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APOD: 2014 March 4 – Sun and Prominence

APOD: 2014 March 4 – Sun and Prominence

01 de agosto de 2026
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APOD: 2014 March 4 – Sun and Prominence

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

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Sun and Prominence

Explanation: 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 .

Date March 4, 2014
Credit Image Credit & Copyright: jp-Brahic
Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

NASA

Agência Espacial Americana

Fonte original