Two worlds orbiting a distant star are about to become a snack of cosmic proportions.
Astronomers1 announced today that the planets Kepler-56b and Kepler-56c will be swallowed by their star in a short time by
astronomical2 standards. Their ends will come in 130 million and 155 million years, respectively. "As far as we know, this is the first time two known exoplanets in a single system have a predicted 'time of death,'" says lead author Gongjie Li of the Harvard-Smithsonian Center for Astrophysics (CfA).
She presented her research today at a meeting of the American Astronomical Society.
The Kepler-56 system provides a glimpse into the future of our solar system. In about five billion years our Sun will become a red giant star,
swelling3 to immense proportions and
engulfing4 Mercury and Venus.
The star Kepler-56 is becoming a red giant star as well. It already has ballooned out to four times the Sun's size. As it ages, it will continue to expand outward. Not only will the star grow larger, but its tides will get stronger, dragging its planets inward to their
eventual5 doom6.
Kepler-56b orbits its host star once every 10.5 days, while Kepler-56c orbits every 21.4 days. Both of them are much closer to their star than Mercury is to the Sun. As a result, they will meet their fate much faster. Li and her collaborators calculated the evolution of both the star's size (using the publicly available MESA code) and the planets' orbits to predict when the planets will be destroyed.
Even before they vanish, the two planets will be subjected to immense heating from the
steadily7 growing star. Their atmospheres will begin to boil off, and the planets themselves will be stretched into egg shapes by stellar tides.
The only
survivor8 in the system will be Kepler-56d, a gas giant planet circling in a 3.3-Earth-year orbit. It will watch from a safe distance as its two
sibling9 worlds meet their
demise(死亡,终止).
The Kepler-56 planetary system also is notable for being the first "
tilted10" multiplanet system to be discovered. The orbits of the inner two planets are tipped significantly from the star's
equator(赤道). This was unexpected since planets form from the same disk of gas and dust as the star, so they should orbit in nearly the same plane as the star's equator (as do the planets in our solar system).
The team was able to better
constrain12 the
tilt11 of these planets, compared to earlier work. They found that the most probable
tilt(倾斜) was either 37 or 131 degrees.
Li and her colleagues also investigated the
inclination13(倾向,爱好) of the outer planet and
determined14 that its orbit is likely to be tilted relative to the star as well. Future observations should help astronomers to characterize this system, and to explain how it became so
skewed(歪斜的).