Kepler-444 has ancient planetary system
Space telescope discovers five exoplanets orbiting a star in the constellation of Cygnus
The planetary system around the star Kepler-444 appears like a distant version of our own inner solar system: Even though not four, but five small planets orbit the host star, their sizes all lie between those of Mercury and Venus.
The exoplanets orbit Kepler-444 in less than ten days or, equivalently, at less than one-tenth Earth’s distance from the Sun. The age of the system is a surprise: with 11.2 billion years, it is almost two and a half times as old as our solar system. So far, no other system of comparable age is known to host Earth-sized planets.
The team carried out the research using asteroseismology: with the help of the Kepler Space Observatory the researchers listened to the natural resonances of the host star which are caused by sound waves trapped within it. “These oscillations lead to miniscule variations in its brightness which allow us to measure its diameter, mass, and age”, says Saskia Hekker from the Max Planck Institute for Solar System Research.
The planets were detected from the dimming that occurs when they passed in front of the star. This fractional fading in the intensity of the light received from the star enables scientists to accurately measure the sizes of the planets relative to the size of the star.
The Kepler Space Observatory has been searching for exoplanets since 2009. Over a period of four years it repeatedly turned its gaze to star Kepler-444. “Long, uninterrupted observations are necessary to observe the weak pulsations. Only with the exquisite, high quality data from the Kepler mission has this been possible”, explains Dr. Timothy White from the University of Göttingen.
"There are far-reaching implications from this discovery”, says Tiago Campante from the University of Birmingham, who led the research. It proves that Earth-sized planets have formed throughout most of the Universe’s 13.8-billion-year history. Hekker clarifies that “We therefore think it is possible that worlds which could support life may have existed even in this early phase of the Universe’s evolution.
Since the beginning of this year, Saskia Hekker heads the new Max Planck Research Group “Stellar Ages and Galactic Evolution” at the MPS. After receiving her doctorate in 2007 at the University of Leiden in the Netherlands, she did research at the Royal Observatory of Belgium and at the University of Birmingham in England. In 2011 she received the prestigious Veni Fellowship of the Netherlands Organization for Scientific Research to continue her work at the Astronomical Institute "Anton Pannenkoek" of the University of Amsterdam. Since 2013 Hekker’s scientific home is the MPS in Göttingen where she was awarded a Starting Grant of the European Research Council.