This week, the Sun erupted with a powerful solar flare, and the incident was caught in real-time by NASA’s Solar Dynamics Observatory. NASA has shared remarkable footage of the event, which took place on January 20, peaking at 1:01 a.m. ET.
“Solar flares are powerful bursts of energy,” NASA writes. “Flares and solar eruptions can impact radio communications, electric power grids, navigation signals, and pose risks to spacecraft and astronauts.”
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NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the right side of this image of the Sun – on January 20. The image from SDO’s Atmospheric Imaging Assembly 131 Ångström channel (colorized in teal) shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares. Credits: NASA/SDOThe Solar Dynamics Observatory constantly observes this sun, waiting to capture moments like this and seeing how the star changes over time. The image is colorized into this blue shade to better show off the flare event, with the blue representing the extreme ultraviolet light given off by the Sun due to its heat. As well as the whole-Sun image above, NASA also released a close-up clip which shows the flaring region in more detail:
A zoom in on the flaring region. Credits: NASA/SDOThis was classified as a M5.5 solar flare, making it one of the more intense types of flare to have been spotted. According to the Space Weather Prediction Center, there are five levels to measure solar flare intensity, each designated by a letter. The lowest is the A level, followed by B, C, M, and X flares, with each level giving off X-rays ten times more powerful than the level below. As an M flare, this event was on the stronger end of the scale, though not quite as dramatic as the X-1 class flare observed in October last year.
Stunning space station video shows glorious aurora over Earth
NASA has released a breathtaking time-lapse video showing a recent aurora over Earth.
The footage was captured by a camera on the International Space Station (ISS), which orbits our planet at an altitude of around 250 miles. Besides the Earth and the gorgeous green aurora, it also shows several of the station’s solar panels moving slowly to capture the sun's rays.
Hubble captures a cosmic sea monster with this image of a jellyfish galaxy
This week's image from the Hubble Space Telescope shows a special and delightful cosmic object: a jellyfish galaxy. These galaxies are named for their larger main body with tendrils that float along after them, like the sea creatures.
This particular jellyfish galaxy is called JO201, and is located in the constellation of Cetus. Appropriately for the sea theme, Cetus is a constellation named after a Greek mythological sea monster that sometimes had the body of a whale or serpent along with the head of a boar. In the image, you can see the main body of the galaxy in the center, with the trailing tendrils spreading down toward the bottom of the frame.
Roman Space Telescope will survey the sky 1,000 times faster than Hubble
Since its launch in 2021, the James Webb Space Telescope has been delighting space fans with its stunning views of space objects near and far. But NASA has another space telescope in the works that will be able to help answer even more of the big questions in astronomy. The Nancy Grace Roman Space Telescope, set to launch in 2027 and colloquially known as Roman, will look at vast areas of space to help cosmologists understand the universe on a large scale.
In astronomy research, it's important to be able to look both in very great detail and on a very wide scale. Telescopes like Hubble and James Webb have exceptional sensitivity, so they can look at extremely distant objects. Roman will be different, aiming to get a broad view of the sky. The image below illustrates the differences between the telescopes, showing what Roman and Hubble can capture in one go and comparing Hubble's detailed, but narrow view to Roman's much wider view.
