Baily's Beads and Prominences - 2017 Total Solar Eclipse
In the first several seconds after the total eclipse ends, a series of dazzlingly bright beads appear along the edge of the Moon and quickly merge to become the crescent Sun. They are formed by sunlight shinning through deep valleys along the irregular limb of the Moon. Francis Baily (Wikipedia) first described this effect after the annular eclipse of 1836. They are known as Baily's Beads in his honor.
Several large solar prominences (Wikipedia) are also visible. Solar prominences are a large, bright features anchored to the Sun's surface in the photosphere, and extend outwards into the Sun's hot outer atmosphere, the solar corona. The bright red arc along the edge of the Moon is the Sun's chromosphere (Wikipedia) (a thin layer that sits just above the solar photosphere).
This image is available as a Custom Print.
Additional eclipse photos can be seen at: 2017 Total Solar Eclipse Photo Gallery.
For more information on this event, see: EclipseWise 2017 Total Solar Eclipse.
Technical Details
- Title: Baily's Beads and Prominences - 2017 Total Solar Eclipse
- Date/Time: 2017 Aug 21 at 17:45 UTC
- Eclipse Circumstances: Altitude = 54°, Azimuth = 143°, HA = -1.41
- Location: Casper College, Casper, WY
- Mount: Losmandy G-11 German Equatorial Mount
- Telescope: Vixen ED100SF Refractor (100mm, f/9, fl=900 mm)
- Camera: Nikon D810
- Exposure: 1/1000 sec, f/9, ISO 200
- File Name: TSE2017-C1066w.jpg
- Processing (Adobe Camera Raw): Exposure Adjustment, Clarity, Sharpening, Noise Reduction
- Processing (Adobe Photoshop CC2017): Curves, Layers
- Rights: Copyright 2017 by Fred Espenak. All Rights Reserved. See: Image Licensing.
