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Birthday · March 4, 2014

Sun and Prominence

March 4, 2014

In the grand ledger of cosmic time, a human life is breathtakingly brief. But brevity is not insignificance.

Sun and Prominence

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APOD published March 4, 2014. Credit: jp-Brahic. A publication-date match, not a photo taken on your date. Independent of NASA.

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Sun and Prominence

Original APOD · March 4, 2014

Dramatic prominences can sometimes be seen looming just beyond the edge of the sun. Such was the case last week as a large prominence, visible above, highlighted a highly active recent Sun. A waving sea of hot gas is visible in the foreground chromosphere in great detail as it was imaged in one specific color of light emitted by hydrogen. A solar prominence is a cloud of solar gas held just above the surface by the Sun's magnetic field. The Earth, illustrated in the inset, is smaller than the prominence. Although very hot, prominences typically appear dark when viewed against the Sun, since they are slightly cooler than the photosphere below them. A quiescent prominence typically lasts about a month, and may erupt in a Coronal Mass Ejection (CME) expelling hot gas into the Solar System, some of which may strike the Earth and trigger auroras.

Image credit: jp-Brahic

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