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The scale of a solar prominence

27,008 次观看 • 1 年前 •via X (Twitter)

10 条评论

Ali 的头像
Ali1 年前

Woooo

RafaSimon 的头像
RafaSimon1 年前

Hey @grok explain Solar Prominence like you are sir David Attenborough

Grok 的头像
Grok1 年前

Picture, if you will, the Sun, a colossal orb of fire, its surface alive with restless energy. Here, great arches of plasma rise—solar prominences, sculpted by invisible magnetic forces. These radiant loops, stretching over 800,000 kilometers, dwarf our Earth, a mere speck at 12,700 kilometers wide. Composed of charged hydrogen and helium, they glow red against the cosmic void, yet appear as dark filaments against the Sun’s blazing disk. Some endure for months, others erupt, hurling plasma into space, stirring auroras or troubling our satellites. Their formation, a dance of magnetic fields, remains a mystery, studied yet not fully unraveled, a testament to the Sun’s untamed grandeur.

Barbara 💕🕊️🌎 的头像
Barbara 💕🕊️🌎1 年前

This is mesmerizing🤩

Ag 的头像
Ag1 年前

Sorry, I measue things in "soccer fields".

Eon 的头像
Eon1 年前

After conquering Mars, we need to make a Cybertruck pass through one of those rings and return to us.

GlobalStatsX 的头像
GlobalStatsX1 年前

Nice

Shawn 的头像
Shawn1 年前

Jeez sure glad we aren’t that close to it

Shawn 的头像
Shawn1 年前

Explains the heat wave currently

Stats Globe 的头像
Stats Globe1 年前

🌅 Solar prominences are large, bright, and cool loops or arches of ionized gas (plasma) that extend from the Sun's surface into its corona. They are anchored to the Sun's surface and can extend for thousands of kilometers into space. When viewed against the bright solar disk, they appear as dark filaments.

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