What processes provide energy to the solar wind as it travels away from the Sun and throughout the solar system? This is what a recent study published in Science hopes to address as an international team of researchers investigated the processes responsible for providing energy to the solar wind as it leaves the Sun and traverses the rest of the solar system. This study holds the potential to help astronomers better understand the Sun’s processes, which could also provide insight into the processes of other stars, as well.

“Our study addresses a huge open question about how the solar wind is energized and helps us understand how the Sun affects its environment and, ultimately, the Earth,” said Dr. Yeimy Rivera, who is a postdoctoral fellow at the Center for Astrophysics | Harvard & Smithsonian and lead author of the study. “If this process happens in our local star, it’s highly likely that this powers winds from other stars across the Milky Way galaxy and beyond and could have implications for the habitability of exoplanets.”

For the study, the researchers used solar wind data from NASA’s Parker Solar Probe and the joint NASA-ESA Solar Orbiter collected within two days of each other due to the spacecraft being aligned with each other, enabling this research to be conducted. For context, the Parker Solar Probe is currently orbiting inside the Sun’s corona while Solar Orbiter is orbiting approximately halfway between the Earth and the Sun. In the end, the researchers found the solar wind’s acceleration that occurs between the Sun and the Earth is due to what are called “Alfvén waves”, which transport energy through the solar plasma. However, researchers haven’t been able to measure Alfvén waves until now.

“There are many open clusters in the galaxy. However, not all open clusters have the same level of interest to astronomers,” Ignacio Negueruela, a researcher at the Universidad de Alicante who was part of the team behind the discovery of supergiants in Barbá 2, told Space.com. “Clusters rich in red supergiants are very rare and tend to be very far away, but they play a crucial role in understanding key aspects in the evolution of massive stars.”

The intimidating size and power of supergiants means these monster stars burn through their nuclear fuel much faster than stars like the sun. Whereas our star will exist in its main sequence lifetime for around 10 billion years, supergiants are estimated to last just a few million years.

The short lifetime of supergiants means that while open clusters like Barbá 2 are common, with over 1,100 already discovered in the Milky Way alone, finding one packed with red supergiants is extremely rare.

Logistics companies on the ground solve similar problems every day and transport goods and commodities across the globe. So, researchers can study how these companies manage their logistics to help space companies and agencies figure out how to successfully plan their mission operations.

One NASA-funded study in the early 2000s had an idea for simulating space logistics operations. These researchers viewed orbits or planets as cities and the trajectories connecting them as routes. They also viewed the payload, consumables, fuel and other items to transport as commodities.

This approach helped them reframe the space mission problem as a commodity flow problem – a type of question that ground logistics companies work on all the time.