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A Dead Star Caught Feeding

NASA's XRISM telescope watched a city-sized dead star swallow gas from a giant neighbor — and clocked it falling at 335,000 mph.

Image: NASA/JPL-Caltech

The Number That Matters

Gas is pouring onto the dead star at about 335,000 mph (540,000 kph). It is the first time anyone has directly watched a stellar wind land on one.

Image: NASA/JPL-Caltech

Meet GX 301-2

The eater is a neutron star called GX 301-2. It packs more than the Sun's mass into a ball roughly 12 miles wide, and spins once every 11 minutes.

Image: NASA/JPL-Caltech

Its Giant Neighbor

The gas comes from Wray 977, a blue hypergiant about 40 times the Sun's mass and 60 times its size. Stars that big shed material constantly.

Image: NASA/ESA

What a Stellar Wind Is

A hypergiant's outer layers stream away as a hot wind. Whatever drifts close to the neutron star is caught by its gravity and dragged down.

Image: NASA/ESA Hubble Space Telescope

Where Such Cores Come From

Neutron stars are what big stars leave behind. The Crab Nebula, seen here, hides one at its heart, born in a supernova people watched in 1054.

Image: NASA/JPL-Caltech/ESA/CXC

A 41.5-Day Orbit

Massive stars often come in pairs. This one laps its partner every 41.5 days, and twice an orbit it hits thicker gas and blazes in X-rays.

Image: NASA/ESA Hubble Space Telescope

Sixteen Hours in February

XRISM watched the pair on Feb. 1, 2025, for about 16 hours, catching the tail end of one of those flares with its Resolve instrument.

Image: NASA/Goddard Space Flight Center

How Resolve Caught It

Nested foil mirrors funnel X-rays onto the detector. Iron lines in the spectrum shifted red — the fingerprint of gas racing away from us.

Image: NASA/Goddard Space Flight Center

Where It Sits

The system lies about 13,000 light-years away in Crux, the Southern Cross — far too faint and far too distant to pick out with the naked eye.

Image: NASA/JPL-Caltech/ESA/CXC/STScI

Why It Matters

Watching wind turn into X-rays shows how the densest objects in the universe grow. The results were published Sept. 18 in Science Advances.

Image: NASA/JPL-Caltech
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