Integrating Model-Based Systems Engineering and Fault Management to Enable Autonomous Space Missions

Integrating Model-Based Systems Engineering and Fault Management to Enable Autonomous Space Missions

Fully autonomous space mission operations require the ability to detect faults and compensate for them without human intervention. To address this challenge and provide model-based support for system design and operations, it is important to connect fault management (FM) and model-based systems engineering (MBSE). This approach was successfully demonstrated with the model-based generation of a failure modes and effects analysis and fault trees using NASA’s HelioSwarm mission early design information.

A group of nine satellites consisting of one hub surrounded by eight small satellites.
Artist’s conception of the future HelioSwarm mission in orbit.
Credit: HelioSwarm Project Team

As NASA strives to push the boundaries of space travel with the Artemis program and the agency’s upcoming deep-space science missions, increased system autonomy and resiliency have inevitably become key technology needs. Autonomous operations require fault management (FM) software to detect issues that occur in space so they can be mitigated automatically without human intervention. Designing autonomous missions requires a multi-disciplinary approach that connects FM with the model-based systems engineering (MBSE) approach used in mission design to ensure that resilient, fault-tolerant systems are architected, modeled, and integrated during the design phase.

To address this need, NASA awarded a Phase II Small Business Innovation Research (SBIR) contract to Qualtech Systems Inc. (QSI) for development of FM capabilities and enhancements to its commercially available toolset, TEAMS® (a product that resulted from commercialization of the company’s earlier NASA-sponsored SBIR work), to support HelioSwarm and other NASA heliophysics missions.

The QSI Approach

One of the most important tasks in this effort was to connect system health management (SHM) and FM to the systems engineering (SE) process. Together, SHM/FM consists of a set of mechanisms that ensure that mission goals are achieved by preventing failures from occurring, or detecting and then mitigating them if they do occur. The SE process coordinates, cross-checks, and integrates system elements to achieve mission goals and is integral during the design, specification, and verification and validation (V&V) of systems. NASA often employs a model-based approach for its SE process, using Systems Modeling Language (SysML) as the framework.

Despite their inherently close relationship to SE in practice, SHM/FM practices have typically not been tightly integrated with SE. Often, SHM/FM is incorporated only after a nominal system is designed, which essentially makes SHM/FM a bandage fix for problems after they occur, without considering how issues might have been prevented. In addition, SE and SHM/FM often involve separate sets of subject matter experts with stove-piped knowledge repositories. This situation can lead to use of modeling methodologies and analyses processes that yield inconsistent results, and can potentially result in inefficiencies throughout the mission life cycle.

This NASA-funded QSI team’s approach integrates SHM/FM directly within the MBSE process from the beginning of a project. This method enables the FM design to be evaluated in an operational context by showing how the SHM/FM schemes mitigate the effects of simulated component-level physical and functional failures. This technique also facilitates trade studies to evaluate the merits of various FM architectures during the design phase.

Under this SBIR effort, QSI worked with the SysML v2 Submission Team (SST) — an assorted group of end users, vendors, academics, and government liaisons involved in the development of specifications for SysML v2, which is the latest iteration of SysML. The QSI team incorporated FM concepts and modeling standards into SysML v2, then they demonstrated how SysML v2 models could translate to the failure space models produced by the QSI toolset.

This capability enables systems engineers to use QSI’s commercial modeling tool set andanalyze the FM aspects of a system design captured in SysML v2. By capturing the causes and impacts of failures, QSI’s toolset enables mission designers to perform Fault Modes, Effects, and Criticality Analyses (FMECAs) and Fault Tree Analyses (FTAs) to analyze, quantify, and improve the diagnostics and availability of the system. Furthermore, the toolset recommends design improvements (e.g., optimal location of sensors onboard the spacecraft) based on the results from such analyses, and it provides these recommendations in industry-standard formats that can be easily understood and incorporated into the design.

During this SBIR effort, theQSI toolset was also enhanced to interface with an MBSE framework and facilitate the creation, evaluation, and selection of FM concepts for a mission design. The toolset now enables FM concepts to be tested early in the design process so that adequate detection and diagnosis can be built into the system design, which could potentially lower the total cost of development, facilitate enhanced communication and coordination among mission team members, and reduce development risks (cost and schedule).

