Jump to content

NASA’s SpaceX Crew-8 Concludes Space Station Scientific Mission


Recommended Posts

  • Publishers
Posted

6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA astronauts Michael Barratt, Matthew Dominick, and Jeanette Epps and Roscosmos cosmonaut Alexander Grebenkin are returning to Earth after months aboard the International Space Station conducting scientific experiments and technology demonstrations for the agency’s SpaceX Crew-8 mission. The four launched on March 3 aboard a SpaceX Dragon spacecraft from NASA’s Kennedy Space Center in Florida.

Here’s a look at some scientific milestones accomplished during their mission:

Revealing resistant microorganisms

NASA astronaut Jeanette Epps extracts DNA for the Genomic Enumeration of Antibiotic Resistance in Space experiment, which surveys the station for antibiotic-resistant organisms and sequences their DNA to examine adaptations to space. Results could support development of measures to protect astronauts and people in buildings and facilities on Earth, such as hospitals, from resistant bacteria.

Epps, wearing a black t-shirt, pants, headband, and white gloves, uses a pipette to fill a rack of small vials. The rack sits on a blue metal work surface along with other equipment and cords. A laptop is attached to the Velcro strips on her pants leg.
NASA

Brain organoid models

NASA astronaut Mike Barratt processes samples for Human Brain Organoid Models for Neurodegenerative Disease & Drug Discovery. This investigation uses human brain organoids created with stem cells from patients to study neuroinflammation, a common feature of neurodegenerative conditions such as Parkinson’s disease. The organoids provide a platform to study these diseases and their treatments and to potentially address how extended spaceflight affects the brain.

Wearing a long-sleeved dark blue shirt, a headset, and glasses, Barratt is looking through the clear top of the Life Sciences Glovebox. His gloved hands inside the box hold two sample syringes, and two more are taped to the back wall of the box.
NASA

Bioprinting human tissues

Tissue samples bioprinted in microgravity are higher quality than those printed on the ground. NASA astronaut Matthew Dominick processes cardiac tissue samples for the Redwire Cardiac Bioprinting Investigation. Results could advance the production of organs and tissues for transplant and improve 3D printing of foods and medicines on future long-duration space missions.

Dominick, wearing a headlamp and black polo shirt with a US flag decal on the left sleeve, smiles at the camera. His arms are inside the plastic sleeves of a portable glovebox, and a laptop is visible just above and to the left of the glovebox.
NASA

Growing better drugs

NASA astronaut Mike Barratt works on Pharmaceutical In-space Laboratory – 02, which uses the station’s Advanced Space Experiments Processor to study how microgravity affects the production of various types of protein crystals. The ability to produce better crystals could lead to manufacturing improvements and new applications and better performance for pharmaceutical compounds, potentially providing more positive patient experiences.

Barratt is wearing a dark blue t-shirt, green pants, and a headset. He is peering at his hands inside the sleeves of a portable glovebox, holding a sample cassette, a silver box the size and shape of a briefcase.
NASA

Alloy solidification

NASA astronaut Jeanette Epps works on Materials Science Lab Batch 3a, two projects investigating the solidification of metallic alloys in space. Insights gained could help improve alloy solidification processes on the ground, supporting the development of materials with superior chemical and physical properties for applications in space and on Earth.

Wearing a long-sleeved black shirt and white gloves, Epps is smiling and holding a silver soup-can-sized canister in her left hand and guiding a long silver rod attached to it into an opening in the Material Science Laboratory, a metal circular device with white plastic edging.
NASA

Fueling the flames

The Solid Fuel Ignition and Extinction- Growth and Extinction Limit investigation determines how fuel temperature affects material flammability. This image shows the fuel surface during a burn (the black part of the sphere) and the distance traveled by the flame (blue). Results could improve researchers’ understanding of fire growth and inform the development of optimal fire suppression techniques to protect crews on future missions.

