Celebrating 20 years of NASA's Chandra X-ray Observatory
(Illustration: NASA/CXC & J.Vaughan)
Since its launch on July 23, 1999, the Chandra X‐ray Observatory has helped revolutionize our understanding of the Universe. As NASA’s flagship mission for X‐ray astronomy and part of the “Great Observatories,” Chandra is a telescope designed to detect X‐ray emission from very hot regions of the Universe such as exploded stars, clusters of galaxies, and matter around black holes.
Because X‐rays are absorbed by Earth’s atmosphere, Chandra orbits high above it. Its elliptical path takes the spacecraft from just under 16,000 km (10,000 miles) on its closest approach out to a distance of 139,000 km (86,500 mi) from Earth.
Chandra carries four very sensitive mirrors nested inside each other. X‐rays from space, which are highly energetic, strike the insides of the hollow shells and are focused onto electronic detectors at the end of the 9.2-meter (30‐foot) optical bench. Depending on which detector is used, very detailed images or spectra (the amount of X-rays over a range of wavelengths) of the cosmic source can be made and analyzed.
Chandra has the ability to make exquisite X‐ray images of star clusters, supernova remnants, galactic eruptions, and collisions between clusters of galaxies. This has allowed scientists using Chandra to probe the geometry of space‐time around black holes, trace the dispersal of elements by supernovas, and reveal whirling neutron stars generating streams of high‐energy particles. The telescope has also been used to study cosmic phenomena as diverse as comets and planets in our Solar System to the effects of dark matter and dark energy on the Universe itself.
As Chandra expands the realm of the known, it continues to raise new questions and point the way for future exploration. To commemorate Chandra’s 20 years in space, we’ve put together 20 facts about Chandra. This, of course, is just a sample of all of the wonderous things Chandra has done and can do in the future.
Credit: NASA/CXC/SAO
20 (Facts) for 20 (Years) with Chandra
Here’s to another 20 years!
Megan Watzke is the public affairs officer for the Chandra X-ray Observatory, a position she has held since 2000. Her responsibilities include the dissemination of Chandra’s science results to the general public through press releases, press conferences, informal education, and other activities. | ![]() |
Kimberly K. Arcand is the Visualization Lead for NASA’s Chandra X-ray Observatory, which has its headquarters at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts. She studies the perception and comprehension of data visualization across the novice-expert spectrum and is active in the creation, distribution, and evaluation of large-scale science and technology communications projects. | ![]() |