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NASA’s IXPE Marks Two Years of Groundbreaking X-ray Astronomy


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On Dec. 9, astronomers and physicists will commemorate two years of landmark X-ray science by NASA’s IXPE (Imaging X-ray Polarimetry Explorer) mission.

IXPE is the joint NASA-Italian Space Agency mission to study polarized X-ray light. Polarization is a characteristic of light that can help reveal information about where that light came from, such as the geometry and inner workings of the ultra-powerful energy sources from which it emanates.

A gif of IXPE deploying in space before starting its science operations to study the cosmos.
A gif of IXPE deploying in space before starting its science operations to study the cosmos.
NASA

Launched Dec. 9, 2021, IXPE orbits Earth some 340 miles high, studying X-ray emissions from powerful cosmic phenomena thousands to billions of light-years from Earth, including quasars, blazars, remnants of supernova explosions such as neutron stars, and high-energy particle streams spewing from the vicinity of black holes at nearly the speed of light.

“Adding X-ray polarization to our arsenal of radio, infrared, and optical polarization is a game changer,” said Alan Marscher, a Boston University astronomer who leads a research group that uses IXPE’s findings to analyze supermassive black holes.

“We’re all familiar with X-rays as a diagnostic medical tool for humans. Here we’re using them in a different way, but they are again revealing information that is otherwise hidden from us,” said Stanford University researcher Josephine Wong, who co-authored findings in October based on IXPE studies of the pulsar wind nebula MSH 15-52, some 16,000 light-years from Earth.

Martin Weisskopf, the astrophysicist who led the development of IXPE and served as its principal investigator until his retirement from NASA in spring 2022, agreed.

There can be no question that IXPE has shown that X-ray polarimetry is important and relevant to furthering our understanding of how these fascinating X-ray systems work.

Martin Weisskopf

Martin Weisskopf

Retired IXPE Principal Investigator

Scientists have long understood, for example, the fundamentals of blazars such as Markarian 501 and Markarian 421. A blazar is a massive black hole feeding off material swirling around it in a disk, creating powerful jets of high-speed cosmic particles which rush away in two directions perpendicular to the disk. But how are those particles accelerated to such high energies? IXPE data published in November 2022 in the journal Nature identified the culprit at Markarian 501 as a shock wave within the jet.

This NASA illustration shows the structure of a black hole jet as inferred by recent observations of the blazar Markarian 421 by the Imaging X-ray Polarimetry Explorer (IXPE).
This NASA illustration shows the structure of a black hole jet as inferred by recent IXPE observations of the blazar Markarian 421. The jet is powered by an accretion disk, shown at the bottom of the image, which orbits and falls into the black hole over time. Helical magnetic fields are threaded through the jet. IXPE observations have shown that the X-rays must be generated in a shock originating within material spiraling around the magnetic fields. The inset shows the shock front itself. X-rays are generated in the white region nearest the shock front, whereas optical and radio emission must originate from more turbulent regions further away from the shock.
NASA/Pablo Garcia

“This is a 40-year-old mystery that we’ve solved,” said Yannis Liodakis, a NASA Postdoctoral Program researcher at NASA’s Marshall Space Flight Center in Huntsville, Alabama. “We finally had all of the pieces of the puzzle, and the picture they made was clear.”

IXPE also conducted unprecedented studies of three supernova remnants – Cassiopeia A, Tycho, and SN 1006 – helping scientists further their understanding of the origin and processes of the magnetic fields surrounding these phenomena.

IXPE is even shedding new light on fundamental mechanisms of our own galaxy. According to studies IXPE conducted in early 2022, Sagittarius A*, the supermassive black hole at the center of the Milky Way, woke up about 200 years ago to devour gas and other cosmic detritus, triggering an intense, short-lived X-ray flare. By combining data from IXPE, Chandra, and the European Space Agency’s XMM-Newton mission, researchers determined the event occurred around the start of the 19th century.

“We know change can happen to active galaxies and supermassive black holes on a human timescale,” said IXPE project scientist Steve Ehlert at NASA Marshall. “IXPE is helping us better understand the timescale on which the black hole at the center of our galaxy is changing. We’re eager to observe it further to determine which changes are typical and which are unique.”

A red and orange circle on a black starry background. A portion of the upper left is purple with lines on it.
This new image of supernova remnant SN 1006 combines data from IXPE and NASA’s Chandra X-ray Observatory. The red, green, and blue elements reflect low, medium, and high energy X-rays, respectively, as detected by Chandra. The IXPE data, which measure the polarization of the X-ray light, is show in purple in the upper left corner, with the addition of lines representing the outward movement of the remnant’s magnetic field.
X-ray: NASA/CXC/SAO (Chandra); NASA/MSFC/Nanjing Univ./P. Zhou et al. (IXPE); IR: NASA/JPL/CalTech/Spitzer; Image Processing: NASA/CXC/SAO/J.Schmidt

IXPE has also supported observations of unanticipated cosmic events – such as the brightest pulse of intense radiation ever recorded, which abruptly swept through our solar system in October 2022.

The pulse stemmed from a powerful gamma-ray burst likely to occur no more than once in 10,000 years, researchers said. Backing up data from NASA’s Fermi Space Telescope and other imagers, IXPE helped determine how the powerful emission was organized and confirmed that Earth imagers viewed the jet almost directly head-on.

