{"id":43750,"date":"2025-09-25T18:09:04","date_gmt":"2025-09-25T10:09:04","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/a-cosmic-carpool-is-traveling-to-a-distant-space-weather-observation-post\/"},"modified":"2025-09-25T18:09:04","modified_gmt":"2025-09-25T10:09:04","slug":"a-cosmic-carpool-is-traveling-to-a-distant-space-weather-observation-post","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/a-cosmic-carpool-is-traveling-to-a-distant-space-weather-observation-post\/","title":{"rendered":"A \u201ccosmic carpool\u201d is traveling to a distant space weather observation post"},"content":{"rendered":"

Scientists loaded three missions worth nearly $1.6 billion on a SpaceX Falcon 9 rocket for launch Wednesday, toward an orbit nearly a million miles from Earth, to measure the supersonic stream of charged particles emanating from the Sun.<\/p>\n

One of the missions, from the National Oceanic and Atmospheric Administration (NOAA), will beam back real-time observations of the solar wind to provide advance warning of geomagnetic storms that could affect power grids, radio communications, GPS navigation, air travel, and satellite operations.<\/p>\n

The other two missions come from NASA, with research objectives that include studying the boundary between the Solar System and interstellar space and observing the rarely seen outermost layer of our own planet\u2019s atmosphere.<\/p>\n

All three spacecraft were mounted to the top of a Falcon 9 rocket for liftoff at 7:30 am EDT (11:30 UTC) on Wednesday from NASA\u2019s Kennedy Space Center in Florida. The rocket arced on a trajectory heading east from Florida\u2019s Space Coast, shed its reusable first stage booster for a landing offshore, then fired its upper stage engine twice to propel the trio of missions into deep space.<\/p>\n

A few minutes later, each of the spacecraft separated from the Falcon 9 to begin a multi-month journey toward their observing locations in halo orbits around the L1 Lagrange point, a gravitational balance point roughly 900,000 miles (1.5 million kilometers) from Earth toward the Sun. The combined pull from the Earth and Sun at this location provides a stable region for satellites to operate in, and a good location for instruments designed for solar science.<\/p>\n

\n

\"\"<\/p>\n

Liftoff of IMAP and its two co-passengers on a Falcon 9 rocket.<\/p>\n

Credit:
\n SpaceX<\/p>\n<\/figure>\n

Seeing the big picture<\/h2>\n

The primary mission launched on Wednesday is called the Interstellar Mapping and Acceleration Probe (IMAP). The spin-stabilized IMAP spacecraft is shaped like a donut, with a diameter of about 8 feet (2.4 meters) and 10 science instruments looking inward toward the Sun and outward toward the edge of the heliosphere, the teardrop-shaped magnetic bubble blown outward by the solar wind.<\/p>\n

,<\/p>\n

At the edge of the heliosphere, the solar wind runs up against the interstellar medium, the gas, dust, and radiation in the space between the stars. This boundary remains a poorly understood frontier in space science, but it\u2019s important because the heliosphere protects the Solar System from damaging galactic cosmic rays.<\/p>\n

\u201cIMAP is a mission of firsts,\u201d said Nicky Fox, associate administrator of NASA\u2019s science mission directorate. \u201cIt\u2019ll be the first spacecraft dedicated to mapping the heliosphere\u2019s outer boundary, a key piece in the heliophysics puzzle about the Sun\u2019s influence on our Solar System. To do this, IMAP will spin every 15 seconds to measure the invisible using a very comprehensive suite of revolutionary instruments.\u201d<\/p>\n

During each rotation, IMAP\u2019s sensors will scoop up all sorts of stuff: ions traveling 1 million miles per hour in the solar wind, interstellar dust particles, and energetic neutral atoms kicked back into the Solar System from the edge of the heliosphere.<\/p>\n

