Giant ghostly 'hand' stretches through space in new X-ray views

NASA's Chandra X-ray Observatory captured this imagery of a huge, hand-shaped feature, which was spawned by a supernova explosion and its aftermath in a patch of space about 17,000 light-years from Earth.
NASA's Chandra X-ray Observatory captured this imagery of a huge, hand-shaped feature, which was spawned by a supernova explosion and its aftermath in a patch of space about 17,000 light-years from Earth. (Image credit: NASA/SAO/NCSU/Borkowski et al.)

An enormous ghostly hand stretches through the depths of space, its wispy fingers pressing against a glowing cloud.

It sounds like science fiction, but it's quite real, as imagery gathered by NASA's Chandra X-ray Observatory shows. 

The "hand" was spawned by the death of a massive star in a supernova explosion, which left behind a fast-spinning, superdense stellar corpse known as a pulsar, Chandra team members said in a description of the dramatic images

Related: Amazing photos by NASA's Chandra X-Ray Observatory

That pulsar has blown a bubble of energetic particles around itself, which, combined with the debris blasted out by the supernova explosion, created the hand-like structure that stretches 150 light-years. The glowing feature that it's reaching for, meanwhile, is a mammoth gas cloud known as RCW 89.

The supernova remnant at the heart of the hand, called MSH 15-52, lies about 17,000 light-years from Earth. Astronomers think the light from its explosion reached us about 1,700 years ago, making MSH 15-52 one of the youngest supernova remnants known in our Milky Way galaxy, Chandra team members said.

Related: Haunting Photos: The Spookiest Nebulas in Space

Chandra has imaged the hand before; it was the subject of an April 2009 photo release, for example. But a recent study took a deep dive into the hand's dynamics, using Chandra imagery from 2004, 2008, 2017 and 2018. 

The research, which was published in The Astrophysical Journal Letters in June 2020, found that the supernova blast wave, which lies at the hand's fingertips, is traveling at about 9 million mph (14.5 million kph) and material closer to the palm is moving even faster, in excess of 11 million mph (17.7 kph).

"While these are startling[ly] high speeds, they actually represent a slowing down of the remnant. Researchers estimate that to reach the farthest edge of RCW 89, material would have to travel on average at almost 30 million miles per hour [48.2 million kph]," Chandra team members wrote in the image description. 

"This difference in speed implies that the material has passed through a low-density cavity of gas and then been significantly decelerated by running into RCW 89," they added.

The dead star likely created such a cavity shortly before exploding, when it shed much of its outer hydrogen layer, Chandra team members said.

Chandra has been eyeing the cosmos in X-ray light for more than two decades. The telescope launched to Earth orbit aboard the space shuttle Columbia in July 1999.

Chandra is one of four NASA "Great Observatories," which launched between 1990 and 2003. The others are the Hubble Space Telescope, which remains active today (though it's dealing with a computer glitch at the moment); the Compton Gamma Ray Observatory, which launched in 1991 and ended its mission in 2000; and the infrared-optimized Spitzer Space Telescope, which launched in 2003 and was taken out of service last year.

Mike Wall is the author of "Out There" (Grand Central Publishing, 2018; illustrated by Karl Tate), a book about the search for alien life. Follow him on Twitter @michaeldwall. Follow us on Twitter @Spacedotcom or Facebook. 

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Mike Wall
Senior Space Writer

Michael Wall is a Senior Space Writer with and joined the team in 2010. He primarily covers exoplanets, spaceflight and military space, but has been known to dabble in the space art beat. His book about the search for alien life, "Out There," was published on Nov. 13, 2018. Before becoming a science writer, Michael worked as a herpetologist and wildlife biologist. He has a Ph.D. in evolutionary biology from the University of Sydney, Australia, a bachelor's degree from the University of Arizona, and a graduate certificate in science writing from the University of California, Santa Cruz. To find out what his latest project is, you can follow Michael on Twitter.