Perhaps most exciting to space scientists is how IXPE data is upending conventional wisdom about various classes of high-energy sources.

“So many of the polarized X-ray results we’ve seen over the past two years were a big surprise, tossing theoretical models right out the window,” Ehlert said.

Seeing results we didn’t anticipate sparks new questions, new theories. It’s really exciting!

Steve Ehlert

Steve Ehlert

IXPE Project Scientist

That excitement continues to build among IXPE partners around the world. In June, the mission was formally extended for 20 months beyond its initial two-year flight, meaning IXPE will continue to observe high-energy X-ray emissions across the cosmos through at least September 2025.

The new year also will mark the start of the IXPE General Observer Program, which invites astrophysicists and other space scientists around the world to propose and take part in studies using the IXPE telescope. Beginning in February 2024, as much as 80% of IXPE’s time will be made available to the broader scientific community.

About the IXPE Mission

IXPE is a collaboration between NASA and the Italian Space Agency with partners and science collaborators in 12 countries. IXPE is led by NASA’s Marshall Space Flight Center. Ball Aerospace, headquartered in Broomfield, Colorado, manages spacecraft operations together with the University of Colorado’s Laboratory for Atmospheric and Space Physics in Boulder.

Elizabeth Landau
NASA Headquarters
elizabeth.r.landau@nasa.gov
202-358-0845

Jonathan Deal
NASA’s Marshall Space Flight Center
256-544-0034
jonathan.e.deal@nasa.gov

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      James Lovell, left, and Fred Haise practice setting up science equipment, the American flag, and the S-band antenna.NASA Lovell, left, and Haise practice collecting rock samples. NASA John Young, left, and Charles Duke train to collect rock samples. NASA Fred Haise, left, and James Lovell practice lowering the Apollo Lunar Surface Experiment Package from the Lunar Module.NASA Lovell, left, and Haise practice setting up the experiments. NASA Lovell, left, and Haise practice drilling for the Heat Flow Experiment. NASA During their 35 hours on the Moon’s surface, Lovell and Haise planned to conduct two four-hour spacewalks to set up the Apollo Lunar Surface Experiment Package (ALSEP), a suite of four investigations designed to collect data about the lunar environment after the astronauts’ departure, and to conduct geologic explorations of the landing site. The four experiments included the: 
      Charged Particle Lunar Environment Experiment designed to measure the flexes of charged particles  Cold Cathode Gauge Experiment designed to measure the pressure of the lunar atmosphere  Heat Flow Experiment designed to make thermal measurements of the lunar subsurface  Passive Seismic Experiment designed to measure any moonquakes, either naturally occurring or caused by artificial means   As an additional investigation, the astronauts planned to deploy and retrieve the Solar Wind Composition experiment, a sheet of aluminum foil to collect particles from the solar wind for analysis by scientists back on Earth after about 20 hours of exposure on the lunar surface. 

      Apollo 14 astronauts Eugene Cernan, left, Joe Engle, Edgar Mitchell, and Alan Shepard with geologist Richard Jahns in the Pinacates Mountains of northern Mexico. NASA Shepard, left, Engle, Mitchell, and Cernan training with the Modular Equipment Transporter, accompanied by geologist Jahns. NASA With one lunar mission just two months away, NASA continued preparations for the following flight, Apollo 14, then scheduled for October 1970 with a landing targeted for the Littrow region of the Moon, an area scientists believed to be of volcanic origin. Apollo 14 astronauts Alan Shepard, Stuart Roosa, and Edgar Mitchell and their backups Eugene Cernan, Ronald Evans, and Joe Engle  learned spacecraft systems in the simulators. Accompanied by a team of geologists led by Richard Jahns, Shepard, Mitchell, Cernan, and Engle participated in a geology expedition to the Pinacate Mountain Range in northern Mexico Feb. 14-18, 1970. The astronauts practiced using the Modular Equipment Transporter, a two-wheeled conveyance to transport tools and samples on the lunar surface. 

      Mail out of the Apollo 12 lunar samples. Apollo 12 astronauts Charles Conrad, left, Richard Gordon, and Alan Bean ride in a motorcade in Lima, Peru.NASA On Feb. 13, 1970, NASA began releasing Apollo 12 lunar samples to 139 U.S. and 54 international scientists in 16 countries, a total of 28.6 pounds of material. On Feb. 16, Apollo 12 astronauts Charles Conrad, Richard Gordon, and Alan Bean, accompanied by their wives and NASA and State Department officials, departed Houston’s Ellington Air Force Base for their 38-day Bullseye Presidential Goodwill World Tour. They first traveled to Latin America, making stops in Venezuela, Peru, Chile, and Panama before continuing on to Europe, Africa, and Asia. 
      The groundbreaking science and discoveries made during Apollo missions has pushed NASA to explore the Moon more than ever before through the Artemis program. Apollo astronauts set up mirror arrays, or “retroreflectors,” on the Moon to accurately reflect laser light beamed at them from Earth with minimal scattering or diffusion. Retroreflectors are mirrors that reflect the incoming light back in the same incoming direction. Calculating the time required for the beams to bounce back allowed scientists to precisely measure the Moon’s shape and distance from Earth, both of which are directly affected by Earth’s gravitational pull. More than 50 years later, on the cusp of NASA’s crewed Artemis missions to the Moon, lunar research still leverages data from those Apollo-era retroreflectors. 

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