Researchers from Lund University used Gaia data to map white dwarf movements, discovering two distinct sequences that reveal new details about their evolution.
White dwarfs were once normal stars similar to the Sun but then collapsed after exhausting all their fuel. Historically, these interstellar remnants have been difficult to study. A recent study from astronomers at Sweden’s Lund University, however, reveals new information about the movement patterns of these perplexing stars.
White dwarfs have a radius of about 1 percent that of the Sun’s. They have roughly the same mass, which means they have an astonishing density of about 1,000 kg (2,200 pounds) per cubic centimeter. After billions of years, white dwarfs will cool down to a point where they no longer emit visible light, and transform into so-called black dwarfs.
The First White Dwarf and New Findings on Movement Patterns
40 Eridani A was the first white dwarf discovered. It is a bright celestial body 16.2 light-years away from Earth, surrounded by a binary system consisting of the white dwarf 40 Eridani B and the red dwarf 40 Eridani C. Ever since it was discovered in 1783, astronomers have tried to learn more about white dwarfs in order to gain a deeper understanding of the evolutionary history of our home galaxy.
In a study published in the journal Monthly Notices of the Royal Astronomical Society, a research team can present new findings of how the collapsed stars move.
Mapping White Dwarf Movements with the Gaia Space Telescope
“Thanks to observations from the Gaia space telescope, we have for the first time managed to reveal the three-dimensional velocity distribution for the largest catalog of white dwarfs to date. This gives us a detailed picture of their velocity structure with unparalleled detail,” says Daniel Mikkola, doctoral student in astronomy at Lund University.
Thanks to Gaia, researchers have measured positions and velocities for about 1.5 billion stars. But only recently have they been able to completely focus on the white dwarfs in the Solar neighborhood.
“We have managed to map the white dwarfs’ velocities and movement patterns. Gaia revealed that there are two parallel sequences of white dwarfs when looking at their temperature and brightness. If we study these separately, we can see that they move in different ways, probably as a consequence of them having different masses and lifetimes,” says Daniel Mikkola.
The results can be used to develop new simulations and models to continue to map the history and development of the Milky Way. Through an increased knowledge of the white dwarfs, the researchers hope to be able to straighten out a number of question marks surrounding the birth of the Milky Way.
“This study is important because we learned more about the closest regions in our galaxy. The results are also interesting because our own star, the Sun, will one day turn into a white dwarf just like 97 percent of all stars in the Milky Way,” concludes Daniel Mikkola.
Reference: “The velocity distribution of white dwarfs in Gaia EDR3″ by Daniel Mikkola, Paul J McMillan, David Hobbs and John Wimarsson, 22 February 2022, Monthly Notices of the Royal Astronomical Society.
DOI: 10.1093/mnras/stac434
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