The Royal Astronomical SocietyResearchers 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.

Figure 1: A new way to detect planets that orbit around dead stars.

Figure 1 shows thatthe 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. [1]

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.” [2]

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

The staff has measured the adjustments within the brightness of the 4 CVs. Using this, they’ve calculated the “distances and masses of potential third bodies in the systems based on the brightness changes in each system.” The examiner relies on the “intrinsic change in luminosity” that may be noticed from completely different angles.

“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 stated.

As per the staff, two of the 4 CVs they studied have “bodies resembling planets” orbiting them.The examiner, stated, has yielded a promising new method for locating planets in orbit round Cataclysmic Variables. [3]

References:

1. https://gadgets360.com/science/news/planets-orbiting-violent-dead-stars-discovery-researchers-cataclysmic-variables-3192032
2. https://www.adeex.in/news/new-method-to-discover-exoplanets-orbiting-violent-dead-stars-suggested-by-researchers/
3. https://www.today24x7.com/News/how-scentists-plan-to-detect-exoplanets-orbiting-violent-dead-stars/

Cite this article:

Sri Vasagi K (2022), New Method to Detect Exoplanets Orbiting Violent Dead Stars, Anatechmaz, pp.270