For the first time, astronomers have determined the shape of the heliosphere, mapping in 3D the boundary that marks the end of the solar wind for our star in space.
This discovery, the which published results of were recently in The Astrophysical Journal, will help to better understand the environment of the solar system and how it interacts with interstellar space. Read also Scientists are optimistic… Has the sun returned to give birth to sunspots again? The coolest and closest images from the Solar Spectrogram project are now available to the public Soho Telescope.. 25 years of staring at the sun Threatens communications and satellites.. hurricanes of plasma ravaging the upper atmosphere of the Earth
unknown edge
astronomer Dan Reisenfeld of Los Alamos National Laboratory says in the press release “Physical models theorized these limits years ago,” lab’s . “But this is the first time that we have actually been able to measure it and make a 3D map of it,” the lead author of the study adds in a statement published on the lab’s website.
Theoretically, the edge of the heliosphere is not unknown to scientists, as they actually realized its existence when the Voyager 1 and Voyager 2 probes crossed this edge on their way to the outer space of the solar system.
The edge of the heliosphere is an interesting place for scientists, as the solar wind loses its speed. These winds are released by our star in the form of streams of charged particles in all directions at supersonic speed.
But as it penetrates into space, it gradually loses its strength so that it is no longer sufficient to push the pressure of the currents of charged particles coming from interstellar space. At the edge of the heliosphere, the solar wind stops completely. Interstellar space contains a low density of atoms, but it is dominated by cosmic winds blowing between the stars, which are enough to repel the advance of the solar wind.
The bat inspires scientists
Despite consensus scientists and grandparents this limit, the shape remained subject debate and differences among them, according ” Science Alert ” (ScienceAlert) scientific.
Scientists realize that they cannot accurately survey the edge of the heliosphere because of the enormous distance that separates us from it. The Voyagers 1 and 2 probes were at distances of 121 and 119 AU (an AU equals 150 million km) from the Sun respectively when they reached this edge, and it took decades to get there. It is about 4 times the distance between the Sun and Neptune, the farthest planet from it.
But that doesn’t mean you can’t look from afar to determine what this edge looks like. Reisenfeld and his team used data from NASA’s Interstellar Boundary Explorer IBEX satellite, an observatory that measures particles coming from the edge of the heliosphere.
Some of these particles are what scientists call “active neutral atoms”, which are atoms that are generated by collisions between solar wind particles and interstellar wind particles, and the strength of their signals depends on the strength of the solar wind at the time of the collision. The solar wind, like the wind on Earth, does not always blow with the same intensity. .
Decoding this signal to determine the edge of the heliosphere is somewhat similar to the way a bat uses sound waves to map its physical surroundings. The signal strength and the time interval between transmitting and receiving can reveal the shape and distance of obstacles.
sexy shape
According to the lead author, the IBEX satellite used the same method to capture the signal of “active neutral atoms” returning after two to 6 years, depending on the energy of these atoms and the direction of the satellite’s “look” through the heliosphere.
Using this time difference and data from an entire solar cycle between 2009 and 2019, the researchers were able to create a 3-D map of the heliosphere.
Although the map created is still a bit rough, according to the researchers, it does reveal interesting things about the heliosphere. Its shape, for example, is now known, and is somewhat similar to that of a comet with a tail of at least 350 AU.
In contrast, the minimum radial distance is between 110 and 120 astronomical units, consistent with what was recorded by the Voyager 1 and 2 probes. While the heliosphere extends at high latitudes between 150 and 175 AU.
The IBEX mission will continue until at least 2025. The interstellar mapping and acceleration probe is scheduled to begin in 2025, starting when IBEX has stopped. The team hopes that these two missions will provide more data to help determine the shape of the heliosphere more precisely.