The HelioSwarm Demonstration

HelioSwarm will transform our understanding of turbulence in the solar wind and the connected Sun–Earth system. The mission uses a constellation, or “swarm,” of one hub and eight co-orbiting small satellites to make the first simultaneous, multiscale measurements of magnetic-field fluctuations and proton flows in the dynamic cislunar space environment. Because plasma turbulence transfers energy across many scales, from fluid-scale motions to kinetic-scale particle dynamics, it cannot be fully understood from a single measurement point, or from measurements at only a single scale. HelioSwarm’s spacecraft will fly with separations ranging from tens to thousands of kilometers, allowing scientists to reconstruct the three-dimensional structure and dynamics of turbulent space plasma. These observations will reveal how energy moves through the solar wind, transforming our understanding of fundamental plasma processes that operate near Earth, around the Sun, and throughout the universe.

Plasma turbulence is the process by which energy contained in fluctuating magnetic fields and plasma motion cascades from large to smaller spatial scales. When the cascade approaches small spatial scales associated with kinetic dissipation, the energy transfers into particle heat. Without turbulent cascades in space plasmas, most of the universe would be far colder than observed. Because of the fundamental thermodynamic role it plays in fluids, including space plasmas, many contend that turbulent fluids are the most important unsolved problem in classical physics.

The QSI team created a SysML v2 design model of HelioSwarm subsystems and top-level mission requirements, capturing the flowdown from mission goals to the design. The team then used its enhanced toolset to translate the HelioSwarm SysML v2 model into an FM model. The HelioSwarm models consist of key subsystems of the hub spacecraft and eight node satellites, including subsystems for command and data handling; electric power; attitude control; propulsion, thermal, and separation hardware payload sensors; and ground and space communications. Using the QSI toolset, mission designers then generated FMECAs and FTAs that were translated into a standardized SysML report. Furthermore, these FM analyses generated recommendations (e.g., for sensor placement) that were provided as proposed updates to the system design. This process will support the design of small spacecraft swarms with inherent redundancy to enhance science observations and other NASA goals, such as providing mission support for lunar surface operations.

Relevance to future NASA missions and non-NASA applications

The technology developed via this latest SBIR effort could be of high value for future NASA missions — especially those that require autonomous operation. The QSI TEAMS® toolset was baselined for Vehicle Systems Management functions on NASA’s Gateway project and retains applicability to future human-rated spacecraft. System design engineers could use this technology to incorporate fault mitigation strategies to improve design with additional insight into the overall system resilience — right at the beginning of the design phase.

This technology may also have applications outside of NASA. Comprehensive and efficient FM analyses and architecture trade studies are of critical importance to complex and high-value military systems such as aircraft, surface ships, submarines, and even modern ground-fighting vehicles. Additionally, this technology could be applicable to emerging commercial space systems, civilian aircraft and maritime systems, transportation, and power generation and distribution equipment.
 
For additional details about this effort, see the relevant TechPort entries: here, here, and here.
Project Lead(s): Dr. Sudipto Ghoshal, Mr. Deepak Haste, Qualtech Systems, Inc.
Sponsoring Organization(s): NASA Ames Research Center

Share

Details

Last Updated
Aug 25, 2026
Editor
NASA Science Editorial Team

Powered by WPeMatico

Get The Details…

NASA, ESA Astronauts Suiting Up for Antenna Installation Spacewalk

NASA, ESA Astronauts Suiting Up for Antenna Installation Spacewalk

Astronauts Anil Menon of NASA and Sophie Adenot of ESA pose for their official portraits while wearing spacesuits at the Johnson Space Center in Houston, Texas.
Astronauts Anil Menon of NASA and Sophie Adenot of ESA pose for their official portraits while wearing spacesuits at the Johnson Space Center in Houston, Texas.
NASA

NASA is streaming live coverage as two astronauts prepare for a spacewalk outside the International Space Station. The spacewalk is scheduled to begin at approximately 8:35 a.m. EDT and last about six and a half hours. Watch online at: https://www.nasa.gov/live

NASA astronaut Anil Menon and ESA (European Space Agency) astronaut Sophie Adenot will step outside the station’s Quest airlock to continue the installation of a replacement Space‑to‑Ground antenna. The antenna is a critical link that enables high‑speed data transmission between NASA’s Mission Control Center in Houston and the space station. 