An acrylic sphere hangs from a rod in the middle of this image, a bright blue flame arcing around the bottom of it. The sphere is mottled black on its lower two-thirds and smooth near its top. A greenish, unburned sphere hangs off to its left, and a bright green wire coil (the igniter) is visible in the lower foreground. The entire image is tinged green.
NASA

Very long-distance calls

NASA astronaut Jeanette Epps wraps up an ISS Ham Radio session on April 10, with students in Italy. The program connects students and enthusiasts with astronauts in space via amateur radio. Participants study space, radio waves, and related topics to prepare questions before their scheduled call.

Epps, smiling at the camera, is wearing a black t-shirt and headband, holding a tablet in her left hand and placing the mic on the wall-mounted ham radio with her right. A video camera is mounted just above it. The walls around her are covered in multiple cords, rails, and straps, and just over her right shoulder are several mission stickers on a wall.
NASA

Student robotics competition

For Astrobee-Zero Robotics, students compete to have their code control one of the space station’s Astrobee robots. The experience helps inspire the next generation of scientists, engineers, and explorers. NASA astronaut Mike Barratt works with the Astrobee robot named Bumble during operations for the project.

Barratt, wearing a long-sleeved blue shirt with an expedition patch on its chest, faces the camera. Just to his right floats Bumble, a cube-shaped robot about the size of a toaster oven. Its sides are black with a white panel in the middle that has camera lenses and two bright blue lights near the bottom. There is a laptop to his right.
NASA

Immune function in space

NASA astronaut Jeanette Epps prepares samples for Immunity Assay, a study of how spaceflight affects immune function. Previously, astronaut immune function could only be examined pre- and postflight, but a newly developed assay allows for testing during flight. This capability provides a more precise assessment of the immune changes that happen in space.

Epps wears a red t-shirt, black pants, and white gloves. She is holding a large syringe in her right hand and is using a blue clip in her left hand to attach a sample tube to the blue lab work table. There are multiple plastic bags across the front of the table and a cluster of pink bags on its upper right. The wall behind it holds various supplies, such as tape, scissors, and pens.
NASA

Getting weighed in weightlessness

The Space Linear Acceleration Mass Measurement Device calculates a crew member’s mass based on Newton’s Second Law of Motion, which states force equals mass times acceleration. NASA astronaut Matthew Dominick performs maintenance on the device, used in support of multiple NASA and ESA (European Space Agency) investigations on how spaceflight affects the body.

Dominick, wearing a red t-shirt and dark green pants, is looking down and smiling. In front of him is a square silver brace with blue padding on its end with silver arms extending above and below it, also with blue padding. Above the brace is a large schematic poster showing how to use the device, and a laptop is mounted off to the left.
NASA

Satellites for science

NASA astronaut Mike Barratt prepares for the Nanoracks Cubesat Deployer Mission 27on April 16. The mission deployed seven research satellites: a reflectometer to measure sea ice, tests of telemetry instruments and solar cells, a hyperspectral thermal imager, a gamma-ray burst detector, a new remote sensing technique, and a magnetic field measurement test.

Barratt, wearing a long-sleeved black shirt, khaki pants, and white gloves, looks at the camera and gestures at the hardware in front of him, two large rectangular drawers mounted sideways on a rack extending out from a circular hatch behind him. The open door of the hatch is to his left, and the blue and yellow boxy Astrobee robots are attached to their docks on the wall to his right.
NASA

Remote-controlled robots

NASA astronaut Jeanette Epps remotely manipulates a robot on the ground for Surface Avatar. The investigation tests system ergonomics, operator response to feedback, and the potential challenges for actual orbit-to-ground remote control. Such operation is an important capability for future exploration missions to the Moon and Mars.

Epps wears a long-sleeved black shirt and a headset and uses her right hand to interact with a laptop mounted to the wall in front of her. On the screen is a simulation of a robot operating on a planetary surface.
NASA

The power of photographs

NASA astronauts Mike Barratt, Matthew Dominick, and Loral O’Hara take photographs in the station’s cupola, adding to the more than 4.7 million images produced for Crew Earth Observations. These images support scientific studies on topics ranging from aquatic organisms and icebergs to the effects of artificial lighting at night and inform the response of decision-makers to natural disasters such as volcanoes and floods.

