Astronomers Have Found a Naked Hot Jupiter Steaming Up The Neighbourhood


Ever marvel what Jupiter would seem like bare, with out its thick coat of turbulent clouds? An exoplanet 575 light-years away is likely to be the reply to the query you did not ask.


The exoplanet is a fuel large known as WASP-62b, and, in response to an evaluation of starlight that handed by its ambiance, the exoplanet is totally starkers. There’s not even a whisper of cloud or haze.

Instead, the ambiance is totally clear – one thing that isn’t solely nearly vanishingly uncommon in exoplanets, however provides us a distinctive alternative to see inside and see what the ambiance is made from.

“I’ll admit that at first I wasn’t too excited about this planet,” stated astronomer Munazza Alam of the Harvard & Smithsonian Center for Astrophysics, who has been working to characterise the atmospheres of confirmed exoplanets. “But once I started to take a look at the data, I got excited.”

When it was found in 2012 (and in follow-up research) WASP-62b appeared to be fairly par for the exoplanet course. It’s about 1.4 occasions the dimensions and 0.57 occasions the mass of Jupiter, orbiting a younger yellow-white dwarf star a little larger than the Sun, known as WASP-62.

It’s additionally, as with most confirmed exoplanets, on a pretty shut orbit, though WASP-62b is nearer to its star than many exoplanets – its orbital interval is simply 4.41 days. This means this can be very scorching, with a mean temperature of round 1,330 Kelvin, subsequently falling into the class of “scorching Jupiter“.


At these temperatures, WASP-62b is greater than seemingly evaporating, like a puddle on a scorching day (however far more slowly).

Because it is comparatively near Earth, and since it passes between us and its star on such a quick interval, WASP-62b was a good candidate for attempting to characterise its ambiance. That’s as a result of when an exoplanet passes in entrance of its star, the starlight adjustments, as some wavelengths of the incoming gentle are absorbed by atoms within the ambiance.

Different chemical components take up completely different wavelengths, so this spectral info can be utilized to see what the exoplanet’s gaseous envelope is made from.

When Alam and her workforce took a take a look at the spectra from three transits of WASP-62b, they discovered one thing actually uncommon: a full set of absorption traces from sodium. In most exoplanet atmospheres, the sodium signature is often partially or absolutely obscured by clouds or haze.

The robust sodium signature from WASP-62b additionally has a very broad base, brought on by one thing known as stress broadening. This might solely occur deep within the exoplanet’s ambiance, at greater pressures. For the sign to be rising so clearly from so deep contained in the ambiance means that there aren’t any clouds to forestall its emergence.


“This is smoking gun evidence that we are seeing a clear atmosphere,” Alam stated.

That makes WASP-62b a very uncommon beast certainly – lower than seven % of the exoplanets found thus far are anticipated to have a clear ambiance. And just one different has been recognized – WASP-96b, a scorching Saturn 1,160 light-years away.

Not solely is WASP-62b nearer and greater, it’s excellently positioned for follow-up research. It falls in a area that may be repeatedly noticed by the James Webb Space Telescope (JWST), known as the Continuous Viewing Zone. This makes it the one fuel large exoplanet, and the one exoplanet with a clear ambiance, on this area. It is subsequently a superb candidate for follow-up remark when the telescope lastly begins operations.

So what’s inside that ambiance? According to the information and simulations, the workforce count on that the JWST would have the ability to detect water, iron hydride, ammonia, carbon monoxide and dioxide, methane, and silylydine, all along with sodium.

Clearly figuring out these ought to reveal each the metallicity and the carbon-to-oxygen ratio inside WASP-62b’s ambiance. The carbon-to-oxygen ratio is especially thrilling – it may be used to understand situations inside the planet-forming disc when the planet was being born, and assist us higher perceive planetary formation processes.

“WASP-62 is the only star in the JWST CVZ with a known transiting giant planet that is bright enough for high-quality atmospheric characterisation via transit spectroscopy. JWST transit programs require many repeated visits, which ideally could be scheduled at any time of the year and executed quickly,” the researchers wrote of their paper.

“WASP-62b is therefore one of the most readily accessible targets for atmospheric studies with JWST.”

The analysis has been revealed in The Astrophysical Journal Letters.


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