This exo-oddball was found during an observing campaign seeking out new worlds around a group of young stars. GU Psc, a star that is roughly a third of the size of our sun, was recently identified as a member of the AB Doradus group and became a ripe target for this exoplanetary search.
These young AB Doradus stars are around 100 million years old and make attractive targets for exoplanetary searches through direct means. As the stars are so young, any planets in tow will still be hot after recently forming from stellar material. Therefore, by their nature, these worlds are radiating energy into space, illuminated in infrared light.
The most common methods used to detect exoplanets include the “transit” method and the “radial velocity” method. The former has been made famous by NASA’s Kepler space telescope that stared at one patch of the sky to see exoplanets drift in front of their parent stars, slightly dimming the starlight. The radial velocity method is commonly used by ground-based observatories that watch for the slight frequency shift of starlight caused by the gravitational wobble of an orbiting exoplanet.
Direct imaging, however, can be a hard task and very few exoplanets have been discovered by this means. But in the case of GU Psc b, the young gas giant world was identified by an international team using several observatories. This research has been published in the Astrophysical Journal.
“Planets are much brighter when viewed in infrared rather than visible light, because their surface temperature is lower compared to other stars,” said team leader Marie-Ève Naud, PhD student at the Department of Physics at the Université de Montréal. “This allowed us to identify GU Psc b.”
But the exoplanetary search wasn’t easy. “We observed more than 90 stars and found only one planet, so this is truly an astronomical oddity!” added Naud.
Read more at Discovery News
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