“The discovery of M51-ULS-1b has established that external galaxies host candidate planets,” they added. It is within the reach of the present generation of X-ray telescopes to develop information about the population of planets orbiting XRBs and for future generations of instruments to develop a comprehensive view.” “An equally thorough study of independent datasets will be important to develop better statistics. “Our discovery of a single transit will lead to more detailed studies of planets and other low-radius objects in external galaxies,” they wrote. “This phenomenon is to be contrasted with planetary transits of stars, which produce relatively small dips in flux across wavebands.”Īccording to the authors, M51-ULS-1b is likely a gas-giant planet with a radius slightly smaller than that of Saturn. “There were no simultaneous observations in the optical or infrared, but the regions emitting at these longer wavelengths are so large in comparison with the XRS that there would likely not have been a detectable decline in emission.” “It completely blocked the X-rays from M51-ULS-1 for a time interval of 20-30 minutes, with the excursion from baseline lasting roughly 3 hours.”
“M51-ULS-1b is the first planet candidate discovered when it passed in front of an XRS whose size is comparable to its own,” the researchers wrote. The newfound planet candidate, named M51-ULS-1b, produced a full, short-lived eclipse of the binary system. One of its members is a compact object, either a neutron star or black hole, and the other is a massive star. M51-ULS-1 is a massive binary system located at the edge of a young stellar cluster. This X-ray source is between 100,000 and one million times brighter in X-ray emission than is the Sun at all wavelengths combined. They identified a single transit candidate in M51-ULS-1, one of the brightest XRSs known in Messier 51. Using X-ray data from Chandra, the astronomers searched for possible planet transits in XRSs in three galaxies: Messier 51, Messier 101 and Messier 104. “Luminous XRSs in external galaxies can be spatially resolved, and we can measure the count rate and X-ray emission from each source as a function of time.” “External galaxies host relatively small numbers - a handful to several hundred - of bright X-ray sources (XRSs),” they added. “Yet each external galaxy occupies such a small area of the sky that the high projected stellar density makes it difficult to study individual stars in enough detail to detect the signatures of planets through either radial velocity measurements or transit detection, the two methods responsible for the discovery of more than 4,300 exoplanets.” Rosanne Di Stefano from the Harvard & Smithsonian Center for Astrophysics and her colleagues wrote in their paper. The conditions under which the known planets formed exist in other galaxies as well,” Dr. “Planets are ubiquitous in the Milky Way.
Image credit: Di Stefano et al., arXiv: 2009.08987.
This Chandra/ACIS-S image shows XRSs (colored points) in Messier 51 M51-ULS-1 is the orange source in the center of the blue box diffuse emission is from hot gas.
0 kommentar(er)
