NASA Launches New Mission to Explore Universe's Most Dramatic Objects

NASA's Imaging X-ray Polarimetry Explorer (IXPE) mission launched at 1 a.m. EST Thursday on a SpaceX Falcon 9 rocket from NASA's Kennedy Space Center in Florida.

Above: A SpaceX Falcon 9 rocket launches with NASA's Imaging X-ray Polarimetry Explorer (IXPE) spacecraft onboard from Launch Complex 39A, Thursday, Dec. 9, 2021, at NASA's Kennedy Space Center in Florida. (NASA/Joel Kowsky)

A joint effort with the Italian Space Agency, the IXPE observatory is NASA's first mission dedicated to measuring the polarization of X-rays from the most extreme and mysterious objects in the universe – supernova remnants, supermassive black holes, and dozens of other high-energy objects.

"IXPE represents another extraordinary first," said Thomas Zurbuchen, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. "Together with our partners in Italy and around the world, we've added a new space observatory to our fleet that will shape our understanding of the universe for years to come. Each NASA spacecraft is carefully chosen to target brand new observations enabling new science, and IXPE is going to show us the violent universe around us – such as exploding stars and the black holes at the center of galaxies – in ways we've never been able to see it."

The rocket performed as expected, with spacecraft separation taking place 33 minutes into flight. Approximately one minute later, the spacecraft unfurled its solar arrays. IXPE entered its orbit around Earth's equator at an altitude of approximately 372 miles (600 kilometers). About 40 minutes after launch, mission operators received the first spacecraft telemetry data.

"It is an indescribable feeling to see something you've worked on for decades become real and launch into space," said Martin Weisskopf, IXPE's principal investigator at NASA's Marshall Space Flight Center in Huntsville, Alabama. Weisskopf came up with the idea for the spacecraft and has conducted seminal experiments in X-ray astronomy since the 1970s. "This is just the beginning for IXPE. We have much work ahead. But tonight, we celebrate!"

IXPE carries three state-of-the-art space telescopes with special polarization-sensitive detectors. Polarization is a property of light that holds clues to the environment from which the light originates. The new mission builds on and complements the scientific discoveries of other telescopes, including the Chandra X-ray Observatory, NASA's flagship X-ray telescope. First light operations are scheduled to begin in January.

NASA Marshall manages the IXPE mission for the agency's Science Mission Directorate as a project of the NASA's Explorers Program. IXPE is an international collaboration between NASA, the Italian Space Agency, along with partners and providers in 12 other countries. Marshall built the three X-ray telescopes. The Italian Space Agency contributed IXPE's polarization detectors. Ball Aerospace in Broomfield, Colorado, provided the spacecraft and manages spacecraft operations at the University of Colorado Boulder's Laboratory for Atmospheric and Space Physics. NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the Explorers Program.

NASA's IXPE Sends First Science Image

NASA's Imaging X-Ray Polarimetry Explorer, which launched Dec. 9, 2021, has delivered its first imaging data since completing its month-long commissioning phase.

Above: This image of the supernova remnant Cassiopeia A combines some of the first X-ray data collected by NASA's Imaging X-ray Polarimetry Explorer, shown in magenta, with high-energy X-ray data from NASA's Chandra X-Ray Observatory, in blue. (NASA/CXC/SAO/IXPE)

All instruments are functioning well aboard the observatory, which is on a quest to study some of the most mysterious and extreme objects in the universe.

IXPE first focused its X-ray eyes on Cassiopeia A, an object consisting of the remains of a star that exploded in the 17th century. The shock waves from the explosion have swept up surrounding gas, heating it to high temperatures and accelerating cosmic ray particles to make a cloud that glows in X-ray light. Other telescopes have studied Cassiopeia A before, but IXPE will allow researchers to examine it in a new way.

In the image above, the saturation of the magenta color corresponds to the intensity of X-ray light observed by IXPE. It overlays high energy X-ray data, shown in blue, from NASA's Chandra X-Ray Observatory. Chandra and IXPE, with different kinds of detectors, capture different levels of angular resolution, or sharpness. An additional version of this image is available showing only IXPE data. These images contain IXPE data collected from Jan. 11 to 18.

After Chandra launched in 1999, its first image was also of Cassiopeia A. Chandra's X-ray imagery revealed, for the first time, that there is a compact object in the center of the supernova remnant, which may be a black hole or neutron star.

"The IXPE image of Cassiopeia A is as historic as the Chandra image of the same supernova remnant," said Martin C. Weisskopf, the IXPE principal investigator based at NASA's Marshall Space Flight Center in Huntsville, Alabama. "It demonstrates IXPE's potential to gain new, never-before-seen information about Cassiopeia A, which is under analysis right now."

Above: This image from NASA's Imaging X-ray Polarimetry Explorer maps the intensity of X-rays coming from the observatory's first target, the supernova remnant Cassiopeia A. Colors ranging from cool purple and blue to red and hot white correspond with the increasing brightness of the X-rays. The image was created using X-ray data collected by IXPE between Jan. 11-18. (NASA)

A key measurement that scientists will make with IXPE is called polarization, a way of looking at how X-ray light is oriented as it travels through space. The polarization of light contains clues to the environment where the light originated. IXPE's instruments also measure the energy, the time of arrival, and the position in the sky of the X-rays from cosmic sources.

"The IXPE image of Cassiopeia A is bellissima, and we look forward to analyzing the polarimetry data to learn even more about this supernova remnant," said Paolo Soffitta, the Italian principal investigator for IXPE at the National Institute of Astrophysics (INAF) in Rome.

With polarization data from Cassiopeia A, IXPE will allow scientists to see, for the first time, how the amount of polarization varies across the supernova remnant, which is about 10 light-years in diameter. Researchers are currently working with the data to create the first-ever X-ray polarization map of the object. This will reveal new clues about how X-rays are produced at Cassiopeia A.

"IXPE's future polarization images should unveil the mechanisms at the heart of this famous cosmic accelerator," said Roger Romani, an IXPE co-investigator at Stanford University. "To fill in some of those details, we've developed a way to make IXPE's measurements even more precise using machine learning techniques. We're looking forward to what we'll find as we analyze all the data."

IXPE launched on a Falcon 9 rocket from Cape Canaveral, and now orbits 370 miles (600 kilometers) above Earth's equator. The mission is a collaboration between NASA and the Italian Space Agency with partners and science collaborators in 12 countries. Ball Aerospace, headquartered in Broomfield, Colorado, manages spacecraft operations.