editors note: prior to coming to texas a&m university in 2008 darren depoy spent 18 years at the ohio state university building both the astronomy program along with an international reputation for excellence in astronomical instrumentation together with fellow texas a&m astronomer jennifer marshall he built the first kelt system used in the set of measurements involved in new research out of ohio state detailed below a system that was later duplicated and installed in the southern hemisphere to complement the original one observing the northern hemisphere skies depoy and marshall both members of the george p and cynthia woods mitchell institute for fundamental physics and astronomy and astronomical instrument builders in the charles r 62 and judith g munnerlyn astronomical laboratory are cited in the teams paper as among those essential for the initiation and successful operation of the kelt-north and kelt-south surveys their brief comments on the discovery are below: depoy: its a pretty weird planet this discovery hints that the process of planet formation is even more diverse than we thought and that it happens around stars more massive than the sun marshall: weve found several planets but nothing as interesting as this one kelt-9b (red) is tidally locked to its star kelt-9 (white) just as the moon is to earth (credit: robert hurt nasa/jpl-caltech) a newly discovered jupiter-like world is so hot that its stretching the definition of the word planetwith a day-side temperature of 4 600 kelvin (more than 7 800 degrees fahrenheit) planet kelt-9b is hotter than most stars and only 1 200 kelvin (about 2 000 degrees fahrenheit) cooler than our own sun in this weeks issue of the journal nature and at a presentation at the the 230th meeting of the american astronomical society an international research team led by astronomers at the ohio state university and vanderbilt university describes a planet with some very unusual features for instance its a gas giant 28 times more massive than jupiter but only half as dense because the extreme radiation from its host star has caused its atmosphere to puff up like a balloon and because it is tidally locked to its star as the moon is to earth the day side of the planet is perpetually bombarded by stellar radiation making it so hot that molecules such as water carbon dioxide and methane cant form there the properties of the night side are still mysterious molecules may be able to form there but probably only temporarily its a planet by any of the typical definitions based on mass but its atmosphere is almost certainly unlike any other planet weve ever seen just because of the temperature of its day side said scott gaudi professor of astronomy at ohio state and a leader of the study kelt-9b orbits a star dubbed kelt-9 which is more than twice as large and nearly twice as hot as our sun keivan stassun a professor of physics and astronomy at vanderbilt who directed the study with gaudi said kelt-9 radiates so much ultraviolet radiation that it may completely evaporate the planet or if gas giant planets like kelt-9b possess solid rocky cores as some theories suggest the planet may be boiled down to a barren rock like mercury animation of kelt-9bs orbit around kelt-9 (credit: robert hurt nasa/jpl-caltech) that is if the star doesnt grow to engulf it first kelt-9 will swell to become a red giant star in about a billion years stassun said the long-term prospects for life or real estate for that matter on kelt-9b are not looking good given that its atmosphere is constantly blasted with high levels of ultraviolet radiation the planet may even be shedding a tail of evaporated planetary material like a comet gaudi added while gaudi and stassun spend a lot of time developing missions designed to find habitable planets in other solar systems the scientists said theres a good reason to study worlds that are unlivable in the extreme as has been highlighted by the recent discoveries from the mearth collaboration the planet around proxima centauri and the astonishing system discovered around trappist-1 the astronomical community is clearly focused on finding earth-like planets around small cooler stars like our sun gaudi said they are easy targets and theres a lot that can be learned about potentially habitable planets orbiting very low-mass stars in general on the other hand because kelt-9bs host star is bigger and hotter than the sun it complements those efforts and provides a kind of touchstone for understanding how planetary systems form around hot massive stars stassun added as we seek to develop a complete picture of the variety of other worlds out there its important to know not only how planets form and evolve but also when and under what conditions they are destroyed how was this new planet found in 2014 astronomers using the kelt-north telescope at winer observatory in arizona noticed a tiny drop in the stars brightness only about half of one percent that indicated a planet may have passed in front of the star the brightness dipped once every 15 days the amount of time it takes for the planet to complete a yearly circuit around its star subsequent observations confirmed the signal to be due to a planet and revealed it to be what astronomers call a hot jupiter the ideal kind of planet for the kelt telescopes to spot kelt is short for kilodegree extremely little telescope astronomers at ohio state vanderbilt and lehigh university jointly operate two kelts (one each in the northern and southern hemispheres) in order to fill a large gap in the available technologies for finding extrasolar planets the research is featured on the cover of the june 19 2017 issue of nature (credit: nature) other telescopes are designed to look at very faint stars in much small sections of the sky and at very high resolution the kelts in contrast look at millions of very bright stars at once over broad sections of sky and at low resolution its a low-cost means of planet hunting using mostly off-the-shelf technology whereas a traditional astronomical telescope costs millions of dollars to build the hardware for a kelt telescope runs less than $75 000 this discovery is a testament to the discovery power of small telescopes and the ability of citizen scientists to directly contribute to cutting-edge scientific research said joshua pepper lehigh astronomer and assistant professor of physics who built the two kelt telescopes the astronomers hope to take a closer look at kelt-9b with other telescopes including nasas spitzer and hubble space telescopes (hst) and eventually the james webb space telescope observations with hst would enable them to see if the planet really does have a cometary tail and allow them to determine how much longer that planet will survive its current hellish condition study co-authors from ohio state include daniel j stevens marshall c johnson matthew penney andrew gould and richard pogge all of the department of astronomy american partner institutions include vanderbilt university fisk university pennsylvania state university the harvard-smithsonian center for astrophysics las cumbres observatory global telescope network university of notre dame lehigh university nasa ames research center bay area environmental research institute swarthmore college ipac brigham young university university of california-santa cruz university of wyoming louisiana state university university of louisville spot observatory in nashville westminster college kutztown university university of hawaii university of washington texas a&m university wellesley college and winer observatory in sonoita az international team members are from denmark italy japan portugal switzerland australia germany and south africa the study was largely funded by the national science foundation (nsf) through an nsf career grant nsf paare grant and an nsf graduate research fellowship additional support came from nasa via the jet propulsion laboratory and the exoplanet exploration program; the harvard future faculty leaders postdoctoral fellowship; theodore dunham jr grant from the fund for astronomical research; and the japan society for the promotion of science the teams nature paper a giant planet undergoing extreme-ultraviolet irradiation by its hot massive-star host can be viewed online along with related figures and captions -atm- contact: pam frost gorder (614) 292-9475 or gorder1@osuedu or scott gaudi (614) 292-1914 or gaudi1@osuedu