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Coming in Hot — NASA's Chandra Checks Habitability of Exoplanets
Visual Description:

  • X-ray observations of nearby stars are helping astronomers identify the best targets to search for exoplanets with conditions suitable for life.

  • Such planets could be directly imaged in searches with a future generation of telescopes.

  • Harmful radiation from a star in the form of X-rays and ultraviolet could damage or even destroy a planet’s atmosphere.

  • Researchers used NASA’s Chandra X-ray Observatory and ESA’s XMM-Newton to look at 57 exoplanets.

This graphic shows a three-dimensional map of stars near the Sun. These stars are close enough that they could be prime targets for direct imaging searches for planets using future telescopes. The blue haloes represent stars that have been observed with NASA’s Chandra X-ray Observatory and ESA’s XMM-Newton. The yellow star at the center of this diagram represents the position of the Sun. The concentric rings show distances of 5, 10, and 15 parsecs (one parsec is equivalent to roughly 3.2 light-years).

Astronomers are using these X-ray data to determine how habitable exoplanets may be based on whether they receive lethal radiation from the stars they orbit, as described in our latest press release. This type of research will help guide observations with the next generation of telescopes aiming to make the first images of planets like Earth.

Researchers examined stars that are close enough to Earth that telescopes set to begin operating in the next decade or two — including the Habitable Worlds Observatory in space and Extremely Large Telescopes on the ground — could take images of planets in the stars’ so-called habitable zones. This term defines orbits where the planets could have liquid water on their surfaces.

There are several factors influencing what could make a planet suitable for life as we know it. One of those factors is the amount of harmful X-rays and ultraviolet light they receive, which can damage or even strip away the planet’s atmosphere.

Based on X-ray observations of some of these stars using data from Chandra and XMM-Newton, the research team examined which stars could have hospitable conditions on orbiting planets for life to form and prosper. They studied how bright the stars are in X-rays, how energetic the X-rays are, and how much and how quickly they change in X-ray output, for example, due to flares. Brighter and more energetic X-rays can cause more damage to the atmospheres of orbiting planets.

The researchers used almost 10 days of Chandra observations and about 26 days of XMM observations, available in archives, to examine the X-ray behavior of 57 nearby stars, some of them with known planets. Most of these are giant planets like Jupiter, Saturn or Neptune, while only a handful of planets or planet candidates could be less than about twice as massive as Earth.

These results were presented at the 244th meeting of the American Astronomical Society meeting in Madison, Wisconsin, by Breanna Binder (California State Polytechnic University in Pomona).

NASA's Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory's Chandra X-ray Center controls science from Cambridge, Massachusetts and flight operations from Burlington, Massachusetts.


Visual Description:

This video shows a three-dimensional map of stars near the Sun on the left side of our screen and a dramatic illustration of a star with a planet orbiting around it on the right side.

The star map on the left shows many circular dots of different colors floating within an illustrated three-sided box. Each wall of the box is constructed in a grid pattern, with straight lines running horizontally and vertically like chicken wire. Dots that are colored blue represent stars that have been observed with NASA's Chandra and ESA's XMM-Newton.

Suspended in the box, at about the halfway point, is a series of three concentric circles surrounding a central dot that indicates the placement of our Sun. The circles represent distances of 5, 10, and 15 parsecs. One parsec is equivalent to roughly 3.2 light-years.

In the animation, the dot filled, chicken wire box spins around slowly, first on its X axis and then on its Y axis, providing a three-dimensional exploration of the plotted stars.


Fast Facts for Exoplanet Survey:
Credit  Movie: Cal Poly Pomona/B. Binder; Illustration: NASA/CXC/M.Weiss
Release Date  June 12, 2024
Category  Exoplanet, Normal Stars & Star Clusters
Observation Dates  41 Chandra observations between May 7, 2000 and May 27, 2023
Observation Time  227 hours (9 days, 11 hours)
Obs. ID  616, 641, 1886, 4199, 7428, 8904, 9931, 10825, 10976-10979, 12337, 12338, 12393, 12396, 12397, 13644, 13646, 13769, 14401, 14402, 14474, 15565-15567, 17317, 17318, 20162-20164, 21071, 22292, 22293, 22327, 22328, 22352-22354, 27852, 49899
Instrument  ACIS
References Binder, B. et al., AAS meeting #244, 2024
Distance Estimate  A range between 4.2 and 62 light-years.
distance arrow
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