Three astronauts, all wearing black, are facing the camera in the cupola, where Earth is visible through the window above them. Barratt, on the left, holds a handrail with his left hand and points a camera toward Earth with his right hand, squinting his left eye. Dominick, center, smiles up at the window, and O’Hara, on the right, uses both hands to point a camera with a large lens at Earth. The camera obscures her face.
NASA

Reflections on the Moon

For Earthshine from ISS, astronauts photograph the Moon throughout the lunar cycle to study changes in the light it reflects from Earth. Results could help validate the concept of observing Earth’s climate from satellite-borne instruments and add to researchers’ understanding of how the planet’s climate is changing.

The Moon is a bright white crescent in the center of this image, surrounded by the blackness of space.
NASA

Packing a Dragon

NASA astronauts Matthew Dominick and Tracy C. Dyson pack frozen samples into the SpaceX Dragon spacecraft for return to Earth and analysis by researchers. The spacecraft launched to the orbiting laboratory on March 21 for NASA’s SpaceX 30th commercial resupply services mission, carrying scientific experiments and supplies, and returned to Earth on April 30.

Dominick, in the foreground, is wearing a blue t-shirt and special black and blue gloves, facing the camera, and holding one of the cold storage trays, a silver metal basket the size of a cat carrier. Behind him is Dyson, wearing a red t-shirt and the same kind of gloves and holding a black box between her hands. Four circular doors to the cold stowage unit are on the wall in front of Dominick.
NASA

Cygnus delivers

Northrop Grumman’s Cygnus cargo spacecraft attached to the Canadarm2 robotic arm before being released from the space station on July 12. NASA’s Northrop Grumman 20th commercial resupply services mission arrived Feb. 1 with experiments on 3D printing, robotic surgery, tissue cartilage, and more.

At the top of the image are the curved silver undersides of three of the space station’s modules. A long, jointed robotic arm extends down from the module on the right. Attached to its end is the silver cylindrical spacecraft with two round, gold solar panels on either side. The blue Earth is visible to the left, and sunlight glints off Cygnus.
NASA

Melissa Gaskill

International Space Station Research Communications Team

NASA’s Johnson Space Center

Download high-resolution photos and videos of the research mentioned in this article. Search this database of scientific experiments to learn more about those mentioned in this article.

