4 min read<\/p>\n
Preparations for Next Moonwalk Simulations Underway (and Underwater)<\/h1>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n![\"The](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/perseus-ixpe-vs-cxo.jpg?w=2048\")
<\/a><\/figure>\nTwo composite images show side-by-side observations of the Perseus Cluster from NASA\u2019s IXPE (Imaging X-Ray Polarimetry Explorer) and Chandra X-ray Observatory. Scientists used data from both observatories, along with data from Nuclear Spectroscopic Telescope Array (NuSTAR), and Neil Gehrels Swift Observatory, to confirm measurements of the galaxy cluster.<\/div>\nX-ray: (Chandra) NASA\/CXC\/SAO, (IXPE) NASA\/MSFC; Image Processing: NASA\/CXC\/SAO\/N. Wolk and K. Arcand<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nWritten by Michael Allen<\/em><\/p>\nAn international team of astronomers using NASA\u2019s IXPE (Imaging X-ray Polarimetry Explorer) has identified the origin of X-rays in a supermassive black hole\u2019s jet, answering a question that has been unresolved since the earliest days of X-ray astronomy. Their findings are described in a paper published in The Astrophysical Journal Letters, by the American Astronomical Society, Nov. 11.<\/p>\n
The IXPE mission observed the Perseus Cluster, the brightest galaxy cluster i observable in X-rays, for more than 600 hours over a 60-day period between January and March. Not only is this IXPE\u2019s longest observation of a single target to date, it also marks IXPE\u2019s first time observing a galaxy cluster.<\/p>\n
Specifically, the team of scientists studied the polarization properties of 3C 84, the massive active galaxy located at the very center of the Perseus Cluster. This active galaxy is a well-known X-ray source and a common target for X-ray astronomers because of its proximity and brightness.<\/p>\n
Because the Perseus Cluster is so massive, it hosts an enormous reservoir of X-ray emitting gas as hot as the core of the Sun. The use of multiple X-ray telescopes, particularly the high-resolution imaging power of NASA\u2019s Chandra X-ray Observatory was essential to disentangle the signals in the IXPE data. Scientists combined these X-ray measurements with data from the agency\u2019s Nuclear Spectroscopic Telescope Array (NuSTAR) mission and Neil Gehrels Swift Observatory.<\/p>\n
Fast facts<\/strong><\/h2>\n\n- Polarization measurements from IXPE carry information about the orientation and alignment of emitted X-ray light waves. The more X-ray waves traveling in sync, the higher the degree of polarization.<\/li>\n
- X-rays from an active galaxy like 3C 84 are thought to originate from a process known as inverse Compton scattering, where light bounces off particles and gains energy. The polarization measurements from IXPE allow us to identify the presence of either inverse Compton scattering or other scenarios.<\/li>\n
- \u201cSeed photons\u201d is the term for the lower-energy radiation undergoing the energizing process of inverse Compton scattering.<\/li>\n
- You may remember the Perseus Cluster from this sonification replicating what a Black Hole sounds like<\/a> from May 2022.<\/li>\n<\/ul>\n
\u201cWhile measuring the polarization of 3C 84 was one of the key science goals, we are still searching for additional polarization signals in this galaxy cluster that could be signatures of more exotic physics,\u201d said Steven Ehlert, project scientist for IXPE and astronomer at NASA\u2019s Marshall Space Flight Center in Huntsville.<\/p>\n
\n\n\n![\"Chandra](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/perseus-cxo-ixpe.jpg?w=2048\")
<\/a><\/figure>\nChandra & IXPE composite image of the Perseus Cluster.<\/div>\nX-ray: (Chandra) NASA\/CXC\/SAO, (IXPE) NASA\/MSFC; Image Processing: NASA\/CXC\/SAO\/N. Wolk and K. Arcand<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n\u201cWe\u2019ve already determined that for sources like 3C 84, the X-rays originated from inverse Compton scattering,\u201d said Ioannis Liodakis, a researcher at the Institute of Astrophysics \u2013 FORTH in Heraklion, Greece, and lead author on the paper. \u201cWith IXPE observations of 3C 84 we had a unique chance to determine the properties of the seed photons.\u201d<\/p>\n
The first possible origin scenario for the seed photons is known as synchrotron self-Compton, where lower-energy radiation originates from the same jet that produces the highly energetic particles.<\/p>\n
In the alternative scenario known as external Compton, seed photons originate from background radiation sources unrelated to the jet.<\/p>\n
\u201cThe synchrotron self-Compton and external Compton scenarios have very different predictions for their X-ray polarization,\u201d said Frederic Marin, an astrophysicist at the Strasbourg Astronomical Observatory in France and co-author of the study. \u201cAny detection of X-ray polarization from 3C 84 almost decisively rules out the possibility of external Compton as the emission mechanism.\u201d<\/p>\n
Throughout the 60-day observation campaign, optical and radio telescopes around the world turned their attention to 3C 84 to further test between the two scenarios.<\/p>\n
NASA\u2019s IXPE measured a net polarization of 4% in the X-rays spectrum, with comparable values measured in the optical and radio data. These results strongly favor the synchrotron self-Compton model for the seed photons, where they come from the same jet as the higher-energy particles.<\/p>\n
\u201cSeparating these two components was essential to this measurement and could not be done by any single X-ray telescope, but by combining the IXPE polarization data with Chandra, NuSTAR, and Swift, we were able to confirm this polarization measurement was associated specifically with 3C 84,\u201d said Sudip Chakraborty, a researcher at the Science and Technology Institute of the Universities Space Research Association in Huntsville, Alabama, and co-author on the paper.<\/p>\n
