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Short-Period Hot Jupiter Discovered Circling HAT-P-68 | Astronomy


Astronomers using data from the HATNet (Hungarian-made Automated Telescope Network) survey have discovered a transiting giant planet orbiting the K5-type dwarf star HAT-P-68.
An artist’s impression of the hot-Jupiter exoplanet HAT-P-68b and its parent star HAT-P-68 (also known as GSC 1925-01046 and 2MASS 07535598+2356176), a K5-type dwarf star with a mass of 0.68 solar masses and a radius of 0.67 solar radii. Image credit: Sci-News.com.
“The discoveries of planets with orbital periods shorter than 10 days provide advantages to resolving current theoretical challenges in the field,” said University of Washington astronomer Bethlee Lindor and colleagues.
“For instance, explaining the inflated radii of hot Jupiters remains a theoretical puzzle that may be elucidated by building up a larger sample objects to disentangle the effects of age, orbital separation, irradiation, composition and mass on the radii of these planets.” ....

Bethleem Lindor , Bethlee Lindor , University Of Washington , Hatnet Automated Telescope Network , Hungarian Made Automated Telescope Network , Transiting Hot Jupiter , பல்கலைக்கழகம் ஆஃப் வாஷிங்டன் , பசி செய்து தானியங்கி தொலைநோக்கி வலைப்பின்னல் ,