During a 6‑hour, 23‑minute spacewalk on Aug. 18, Menon and Adenot removed a failed Space‑to‑Ground antenna and secured it to the station’s truss structure. The astronauts needed more time than expected to disconnect electrical cables and loosen bolts, delaying installation of the replacement antenna.  

Menon will serve as crew member 1 in the suit with red stripes, while Adenot will serve as crew member 2 in an unmarked suit.

U.S. spacewalk 98 will be Menon’s third and Adenot’s second. It also will be the 283rd spacewalk in support of space station assembly, maintenance, and upgrades. 

Learn more about station activities by following the space station blog, @space_station on X, as well as the ISS Facebook and ISS Instagram accounts.

Get the latest from NASA delivered every week. Subscribe here.

Powered by WPeMatico

Get The Details…

Mark A. Garcia

NASA Sets Coverage for Roman Space Telescope Launch from Florida

NASA Sets Coverage for Roman Space Telescope Launch from Florida

NASA’s Nancy Grace Roman Space Telescope is encapsulated within the payload fairing at the agency’s Kennedy Space Center in Florida, ahead of mating to a SpaceX Falcon Heavy rocket for launch.
Credit: NASA/Sydney Rohde (Rocz)

Coverage plans are ready for NASA’s Nancy Grace Roman Space Telescope prelaunch and launch activities. Roman is NASA’s next-generation observatory designed to explore some of the universe’s biggest mysteries, including dark energy.

NASA and SpaceX are targeting Roman’s liftoff for no earlier than 7:26 a.m. EDT Sunday, Aug. 30, aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida. Launch coverage begins at 6:20 a.m.

Live coverage of these events will stream through a variety of platforms. Learn where to watch online:

https://www.nasa.gov/live

Named for NASA’s first chief astronomer, the Nancy Grace Roman Space Telescope will pair sharp infrared vision with a field of view at least 100 times larger than the agency’s Hubble Space Telescope. Its crisp, sweeping surveys will help scientists investigate dark energy and dark matter, discover and characterize exoplanets, map billions of galaxies, study black holes, and explore objects from our own solar system to the edge of the observable universe.

After launch and separation from the rocket, Roman will travel to the second Sun-Earth Lagrange point, or L2, about one million miles from Earth. The mission has a five-year primary lifetime with a goal of operating for 10 years, and Roman’s science data will be publicly available after processing.

NASA’s mission coverage is as follows (all times are Eastern and subject to change based on real-time operations):

Saturday, Aug. 29

9 a.m.: NASA’s Roman Space Telescope Mission Science Briefing: The briefing will take place in the NASA Kennedy Press Site auditorium with the following participants:

  • Shawn Domagal-Goldman, director, Astrophysics Division, NASA Headquarters
  • Julie McEnery, Roman telescope senior project scientist, NASA Goddard Space Flight Center
  • Vanessa Bailey, Roman Coronagraph Instrument scientist, NASA Jet Propulsion Laboratory
  • Kristen McQuinn, Roman Science Operations Center lead, Space Telescope Science Institute
  • Lee Armus, Roman Science Support Center lead, Caltech/IPAC

Media may ask questions in person or by phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the NASA Kennedy newsroom no later than one hour before the briefing at: ksc-newsroom@mail.nasa.gov.

10:30 a.m.: NASA’s Roman Space Telescope Prelaunch News Conference: The news conference will take place in the NASA Kennedy Press Site auditorium with the following participants:

  • Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters
  • Lucas Paganini, Roman telescope program executive, NASA Headquarters
  • Jackie Townsend, Roman telescope project manager, NASA Goddard
  • Denton Gibson, launch director, NASA’s Launch Services Program, NASA Kennedy
  • Julianna Scheiman, director, NASA Science and Dragon Programs, SpaceX
  • Justin McReynolds, launch weather officer, 45th Weather Squadron, U.S. Space Force

Media may ask questions in person or by phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the NASA Kennedy newsroom no later than one hour before the briefing at: ksc-newsroom@mail.nasa.gov.