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • By NASA
      Credit: NASA NASA has selected SpaceX of Starbase, Texas, to provide launch services for the Near-Earth Object (NEO) Surveyor mission, which will detect and observe asteroids and comets that could potentially pose an impact threat to Earth.
      The firm fixed price launch service task order is being awarded under the indefinite delivery/indefinite quantity NASA Launch Services II contract. The total cost to NASA for the launch service is approximately $100 million, which includes the launch service and other mission related costs. The NEO Surveyor mission is targeted to launch no earlier than September 2027 on a SpaceX Falcon 9 rocket from Florida.
      The NEO Surveyor mission consists of a single scientific instrument: an almost 20-inch (50-centimeter) diameter telescope that will operate in two heat-sensing infrared wavelengths. It will be capable of detecting both bright and dark asteroids, the latter being the most difficult type to find with existing assets. The space telescope is designed to help advance NASA’s planetary defense efforts to discover and characterize most of the potentially hazardous asteroids and comets that come within 30 million miles of Earth’s orbit. These are collectively known as near-Earth objects, or NEOs.
      The mission will carry out a five-year baseline survey to find at least two-thirds of the unknown NEOs larger than 140 meters (460 feet). These are the objects large enough to cause major regional damage in the event of an Earth impact. By using two heat-sensitive infrared imaging channels, the telescope can also make more accurate measurements of the sizes of NEOs and gain information about their composition, shapes, rotational states, and orbits.
      The mission is tasked by NASA’s Planetary Science Division within the agency’s Science Mission Directorate at NASA Headquarters in Washington. Program oversight is provided by NASA’s Planetary Defense Coordination Office, which was established in 2016 to manage the agency’s ongoing efforts in planetary defense. NASA’s Planetary Missions Program Office at the agency’s Marshall Space Flight Center in Huntsville, Alabama, provides program management for NEO Surveyor. The project is being developed by NASA’s Jet Propulsion Laboratory in Southern California.
      Multiple aerospace and engineering companies are contracted to build the spacecraft and its instrumentation, including BAE Systems SMS (Space & Mission Systems), Space Dynamics Laboratory, and Teledyne. The Laboratory for Atmospheric and Space Physics at the University of Colorado, Boulder, will support operations, and the Infrared Processing and Analysis Center at the California Institute of Technology (Caltech) in Pasadena, California, is responsible for processing survey data and producing the mission’s data products. Caltech manages JPL for NASA. Mission team leadership includes the University of California, Los Angeles. NASA’s Launch Services Program at the agency’s Kennedy Space Center in Florida is responsible for managing the launch service.
      For more information about NEO Surveyor, visit:
      https://science.nasa.gov/mission/neo-surveyor/
      -end-
      Tiernan Doyle / Joshua Finch
      Headquarters, Washington
      202-358-1600 / 202-358-1100
      tiernan.doyle@nasa.gov / joshua.a.finch@nasa.gov
      Patti Bielling
      Kennedy Space Center, Florida
      321-501-7575
      patricia.a.bielling@nasa.gov
      Share
      Details
      Last Updated Feb 21, 2025 LocationNASA Headquarters Related Terms
      Kennedy Space Center Launch Services Office Launch Services Program NEO Surveyor (Near-Earth Object Surveyor Space Telescope) Planetary Defense Coordination Office Planetary Science Division Science Mission Directorate Space Operations Mission Directorate View the full article
    • By NASA
      Gateway’s HALO (Habitation and Logistics Outpost) in a cleanroom at Thales Alenia Space in Turin, Italy. After final installations are complete, it will be packaged and transported to the United States for final outfitting before being integrated with Gateway’s Power and Propulsion Element and launched to lunar orbit. Thales Alenia Space Through the Artemis campaign, NASA will send astronauts on missions to and around the Moon. The agency and its international partners report progress continues on Gateway, the first space station that will permanently orbit the Moon, after visiting the Thales Alenia Space facility in Turin, Italy, where initial fabrication for one of two Gateway habitation modules is nearing completion.
      Leaders from NASA, ESA (European Space Agency), and the Italian Space Agency, as well as industry representatives from Northrop Grumman and Thales Alenia Space, were in Turin to assess Gateway’s HALO (Habitation and Logistics Outpost) module before its primary structure is shipped from Italy to Northrop Grumman’s Gilbert, Arizona site in March. Following final outfitting and verification testing, the module will be integrated with the Power and Propulsion Element at NASA’s Kennedy Space Center in Florida.
