SPACE/COSMOS
Solar flares over 6 times hotter than previously thought
image:
A solar limb flare with a comparatable scale of Earth
view moreCredit: Created by Alexander Russell (University of Andrews) using the open-source SunPy Python package and data from NASA’s Solar Dynamics Observatory space telescope via NASA EPIC Team
New research from the University of St Andrews has proposed that particles in solar flares are 6.5 times hotter than previously thought and provided an unexpected solution to a 50-year-old mystery about our nearest star.
Solar flares are sudden and huge releases of energy in the Sun’s outer atmosphere that heat parts of it to greater than 10 million degrees. These dramatic events greatly increase the solar X-rays and radiation reaching Earth and are hazardous to spacecraft and astronauts, as well as affecting our planet’s upper atmosphere.
The research, published today in Astrophysical Journal Letters, looked at evidence of how flares heat solar plasma to greater than 10 million degrees. This solar plasma is made up of ions and electrons. The new research argues that solar flare ions, positively charged particles that make up half of the plasma, can reach over 60 million degrees.
Looking at data from other research areas, the team, led by Dr Alexander Russell, Senior Lecturer in Solar Theory from the School of Mathematics and Statistics, realised that solar flares are very likely to heat the ions more strongly than the electrons.
Dr Russell, said: “We were excited by recent discoveries that a process called magnetic reconnection heats ions 6.5 times as much as electrons. This appears to be a universal law, and it has been confirmed in near-Earth space, the solar wind and computer simulations. However, nobody had previously connected work in those fields to solar flares.”
“Solar physics has historically assumed that ions and electrons must have the same temperature. However, redoing calculations with modern data, we found that ion and electron temperature differences can last for as long as tens of minutes in important parts of solar flares, opening the way to consider super-hot ions for the first time.”
“What’s more,” he added, is that the new ion temperature fits well with the width of flare spectral lines, potentially solving an astrophysics mystery that has stood for nearly half a century.”
There has been a long-standing question since the 1970s about why flare spectral lines, bright enhancements in the solar radiation at specific “colours” in extreme-ultraviolet and X-ray light, are broader than expected. Historically, it was believed that this could only be due to turbulent motions, but that interpretation has come under pressure as scientists have tried to identify the nature of the turbulence. After nearly 50 years, the new work argues for a paradigm shift where the ion temperature can make a large contribution to explaining the enigmatic line widths of solar flare spectra.
Solar flares
Credit
Created by Alexander Russell (University of Andrews) using the open-source SunPy Python package and data from NASA’s Solar Dynamics Observatory space telescope via NASA EPIC Team
Journal
The Astrophysical Journal Letters
Method of Research
Data/statistical analysis
Subject of Research
Not applicable
Article Title
Solar Flare Ion Temperatures
Article Publication Date
3-Sep-2025
SwRI-proposed mission could encounter and explore a future interstellar comet like 3I/ATLAS up close
Development study sets mission objectives and trajectory of journey to interstellar comet, as well as probability of success in locating a target
image:
Upper left panel: Comet 3I/ATLAS as observed soon after its discovery. Upper right panel: Halley’s comet’s solid body as viewed up close by ESA’s Giotto spacecraft. Lower panel: The path of comet 3I/Atlas relative to the planets Mercury through Saturn and the SwRI mission interceptor study trajectory if the mission were to be launched this year. The red arc in the bottom panel is the mission trajectory from Earth to interstellar comet 3I/ATLAS.
view moreCredit: NASA/ESA/UCLA/MPS
SAN ANTONIO — September 3, 2025 — Southwest Research Institute (SwRI) has completed a mission study detailing how a proposed spacecraft could fly by an interstellar comet, providing remarkable insights into the properties of bodies originating beyond our solar system. The internally funded SwRI project developed the mission design, scientific objectives, payload and key requirements based on previous interstellar object (ISO) detections. Using the recent discovery of 3I/ATLAS, the team validated the mission concept, determining that 31/ATLAS could have been intercepted and observed by the proposed spacecraft.
In 2017, the object designated 1I/‘Oumuamua became the first interstellar comet (ISC) detected in the solar system. Its identification and naming nomenclature starts with the number 1, because it’s the first such object to be discovered, followed by an “I” for interstellar, and “ʻOumuamua,” which is the object’s given name — a Hawaiian word meaning “a messenger from afar arriving first.” Its discovery was soon followed by the discovery of the second interstellar comet, ISC 2I/Borisov in 2019, and now this year, ISC 3I/ATLAS, which made worldwide headlines as it became the third officially recognized interstellar object to cross into our solar system. As new astronomical facilities like the National Science Foundation’s Vera Rubin Observatory develop new surveys and those capabilities expand, astronomers expect to discover many more ISCs over the next decade.
“These new kinds of objects offer humankind the first feasible opportunity to closely explore bodies formed in other star systems,” said SwRI Associate Vice President Dr. Alan Stern, a planetary scientist who led the study project. “An ISC flyby could give unprecedented insights into the composition, structure and properties of these objects, and it would significantly expand our understanding of solid body formation processes in other star systems.”
Scientists estimate that numerous interstellar objects of extrasolar origin pass inside Earth’s orbit each year, and that as many as 10,000 pass inside the Neptune’s orbit in any given year. The SwRI-led internal research study tackled the unique design challenges and defined the costs and payload needs associated with an ISC mission. The mission concept could be later proposed to NASA. The hyperbolic trajectories and high velocities of these objects preclude orbiting them with current technology, but the SwRI study showed that flyby reconnaissance is feasible and affordable.
“The trajectory of 3I/ATLAS is within the interceptable range of the mission we designed, and the scientific observations made during such a flyby would be groundbreaking,” said SwRI’s Matthew Freeman, the study’s project manager.” The proposed mission would be a high-speed, head-on flyby that would collect a large amount of valuable data and could also serve as a model for future missions to other ISCs.”
SwRI scientists and their external collaborators in the study established the major, comprehensive scientific objectives for a mission to an ISC. Determining the physical properties of the body would offer insights to its formation and evolution. Examining the ISC composition could help explain its origins and interpret how evolutionary forces have affected the comet since its formation. Yet another objective is to thoroughly investigate the nature of the object’s coma, the escaping atmosphere emanating from its central body.
To develop mission trajectory options, SwRI developed software that generated a representative, synthetic population of ISCs then calculated a minimum energy trajectory from Earth to the path of each comet. The software’s calculations showed that a low-energy rendezvous trajectory is possible, and in many cases would require less launch and in-flight velocity change resources than many other solar system missions. SwRI orbital mechanics expert, Dr. Mark Tapley, used this software to calculate the trajectory that the proposed spacecraft could have taken from Earth to intercept 3I/ATLAS. He found that the mission designed by SwRI’s study could have reached 3I/ATLAS.
“The very encouraging thing about the appearance of 3I/ATLAS is that it further strengthens the case that our study for an ISC mission made,” said Tapley. “We demonstrated that it doesn’t take anything harder than the technologies and launch performance like missions that NASA has already flown to encounter these interstellar comets.”
For more information, visit https://www.swri.org/markets/earth-space/space-research-technology.
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