11:45 a.m.: NASA Administrator Jared Isaacman is expected to fly past the Nancy Grace Roman Space Telescope and Falcon Heavy rocket on the launchpad in his jet. The flyby will be shown live on the same stream as the prelaunch news conference, with a view of the launch pad during the transition. The flyby is subject to weather and operational considerations.

12 p.m.: In-person interviews will take place in the NASA Kennedy Press News Center:

  • Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters
  • Lucas Paganini, Roman telescope program executive, NASA Headquarters
  • Dalia Kirschbaum, acting director, Sciences and Exploration Directorate, NASA Goddard
  • Josh Schlieder, Roman telescope project scientist, NASA Goddard
  • Jason Hylan, Roman telescope flight segment and observatory manager, NASA Goddard
  • Bertrand Mennesson, Roman Coronagraph Instrument project scientist, NASA JPL
  • Jeff Hanke, president, Space Systems, Space and Mission Systems, L3Harris Technologies 
  • Wendy Minotti, program manager, Exquisite Imaging, Space and Mission Systems, L3Harris Technologies
  • Bonnie Patterson, vice president and general manager, Civil Space, Space and Mission Systems, BAE Systems
  • Sarah Lipscy, director, Strategic Operations, Space and Mission Systems, BAE Systems

Previously credentialed media interested in scheduling an interview should contact the NASA Kennedy newsroom at: ksc-newsroom@mail.nasa.gov.

Sunday, Aug. 30

6:20 a.m.: Launch coverage begins.

7:26 a.m.: Launch

9:30 a.m.: Postlaunch news conference with the following participants:

  • NASA Administrator Jared Isaacman
  • Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters
  • Jackie Townsend, Roman telescope project manager, NASA Goddard
  • Julie McEnery, Roman telescope senior project scientist, NASA Goddard
  • Denton Gibson, launch director, NASA’s Launch Services Program, NASA Kennedy

Media may ask questions in person or by phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the NASA Kennedy newsroom no later than one hour before the news conference at: ksc-newsroom@mail.nasa.gov.

Audio-only coverage

Audio-only coverage of the launch will be carried on the NASA “V” circuits, accessible by dialing 321-867-1220 or 321-867-1240. On launch day, mission audio countdown activities without NASA broadcast commentary will be carried on 321-867-7135.

Launch audio also will be available on Launch Information Service and Amateur Television System’s VHF radio frequency 146.940 MHz and KSC Amateur Radio Club’s UHF radio frequency 444.925 MHz, FM mode, heard within Brevard County on the Space Coast.

NASA website launch coverage

Launch day coverage will be available on the NASA website, including the livestream and blog updates as countdown milestones occur. On-demand streaming video and launch photos will be available shortly after liftoff. Follow mission updates on the Roman launch blog.

Attend launch virtually

Members of the public may register to attend the Roman launch virtually. NASA’s Virtual Guest Program includes curated launch resources, notifications about related opportunities or schedule changes, and a stamp for the NASA virtual guest passport following launch.

Watch, engage on social media

Let people know you’re watching the mission on X, Facebook, and Instagram by following and tagging these accounts:

The Roman telescope is managed at NASA Goddard with participation by the agency’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a team of scientists from various research institutions. The primary industrial partners are BAE Systems Inc., L3Harris Technologies, and Teledyne Scientific & Imaging. Contributions to Roman also are made by ESA (European Space Agency), JAXA (Japan Aerospace Exploration Agency), the French space agency CNES (Centre National d’Études Spatiales), and the Max Planck Institute for Astronomy in Germany. NASA’s Launch Services Program, based at Kennedy, manages the launch service for the Roman mission.