      “Building and testing hardware for Gateway is truly an international collaboration,” said Jon Olansen, manager, Gateway Program, at NASA’s Johnson Space Center in Houston. “We’re excited to celebrate this major flight hardware milestone, and this is just the beginning – there’s impressive and important progress taking shape with our partners around the globe, united by our shared desire to expand human exploration of our solar system while advancing scientific discovery.”
      Gateway’s HALO (Habitation and Logistics Outpost) in a cleanroom at Thales Alenia Space in Turin, Italy. After final installations are complete, it will be packaged and transported to the United States for final outfitting before being integrated with Gateway’s Power and Propulsion Element and launched to lunar orbit.Thales Alenia Space To ensure all flight hardware is ready to support Artemis IV — the first crewed mission to Gateway – NASA is targeting the launch of HALO and the Power and Propulsion Element no later than December 2027. These integrated modules will launch aboard a SpaceX Falcon Heavy rocket and spend about a year traveling uncrewed to lunar orbit, while providing scientific data on solar and deep space radiation during transit.
      Launching atop HALO will be ESA’s Lunar Link communication system, which will provide high-speed communication between the Moon and Gateway. The system is undergoing testing at another Thales Alenia Space facility in Cannes, France.
      Once in lunar orbit, Gateway will continue scientific observations while awaiting the arrival of Artemis IV astronauts aboard an Orion spacecraft which will deliver and dock Gateway’s second pressurized habitable module, the ESA-led Lunar I-Hab. Thales Alenia Space, ESA’s primary contractor for the Lunar I-Hab and Lunar View refueling module, has begun production of the Lunar I-Hab, and design of Lunar View in Turin.
      Teams from NASA and ESA (European Space Agency), including NASA astronaut Stan Love (far right) and ESA astronaut Luca Parmitano (far left) help conduct human factors testing inside a mockup of Gateway’s Lunar I-Hab module.Thales Alenia Space Northrop Grumman and its subcontractor, Thales Alenia Space, completed welding of HALO in 2024, and the module successfully progressed through pressure and stress tests to ensure its suitability for the harsh environment of deep space.
      Maxar Space Systems is assembling the Power and Propulsion Element, which will make Gateway the most powerful solar electric propulsion spacecraft ever flown. Major progress in 2024 included installation of Xenon and chemical propulsion fuel tanks, and qualification of the largest roll-out solar arrays ever built. NASA and its partners will complete propulsion element assembly, and acceptance and verification testing of next-generation electric propulsion thrusters this year.
      The main bus of Gateway’s Power and Propulsion Element undergoes assembly and installations at Maxar Space Systems in Palo Alto, California.Maxar Space Systems SpaceX will provide both the Starship human landing system that will land astronauts on the lunar surface during NASA’s Artemis III mission and ferry astronauts from Gateway to the lunar South Pole region during Artemis IV, as well as provide logistics spacecraft to support crewed missions.
      NASA also has selected Blue Origin to develop Blue Moon, the human landing system for Artemis V, as well as logistics spacecraft for future Artemis missions. Having two distinct lunar landing designs provides flexibility and supports a regular cadence of Moon landings in preparation for future missions to Mars.
      CSA (Canadian Space Agency) is developing Canadarm3, an advanced robotics system, and JAXA (Japan Aerospace Exploration Agency) is designing and testing Lunar I-Hab’s vital life support systems, batteries, and a resupply and logistics vehicle called HTV-XG.
      NASA’s newest Gateway partner, the Mohammad Bin Rashid Space Centre (MBRSC) of the United Arab Emirates, kicked off early design for the Gateway Crew and Science Airlock that will be delivered on Artemis VI. The selection of Thales Alenia Space as its airlock prime contractor was announced by MBRSC on Feb. 4.
      Development continues to advance on three radiation-focused initial science investigations aboard Gateway. These payloads will help scientists better understand unpredictable space weather from the Sun and galactic cosmic rays that will affect astronauts and equipment during Artemis missions to the Moon and beyond.
      The Gateway lunar space station is a multi-purpose platform that offers capabilities for long-term exploration in deep space in support of NASA’s Artemis campaign and Moon to Mars objectives. Gateway will feature docking ports for a variety of visiting spacecraft, as well as space for crew to live, work, and prepare for lunar surface missions. As a testbed for future journeys to Mars, continuous investigations aboard Gateway will occur with and without crew to better understand the long-term effects of deep space radiation on vehicle systems and the human body as well as test and operate next generation spacecraft systems that will be necessary to send humans to Mars.
