Exoplanet Study Suggests our Solar System is the Norm
The two most effective methods for detecting extrasolar planets are the radial-velocity method and the transit method. The radial-velocity method detects planets through the reflex motion induced by the planet on the star’s velocity on the radial direction (hence the name). This velocity variation is detected through the Doppler effect, the same that leads to a pitch change in the sound of an traveling ambulance. On the other hand, a planetary transit is akin to a mini-eclipse. As a planet travels around the star, its orbit can locate it in front of the star, and the light we collect from the star is reduced because the planet blocks part of it (even though we cannot image the planet).
We simulated planetary systems with frequencies as reported by HARPS survey (that detects basically all the systems, independently of their inclination angle), and attributed to them different relative inclinations. The frequency of transiting systems was calculated and compared with the values reported by Kepler. We showed that a match can be obtained for double-transiting systems only if they are very strongly aligned with a common plane (the system’s plane). This alignment has to be close to 1 degree, and only reaches 5 degrees on very extreme cases (extreme on the sense of the assumption on how a planetary mass translates to a radius).
These results show consistently that the planets’ orbits are predominantly aligned, reinforcing the idea that planets form on a disk and suggesting for the first time that violent encounters between planets are not frequent. This provides a very important clue about the formation and evolution of exoplanets, a domain in which several open questions remain. Even though the Solar System’s organization is more often the exception than the rule, this study shows that the high degree of alignment of our system might well be the norm.
Pedro Figueira (CAUP), the article’s first author stated: “These results show us that the way our solar system formed must be common. Its structure is the same as the other planetary systems we studied, with all planets orbiting roughly in the same plane.”