THIS Is What Astronomers Spotted In Venus’ Atmosphere: A Massive ‘Bulge’!

Group of astronomers has spotted a massive bow-shaped ‘bulge’ in Venus upper atmosphere, and they are trying to explain how it could withstand the gush of sulfuric acid clouds that are spinning faster than the planet itself.

Scientists guess that the 10,000-km structure is the result of the largest gravity wave ever seen in our solar system.


The infrared image above is showing us the massive wave stretching from Venus north to south pole. It was first spotted by Japan’s Akatsuki probe back in December.

The wave remain on the planet hot atmosphere for four days straight, even facing the powerful Venus’ 359 km/h winds.

But after four days it vanished from above the clouds.

The Akatsuki team says that all the evidence is showing us that the bulge is actually a massive gravity wave – something that occurs when a fluid material, such as a liquid, gas, or plasma, is jostled out of a position of equilibrium.

They suggest that, given the intense speed and shape of Venus’ sulphuric acid winds, the only structure that could withstand all that is a massive gravity wave – despite the fact that no one had predicted that they could grow this big

“The present study shows direct evidence of the existence of stationary gravity waves, and it further shows that such stationary gravity waves can have a very large scale – perhaps the greatest ever observed in the Solar System,” the team reports.


It is really strange how something this big can even survive Venus’ atmosphere, the planet acid clouds are moving faster than the planet itself rotates on its axis.

And as fast as those acid clouds are, the planet’s rotation is painfully slow – one day on Venus lasts longer than it takes for the planet to complete its orbit of the Sun.


First of all, gravity wave and gravitational waves are totally different things,

so don’t get the two mixed up.

Gravitational waves are ripples in spacetime that were directly detected in early 2016 – the first time since Einstein predicted them over 100 years ago.

Gravity waves, on the other hand, are far more simple – we have them here on Earth, and they’re basically just a ripple or disturbance in the density of a planet’s atmosphere.

It’s thought that Venus’ massive gravity wave formed due to its towering mountain ranges.

As Emma Grey Ellis explains for Wired, if wind is rushing over an uneven surface – such as a jagged mountain range, or even a turbulent ocean – tension is created between air particles wanting to move up, and gravity wanting to push them back down.


This jostling for equilibrium is what causes gravity waves on Earth – like over the Andes in Patagonia – and the Akatsuki team says it’s no coincidence that this phenomenon keeps appearing over Venus’ highlands.

They suggest that surface winds on Venus triggered the formation of the massive gravity wave when they pummelled into the 4,500-metre-high(14,764 feet) Aphrodite Terra mountain range that looms near the planet’s equator.

“We suppose that highlands are a key to generating the stationary gravity waves, because most of the bows – and we have found more than 15 bows so far – have appeared above the highlands at their centres,” one of the researchers, Makoto Taguchi from Rikkyo University, told Ellis.

While the researchers are confident in their explanation, many questions remain, including the mystery of how the gravity wave got so high above the surface in the first place.

The team hopes to address that question with further observations of the planet, and with that insight, we might finally be able to answer an even bigger question – how did Venus’ crazy super-rotation occur?

“We don’t entirely understand how the atmosphere comes to this super-rotating state, but gravity waves are one contributing factor,” Gerald Schubert, a geophysicist at the University of California, Los Angeles, who wasn’t involved in the study, told Wired.

“The feature probably arising at least in part by gravity waves will tell us more about the role they play in the atmospheric dynamics.”

The research has been published in Nature Geoscience.

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