Meet the stars that spin so quickly they squash themselves into the shape of a pumpkin.
What happens when a star spins really rapidly? Its spherical shape can squash into the shape of a pumpkin. The rapid rotation is thought to be caused by the merging of two binary stars into one. Astronomers using observations from NASA's Kepler and Swift missions discovered a batch of 18 of these rapidly spinning stars by detecting X-rays they produce at more than 100 times the peak levels ever seen from the Sun. These rare stars were found as part of an X-ray survey of the original Kepler field of view, a patch of the sky comprising parts of the constellations Cygnus and Lyra. From May 2009 to May 2013, Kepler measured the brightness of more than 150,000 stars in this region to detect the regular dimming from planets passing in front of their host stars. These stars rotate every few days, while our own Sun takes an entire month to complete one rotation, and the rapid spinning drives increased levels of stellar activity such as starspots, flares and prominences, which generate X-rays. The most intense X-ray emission comes from an orange giant named KSw 71. This red giant is more than 10 times larger than our sun, and it rotates fully in just 5.5 days. Watch the video to learn more.
Learn about the formation of Pumpkin Stars, from their rapid spin to their intense X-ray emissions.
KSw 71 is the most extreme Pumpkin Star. It is larger, cooler and redder than our Sun, and rotates four times as fast.
Eighteen Pumpkin Stars were found in Kepler’s field of view.
Pumpkin stars form when two Sun-like stars merge.
Newly formed Pumpkin stars have an excretion disk, which will dissipate over the next 100 million years.
For More Information
Please give credit for this item to:
NASA's Scientific Visualization Studio