Absolutely Amazing!!!!!

Absolutely Amazing!!!!!

Can you name a few planets where it rains things? I was telling my little sister how it rains neon on Jupiter and she wants to know more.

Hello, we can find other types of rain not only on other planets, but also on moons and even brown dwarfs.

For example because of the high temperature some brown dwarfs can raining molten-iron.

image

and there is also rain of hydrocarbons (methane and liquid ethane) on Saturn’s moon Titan.

image

We can also mention diamond rain in Neptune, sulfuric acid rain on Venus and rain of glass on the exoplanet HD 189733b.

Below I will leave some links to that:

Sulfuric acid rain on Venus

Diamond Rain in Neptune

Rain of glass on exoplanet HD 189733b

Images credit: NASA/JPL-Caltech/University of Western Ontario/Stony Brook University & David A. Hardy (AstroArt) 

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8 years ago

Wow

amyleigh81 - Life
7 years ago
Roll That Shit

Roll that Shit


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7 years ago

Very Interesting

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4 years ago

There's NO better favor in the world that you could do for yourself than truly "LOVE YOURSELF"!!

“Love Yourself” By Enkel Dika On INPRNT

“Love Yourself” by Enkel Dika on INPRNT


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7 years ago

Absolutely amazing!!

The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature
The Upper Atmosphere Of The Sun Is Dominated By Plasma Filled Magnetic Loops (coronal Loops) Whose Temperature

The upper atmosphere of the Sun is dominated by plasma filled magnetic loops (coronal loops) whose temperature and pressure vary over a wide range. The appearance of coronal loops follows the emergence of magnetic flux, which is generated by dynamo processes inside the Sun. Emerging flux regions (EFRs) appear when magnetic flux bundles emerge from the solar interior through the photosphere and into the upper atmosphere (chromosphere and the corona). The characteristic feature of EFR is the Ω-shaped loops (created by the magnetic buoyancy/Parker instability), they appear as developing bipolar sunspots in magnetograms, and as arch filament systems in Hα. EFRs interact with pre-existing magnetic fields in the corona and produce small flares (plasma heating) and collimated plasma jets. The GIFs above show multiple energetic jets in three different wavelengths. The light has been colorized in red, green and blue, corresponding to three coronal temperature regimes ranging from ~0.8Mk to 2MK. 

Image Credit: SDO/U. Aberystwyth

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