In the heart of the Milky Way, the stars appear younger than expected.
NASA, Caltech, Susan Stolovy (SSC, Caltech)
Stars in the core of our galaxy may indeed be nearly immortal, harnessing dark matter for energy.
Over two decades ago, astronomers observed oddities among the stars at the Milky Way’s center. Their emitted light suggests they are younger than their mass would indicate; this phenomenon is termed the “Youth Paradox.” Furthermore, there’s a surprising scarcity of older stars in this region, referred to as the “aging difficulty problem.”
Currently, Isabelle John from the University of Stockholm and her team employed computer simulations to propose that dark matter might hold the key to resolving both issues.
It’s established that the centers of galaxies possess high densities of dark matter. The researchers simulated the interactions of dark matter particles with stars and found that upon collision with a star’s atomic nucleus, a particle loses energy and can become trapped there. If other dark matter particles are also present at the same site, they can annihilate each other, generating bursts of energy that illuminate the stars.
Stars typically age due to a lack of fusion fuel, but dark matter could serve as an extra energy source, extending their longevity. Given the substantial amount of dark matter surrounding the galactic center, this mechanism may effectively grant stars a form of immortality, according to John.
She notes that the team’s simulations are based on broad assumptions regarding dark matter and align qualitatively with historical observations. However, further empirical data could enhance our understanding, prompting additional telescope observations to gather fresh insights on dark matter and verify if the stars at the Milky Way’s core can indeed achieve eternal life, as their nature remains poorly understood.
Mark Pinne from Ohio State University emphasizes the importance of interpreting simulations of stars situated away from the galaxy’s center. He points out that since there exists comprehensive observational data on stars near Earth, the anticipated impacts of dark matter should be cross-verified with this information.
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Source: www.newscientist.com
