Astronomers have figured out how exoplanets revolve around their pulsars

A team of scientists looked for signals indicating the presence of satellite planets with masses 100 times greater

mass of the Earth, and a period of revolution from 20 days to17 years. Of the 10 potential objects, the most promising is the PSR J2007+3120 system, with the possibility of hosting at least two planets with masses several times larger than Earth and orbital periods of 1.9 and ~3.6 years.

The results of the work indicate the absenceoffsets for specific planetary masses or orbital periods in pulsar systems. However, the study provides information about the shape of the orbits of these planets: unlike the near-circular orbits of our solar system, these planets revolve around their stars in highly elliptical trajectories. This indicates that the process of formation of "pulsar-planet" systems is very different from traditional "star-planet" systems.

Pulsars are incredibly interesting and exoticobjects. Exactly 30 years ago, the first extrasolar planets were discovered around a pulsar, but we have yet to understand how these planets can form and survive in such extreme conditions. And also find out how common they are and what they look like.

Juliana Nitsu, PhD, student at the University of Manchester

Processes that make the planetsform and survive around pulsars are currently unknown. The study, which studied 800 pulsars, was conducted by the Jodrell Bank Observatory. It showed that less than 0.5% of all known pulsars could contain Earth-mass planets.

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