A team of European astronomers, using the SOPHIE
spectrograph at the Observatoire de Haute-Provence (France), confirmed
the presence of Kepler-88 c, an unseen planet that was previously
predicted thanks to the gravitational perturbation it caused on its
transiting brother planet, Kepler-88 b.
Searching for periodic transits in hundred of thousand of stars was the
primary goal of the Kepler space telescope. More than 3500 of such
periodic transits were found during the 4 years of the mission. However,
not all the planets located in the Kepler field-of-view are transiting
their host star. Indeed, if their orbital plane is slightly misaligned
(only a few degrees is enough) with the line of sight from the Earth,
the planet is not transiting and thus, is “unseen” from the Kepler
spacecraft
Planets that share the same host star gravitationally interact with
each other. This interaction between planets can cause perturbations in
the predicted times of transit of planets [
3]
in multi-planetary systems. “This is called Transit Timing Variations
(TTV)” explains the leading author of the paper, Susana Barros, a
researcher at the Laboratoire d’Astrophysique de Marseille (LAM).
The TTV technique is sensitive to planets in multiple systems down to
the mass of the Earth, and can therefore be used to unveil the
existence of non-transiting planets, that cause perturbations in the
orbital motion of transiting planets.
.
This is the case of the Kepler-88 system, which hosts a transiting
planet (Kepler-88 b), discovered by the Kepler space telescope [
4]
(NASA) , that is strongly perturbed by a non-transiting planet
(Kepler-88 c). “This system presents such strong interactions that it
has earned the nickname of the king of transit variations” adds Rodrigo
Díaz, a researcher working at the Geneva Observatory (OAUG).
A careful analysis of the dynamical interaction between planets,
previously performed by a team led by David Nesvorný (Boulder
University), predicted that this system had two planets near a
two-to-one resonance (the orbital period of the unseen outer-planet is
exactly two times longer than the the transiting inner-planet). This
configuration is similar to the Earth and Mars in the Solar System, with
Mars orbiting the Sun in nearly 2 years.
Using the SOPHIE velocimeter, the team independently measured [
5] the mass of Kepler-88 c. “SOPHIE is a French instrument capable of measuring the velocity of stars [
6]
with a precision equivalent to the speed of a bicycle. It has been used
to characterize nearly 20 Kepler planets so far” adds Alexandre
Santerne a researcher at Centro de Astrofísica da Universidade do Porto
(CAUP) and responsible of the observations of Kepler targets with
SOPHIE.
The inferred mass for the unseen planet is in perfect agreement with
the value that was predicted from TTV. “This is the first time that the
mass of an unseen exoplanet inferred based on Transit Timing Variation
is independently confirmed by another technique” comments Susana Barros.
This result therefore confirms TTV as a valid technique to detect
unseen planets and explore multi-planet systems. TTV has already been
used to determine the mass of more than 120 exoplanets detected by
Kepler, around 47 planetary systems, down to a few Earth-mass planets.
"This independent confirmation is a very important contribution to
the statistical analyses of the Kepler multiple planet systems. It helps
to better understand the dynamical interactions and the formation of
planetary systems. This also permits to anticipate the future
exploration of exoplanetary systems from space as would do the PLATO
mission " concludes Magali Deleuil, professor at Aix-Marseille University and leader of LAM’s exoplanet research.
Neptune was the first planet detected based on the gravitational
influence it had on another planet (Uranus). The French mathematician
Urbain Le Verrier calculated that the anomalies in Uranus orbit were due
to a two-to-one resonance from a previously unseen planet. His
calculation led Johann Gottfried Galle to find Neptune on September 23rd
1846
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