The first all-sky X-ray map to be released in 30 years reveals new wonders of the hot and energetic universe.

The eRosita mission has captured a full view of the X-ray sky. The plane of the Milky Way Galaxy runs along the center of this image. The photons are color-coded by energy: red 300‐600 electron volts (eV), green for 600 to 1,000 eV, and blue for 1,000 to 2,300 eV. Along the galactic plane, gas absorbs all but the highest-energy photons. A number of individual sources and structures are visible and are labeled in the image below.
J. Sanders, H. Brunner & eSASS team (MPE) / E. Churazov, M. Gilfanov (on behalf of IKI)

The eRosita space telescope, which launched in July 2019, has completed its first full sweep across the sky, mapping both hemispheres and cataloging more than 1 million X-ray sources. This is only the first all-sky map to be delivered: The mission plans to create seven more maps, combining them to achieve unprecedented sensitivity to the whole X-ray sky.

One of the key science goals of this mission is to find new galaxy clusters, more distant than ones discovered before, and use them to track the growth of cosmic structure over time. But the multiple maps enable the mission to study other sources, too, including ephemeral ones like flares of light coming from around black holes.

X-ray Vision

The eRosita telescope flies on the Spektrum-Röntgen-Gamma spacecraft, a joint German-Russian mission that operates at the L2 Lagrange point, 1.5 million kilometers (900,000 miles) away on the opposite side of Earth from the Sun. As the telescope rotates, it scans the X-ray sky with seven cameras, taking exposures of 150 to 200 seconds over most of the sky. (The poles have longer exposure times.) The images record photon energies between 300 and 5,000 electron volts.

In half a year, the mission has already doubled the number of known sources collected since the start of X-ray astronomy in the 1960s. Some of these sources are pointed out below:

Labeled all-sky map
This annotated version of the all-sky map points out several galaxy clusters (e.g., Coma, Virgo, Fornax, and Perseus), point sources (e.g., Sco X-1), and extended supernova remnants (SNR). One of the most conspicuous sources is the North Polar Spur, a bubble of hot gas. Its distance is unknown, so astronomers aren't sure if it's a nearby supernova remnant, or a larger shell associated with the galactic center.
J. Sanders, H. Brunner & eSASS team (MPE) / E. Churazov, M. Gilfanov (on behalf of IKI)

This sky is decidedly different from the one we see at night. Only the hottest gases and the most extreme and active sources emit X-rays. While the mission sees some stars, whose magnetic activity creates X-ray-emitting flares, most of the sources are active galactic nuclei, in which hot gases swirl into the maw of supermassive black holes. Other X-ray sources include the hot gases released in supernovae explosions and the far more tenuous gas in and around our galaxy.

The active galaxies that pepper the sky — and account for more than three-quarters of the tally — outnumber eRosita’s true quarry: galaxy clusters. The hot gas spread out in the vast space between galaxies emits X-rays. So by looking for these X-ray blobs, the telescope can find galaxy clusters back to when the universe was only half its current age. Galaxy clusters mark junctures in the cosmic web, so by plotting a large number of clusters over billions of years, astronomers can watch large-scale structures evolve. With more than 20,000 clusters spotted so far, the mission is on track to find more than 100,000 when its surveys are complete.

The researchers continue to analyze the first results even as the mission begins its second round of sky-mapping. The eRosita mission will start making its data public around the summer of 2022, says eRosita principal investigator Peter Predehl (Max Planck Institute for Extraterrestrial Physics, Germany).

Zoom In

Explore regions of eRosita's all-sky map using the Worldwide Telescope.

Vela Supernova Remnant

(Hint: Use the toolbox controls at the upper right to change the background to ROSAT/RASS, then use the cross-fader to see how much eRosita has improved upon the previous all-sky X-ray survey, released 20 years ago.)

The Large Magellanic Cloud

Explore other Worldwide Telescope views here:
Shapley Supercluster
Carina Nebula


You must be logged in to post a comment.