In the past decade, thousands of planets have been discovered beyond our Solar System. These planets have provided astronomers with the opportunity to study planetary systems that have defied our preconcieved notions. This includes particularly massive gas giants that are many times the size of Jupiter (aka. “super-Jupiters”). And then there are those that orbit particularly close to their suns, otherwise known as “hot-Jupiters”.
Conventional wisdom indicates that gas giants should exist far from their suns and have long orbital periods that can last for a decade or longer. However, in a recent study, an international team of astronomers announced the detection of a “hot-Jupiter” with the shortest orbital period to date. Located 1,060 light-years away from Earth, this planet (NGTS-10b) takes just 18 hours to complete a full orbit of its sun.
As the team states in their study, which recently appeared in the Monthly Notices of the Royal Astronomical Society (MNRAS), the planet was discovered by the
Specifically, the NGTS is concerned with finding Neptune and super-Earth sized exoplanets around bright stars. To date, the majority of large planets that have short orbital periods have been hot-Jupiters, which are the easiest to spot using passing in front of their star relative to the observer (aka. the Transit Method) – especially with ground-based telescopes.
Dr. James McCormac – a post-doctoral research fellow with the University of Warwick’s Center for Exoplanets and Habitability and a member of the NGTS – was also the lead author on the study. As he explained to Universe Today via email:
“The Next Generation Transit Survey (NGTS) is a robotic exoplanet survey designed to discover Neptune-sized exoplanets. It consists of 12 identical 20cm telescopes and is located at the European Southern Observatory in Chile. We measure the minuscule drop (as low as 0.1%) in the light intensity as a planet transits across the face of its star. To date, we have found 9 new transiting exoplanets, including 1 Neptune-like planet (NGTS-4b).”
Most of the hot-Jupiters discovered have orbital periods of around 10 days, which is what makes NGTS-4b particularly special. While ultra-short period hot-Jupiters (those with orbital periods of less than twenty-four hours) are theoretically the easiest to detect but have proven to be extremely rare. To date, only 6 of the 337 hot-Jupiters discovered have had orbital periods shorter than a day.
Using NGTS data, McCormac and his colleagues determined that NGTS-10b is about the same size as Jupiter but with roughly twice the mass. It’s host star, NGTS-10, is a relatively-active K5V main sequence orange dwarf star, which means that it is slightly smaller, dimmer and cooler than our Sun. But given how close NGTS-10b is in its orbit, the planet gets all the heat and radiation it can handle!
With an orbital period of just 18 hours, NGTS-10b is not only the shortest-period planet observed to date. It also places it
“These close-in giant planets are expected to interact with their stars tidally and eventually spiral into the star and become consumed. So, either we are very lucky to catch planets like NGTS-10b as they spiral in, or the tidal interaction processes are less efficient than we expect and the ultra-short period planets may survive at these close-in separations for long periods of time.”
In short, NGTS-10b has an orbit that places it within 1.46 ± 0.18 Roche radii of its host star, which means that it is slowly spiraling inward. At the rate they calculated, McCormac and his team estimate that its orbital period will shorten by 7 seconds over the coming decades and the planet will eventually be torn to pieces by NGTS-10.
“If the tidal interaction processes are efficient, then NGTS-10b will slowly spiral in over the next 38 million years and become consumed by the star,” McCormac said. “However, if they are less efficient the planet could live at its current separation for much longer. We hope to make further measurements in the future to determine the fate of NGTS-10b.”
In the coming decade, McCormac and his colleagues hope to conduct further observations of NGTS-10b to see if it shows any signs of in-spiral towards its star. Directly measuring the rate of infall (should there be any) will allow astronomers to place tighter constraints on the efficiency of tidal interactions between stars and planets.