\u201cThese energetic neutral atoms act as cosmic messengers,\u201d said David McComas, IMAP\u2019s principal investigator from Princeton University. \u201cThey\u2019re unaffected by magnetic fields so they can propagate all the way in from the boundaries to Earth\u2019s orbit and be measured by IMAP.\u201d<\/p>\n

Tracking these energetic neutral atoms will allow scientists to map the boundary of the heliosphere and what shapes it. The Sun\u2019s movement through the Milky Way galaxy forms a shock wave on the front side of the heliosphere, similar to the wave created by the bow of a ship moving through water.<\/p>\n

\n

\"\"<\/p>\n

Artist\u2019s illustration of the IMAP spacecraft in orbit.<\/p>\n

Credit:
\n NASA<\/p>\n<\/figure>\n

\u201cWe ended up with this fabulous observatory that measures everything,\u201d McComas said. \u201cThe particles coming out from the Sun are moving out in the solar wind to get to the outer heliosphere. Some fraction of them become neutralized and come right back, and we observe them a few years later as ENAs (energetic neutral atoms). So, we\u2019re really observing the entire life cycle of this particle energization and how it interacts at the boundaries of the heliosphere.\u201d<\/p>\n

,<\/p>\n

IMAP follows a much smaller mission, named IBEX, that carried just two instruments to begin probing the edge of the heliosphere in 2008. IBEX discovered an unexpected ribbon-like pattern of energetic neutral emissions coming from the front of the heliosphere. Scientists have developed several theories to explain the ribbon signature. One of the theories postulates that the ribbon represents a group of particles that somehow leaked from the heliosphere and bounced around interstellar space before returning to the Solar System.<\/p>\n

\u201cIt was found that interstellar matter, particles, and neutrals streaming in from outside the Solar System, actually\u2026 have a significant effect in how the entire heliosphere behaves,\u201d said Shri Kanekal, IMAP\u2019s mission scientist at NASA\u2019s Goddard Space Flight Center.<\/p>\n

IBEX\u2019s discoveries fueled enthusiasm among space scientists for a more sophisticated follow-up mission like IMAP. NASA selected IMAP for development in 2018, and the $782 million mission will spend at least two years conducting scientific observations. The spacecraft was built at the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland.<\/p>\n

\n

\"\"<\/p>\n

The ribbon remains one of IBEX\u2019s biggest discoveries. It refers to a vast, diagonal swath of energetic neutrals, painted across the front of the heliosphere.<\/p>\n

Credit:
\n NASA\/IBEX<\/p>\n<\/figure>\n

\u201cImmense value\u201d<\/h2>\n

Two years after NASA approved IMAP for development, the agency\u2019s heliophysics division selected another mission to head for the L1 Lagrange point. This smaller spacecraft, called the Carruthers Geocorona Observatory, hitched a ride to space with IMAP on Wednesday.<\/p>\n

The $97 million Carruthers mission carries two co-aligned ultraviolet imagers designed for simultaneous observations of Earth\u2019s exosphere, a tenuous cloud of hydrogen gas that fades into the airless void of outer space about halfway to the Moon. The hydrogen atoms in the exosphere generate a faint glow called the geocorona, which is only detectable in ultraviolet light at great distances. Images of the entire geocorona can\u2019t be collected from a satellite in Earth orbit.<\/p>\n

,<\/p>\n

The mission is named for George Carruthers, an engineer and solar physicist who developed an ultraviolet camera placed on the Moon by the Apollo 16 astronauts in 1972. This camera captured the first view of the geocorona, a term coined by Carruthers himself.<\/p>\n

The 531-pound (241-kilogram) Carruthers observatory was built by BAE Systems, with instruments provided by the University of California Berkeley\u2019s Space Sciences Lab.<\/p>\n

There\u2019s a lot for scientists to learn from the Carruthers mission, because they know little about the exosphere or geocorona.<\/p>\n

\u201cWe actually don\u2019t know exactly how big it is,\u201d said Lara Waldrop, the mission\u2019s principal investigator from the University of Illinois Urbana-Champaign. \u201cWe don\u2019t know whether it\u2019s spherical or oval, how much it changes over time or even the density of its constituent hydrogen atoms.\u201d<\/p>\n

