the planet.

The researchers detected the the quartz nanoparticles in high-altitude clouds utilizing Webb’s Mid-Infrared Instrument, in accordance with new analysis printed Monday in The Astrophysical Journal Letters.

“We had been thrilled,” stated lead research creator David Grant, a researcher on the College of Bristol, in a press release. “We knew from Hubble observations that there have to be aerosols — tiny particles making up clouds or haze — in WASP-17 b’s ambiance, however we didn’t anticipate them to be product of quartz.”

Minerals wealthy in silicon and oxygen, referred to as silicates, are plentiful on Earth, the moon and different rocky our bodies within the photo voltaic system. Silicates are additionally extremely widespread within the Milky Method galaxy. However up to now, the silicate grains detected in exoplanet atmospheres have been magnesium-based, not quartz, which is product of pure silica.

“We totally anticipated to see magnesium silicates,” stated research coauthor Hannah Wakeford, senior lecturer in astrophysics at College of Bristol, in a press release.
“However what we’re seeing as a substitute are possible the constructing blocks of these, the tiny ‘seed’ particles wanted to kind the bigger silicate grains we detect in cooler exoplanets and brown dwarfs.”

The discovering might allow researchers to grasp the supplies used to kind planetary environments a lot totally different from what we all know on Earth.

Wasp-17b takes 3.7 Earth days to finish one orbit round its star. Astronomers targeted their observations on the exoplanet because it crossed in entrance of its star and starlight filtered via its ambiance.

After 10 hours of remark time, the workforce found a signature suggesting the presence of quartz nanoparticles.

The quartz crystals are possible hexagonal in form, just like the a lot bigger geodes we all know on Earth, however each is simply one-millionth of a centimeter — so small that 10,000 of the grains might match aspect by aspect throughout a human hair, in accordance with the analysis. And the particles originate within the ambiance.

A transmission spectrum of the hot gas giant exoplanet WASP-17 b captured by MIRI (Webb's Mid-Infrared Instrument) on March 12-13, 2023, reveals the first evidence for quartz (crystalline silica, SiO2) in the clouds of an exoplanet.

The spectrum was made by measuring the change in brightness of 28 wavelength-bands of mid-infrared light as the planet transited its star. Webb observed the WASP-17 system using MIRI's low-resolution spectrograph for nearly 10 hours, collecting more than 1,275 measurements before, during, and after the transit.

For each wavelength, the amount of light blocked by the planet's atmosphere (white circles) was calculated by subtracting the amount that made it through the atmosphere from the amount originally emitted by the star.

The solid purple line is a best-fit model to the Webb (MIRI), Hubble, and Spitzer data. (The Hubble and Spitzer data cover wavelengths from 0.34 to 4.5 microns and are not shown on the graph.) The spectrum shows a clear feature around 8.6 microns, which astronomers think is caused by silica particles absorbing some of the starlight passing through the atmosphere.  

The dashed yellow line shows what that part of the transmission spectrum would look like if the clouds in WASP-17 b's atmosphere did not contain SiO2.

This marks the first time that SiO2 has been identified in an exoplanet, and the first time any specific cloud species has been identified in a transiting exoplanet.

“WASP-17 b is extraordinarily scorching — round 2,700 levels Fahrenheit (1,500 levels Celsius) — and the stress the place the quartz crystals kind excessive within the ambiance is simply about one-thousandth of what we expertise on Earth’s floor,” Grant stated. “In these situations, strong crystals can kind straight from fuel, with out going via a liquid section first.”

The planet is tidally locked to its star, that means one aspect at all times faces the star and experiences searing temperatures, whereas the everlasting “evening” aspect of the planet is cooler. Whereas the clouds can drift across the planet, they possible vaporize on the recent day aspect, which might ship the quartz particles swirling.

“The winds may very well be shifting these tiny glassy particles round at 1000’s of miles per hour,” Grant stated.

Webb’s delicate detections are permitting researchers to have a greater understanding of the atmospheres, environmental situations and climate on planets outdoors of our photo voltaic system.

Sizzling fuel giants, additionally referred to as Sizzling Jupiters, like WASP-17b are largely composed of hydrogen and helium, together with some water vapor and carbon dioxide. Detecting silica within the planet’s ambiance helps scientists to have a broader sense of WASP-17b’s composition.

“If we solely think about the oxygen that’s in these gases, and neglect to incorporate the entire oxygen locked up in minerals like quartz, we’ll considerably underestimate the overall abundance,” Wakeford stated. “These stunning silica crystals inform us in regards to the stock of various supplies and the way all of them come collectively to form the surroundings of this planet.”

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