Scientists will continue to analyze IXPE\u2019s data from different locations in the Perseus Cluster for different signals.<\/p>\n
More about IXPE<\/strong><\/h2>\nNASA\u2019s IXPE, which continues to provide unprecedented data enabling groundbreaking discoveries about celestial objects across the universe, is a joint NASA and Italian Space Agency mission with partners and science collaborators in 12 countries. The IXPE mission is led by NASA\u2019s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, Inc., headquartered in Falls Church, Virginia, manages spacecraft operations together with the University of Colorado\u2019s Laboratory for Atmospheric and Space Physics in Boulder.<\/p>\n
Learn more about IXPE\u2019s ongoing mission here:<\/p>\n
https:\/\/www.nasa.gov\/ixpe<\/a><\/p>\n\n\n\n\n\n\nShare<\/h2>\n<\/p><\/div>\n\n
![\"The](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2025\/12\/perseus-ixpe-vs-cxo.jpg\")
<\/a><\/figure>Written by Michael Allen<\/em><\/p>\n An international team of astronomers using NASA\u2019s IXPE (Imaging X-ray Polarimetry Explorer) has identified the origin of X-rays in a supermassive black hole\u2019s jet, answering a question that has been unresolved since the earliest days of X-ray astronomy. Their findings are described in a paper published in The Astrophysical Journal Letters, by the American Astronomical Society, Nov. 11.<\/p>\n The IXPE mission observed the Perseus Cluster, the brightest galaxy cluster i observable in X-rays, for more than 600 hours over a 60-day period between January and March. Not only is this IXPE\u2019s longest observation of a single target to date, it also marks IXPE\u2019s first time observing a galaxy cluster.<\/p>\n Specifically, the team of scientists studied the polarization properties of 3C 84, the massive active galaxy located at the very center of the Perseus Cluster. This active galaxy is a well-known X-ray source and a common target for X-ray astronomers because of its proximity and brightness.<\/p>\n Because the Perseus Cluster is so massive, it hosts an enormous reservoir of X-ray emitting gas as hot as the core of the Sun. The use of multiple X-ray telescopes, particularly the high-resolution imaging power of NASA\u2019s Chandra X-ray Observatory was essential to disentangle the signals in the IXPE data. Scientists combined these X-ray measurements with data from the agency\u2019s Nuclear Spectroscopic Telescope Array (NuSTAR) mission and Neil Gehrels Swift Observatory.<\/p>\n \u201cWhile measuring the polarization of 3C 84 was one of the key science goals, we are still searching for additional polarization signals in this galaxy cluster that could be signatures of more exotic physics,\u201d said Steven Ehlert, project scientist for IXPE and astronomer at NASA\u2019s Marshall Space Flight Center in Huntsville.<\/p>\n \u201cWe\u2019ve already determined that for sources like 3C 84, the X-rays originated from inverse Compton scattering,\u201d said Ioannis Liodakis, a researcher at the Institute of Astrophysics \u2013 FORTH in Heraklion, Greece, and lead author on the paper. \u201cWith IXPE observations of 3C 84 we had a unique chance to determine the properties of the seed photons.\u201d<\/p>\n The first possible origin scenario for the seed photons is known as synchrotron self-Compton, where lower-energy radiation originates from the same jet that produces the highly energetic particles.<\/p>\n In the alternative scenario known as external Compton, seed photons originate from background radiation sources unrelated to the jet.<\/p>\n \u201cThe synchrotron self-Compton and external Compton scenarios have very different predictions for their X-ray polarization,\u201d said Frederic Marin, an astrophysicist at the Strasbourg Astronomical Observatory in France and co-author of the study. \u201cAny detection of X-ray polarization from 3C 84 almost decisively rules out the possibility of external Compton as the emission mechanism.\u201d<\/p>\n Throughout the 60-day observation campaign, optical and radio telescopes around the world turned their attention to 3C 84 to further test between the two scenarios.<\/p>\n NASA\u2019s IXPE measured a net polarization of 4% in the X-rays spectrum, with comparable values measured in the optical and radio data. These results strongly favor the synchrotron self-Compton model for the seed photons, where they come from the same jet as the higher-energy particles.<\/p>\n \u201cSeparating these two components was essential to this measurement and could not be done by any single X-ray telescope, but by combining the IXPE polarization data with Chandra, NuSTAR, and Swift, we were able to confirm this polarization measurement was associated specifically with 3C 84,\u201d said Sudip Chakraborty, a researcher at the Science and Technology Institute of the Universities Space Research Association in Huntsville, Alabama, and co-author on the paper.<\/p>\n Scientists will continue to analyze IXPE\u2019s data from different locations in the Perseus Cluster for different signals.<\/p>\n NASA\u2019s IXPE, which continues to provide unprecedented data enabling groundbreaking discoveries about celestial objects across the universe, is a joint NASA and Italian Space Agency mission with partners and science collaborators in 12 countries. The IXPE mission is led by NASA\u2019s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, Inc., headquartered in Falls Church, Virginia, manages spacecraft operations together with the University of Colorado\u2019s Laboratory for Atmospheric and Space Physics in Boulder.<\/p>\n Learn more about IXPE\u2019s ongoing mission here:<\/p>\n https:\/\/www.nasa.gov\/ixpe<\/a><\/p>\nFast facts<\/strong><\/h2>\n
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<\/a><\/figure>More about IXPE<\/strong><\/h2>\n
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