15/11/2017
DEBRIS DISKS AROUND STARS COULD POINT THE WAY TO GIANT EXOPLANETS
According to current estimates,there could be as many as 100 billion planets in the milkyway galaxy alone.
Unfortunately, finding evidence of these planets is tough, time-consuming work.
Luckily a new study led by the Infrared Processing and Analysis Center(IPAC) at Caltech has determined that there may be a shortcul to finding exoplanets using direct imaging.
The solution, they claim, is to look for systems with a circumstellar debris disk, for they are sure to have at least one giant planet.
The study, titled "A Direct Imaging Survey Of Spitzer Detected Debris Disks: Occurrence of Giant Planets in Dusty Systems", recently appeared in the Astronomical journal.
For the sake of this study, Dr.Meshkat and her colleagues examined data on 130 different single-star systems with debris disks, which they then compared to 277 stars that do not appear to host disks.
As Dr.meshkat explained in a recent Nasa press release, this study will be of assistance when it comes time for exoplanet-hunters to select their targets:
"Our research is important for how future missions will plan which stars to observe.
Many planets that have been found through direct imaging have been in systems that had debris disks, and how we know the dust could be indicators of undiscovered worlds".
As study co-author Dimitri Mawet, who is also a JpL Senior research scientist, explained:
"it's possible we don't find small planets in these systems because, early on, these massive bodies destroyed the building blocks of rocky planets, sending them smashing into each other at high speeds instead of gently combining."
As karl Stapelfeldt, the chief scientist of NASA's Exoplanet Exploration Program Office and a Co-author on the study, stated:
"By showing astronomers where future missions such as NASA's James Webb space telescope have their best chance to find giant exoplanets, this research paves the way to future discoveries".