More than three years ago, Steve B. Howell from NASA’s Ames Research Center in Moffett Field, California, put together a team to investigate and characterize the stars that the NASA Kepler mission found to host planets — Mark Everett and David Silva, both at NOAO in Tucson, Arizona, and Paula Szkody from the University of Washington in Seattle.
“One of the main findings of this initial work is that our observations indicate that most of the stars we observed are slightly larger than previously thought and one-quarter of them are at least 35 percent larger,” said Everett. “Therefore, any planets orbiting these stars must be larger and hotter as well. By implication, these new results reduce the number of candidate Earth-size planet analogs detected by Kepler.”
The Kepler mission, a telescope in orbit around the Sun, measures how much a star dims when a planet candidate crosses in front of it. The amount of dimming reveals the relative size of the star and its candidate planet. The research team used the amount of dimming combined with new measurements of the sizes of the stars to determine that the planet candidates are larger than previously thought.
While approximate sizes of most of the host stars were previously known from the star’s colors and brightness, spectra reveal far more. The team acquired spectra using the large ground-based Mayall 4-meter telescope located near Tucson, Arizona. Their observations were made over 48 nights covering the past several years.
“While Kepler is the discovery machine, it takes both Earth-based and space-based telescopes to truly understand exoplanets and how they relate to the stars they orbit,” said Silva.
To date, more than 300 stars have been observed at the Mayall 4-meter from the long list identified by Kepler as hosts of potential planets — referred to as Kepler Objects of Interest (KOIs). The sample contained more faint stars, with distances ranging from 2,800 to over 7,000 light-years, than previous ground-based studies. Such faint KOIs host the majority of high-priority Earth-sized candidate planets identified so far by Kepler. Spectra of these stars were obtained and compared with theoretical models to determine more accurate stellar radii, temperatures, and metallicity — the relative amount of elements heavier than hydrogen and helium in each star. In all, these stars are thought to harbor more than 360 exoplanet candidates. To date, this study represents the largest and faintest uniform sample of spectroscopically characterized exoplanet host stars in the Kepler field of view.
“Determination of accurate stellar sizes allows astronomers to more accurately identify which exoplanets are Earth analogs, fulfilling a key goal of the Kepler mission,” said Howell.
The team plans to make more ground-based spectral observations as there remain over 1,000 KOI stars with small planet candidates to observe in this magnitude range.