The sun's sprung a leak! Enormous coronal hole that is 50-EARTHS-wide spotted on star (but don't worry, it's harmless)
- Coronal holes are regions of corona where magnetic field reaches out into space rather than looping back down
- They were first observed in images taken by astronauts on board NASA's Skylab space station in 1973 and 1974
- Can remain visible to scientists for years, although the exact shape changes all the time
Astronomers have spotted what looks like an enormous chasm sprawled across the sun's surface.
The phenomenon, known as a coronal hole, is 50-Earths-wide and shows up as a vast patch of black on Nasa's newly released image.
Captured by Nasa's Solar Dynamics Observatory on 15 October, the region occurs where a magnetic field fails to loop back down to the sun's surface instead sending out coronal material in what is called a high-speed solar wind stream.
Awe-inspiring: The image, take on 15 October, was taken in wavelengths of 193 Angstroms, which is invisible to the human eye
Nasa said: 'Coronal holes are magnetically open areas that are one source of high-speed solar wind.
'They appear dark when viewed in many wavelengths of extreme ultraviolet light, such as seen here. At times, the solar wind can generate aurora at higher latitudes on Earth.’
While the image may at first look alarming, it does not indicate that we are in any danger. Coronal holes are a common feature on the sun, though they appear at different places - particularly near the poles - and with more frequency at different times of the sun's activity cycle.
They are generally more common when the sun is at a less active point in its 11-year cycle.
The holes' effects are usually harmless, although in some cases satellite communications and high-altitude radio transmissions can be temporarily disrupted.
A coronal hole was also spotted at the beginning of the year (pictured). In January the phenomenon occurred closer to the south pole
They can also trigger the stunning aurora over Earth's skies - although solar flares and coronal mass ejections can also be responsible for the natural wonder.
The high-speed solar winds originating from this coronal hole triggered a geomagnetic storm near Earth that resulted in several nights of auroras earlier this month.
The hole is currently moving westwards - to the right, from Earth's perspective - so solar winds will remain strong, National Oceanic and Atmospheric Administration (NOAA) officials have said.
Coronal holes were first observed in X-ray images taken by astronauts on board Nasa's Skylab space station in 1973 and 1974.
The material that constantly flows from the sun is called the solar wind, which typically 'blows' at around 250 miles (400 km) per second.
When a coronal hole is present, however, the wind speed can double to nearly 500 miles (800 km) per second.
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