      Learn More About Gateway Facebook logo @NASAGateway @NASA_Gateway Instagram logo @nasaartemis Share
      Details
      Last Updated Feb 21, 2025 ContactLaura RochonLocationJohnson Space Center Related Terms
      Artemis Artemis 4 Earth's Moon Exploration Systems Development Mission Directorate Gateway Space Station Humans in Space Johnson Space Center Explore More
      2 min read Lunar Space Station Module Will Journey to US ahead of NASA’s Artemis IV Moon Mission
      A key element of the Gateway lunar space station has entered the cleanroom for final…
      Article 1 week ago 2 min read Advanced Modeling Enhances Gateway’s Lunar Dust Defense
      Ahead of more frequent and intense contact with dust during Artemis missions, NASA is developing…
      Article 1 month ago 2 min read Gateway Tops Off
      Gateway’s Power and Propulsion Element is now equipped with its xenon and liquid fuel tanks.
      Article 3 months ago Keep Exploring Discover More Topics From NASA
      Humans In Space
      Orion Spacecraft
      Human Landing System
      Extravehicular Activity and Human Surface Mobility
      View the full article
    • By NASA
      Live Video from the International Space Station (Official NASA Stream)
    • By NASA
      Live High-Definition Views from the International Space Station (Official NASA Stream)
    • By NASA
      6 Min Read NASA’s PUNCH Mission to Revolutionize Our View of Solar Wind 
      Earth is immersed in material streaming from the Sun. This stream, called the solar wind, is washing over our planet, causing breathtaking auroras, impacting satellites and astronauts in space, and even affecting ground-based infrastructure. 
      NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission will be the first to image the Sun’s corona, or outer atmosphere, and solar wind together to better understand the Sun, solar wind, and Earth as a single connected system.  
      Launching no earlier than Feb. 28, 2025, aboard a SpaceX Falcon 9 rocket from Vandenberg Space Force Base in California, PUNCH will provide scientists with new information about how potentially disruptive solar events form and evolve. This could lead to more accurate predictions about the arrival of space weather events at Earth and impact on humanity’s robotic explorers in space. 
      “What we hope PUNCH will bring to humanity is the ability to really see, for the first time, where we live inside the solar wind itself,” said Craig DeForest, principal investigator for PUNCH at Southwest Research Institute’s Solar System Science and Exploration Division in Boulder, Colorado. 
      This video can be freely shared and downloaded at https://svs.gsfc.nasa.gov/14773.
      Video credit: NASA’s Goddard Space Flight Center Seeing Solar Wind in 3D 
      The PUNCH mission’s four suitcase-sized satellites have overlapping fields of view that combine to cover a larger swath of sky than any previous mission focused on the corona and solar wind. The satellites will spread out in low Earth orbit to construct a global view of the solar corona and its transition to the solar wind. They will also track solar storms like coronal mass ejections (CMEs). Their Sun-synchronous orbit will enable them to see the Sun 24/7, with their view only occasionally blocked by Earth.  
      Typical camera images are two dimensional, compressing the 3D subject into a flat plane and losing information. But PUNCH takes advantage of a property of light called polarization to reconstruct its images in 3D. As the Sun’s light bounces off material in the corona and solar wind, it becomes polarized — meaning the light waves oscillate in a particular way that can be filtered, much like how polarized sunglasses filter out glare off of water or metal. Each PUNCH spacecraft is equipped with a polarimeter that uses three distinct polarizing filters to capture information about the direction that material is moving that would be lost in typical images.  
      “This new perspective will allow scientists to discern the exact trajectory and speed of coronal mass ejections as they move through the inner solar system,” said DeForest. “This improves on current instruments in two ways: with three-dimensional imaging that lets us locate and track CMEs which are coming directly toward us; and with a broad field of view, which lets us track those CMEs all the way from the Sun to Earth.” 
      All four spacecraft are synchronized to serve as a single “virtual instrument” that spans the whole PUNCH constellation. 
      Crews conduct additional solar array deployment testing for NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) satellites at Astrotech Space Operations located on Vandenberg Space Force Base in California on Wednesday, Jan. 22, 2025. USSF 30th Space Wing/Alex Valdez The PUNCH satellites include one Narrow Field Imager and three Wide Field Imagers. The Narrow Field Imager (NFI) is a coronagraph, which blocks out the bright light from the Sun to better see details in the Sun’s corona, recreating what viewers on Earth see during a total solar eclipse when the Moon blocks the face of the Sun — a narrower view that sees the solar wind closer to the Sun. The Wide Field Imagers (WFI) are heliospheric imagers that view the very faint, outermost portion of the solar corona and the solar wind itself — giving a wide view of the solar wind as it spreads out into the solar system.   