For more information about NASA’s Roman telescope, visit:

https://www.nasa.gov/roman

-end-

Alise Fisher
NASA Headquarters, Washington
202-385-1287
alise.m.fisher@nasa.gov

Leejay Lockhart
Kennedy Space Center, Fla.
321-747-8310
leejay.lockhart@nasa.gov

Claire Andreoli
Goddard Space Flight Center, Greenbelt, Md.
301-286-1940
claire.andreoli@nasa.gov

Powered by WPeMatico

Get The Details…
Jessica Taveau

Perseverance Captures Another Phobos Transit

Perseverance Captures Another Phobos Transit

2 Min Read

Perseverance Captures Another Phobos Transit

A dark, irregularly shaped silhouette transits across the lower right portion of a bright orange sun against a pitch-black sky.
PIA26811
Credits:
NASA/JPL-Caltech/ASU/MSSS/SSI

Description

NASA’s Perseverance Mars rover used its Mastcam-Z camera to capture the silhouette of Phobos, one of the two Martian moons, as it crossed in front of the Sun on Aug. 12, 2026, the 1,948th Martian day, or sol, of the mission. 

The animation has been tinted to simulate what a human would see if they were watching the transit from the Martian surface through protective solar eclipse glasses.  

Perseverance has captured several Phobos transits since its landing at Jezero Crater in February 2021. By comparing the various recordings, scientists can refine their understanding of the potato-shaped moon’’ orbit, learning how it is changing. Eons from now, Phobos’ orbit is expected to eventually send the moon toward the Red Planet’s surface.

Arizona State University leads the operations of the Mastcam-Z instrument, working in collaboration with Malin Space Science Systems in San Diego, on the design, fabrication, testing, and operation of the cameras, and in collaboration with the Niels Bohr Institute of the University of Copenhagen on the design, fabrication, and testing of the calibration targets.

NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.

For more about Perseverance: science.nasa.gov/mission/mars-2020-perseverance

Powered by WPeMatico

Get The Details…

Starstruck: NASA Research Shows How Sun’s Ancient History Shaped Earth

Starstruck: NASA Research Shows How Sun’s Ancient History Shaped Earth

6 Min Read

Starstruck: NASA Research Shows How Sun’s Ancient History Shaped Earth

At the center of our solar system, the Sun influences every planet that orbits it. In two recent NASA-funded studies, scientists uncovered how ancient events in the Sun’s history may have helped create Earth’s unique climate and driven previously unexplained climatic shifts.  

In new research, scientists at NASA’s SHIELD (Solar Wind with Hydrogen Ion charge Exchange and Large-Scale Dynamics) center — one of NASA’s DRIVE (Diversify, Realize, Integrate, Venture, Educate) Science Centers — trace the trajectory of the heliosphere, the massive bubble created by our Sun that envelops our solar system, as it moved through our galaxy and influenced Earth’s climate along the way. In another paper, a NASA scientist and coauthors investigate how the younger, dimmer Sun managed to heat Earth by seeding the production of potent greenhouse gases.

A Sun on the move 

Over the last tens of millions of years, Earth’s climate has undergone significant shifts, including notable ice ages in which the global average temperature temporarily dropped by several degrees. During these periods, more frequent climate swings led Earth to warm and cool. To explain these periods of warming and cooling, scientists looked to factors internal to Earth, including orbital changes, greenhouse gases, and ice. But new research suggests changes to the Sun’s environment may be key to understanding Earth’s temperature swings. 

Just as our planet is encased by an atmosphere, so our entire solar system is encased inside a kind of “atmosphere” created by the Sun. This protective bubble, known as the heliosphere, is formed by a continuous solar wind of charged particles streaming out from the Sun in all directions. 

This conceptual animation begins with a view of the Milky Way Galaxy. As we zoom in, we travel to the Local Interstellar Cloud, and then to the heliosphere, the protective bubble that surrounds our solar system. The heliosphere is formed by a continuous stream of charged particles from the Sun, called the solar wind.
NASA’s Goddard Space Flight Center Conceptual Image Lab

Our heliosphere orbits around the center of our galaxy, the Milky Way. Throughout the Sun’s 4.6-billion-year existence, our heliosphere has traversed various regions within our galaxy. In a paper published on Aug. 21 in Annual Review of Astronomy and Astrophysics, researchers at NASA’s SHIELD used computer modeling to reverse-engineer the path of the heliosphere through our galaxy, revealing that the environments it passed through may have triggered changes on Earth.   

Merav Opher, SHIELD’s principal investigator at Boston University, and her team ran simulations that showed the Sun has encountered frigid expanses of gas and dust at least three different times in the past few million years. In these instances, massive interstellar “cold clouds” pushed against the heliosphere to such an extent that it shrank to smaller than Earth’s orbit, stranding our planet outside the Sun’s protective shield. 

