A research team from UCL observed a ring of planetary debris studded with moon-sized structures orbiting close to a white dwarf star, hinting at a nearby planet in the ‘habitable zone.’
What was involved in conducting this study?
Scientists observed WD1054–226, which is a white dwarf star 117 light years away and recorded changes in its light over a span of 18 nights. To record these results, researchers utilised the ULTRACAM high-speed camera on the ESO 3.5m New Technology Telescope (NTT) at the La Silla Observatory in Chile.
In order to better interpret the changes in light, scientists also considered data from the NASA Transiting Exoplanet Survey Satellite (TESS). They discovered pronounced dips in light corresponding to 65 evenly spaced clouds of planetary debris orbiting the star every 25 hours.
Scientists determined that the regularity of the transiting structures suggests that they are kept in such a precise arrangement by a nearby planet. The planet is thought to be similar in size to that of the terrestrial planets in our solar system. The approximate distance between the planet and WD1054–226 is approximately 1.7% of the Earth-Sun distance (roughly 2.5 million kilometres).
What have scientists ascertained regarding white dwarf stars?
The light from WD1054–226 was always somewhat obscured by enormous clouds of orbiting material passing in front of it, which indicated a ring of planetary debris orbiting the star. The habitable zone is the area where the temperature would theoretically allow liquid water to exist on the surface of a planet.
When compared to a star like the Sun, the habitable zone of a white dwarf will be smaller and closer to the star, as white dwarfs give off less light and heat. This is because they are small, dense stars, gradually cooling down in space for the remainder of their lifetimes.
When considering the structures that scientists observed in the study, it is noted that the structures orbit in an area that would have been enveloped by the star while it was a red giant. This indicates that they are likely to have formed or arrived relatively recently, rather than survived from the birth of the star and its planetary system.
It is anticipated that this orbit around the white dwarf was swept clear during the giant star phase of its life. Thus, this recent development indicates that if the star can host water, it could also host life. The area would be habitable for at least two billion years, including at least one billion years into the future.
What do scientists anticipate for the future when considering these results?
Up to 95% of all stars will eventually become white dwarfs. The exceptions are the largest stars that explode and become either black holes or neutron stars.
Therefore, when stars begin running out of hydrogen, they expand and cool, becoming red giants; the Sun will enter this phase in four to five billion years, swallowing Mercury, Venus, and possibly Earth. Once the outer material has gently blown away and hydrogen is exhausted, the hot core of the star remains, slowly cooling over billions of years – this is the star’s white dwarf phase.
At present, planets orbiting white dwarfs are challenging for astronomers to detect because the stars are much fainter than main-sequence stars, such as the Sun. Currently, astronomers have only found tentative evidence of a gas giant orbiting a white dwarf.
Lead author Professor Jay Farihi concluded: “This is the first-time astronomers have detected any kind of planetary body in the habitable zone of a white dwarf.
“The moon-sized structures we have observed are irregular and dusty rather than solid, spherical bodies. Their absolute regularity is a mystery we cannot currently explain. An exciting possibility is that these bodies are kept in such an evenly spaced orbital pattern because of the gravitational influence of a nearby major planet.
“Without this influence, friction and collisions would cause the structures to disperse, losing the precise regularity that is observed. A precedent for this ‘shepherding’ is the way the gravitational pull of moons around Neptune and Saturn help to create stable ring structures orbiting these planets.
“The possibility of a major planet in the habitable zone is exciting and also unexpected; we were not looking for this. However, it is important to keep in mind that more evidence is necessary to confirm the presence of a planet. We cannot observe the planet directly so confirmation may come by comparing computer models with further observations of the star and orbiting debris.
“Since our Sun will become a white dwarf in a few billion years, our study provides a glimpse into the future of our own solar system.”
This study has been published in Monthly Notices of the Royal Astronomical Society.