HAT-P-67 b is 2.08 times the diameter of Jupiter (which has an average diameter of about 88,850 miles [143,000 kilometers]), but HAT-P-67 b is less than 60 percent of Jupiter’s mass. This makes it the least dense planet discovered so far. The large diameter is likely due to the planet’s proximity to its star. Gas giant planets like HAT-P-67 b experience extreme levels of radiation. High-energy X-rays and ultraviolet light from the star ionize the outer gaseous atmosphere of the planet, stripping it of electrons and causing it to heat up and expand. The heated outer atmosphere also begins to escape. This hot, escaping gas is called the exoatmosphere.
HAT-P-67 b was discovered in 2017, so measurements of the hot, ionized exoatmosphere have not yet been attempted. However, the size of the exoatmosphere of other hot Jupiter planets like HD 209458 b (the first transiting planet ever discovered) can be 10 times larger than the already inflated atmosphere. HAT-P-67 b’s star is evolving into a red giant, so it is brighter than it was in the past. Its increasing radiation will cause more heating and more expansion of the planet’s atmosphere in the future.
Assistant Professor, Department of Physics,
Hobart and William Smith Colleges,
Geneva, New York