These exposures — approximately 2 to 3 million years, 6 to 7 million years, and 13 to 14 million years ago — would have exposed Earth’s atmosphere to totally different surroundings. The simulation results match geologic evidence: Elements prevalent in interstellar dust appear in deep-sea sediment core samples, Antarctic snow, and lunar samples during these timelines. 

This animated illustration shows Earth and the Sun protected by the heliosphere, the massive bubble created by our Sun. As our solar system traverses through the galaxy, encounters with massive interstellar “cold clouds” pushed against the heliosphere and caused the heliosphere to shrink past Earth, exposing the planet to cosmic radiation and elements from interstellar space.
NASA’s SHIELD DRIVE Science Center/Merav Opher/Harvard Radcliffe Institute

These heliosphere collapse events may also explain ancient climatic patterns on Earth. In the simulations, when Earth’s atmosphere was exposed to a cold, dense galactic hydrogen cloud, it increased water vapor content and shifted upper-atmospheric dynamics, ultimately altering the conditions at the surface. In summary, our heliosphere’s trips through colder regions in our galaxy may be a key factor in driving some of Earth’s ancient changes in climate, including possible ice ages.  

Next frontier in studying heliophysics 

The SHIELD center is one of several that NASA funds to unlock the next generation of heliospheric research. As a DRIVE Science Center, SHIELD builds a team of researchers with differing expertise, approaches, and opinions to develop a model, or “digital twin,” of the heliosphere that helps reveal how the heliosphere interacts with its surroundings, including dense interstellar clouds. Understanding our unique, habitable solar system will help unravel the mysteries of life’s evolution on Earth and potentially uncover other habitable star systems. 

Young Sun 

In another paper, Vladimir Airapetian, a scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, focuses on a long-standing mystery of how the ancient Sun warmed early Earth enough to sustain life. Three billion years ago, the young Sun was 70% as bright as it is today. Under these dimmer conditions, Earth should have been frozen solid. Yet geological evidence shows stable liquid water already existed long before that. This puzzle — a balmy Earth under a cooler, dimmer Sun — is known as the Faint Young Sun paradox.  

One clue to resolving the paradox comes from young Sun-like stars elsewhere in the galaxy. These “toddler” stars are prone to throwing fits. Specifically, data from NASA’s retired Kepler space telescope shows that young Sun-like stars regularly erupt with massive superflares, flinging high-energy particles in all directions on a daily basis. If our young Sun was like these other stars, Airapetian proposes, the barrage of high-energy solar particles could have triggered chemical reactions that were key to warming early Earth. 

Airapetian’s team simulated early Earth’s atmosphere in a sealed chamber, mixing molecular nitrogen, ammonia, carbon dioxide, and carbon monoxide. They then fired protons into the mixture, simulating the onslaught of particles from superflares. This proton bombardment triggered several changes including the production of nitrous oxide, a greenhouse gas 300 times more potent than carbon dioxide. The research was published in Astrophysical Journal Letters.

This nitrous oxide could help Earth hold onto heat. But not all the nitrous oxide would last. The young Sun’s intense ultraviolet radiation would break some of it down, splitting the molecule back into nitrogen and oxygen. But even if only 10% of the nitrous observed in the experiment survived, Airapetian’s team’s computer simulations confirmed, it would still warm Earth’s equatorial regions to about 41 degrees Fahrenheit (5 degrees Celsius), above water’s freezing point. This smaller amount of nitrous could even accelerate prebiotic synthesis: just-above-freezing temperatures have been found to be more efficient for building complex chains of amino acids than warmer temperatures. 

Unearthing secrets of our star-planet system 

Together, these two studies show that the Sun can lead to surprising implications for Earth. While our planet stands alone in many ways, it was formed and has always existed as part of a star-planet system. Understanding that unique relationship promises new insights about both Earth and the star that sustains it.  

By Desiree Apodaca and Miles Hatfield 
NASA’s Goddard Space Flight Center, Greenbelt, Md. 

Keep Exploring

Discover More Topics From NASA

Powered by WPeMatico

Get The Details…