KEPLER DATA HELPING HONE IN ON ‘OTHER EARTHS’
The discovery of the first exoplanet to have its size and mass measured, and determined to be smaller than that of Earth, increases the range of worlds that Kepler can help scientists discover.
Kepler-138b is the innermost of three planets that orbit Kepler-138, a star less than half the size of the Sun and roughly 30 percent cooler. The Kepler-138 system is located about 200 light-years from Earth in the direction of the constellation Lyra.
The new technique involves the study of not only the transit information gathered about this planet, but also two others in the same stellar system – Kepler 138c and 138d. Both of these worlds are approximately Earth-sized, but their densities have a large variation. Analysis of the combined data from the parent star and all three planets made the discovery possible.
“Each planet periodically slows down and accelerates ever so slightly from the gravity of its neighboring planets,” said Jontof-Hutter, a research associate at the Pennsylvania State University’s Center for Exoplanets and Habitable Worlds. “The slight change in time between transits allows us to measure the masses of the planets.”
The new technique also allows scientists to accurately estimate the density of an exo-planet. With these combined measurements, scientists can infer the composition or material that makes up a particular object. High density exo-planets are more likely to contain more metals than their less-dense counterparts.
This type of discovery should allow scientists to look for ever smaller exo-planets transiting stars. By increasing the sensitivity of the measurements, scientists may one day be able to use the technique to determine with more certainty the habitability of any exo-planets that may be Earth-sized or smaller. Until this discovery, finding planets that were the size of the Earth was considered extremely difficult. Finding an Earth-sized or smaller exo-planet orbiting a star is far more challenging than finding the proverbial needle in a haystack. This new technique could, effectively, reduce the size of the haystack.
The Kepler mission uses the transit method to discover these new worlds. This technique watches for the subtle changes in a star’s brightness as a planet passes in front of it (as seen from Kepler’s viewpoint). The technique has been used to find thousands of exo-planet candidates and has confirmed the existence of hundreds more. The spacecraft was launched in 2009 with a planned primary mission of 3.5 years. Kepler is equipped with a 3.1 ft (0.95 m) primary mirror and an X band communications array.
The main mission of the Kepler spacecraft ended in August, 2013 when the number of reaction wheels dropped from the minimum needed to accurately lock onto candidate stars. A reaction wheel spins similar to a flywheel and is used to hold a spacecraft steady without the need for fuel. It makes a spacecraft lighter and can give them a much longer operational life. Kepler has four reaction wheels on board but needs three operational to be accurate. When the spacecraft lost two of its reaction wheels, the primary mission concluded.
Engineers were not done with Kepler, however. They developed a new technique that allowed the spacecraft to remain stable enough for some observations using only two reaction wheels along with the assistance of the telescope’s thrusters. The new mission was named K2, or “Second Light”. This extended mission continues to find new planet candidates.