It turns out that the existence of life on planets orbiting stars like our sun does not require those stars to be vibrant and powerful. A potential "major planet" that orbits a dying sun and could support life in the future has been found by scientists
The “surprising” discovery was made by
researchers from University College London while watching a white dwarf, the
burning remnants of a star that ran out of hydrogen fuel. It is about 117
light-years away from us. This star, known as WD1054-226, has a ring of
planetary rubble in its orbital habitable zone, also known as the Goldilocks
zone, where temperatures should enable the planet to have liquid water on its
surface.
If the newfound planet is proved to be a
life-sustaining world, it will be the first time a life-sustaining planet has
been identified around a dying sun.
Scientists made the discovery while monitoring
the light from the white dwarf and reported their results in the Royal
Astronomical Society’s Monthly Notices. They discovered strong dips in light
that matched to 65 uniformly distributed clouds of debris that orbited
WD1054-226 every 25 hours, according to their findings.
Jay Farihi, the lead author of the study and
professor at UCL Physics and Astronomy, said: “The moon-sized structures we
have observed are irregular and dusty (e.g. comet-like) rather than solid,
spherical bodies”
He described the structures as a “mystery we
cannot explain,” but suggested one possible and “unexpected” explanation: a
nearby planet.
The idea of a “major planet” in the star’s
habitable zone is thrilling, but he emphasises that such a planet has yet to be
proven. Farihi stated that his team still requires further proof, which may be
tough to get due to the inability to directly view the planet. To gain a
clearer explanation, they may have to depend on computer models along with
additional observations of the star and its circling debris.
The team anticipates that, if a planet exists,
it was just recently formed — and that it would be habitable for at least 2
billion years, including at least 1 billion years in the future.
Their findings may also aid scientists in
developing a better knowledge of our solar system, as more than 95% of all
stars, including our sun, will ultimately become white dwarfs.
Reference(s): Royal
Astronomical Society’s Monthly Notices
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