New Method to Discover Exoplanets Orbiting Violent Dead Stars Suggested by Researchers

Researchers measured the changes in the brightness of four CVs — LU Camelopardalis, QZ Serpentis, V1007 Herculis, and BK Lyncis as part of the study.

New Method to Discover Exoplanets Orbiting Violent Dead Stars Suggested by Researchers

Photo Credit: Departamento de Imagen y Difusion FIME-UANL/ Lic. Debahni Selene Lopez Morales D.R. 2022

An artist’s impression of a CV from point of view of the surface of an orbiting planet

Highlights
  • Planets that orbit around dead stars known as Cataclysmic Variables (CVs)
  • CVs binary star systems with two stars in extreme proximity to each other
  • Researchers measured the changes in the brightness of four CVs

Researchers have suggested a new way to detect planets that orbit around dead stars known as Cataclysmic Variables (CVs), which are essentially binary star systems that have two stars in extreme proximity to each other. The lack of distance between them leads to one star drawing material from the other, thereby dimming the second star. The researchers measured the changes in the brightness of four CVs — LU Camelopardalis, QZ Serpentis, V1007 Herculis, and BK Lyncis — as part of the study.

According to the Royal Astronomical Society, “CVs are typically formed of a small, cool type of star known as a red dwarf star, and a hot, dense star — a white dwarf. Red dwarf stars have a mass between 0.07 and 0.30 solar masses and a radius of around 20 percent of the Sun's, while white dwarf stars have a typical mass of around 0.75 Solar masses and a very small radius similar to that of planet Earth.”

Now, if there is a third entity – a planet, for instance – in the vicinity, it can affect the transfer of material from the donor to the primary star due to its gravitational force. This, in turn, can affect the system's brightness a new study has found.

The study published in the Monthly Notices of the Royal Astronomical Society (MNRAS) is titled: “Testing the third-body hypothesis in the cataclysmic variables LU Camelopardalis, QZ Serpentis, V1007 Herculis, and BK Lyncis.”

The peer reviewed study has been led by Dr. Carlos Chavez from the Universidad Autónoma De Nuevo León in Mexico. Dr Chavez and his team have examined CVs in the study - LU Camelopardalis, QZ Serpentis, V1007 Herculis, and BK Lyncis.

The team has measured the changes in the brightness of the four CVs. Using this, they have calculated the “distances and masses of potential third bodies in the systems based on the brightness changes in each system.” The study is based on the “intrinsic change in luminosity” that can be observed from different angles.

As per the team, two of the four CVs they studied have "bodies resembling planets" orbiting them.

“Our work has proven that a third body can perturb a cataclysmic variable in such a way that can induce changes in brightness in the system. These perturbations can explain both the very long periods that have been observed — between 42 and 265 days — and the amplitude of those changes in brightness,” Dr Chavez said.

The study, the team said, has yielded a promising new technique for finding planets in orbit around Cataclysmic Variables.


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