      “I’m most excited to see the ‘inbetweeny’ activity in the solar wind,” said Nicholeen Viall, PUNCH mission scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “This means not just the biggest structures, like CMEs, or the smallest interactions, but all the different types of solar wind structures that fill that in between area.” 
      When these solar wind structures from the Sun reach Earth’s magnetic field, they can drive dynamics that affect Earth’s radiation belts. To launch spacecraft through these belts, including ones that will carry astronauts to the Moon and beyond, scientists need to understand the solar wind structure and changes in this region. 
      Building Off Other Missions 
      “The PUNCH mission is built on the shoulders of giants,” said Madhulika Guhathakurta, PUNCH program scientist at NASA Headquarters in Washington. “For decades, heliophysics missions have provided us with glimpses of the Sun’s corona and the solar wind, each offering critical yet partial views of our dynamic star’s influence on the solar system.” 
      When scientists combine data from PUNCH and NASA’s Parker Solar Probe, which flies through the Sun’s corona, they will see both the big picture and the up-close details. Working together, Parker Solar Probe and PUNCH span a field of view from a little more than half a mile (1 kilometer) to over 160 million miles (about 260 million kilometers). 
      Additionally, the PUNCH team will combine their data with diverse observations from other missions, like NASA’s CODEX (Coronal Diagnostic Experiment) technology demonstration, which views the corona even closer to the surface of the Sun from its vantage point on the International Space Station. PUNCH’s data also complements observations from NASA’s EZIE (Electrojet Zeeman Imaging Explorer) — targeted for launch in March 2025 — which investigates the magnetic field perturbations associated with Earth’s high-altitude auroras that PUNCH will also spot in its wide-field view.  
      A conceptual animation showing the heliosphere, the vast bubble that is generated by the Sun’s magnetic field and envelops all the planets.
      NASA’s Goddard Space Flight Center Conceptual Image Lab As the solar wind that PUNCH will observe travels away from the Sun and Earth, it will then be studied by the IMAP (Interstellar Mapping and Acceleration Probe) mission, which is targeting a launch in 2025. 
      “The PUNCH mission will bridge these perspectives, providing an unprecedented continuous view that connects the birthplace of the solar wind in the corona to its evolution across interplanetary space,” said Guhathakurta. 
      The PUNCH mission is scheduled to conduct science for at least two years, following a 90-day commissioning period after launch. The mission is launching as a rideshare with the agency’s next astrophysics observatory, SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer).  
      “PUNCH is the latest heliophysics addition to the NASA fleet that delivers groundbreaking science every second of every day,” said Joe Westlake, heliophysics division director at NASA Headquarters in Washington. “Launching this mission as a rideshare bolsters its value to the nation by optimizing every pound of launch capacity to maximize the scientific return for the cost of a single launch.” 
      The PUNCH mission is led by Southwest Research Institute’s offices in San Antonio, Texas, and Boulder, Colorado. The mission is managed by the Explorers Program Office at NASA Goddard for NASA’s Science Mission Directorate in Washington. 
      By Abbey Interrante 
      NASA’s Goddard Space Flight Center, Greenbelt, Md. 
      Header Image:
      An artist’s concept showing the four PUNCH satellites orbiting Earth.
      Credits: NASA’s Goddard Space Flight Center Conceptual Image Lab
      Share








      Details
      Last Updated Feb 21, 2025 Related Terms
      Heliophysics Coronal Mass Ejections Goddard Space Flight Center Heliophysics Division Polarimeter to Unify the Corona and Heliosphere (PUNCH) Science Mission Directorate Solar Wind Space Weather The Sun Explore More
      2 min read Hubble Spies a Spiral That May Be Hiding an Imposter


      Article


      3 hours ago
      3 min read Eclipses to Auroras: Eclipse Ambassadors Experience Winter Field School in Alaska


      Article


      3 days ago
      2 min read NASA Science: Being Responsive to Executive Orders


      Article


      3 days ago
      Keep Exploring Discover More Topics From NASA
      Missions



      Humans in Space



      Climate Change



      Solar System


      View the full article
  • Check out these Videos

×
×
  • Create New...