What scientists do know is that the exosphere plays an important role in shaping how solar storms affect the Earth. The exosphere is also the path by which the Earth is (very) slowly losing atomic hydrogen from water vapor lofted high into the atmosphere. \u201cThis process is extremely slow at Earth, and I\u2019m talking billions of years. It is certainly nothing to worry about,\u201d Waldrop ensures.<\/p>\n

\n

\"\"<\/p>\n

This image illustrates the location of the Sun-Earth L1 Lagrange point, where IMAP, Carruthers, and SWFO-L1 will operate.<\/p>\n

Credit:
\n NOAA<\/p>\n<\/figure>\n

The final spacecraft aboard Wednesday\u2019s launch is the world\u2019s first operational satellite dedicated to monitoring space weather. This $692 million mission is called the Space Weather Follow On-L1, or SWFO-L1, and serves as an \u201cearly warning beacon\u201d for the potentially devastating effects of geomagnetic storms, said Irene Parker, deputy assistant administrator for systems at NOAA\u2019s National Environmental Satellite, Data, and Information Service.<\/p>\n

NOAA\u2019s previous satellites peer down at Earth from low-Earth orbit or geosynchronous orbit, gathering data for numerical weather models and tracking the real-time movement of hurricanes and severe storms. Until now, NOAA has relied upon a hodgepodge of research satellites to monitor the solar wind upstream from Earth. SWFO-L1, also built by BAE Systems, is the first mission designed from the start for real-time, around-the-clock solar wind observations.<\/p>\n

,<\/p>\n

\u201cWe\u2019ll use SWFO-L1 to buy power grid, airline, and satellite operators precious time to act before billion-dollar storms strike,\u201d said Clinton Wallace, director of NOAA\u2019s Space Weather Prediction Center.<\/p>\n

Once on station around the L1 Lagrange point, the satellite will be renamed SOLAR-1 before NOAA declares it operational in mid-2026. The platform hosts four instruments, one of which is a coronagraph to detect the massive eruptions from the Sun that spark geomagnetic storms. The other instruments will sample solar particles as they pass over the spacecraft about a half-hour before they reach our planet.<\/p>\n

These instruments are akin to weather satellites that detect a hurricane\u2019s formation over the remote ocean and hurricane hunters that take direct measurements of the storm to assess its intensity before landfall, NOAA said.<\/p>\n

Bundling IMAP, Carruthers, and SWFO-L1 onto the same rocket saved at least tens of millions of dollars in launch costs. Normally, they would have needed three different rockets.<\/p>\n

Rideshare missions to low-Earth orbit are becoming more common, but spacecraft departing for more distant destinations like the L1 Lagrange point are rare. Getting all three missions on the same launch required extensive planning, a stroke of luck, and fortuitous timing.<\/p>\n

\u201cThis is the ultimate cosmic carpool,\u201d said Joe Westlake, director of NASA\u2019s heliophysics division. \u201cThese three missions heading out to the Sun-Earth L1 point riding along together provide immense value for the American taxpayer.\u201d<\/p>\n

\u201cIt\u2019s like a bus,\u201d Fox said. \u201cYou wait for one and then three come at the same time.\u201d<\/p>\n","protected":false},"excerpt":{"rendered":"

Scientists loaded three missions worth nearly $1.6 billion on a SpaceX Falcon 9 rocket for launch Wednesday, toward an orbit nearly a million miles from Earth, to measure the supersonic stream of charged particles emanating from the Sun. One of the missions, from the National Oceanic and Atmospheric Administration (NOAA), will beam back real-time observations […]<\/p>\n","protected":false},"author":1,"featured_media":43752,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[],"class_list":["post-43750","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/43750"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=43750"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/43750\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media\/43752"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=43750"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=43750"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=43750"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}