Images by Date
Images by Category
Solar System
Stars
Exoplanets
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Quasars
Galaxy Clusters
Cosmology/Deep Field
Miscellaneous
Images by Interest
Space Scoop for Kids
Multiwavelength
Sky Map
Constellations
Photo Blog
Top Rated Images
Image Handouts
Desktops
Fits Files
Visual descriptions
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
AVM/Metadata
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Image Use Policy
Questions & Answers
Glossary of Terms
Videos: Finding Clues in the Ruins of an Ancient Dead Star
Tour: Finding Clues in the Ruins of an Ancient Dead Star
(Credit: NASA/CXC/SAO/A.Jubett)
[Runtime: 03:25]

With closed-captions (at YouTube)

People often think about archaeology happening deep in jungles or inside ancient pyramids. However, a team of astronomers has shown that they can use stars and the remains they leave behind to conduct a special kind of archaeology in space.

Mining data from NASA’s Chandra X-ray Observatory, the team of astronomers studied the relics that one star left behind after it exploded. This “supernova archaeology” result uncovers important clues about a star that self-destructed – probably more than a million years ago.

Today, the system called GRO J1655-40 contains a black hole with nearly seven times the mass of the Sun and a star with about half as much mass. However, this was not always the case.

Originally GRO J1655-40 had two shining stars. The more massive of the two stars, however, burned through all of its nuclear fuel and then exploded in what astronomers call a supernova. The debris from the destroyed star then rained onto the companion star in orbit around it.

With its outer layers expelled, including some striking its neighbor, the rest of the exploded star collapsed onto itself and formed the black hole that exists today. Over time, the black hole and companion star moved closer. When the separation became small enough, the black hole, with its strong gravitational pull, began pulling matter from its companion, wrenching back some of the material its exploded parent star originally deposited.

While most of this material sank into the black hole, a small amount of it fell into a disk that orbits around the black hole. Through the effects of powerful magnetic fields and friction in the disk, material is being sent out into interstellar space in the form of powerful winds.

This is where the X-ray archaeological hunt enters the story. Astronomers used Chandra to observe the GRO J1655-40 system in 2005 when it was particularly bright in X-rays. Chandra detected signatures of individual elements found in the black hole’s winds by getting detailed spectra — giving X-ray brightness at different wavelengths — embedded in the X-ray light.

The team of astronomers digging through the Chandra data were able to reconstruct key physical characteristics of the star that exploded from the clues imprinted in the X-ray light by comparing the spectra with computer models of stars that explode as supernovae. They discovered that the long-gone star destroyed in the supernova was about 25 times the mass of the Sun. It was also much richer in elements heavier than helium in comparison with the Sun.

Look for more supernova archaeology stories with Chandra in the future!


Quick Look: Finding Clues in the Ruins of an Ancient Dead Star
(Credit: NASA/CXC/SAO/A.Jubett)
[Runtime: 00:45]

With narration (video above with voiceover)

Astronomers conducted archaeology in space with NASA’s Chandra X-ray Observatory.

Looking at a double star system, they found individual elements like iron and sulfur.

These elements are flowing away from winds being powered by a black hole.

This helps scientists learn more about the star that exploded to create the black hole.




Return to: Finding Clues in the Ruins of an Ancient Dead Star (March 24, 2025)